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2011: Top Stories from the Best Year Ever for NASA Planetary Science!

2011 – NASA’s Year of the Solar System – The Story of How We Came to Be!
Asteroid Vesta from Dawn – Unveiling a Former Fuzzy Blob with Exquisite Clarity
NASA's Dawn spacecraft achieved orbit at the giant asteroid Vesta in July 2011. The depiction of Vesta is based on images obtained by Dawn's framing cameras. Dawn is an international collaboration of the US, Germany and Italy. Credit: NASA/JPL-Caltech

A year ago, 2011 was proclaimed as the “Year of the Solar System” by NASA’s Planetary Science division. And what a year of excitement it was indeed for the planetary science community, amateur astronomers and the general public alike !

NASA successfully delivered astounding results on all fronts – On the Story of How We Came to Be.

“2011 was definitely the best year ever for NASA Planetary Science!” said Jim Green in an exclusive interview with Universe Today. Green is the Director of Planetary Science for the Science Mission Directorate at NASA HQ. “The Search for Life is a significant priority for NASA.”(…)
Read the rest of 2011: Top Stories from the Best Year Ever for NASA Planetary Science! (2,405 words)


© Ken Kremer for Universe Today, 2011. |
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Post tags: 1 Ceres, 4 vesta, Cassini Saturn, Comet Tempel 1, Comet Wild 2, Curiosity Rover, Dawn Asteroid Orbiter, deep impact mission, Earth, GRAIL Lunar mission, Juno mission, Jupiter, Main Asteroid Belt, Mars, Mars Rovers, Mars Science Laboratory, Mercury, Mercury MESSENGER, Moon, NASA, Opportunity Rover, Search for Life, stardust mission, STARDUST-NExT

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The week in pictures: December 17–30, 2011

Astronomy Magazine News Article – Released:12/30/2011
Astronomy.com News – Presented by Astronomy Magazine

Our Picks of Best Space and Astronomy Images from 2011

First Ever Portrait of the International Space Station and docked Shuttle Endeavour from Soyuz capsule. This image was taken by Expedition 27 crew member Paolo Nespoli from the Soyuz TMA-20 following its undocking on May 23, 2011. It is the first-ever image of a space shuttle docked to the International Space Station. Endeavour at left. European ATV cargo carrier at right. Credit: NASA/Paolo Nespoli

2011 was a picturesque year! The year brought us new discoveries, a new supernova, the end of an era in human spaceflight, and much more. Here’s a look back at some of the best images we’ve posted on Universe Today in 2011, listed in no particular order:

Above, is the first-ever images of a space shuttle docked to the International Space Station were taken by ESA astronaut Paolo Nespoli on May 23, 2011 through a window inside the Soyuz TMA-20 vehicle as he and two crewmates were departing the ISS for their return trip to Earth. See the entire gallery of images of this event here.

(…)
Read the rest of Our Picks of Best Space and Astronomy Images from 2011 (1,176 words)


© nancy for Universe Today, 2011. |
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Post tags: 2011, Astronomy, Astrophotos, space, Space Exploration

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Meteor Showers in 2011

SkyandTelescope.com’s Most Recent Observing Stories

Meteor Showers in 2011

SkyandTelescope.com’s Most Recent Articles

The week in pictures: December 10–16, 2011

Astronomy Magazine News Article – Released:12/16/2011
Astronomy.com News – Presented by Astronomy Magazine

AIC 2011 Videos

SkyandTelescope.com’s Most Recent Articles

DC3 Dreams at AIC 2011

SkyandTelescope.com’s Most Recent Articles

PlaneWave Instruments at AIC 2011

SkyandTelescope.com’s Most Recent Articles

Astro Haven at AIC 2011

SkyandTelescope.com’s Most Recent Articles

Astro Haven at AIC 2011

SkyandTelescope.com’s Most Recent Articles

AIC 2011 Videos

SkyandTelescope.com’s Most Recent News Stories

The week in pictures: December 3–9, 2011

Astronomy Magazine News Article – Released:12/9/2011
Astronomy.com News – Presented by Astronomy Magazine

Watch the Dawn Eclipse of the Moon, Dec. 10, 2011

SkyandTelescope.com’s Most Recent Articles

The week in pictures: November 19–December 2, 2011

Astronomy Magazine News Article – Released:12/2/2011
Astronomy.com News – Presented by Astronomy Magazine

NASA Planetary Science Trio Honored as ‘Best of Whats New’ in 2011- Curiosity/Dawn/MESSENGER

Popular Science magazine names NASA’s Mars Science Laboratory, Dawn and MESSENGER missions as ‘Best of What’s New’ in innovation in 2011. Artist concept shows mosaic of MESSENGER, Mars Science Laboratory and Dawn missions. Credit: NASA/JPL-Caltech

A trio of NASA’s Planetary Science mission’s – Mars Science Laboratory (MSL), Dawn and MESSENGER – has been honored by Popular Science magazine and selected as ‘Best of What’s New’ in innovation in 2011 in the aviation and space category.

The Curiosity Mars Science Laboratory was just launched to the Red Planet on Saturday, Nov. 26 and will search for signs of life while traversing around layered terrain at Gale Crater. Dawn just arrived in orbit around Asteroid Vesta in July 2011. MESSENGER achieved orbit around Planet Mercury in March 2011.

Several of the top mission scientists and engineers provided exclusive comments about the Popular Science recognitions to Universe Today. (…)
Read the rest of NASA Planetary Science Trio Honored as ‘Best of Whats New’ in 2011- Curiosity/Dawn/MESSENGER (726 words)


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Post tags: 1 Ceres, 4 vesta, Curiosity, Curiosity Rover, Dawn Asteroid Orbiter, Dawn mission, Hubble Space Telescope, Mars Science Laboratory, Mercury, Mercury MESSENGER, MESSENGER, MSL, NASA, planet mercury, Search for Life

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The week in pictures: November 12–18, 2011

Astronomy Magazine News Article – Released:11/18/2011
Astronomy.com News – Presented by Astronomy Magazine

Astronomy accepting entries for 2011 outreach award

Astronomy Magazine News Article – Released:11/14/2011
Astronomy.com News – Presented by Astronomy Magazine

Leonid Meteor Shower Peaks – November 17-19, 2011

Leonid meteors seen from 39,000 feet aboard an aircraft during the 1999 Leonids Multi-Instrument Aircraft Campaign (Leonid-MAC). Comet Tempel-Tuttle provides the cometary debris for the Leonid meteor storm, which takes place in mid-November. Credit: NASA/ISAS/Shinsuke Abe and Hajime Yano

Are you ready for a good, predictable meteor shower? Then break out your favorite skywatching gear because the 2011 Leonid meteor shower is already sparkling the skies… (…)
Read the rest of Leonid Meteor Shower Peaks – November 17-19, 2011 (585 words)


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Guest blog: An imager’s take on the 2011 Advanced Imaging Conference

Astronomy magazine Contributing Editor Tony Hallas joined me at The Advanced Imaging Conference (AIC) in Santa Clara, California, November 3–6. This was the eighth annual meeting of this group. More than 300 imagers from around the world attended, and 35 vendors shared (and sold) the latest in astroimaging gear. Below is his take on the event:

Astroimager and vendor Don Goldman chats with a customer at AIC 2011. // Photo by Michael E. BakichAIC was special to me for a variety of reasons. For one thing, it was the first time I attended as a contributing editor of Astronomy magazine. Also, several of the presentations were extremely pertinent to future endeavors with my telescope.

An early presentation by Mike Rice, founder of New Mexico Skies, that dealt with the care and maintenance of telescopes was invaluable. Of special note was his discussion of the corrosion problems that all telescope electronics are prone to. Mike pointed out that most of the plugs and receptacles made for use within the safe confines of a home environment, not out in the wet, corrosive air commonly experienced during a night of imaging. He recommended two products to prevent corrosion: DeoxIT G5 and DeoxIT G5 Gold. The latter is specifically for gold contacts. He also suggested fastening wire bundles to the declination arm of a German equatorial mount to avoid tangles. He concluded with some tips on collimation and answered many questions from the audience.

Mike Rice, founder of New Mexico Skies, gave a talk titled "The 'Hands On' Challenges of Building and Operating an Imaging Observatory and How to Deal with Them." // Photo by Michael E. BakichAstroimager Steve Cannistra gave a great presentation on wide-field imaging. He stressed compositional elements and technical considerations that are necessary for a successful outcome.

Not to be missed was a presentation by Seattle-based marketing director and imager Nick Risinger of what is arguably the greatest astrophoto ever made — a 37,440-exposure mosaic of the night sky complete with Hydrogen-alpha data. He also had his camera setup on display in the vendor area.

Jay GaBany showed how he creates his unique, extremely deep images that reveal impossibly faint detail. He records these data using his camera and telescope, and he adds a healthy dose of compositional acumen.

Another presentation that I found extremely useful occurred on the last day of the conference. Paul Jones, founder of Star Instruments, with help from astroimager Richard Simons spoke about how to collimate Ritchey-Chrétien optics by analysis of the star shapes in the corners of your CCD frame. If all the stars are perfect, your optical system is aligned, but, as happens so often, some of the stars might be distorted by coma and astigmatism due to bad collimation. Essentially, a poorly aligned primary will result in comet-shaped stars, and a poorly collimated secondary will result in astigmatic stars. They offered diagrams and solutions along with a way to keep track of which adjustment does what. Without that, an imager would quickly become frustrated!

R. Jay GaBany's talk, "Awakening Your Astronomical Images" was well-received by AIC attendees. // Photo by Michael E. BakichThis year’s AIC offered many excellent workshops for all levels of imaging, including basic CCD image processing, how to use narrowband filters, how to automate image acquisition, and a “get your feet wet” introduction to PixInsight image processing.

Add to all this excellent meals and camaraderie, and it’s no surprise that AIC 2011 boasted record attendance even in this “down” economy. I look forward eagerly to next year’s event.

To see more than 100 images by many AIC members, visit Astronomy magazine's AIC online photo gallery.

You'll find Michael Bakich's previous conference blogs here (#1), here (#2), here (#3), here (#4), and here (#5).


Astronomy.com blog

The week in pictures: November 5–11, 2011

Astronomy Magazine News Article – Released:11/11/2011
Astronomy.com News – Presented by Astronomy Magazine

Get ready for the 2011 Leonid meteor shower

Astronomy Magazine News Article – Released:11/8/2011
Astronomy.com News – Presented by Astronomy Magazine

Day 1 (part 2) at the Advanced Imaging Conference 2011

I have now experienced a full day at the Advanced Imaging Conference (AIC), in Santa Clara, California. Earlier, I blogged about only the first half of day 1 to keep the length of that entry manageable.

Conference organizers scheduled two concurrent afternoon workshop sessions that paralleled the two in the morning. Those began at 1:30 and 3:30 p.m., and the speakers were the same seven who gave talks this morning.

Most of my afternoon activity occurred in the vendor area. Unlike my trek through there this morning (when it was still closed), the afternoon and evening saw a great deal of activity between attendees and manufacturers.

I chatted with more vendors, all of whom seemed happy about the AIC’s attendance and about the level of interest shown by conference-goers. One in particular was Phil Beffrey, creator of Celestial Parfait. This product is a totally free software program for astronomy and science education that runs on Windows machines. It provides a great-looking star atlas interface for pointing telescopes, it controls CCD and DSLR cameras, and it offers tools so that users can share observations. This is Phil’s first time at AIC and his enthusiasm for promoting education guaranteed that he was never alone. His hope is that astronomy clubs and teachers will begin to use it in their presentations and classes and distribute it directly to members and students. Phil encourages emails telling him a little about your astronomy pursuits. In response, he’ll send you a copy of Celestial Parfait.

The Mount Lemmon SkyCenter, always interested in teaching the latest astroimaging techniques, offered a new product by founder and world-class imager Adam Block. It comes in the form of three 4-gigabyte jump drives. Each features a different deep-sky object and contains a detailed lesson from Adam’s popular Making Every Pixel Count DVD telling how to process the image data, which Adam also included with the lesson! Visit the SkyCenter’s website at http://skycenter.arizona.edu.

I also talked at length to Kevin Nelson, head of Quantum Scientific Imaging (QSI). The company has just released a new CCD camera, its 8.3-megapixel QSI 683. I won’t say a lot about it here because one will soon be on its way to Astronomy magazine and we’ll conduct a full review of it. Look for it in an upcoming issue. This camera will find many homes, however, because QSI integrated a five-position filter wheel really close to the CCD chip. That means the camera can use 1¼" filters, which are dramatically less expensive than other sizes.

You'll find more about the AIC at the conference website. To see more than 100 images by many AIC members, visit Astronomy magazine's AIC online photo gallery. And watch for even more blogs from this super conference throughout the weekend.


Astronomy.com blog

Day 2 (part 2) at the Advanced Imaging Conference 2011

The second half of day 2 at the Advanced Imaging Conference (AIC), in Santa Clara, California, included (for me) more talks and more talking with vendors.

Alex Filippenko, professor of astronomy at the University of California, Berkeley, presented “Hearts of Darkness: Black Holes in Space.” His talk was a roundup of the properties of the various types of black holes.

After Alex, the AIC organizers alotted 1 hour and 45 minutes for its Spotlight Presentations. Three imagers, David Martinez-Delgado, Dean Salman, and Joel Hagen presented talks titled “Stellar Streams,” “Processing Tips Learned from the Sharpless Catalog Project,” and “Photoshop Tips from a NASA Image Processor.” If you’re a long-time reader of Astronomy, you may be familiar with Dean Salman’s images because many have run in the magazine during the past five years.

After supper, Adam Block of the Mount Lemmon SkyCenter would have conducted a “Remote Imaging Demonstration” from the observatory containing the 32-inch Ritchey-Chretien telescope atop Mount Lemmon. The dome, however, had frozen shut and Adam could not free it remotely. Everyone understood, of course, and they still inundated Adam with questions.

One of the showstoppers this year was a 14-foot-wide durotran backlit transparency that showed the region of the California Nebula (NGC 1499). This project, which combines an incredible 128 hours of imaging, was a four-man collaboration among Rogelio Bernal Andreo, Bob Caton, Al Howard, and Eric Zbinden. I spent quite a bit of time talking with the imagers about this amazing project, and you’ll see it as a two-page spread in an upcoming issue of Astronomy.

You’ll find more about the AIC at the conference website. To see more than 100 images by many AIC members, visit Astronomy magazine’s AIC online photo gallery.

 

You’ll find my four previous conference blogs here (#1), here (#2), here (#3), and here (#4). What a great conference! And remember, we still have a report from Contributing Editor Tony Hallas to come. I’m looking forward to that.


Astronomy.com blog

Day 2 at the Advanced Imaging Conference 2011

Day 2 at the Advanced Imaging Conference (AIC), in Santa Clara, California, started with a bang. The AIC Board of Directors presented its prestigious Hubble Award to Ron Wodaski. They bestow this honor on individuals who have demonstrated significant and sustained contributions to the astrophotography community over a period of years. Ron was one of the earliest CCD imagers. Many imagers consider his 2002 book, The New CCD Astronomy, the hobby’s bible. After the short presentation and applause, Ron gave an illustrated lecture.

He recounted a bit of his history, including the impact the book made. He also talked about being one of the first to promote remote access to a large telescope under a dark, steady sky when he opened Black Bird Observatory in New Mexico. It featured a 20-inch telescope and a sensitive CCD camera that was available to anyone with Internet access for a modest hourly fee.

Today, Ron is Director of the Tzec Maun Foundation, a non-profit group offering students and researchers free access to a variety of high-quality astronomical instruments in New Mexico and Australia. The long-anticipated centerpiece will be a state-of-the-art 1-meter telescope located in a refurbished former government tracking station. Ron talked about this fabulous facility. It’s four stories high and the doors weigh 14 tons. That’s impressive, but not as impressive as the dome. It tips the scales at 105 tons!

Eventually, the Tzec Maun Foundation plans to make even this telescope available to astronomers around the world. More than 300 AIC members certainly got excited when they heard that.

You’ll find more about the AIC at the conference website. To see more than 100 images by many AIC members, visit Astronomy magazine’s AIC online photo gallery.

You’ll find my three previous conference blogs here (#1), here (#2), and here (#3). And the conference isn’t over, so I’m not done yet!

 


Astronomy.com blog

The week in pictures: October 29–November 4, 2011

Astronomy Magazine News Article – Released:11/4/2011
Astronomy.com News – Presented by Astronomy Magazine

Day 1 at the Advanced Imaging Conference 2011

I’m at the Advanced Imaging Conference (AIC), which, for the second straight year is being held at the Hyatt Regency Hotel in Santa Clara, California. The 2011 version is the conference’s eighth incarnation. November 4–6. For the third straight year, Astronomy magazine is proud to be an editorial sponsor.

Jay GaBany, one of the conference organizers, confirmed to me that this year’s event is the largest so far. “We have more than 300 attendees,” Jay said, “including eight that arrived and registered just this morning.”

I’m writing this just before lunch, but after the first morning session. Seven speakers have already given talks in two concurrent sessions, one that started at 8 a.m. and the other at 10 a.m. In the earlier session, Adam Block from the University of Arizona’s Mount Lemmon SkyCenter, presented a 2-hour talk titled, “ABCs of Image Processing” to an enthusiastic, packed house. And Mike Rice spoke about “The ‘Hands On’ Challenges of Building and Operating an Imaging Observatory and How to Deal with Them.” Steve Leshin presented “Image Processing with PixInsight,” and John Smith spoke about “Complete Image Acquisition Automation with CCDAutoPilot.”

The 10 a.m. speakers were R. Jay GaBany (“Awakening Your Images”), Bob Denny (“The Next Generation of Observatory Automation”), and Don Goldman (“Narrow Band Imaging.”) All seven speakers will present their talks again this afternoon.

I thought registration was fun, but that could have been because, in addition to the conference agenda, each attendee’s packet contained both Astronomy’s special issue Spectacular Universe, and our November themed “Photo Issue.” Could any two publications be more suited to an imaging conference? And all went inside a plastic bag that proudly displayed the magazine’s name. It’s fun to be a sponsor.

In the vendor area (before it opened) I followed astroimager and Astronomy Contributing Editor Tony Hallas around as he interacted with various CCD manufacturers. Tony told me he already has several new ideas for his monthly “Astroimaging” column. And, from what I saw in the vendor area, there may be a few new reviews ahead as well. He’s planning to write a guest blog (that will appear here) after the conference concludes.

I talked to several vendors about new products. Paul Hobbs from Meade Instruments was happy to show off the company’s new LX800. Meade aimed this line of telescopes straight at astroimagers. Among many high points, the scopes feature the StarLock full-time automatic integrated guider. This unit assists with polar drift-alignment, finds and centers targets, and then automatically locks onto a field star as faint as 11th magnitude for guiding with an error no greater than 1". You don’t need a separate computer, you don’t have to select a guide star, and you don’t even have to focus. Just set up your camera and image. Paul and I sat at the same table at lunch and he was telling me how happy he was with the comments he’d already received. And the conference is barely four hours old!

The folks at Fishcamp Engineering also are busy readying new products. In fact, by the first of the year, the company plans to have four new CCD cameras available. Each will contain a different CCD sensor, so you’ll be able to pick your chip size, resolution, and price. You'll find more about the AIC at the conference website. To see more than 100 images by many AIC members, visit Astronomy magazine's AIC online photo gallery. And watch for more blogs throughout the weekend.


Astronomy.com blog

Previewing the Advanced Imaging Conference 2011

The eighth annual Advanced Imaging Conference (AIC) promises to be the best one yet. The 2011 event is being held at the Hyatt Regency Hotel in Santa Clara, California, November 4–6. For the third straight year, Astronomy magazine is proud to be an editorial sponsor.

This year’s speakers include regular Astronomy contributors Adam Block (“ABCs of Image Processing”), Steve Cannistra (“Wide-field Image Processing”), R. Jay GaBany (“Awakening Your Astronomical Images”), Don Goldman (“Narrowband Filter Selection and Image Processing”), and Dean Salman (“Processing Tips Learned from the Sharpless Catalog Project”).

Ken Crawford, one of the conference’s organizers, told me that he expects about the same number of participants as last year, which would be approximately 300. And he was especially happy to report that 35 manufacturers would be setting up displays.

During the meeting, the AIC Board of Directors will present its most prestigious honor — the Hubble Award — to Ron Wodaski. The organization bestows the Hubble Award “to those individuals who have demonstrated significant and sustained contributions to the astrophotography community over a period of years.” As criteria, the board evaluates production of fine images, popularization through public outreach, technical innovation, scientific contributions, and selfless direct support of other imagers.

The conference committee released this blurb about the 2011 winner: “Ron Wodaski got his start in astrophotography in the 90s. When he couldn’t find the book he was looking for to explain how to do it, he wrote one out of desperation, assuming that if he needed help, so did everyone else. One day, out of the blue, he was offered the job of running the Tzec Maun Foundation by a reader of one of those books, and he said yes. Today, the Foundation offers free telescopes via the Internet to students all over the world.”

After the award presentation, Wodaski will give a talk titled “Cosmic Wonder.” In it, he’ll chat about his love of imaging and how he got started. He also will describe the Tzec Maun Foundation’s new 1-meter telescope to AIC members, and, in his words, “how we’re making it broadly available for research, for serious amateurs like you.”

This year, each attendee’s packet will contain Astronomy’s special issue Spectacular Universe, which contains 250 stunning pictures, every one by an amateur imager. I gave a short presentation about this project at last year’s AIC during which I asked members to send me their best work for inclusion. Many did, and I’m looking forward to personally thanking them during the conference.

To learn more about the 2011 AIC, visit the conference website. To see more than 100 images by many AIC members, visit Astronomy magazine’s AIC online photo gallery. And watch for my blogs and tweets throughout the weekend.


Astronomy.com blog

Large Hadron Collider Finishes 2011 Proton Run

A new loop will be added to CERN's Antiproton Decelerator in 2016 to increase antiproton production at low energies. Credit: CERN

The world’s largest and highest-energy particle accelerator has been busy. At 5:15 p.m. on October 30, 2011, the Large Hadron Collider in Geneva, Switzerland reached the end of its current proton run. It came after 180 consecutive days of operation and four hundred trillion proton collisions. For the second year, the LHC team has gone beyond its operational objectives – sending more experimental data at a higher rate. But just what has it done? (…)
Read the rest of Large Hadron Collider Finishes 2011 Proton Run (688 words)


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S&T’s Audio Sky Tour for November 2011

With the return to Standard Time for North America and Europe, stargazers there can catch some of the evening’s offerings before dinnertime. Venus and Jupiter are planetary bookends at sunset, with Venus lurking low in the western twilight just as the King of Planets rises in the east.
SkyandTelescope.com’s Most Recent Articles

The week in pictures: October 22–28, 2011

Astronomy Magazine News Article – Released:10/28/2011
Astronomy.com News – Presented by Astronomy Magazine

Sky & Telescope December 2011

SkyandTelescope.com’s Most Recent Articles

Sky & Telescope December 2011

SkyandTelescope.com’s Most Recent News Stories

See Jupiter at its 2011 best

Astronomy Magazine News Article – Released:10/24/2011
Astronomy.com News – Presented by Astronomy Magazine

The week in pictures: October 15–21, 2011

Astronomy Magazine News Article – Released:10/21/2011
Astronomy.com News – Presented by Astronomy Magazine

The week in pictures: October 1–7, 2011

Astronomy Magazine News Article – Released:10/7/2011
Astronomy.com News – Presented by Astronomy Magazine

The week in pictures: October 8–14, 2011

Astronomy Magazine News Article – Released:10/14/2011
Astronomy.com News – Presented by Astronomy Magazine

Sky & Telescope November 2011

SkyandTelescope.com’s Most Recent News Stories

S&T’s Audio Sky Tour for October 2011

This is a month of transition: you can spot the Summer Triangle overhead as darkness falls and the winter mix of Orion, his dogs, and Taurus in the hours before sunrise. Jupiter peaks in brightness this month, and it dominates the sky from dusk until dawn.
SkyandTelescope.com’s Most Recent Articles

The week in pictures: September 24–30, 2011

Astronomy Magazine News Article – Released:9/30/2011
Astronomy.com News – Presented by Astronomy Magazine

Sky & Telescope November 2011

SkyandTelescope.com’s Most Recent Articles

The week in pictures: September 17–23, 2011

Astronomy Magazine News Article – Released:9/23/2011
Astronomy.com News – Presented by Astronomy Magazine

On the road: The 2011 Pacific Astronomy and Telescope Show, Day 2

Yesterday, Sunday, September 18, was the last day of the fourth annual Pacific Astronomy and Telescope Show (PATS) in Pasadena, California. One of the conference’s organizers told me that Saturday was the best day (attendance-wise) in the 4-year history of the event.

Since I’ve been here, I’ve seen several products you’ll be reading reviews of in upcoming issues of Astronomy magazine. And I’ve talked to other manufacturers who promised announcements of new gear soon.

Yesterday I gave my talk, “How to Buy Your First Telescope,” to a group of less than 30 people. That number, although disappointing, wasn’t unexpected because the planners scheduled me to speak before noon. Despite the low attendance, we ran out of time at the end because of the number of questions people asked. They were definitely listening.

I’ll be back in the office Tuesday getting ready for my next trip — a star party in Jacksonville, Florida, October 7 to 8, organized by Astronomy Contributing Editor Mike Reynolds. I’ll give a couple of talks and participate in all nighttime public observing sessions. And I’ll be blogging and tweeting. Sounds like fun!

For more on the 2011 PATS show, click here.


Astronomy.com blog

PATS 2011

SkyandTelescope.com’s Most Recent News Stories

On the road: The 2011 Pacific Astronomy and Telescope Show, Day 1

 

It’s that time of year again. I’m in Pasadena, California, spending the weekend (September 16–18) at the fourth annual Pacific Astronomy and Telescope Show (PATS). This gathering gives telescope and astronomy equipment manufacturers the chance to show off to lots of visitors (many of whom are nurturing their first love of our hobby) the chance to look at and discuss the latest astronomy gear. The newest telescopes, mounts, cameras, eyepieces, and accessories are all on display this weekend. And staffing each booth are salespeople and designers ready and eager to impart their knowledge to interested visitors.

 

I arrived a day early to talk to manufacturers (mostly as they’re setting up their booths) before the crush of the weekend crowd eliminated detailed conversations. I’m representing Astronomy magazine (one of the show’s sponsors) as the editor most involved in hobby and equipment stories, so I’ve been eager to learn (and report) what’s hot. But I’m also giving a talk. Because the organizers of PATS aim the get-together at the general public, I’ve chosen "How to Buy Your First Telescope" as my topic. The subject matter is near and dear to me, having helped create a special 16-page booklet by the same name Astronomy readers will find included as part of our November issue. I’m on the schedule for 11:45 a.m. today.

 

Saturday was the first “public day.” About 65 participants met to hear talks by leading astroimagers at the Riverside AstroImaging Workshop (RAW), which always meets the day before PATS. Speakers included Astronomy magazine image contributors Rogelio Bernal Andreo, Ken Crawford, R. Jay GaBany, and Warren Keller. Topics covered ranged from astrophotography for beginners to advanced imaging. Some highlights were “Planning Your Imaging Session,” “Choosing the Right Equipment,” and “Advanced Photoshop Techniques.”

 

I also walked the PATS floor Saturday. Just in the first few hours, I had great conversations with several manufacturers. And I saw new telescopes and accessories by Celestron, Meade, Quantum Scientific Imaging, and Tele Vue, to name a few.

 

Of the 38 booths I counted, there’s a mix of equipment manufacturers, astronomy clubs, and organizations supporting professional observatories.

 

Stay tuned for more blogs and tweets.

 

P.S. Good thing PATS isn’t a star party. Although the temperature is nice, the California sky is totally cloudy today.

 

P.P.S. Funny times at the registration desk: Astronomy magazine is a sponsor, we have a booth set up, and I’m speaking tomorrow, but the organizers of PATS didn’t have a name badge for me. I had to print my own. Good thing I was wearing my staff shirt!

 


Astronomy.com blog

The week in pictures: September 10–16, 2011

Astronomy Magazine News Article – Released:9/16/2011
Astronomy.com News – Presented by Astronomy Magazine

The week in pictures: September 3–9, 2011

Astronomy Magazine News Article – Released:9/9/2011
Astronomy.com News – Presented by Astronomy Magazine

The week in pictures: August 27–September 2, 2011

Astronomy Magazine News Article – Released:9/2/2011
Astronomy.com News – Presented by Astronomy Magazine

Sky & Telescope October 2011

SkyandTelescope.com’s Most Recent News Stories

Sky & Telescope October 2011

SkyandTelescope.com’s Most Recent Articles

The week in pictures: August 20–26, 2011

Astronomy Magazine News Article – Released:8/26/2011
Astronomy.com News – Presented by Astronomy Magazine

Free LIVE Broadcast of Comet Garradd – August 22, 2011

Are you ready for some excitement? How would you like to watch a LIVE broadcast of Comet C2009 P1 Garradd?! Thanks to our good friends at Barket Observatory and clear skies in Israel, we can do just that! Step inside to our virtual observatory… (…)
Read the rest of Free LIVE Broadcast of Comet Garradd – August 22, 2011 (408 words)


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The week in pictures: August 13–19, 2011

Astronomy Magazine News Article – Released:8/19/2011
Astronomy.com News – Presented by Astronomy Magazine

The week in pictures: August 6–12, 2011

Astronomy Magazine News Article – Released:8/12/2011
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The week in pictures: July 30–August 5, 2011

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S&T’s Audio Sky Tour for August 2011

This is your last chance to spot Saturn before it sinks into the evening twilight. But there are many other celestial attractions to look for on August evenings.
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The week in pictures: July 23–29, 2011

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S&T’s Audio Sky Tour for July 2011

Look low in the west at sunset to spy fleet Mercury, toward southwest for Saturn, and in the south for red-hued Antares, the “rival of Mars.”
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Close Approach: Images and Animations of Asteroid 2011 MD

Animation of 2011 MD on Monday, June 27, 2011 at 09:30 UTC. Credit: Ernesto Guido, Nick Howes and Giovanni Sostero at the Faulkes Telescope South. Click for original larger version.

Today, Monday June 27 at about 17:00 UT, asteroid designated as 2011 MD will pass only 12,300 kilometers (7,600 miles) above the Earth’s surface. Here are some images and an animation of the asteroid’s close approach taken around 09:30 UT taken by Ernesto Guido, Nick Howes and Giovanni Sostero at the Faulkes Telescope South through a 2.0-m f/10.0 Ritchey-Chretien and a CCD. The trio of astronomers say that at the time these images were taken, the asteroid had a magnitude of about 14.5. At the moment of its close approach, 2011 MD will be bright as magnitude ~11.8.

The animation above shows the object’s movement in the sky. Each image was 20-second exposure.

See more below from Guido, Howes and Sostero.

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Getting Closer: Images, Video of Asteroid 2011 MD

Asteroid 2011 MD. Credit: Peter Lake

Accomplished amateur astronomer and blogger Peter Lake, a.k.a “AstroSwanny” from Australia captured some of the first images of what will be a very close pass of Earth by asteroid 2011 MD. He actually took the image at 07:00 UTC on June 26th with a 20 inch telescope in New Mexico controlled via his iPhone, through the Global Rent-A-Scope program. Ahh, the wonders of technology! As Peter says, “Its not every day, that an asteroid misses by less than 3-5 earth Radii.”

The asteroid, which was only detected last week, is about 25 to 55 feet (8 to 18 m) across, is expected to pass less than 8,000 miles above Earth’s surface around 1 p.m. EDT (17:00 UT) on Monday, June 27th. The time of closest approach will be observable from South Africa and parts of Antarctica, but the approach will be visible across Australia, New Zealand, southern and eastern Asia, and the western Pacific.

Below is a video he compiled of the his observations of the pass, and used ten 120-second images for the video.

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Is Asteroid 2011 MD Space Junk?

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Is Asteroid 2011 MD Space Junk?

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Get ready for Astronomy magazine’s 2011 Star Products

In the September issue (on sale August 2), Astronomy magazine will once again present its Star Products awards. As before, Contributing Editor Phil Harrington and the Astronomy editorial team put their heads together and came up with a terrific list.

The items in 2011’s Star Products constitute the most innovative astronomy gadgets and gizmos on the market today. Each offers something special, and all reaffirm that it’s a great time to be an amateur astronomer.

This year, we chose 35 products from 28 manufacturers. The winning selections include 17 telescopes, and we also feature eyepieces, binoculars, mounts, a great astroimaging camera, a solar telescope, focusers, three observatory domes, and several accessories.

A concise description accompanies each product, and a full-page, alphabetized table lists the prices and the manufacturers’ websites for readers who want additional information.

Don’t miss this issue because this list will help you find the perfect holiday gift for an observer … or yourself.


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The longest day – Summer Solstice 21st June 2011

Solstice Sunset Credit:Adrian West

June 21st, 2011 is Summer Solstice – the longest day of the year.

This is the time when the Sun is at its highest or most northerly point in the sky in the Northern Hemisphere and when we receive the most hours of daylight. If you live in the Southern Hemisphere it is the reverse, so you will be having “Winter Solstice.”

Also known as “Midsummer” the Summer Solstice gets its name from the Latin for sol (sun) and sistere (to stand still). The Sun reaches its most Northerly point and momentarily stands still before starting its journey South in the sky again until it reaches its most Southerly point “Winter Solstice”, before repeating the cycle. This is basically how we get our seasons.
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Lunar Eclipse Images from Around the World; June 15, 2011

A mosiac of lunar eclipse images by Marko Posavec in Koprivnica, Croatia.

It was an event that hasn’t happened in 11 years and won’t happen again until 2018. The total lunar eclipse of June 15, 2011 didn’t disappoint. Take a look at some of the amazing images taken by astrophotographers from around the world — well, the “eastern” side of the world anyway, as the eclipse wasn’t visible in North America. Our lead image is a fantastic mosaic taken by Marko Posavec in Koprivnica, Croatia. We have another image by Posavic below, but you can see more of his images via his Twitter account.

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Sky & Telescope August 2011

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Sky & Telescope August 2011

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Dragon*Con 2011

The folks at Dragon*Con have decided to decline having me as a guest this year. I already have my plane tickets, hotel booked, so I’m still going to go – I just signed up with a regular membership. It’s too bad, but then, this gives me the freedom to just enjoy the convention as a fan, and not have to participate in panels, help promote the convention through Universe Today, etc. I think we’re still going to do an episode of Astronomy Cast live, just because that’s so much fun. I’m bringing the whole family: wife, kids, even the mother-in-law. Anyway, you’ll see me lurking around the Astronomy Cast booth, or watching panels. It should be a fun vacation. :-) See you there!


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SDO Captures Solar Flare March 19, 2011

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Uranus and Neptune in 2011

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Uranus and Neptune in 2011

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On the Road: American Astronomical Society May 2011 meeting, Tuesday recap

After recovering from Monday’s exertions, I began my second day at the 218th American Astronomical Society (AAS) meeting feeling fresh. Science, especially relating to the worlds around other stars, seemed to be more in focus Tuesday, though amateurs still had their moments to shine.

A simple device mimics a system of transiting exoplanets, helping illustrate exactly what the Kepler mission looks for. // Bill Andrews photoFor instance, the first of the day’s talks, “The Pan-STARRS Wide-Field Imaging Survey” by Nicholas Keiser of the University of Hawaii’s Institute for Astronomy, ended with a question from the audience about the possible assistance that a citizen science project like Galaxy Zoo could provide. Keiser enthusiastically agreed, saying, “Getting non-astronomers involved in astronomy seems to be a highly productive thing.” The talk itself was all about the Panoramic Survey Telescope & Rapid Response System, or Pan-STARRS for short: its specs, goals, and some of its first data and results. (Its biggest aim is to search for potentially life-destroying asteroids, and so far, so good: “None of them are going to hit us,” Keiser said. “Yet.”)

But a conference isn’t all talks and field trips — one of my favorite parts of these things is talking face to face at the poster sessions with some of the people actually doing science. The Kepler mission and its exoplanet search figured prominently in my day’s plans, so I chatted with some of the representatives from SETI (the Search for Extra Terrestrial Intelligence) and Kepler, even getting a chance to play with a simple model of an exoplanet system. By turning a small crank, visitors could move two pea-sized planets around a light bulb, with a nearby light detector showing the corresponding drop in brightness from the transitions across the “star.” What a nifty way to show what Kepler looks for!

I also got a chance to speak with Prabal (rhymes with “trouble”) Saxena of George Mason University, who presented a poster about one of the most distant moons in the solar system, titled “An External Source for Charon’s Atmosphere: Accretion of Pluto’s Atmosphere.” It’s an exciting theory, and not just because it will be experimentally verified (or not) when NASA’s New Horizons probe reaches the Pluto-Charon system in 2015. If Saxena is right, this process of atmospheric accretion could have a significant impact on planetary science. (He also said Astronomy magazine helped him get interested in the subject to begin with; neat!)

The poster sessions at the 218th meeting of the American Astronomical Society are among my favorite events — you never know what interesting research you’ll come across! // Elizabeth Andrews photoNext up was the day’s first official exoplanet talk, “Kepler and the Architecture of Planetary Systems,” which detailed some of the newly discovered properties of the multi-planet systems the Kepler mission has uncovered. “I should be saying ‘planet candidates,' ” said the first speaker, David Latham of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, but he felt almost all of them would prove to be actual planets anyway. Astronomers can now calculate the various eccentricities, orbital resonances, and orbital inclinations of planets within the nearly 200 known multi-exoplanet systems, which are all important in theorizing their formation. The final speaker of this session, Jason Steffen of Fermilab in Illinois, suspects there will turn out to be “more than one way to form a planetary system.”

Things got a little emotional during the Henry Norris Russell Lectureship, as both AAS President Debra Elmegreen and the honoree Margaret Geller of the Smithsonian Astrophysical Observatory in Tucson, Arizona, remembered their longtime friend and collaborator, former AAS President John Huchra. He was supposed to introduce Geller, but his October death took everyone by surprise, so both speakers understandably struggled to keep their composure at times. Geller even went so far as to honor Huchra with a moment of silence, and it was clear she was dedicating the lecture to him. Titled “Mapping the Universe with Redshift Surveys and Weak Lensing,” the actual talk detailed Geller and Huchra’s early exploration of the universe, and the structures they discovered. Some of the details were a little dense, and when Geller at one point said, “Nothing is simple when you’re observing the universe,” I couldn’t help but agree.

After lunch, I headed to a session devoted to various ways of promoting “Astronomy Education & Public Outreach,” a subject Astronomy knows a little something about. All kinds of great ideas came up, from top-down NASA initiatives, to plans to get kids not just excited about science but actually performing real research, to suggestions for college cosmology curricula, re-evaluating what we mean by a “learning disability,” to an individual working hard to promote astronomy to those who might not have expected to like it (this last was Astronomy guest blogger Donald Lubowich of Hofstra University). It’s great to see so much interest in making sure the public stays interested.

This “family portrait” displays all the planet candidates the Kepler Mission has found as they transit (orbit in front of) their parent star, with our Sun and Jupiter displayed alone in the second row. // Photo by NASA/Kepler Science Team/Jason RoweNext was a double dose of heavy science. First, Chris Carilli and Rick Perley, both of the National Radio Astronomy Observatory in Socorro, New Mexico, tag-teamed through their talk, “Early Science with the Expanded Very Large Array (EVLA).” Carilli shared some of the science that’s already come from the 30-year-old array’s total overhaul, “effectively re-imagining” what’s possible in terms of studying star formation, molecular gas, and some of the most distant galaxies; Perley stuck to the upgrades and what they mean for future research, even going so far as to provide a “how to” on scheduling observing time on the EVLA.

Immediately following that was the day’s last session on exoplanets, “Extrasolar Planets: Detection and Characterization.” Now that astronomers have had a few months to play with the extensive Kepler data (released in February), they can make ever more interesting conclusions on the subject (such as the claim from William Borucki of NASA's Ames Research Center in Moffett Field, California, that nearly every candidate star will have, on average, 0.34 planet orbiting it). With the Spitzer Space Telescope helping characterize these potential other worlds and ever-improving technology to find a needle-like planet in haystack-like dusty debris, the future of exoplanet research looks bright — no wonder there’s always so many people at these talks!

The day’s final event was the SPD Hale Prize lecture, “The Sun’s Magnetic Surface,” given by Hendrik Spruit of the Max Planck Institute for Astrophysics in Garching, Germany. Not too many people attended the talk, which is too bad because they missed the random free food that accompanied it (Asian appetizers before and cakes after). Spruit discussed a few ideas behind solar behavior, and frankly described the problems behind much of the standard views. “Observations rule out the main types of models,” he said, insisting that “the magnetic field is not weak!” This alters current views behind sunspot formation and the importance of convection and diffusion in modeling behavior at the Sun’s surface. Spruit acknowledged that his views have their problems, too, but he jovially made it clear that the standard views were more wrong.

And that was Tuesday! It’s hard to believe there’s just one more full day left, but I’ll do my best to keep you updated. And, as always, be sure to follow my live tweets from the conference on @AstronomyMag (#AAS218).

Related blogs:
On the Road: American Astronomical Society May 2011 meeting, Monday recap

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On the Road: American Astronomical Society May 2011 meeting, Wednesday recap

Somehow, the third and final full day of the 218th meeting of the American Astronomical Society (AAS) has come and gone. It seems like just yesterday that I got to beautiful, if not quite sunny, Boston, Massachusetts!

The day began with an unusual talk, “Demographics in Astronomy and Astrophysics.” James Ulvestad of the National Science Foundation (NSF) was careful to stress he was giving his own views and didn’t speak for the NSF as a whole. He spoke about the growing fragmentation of the astronomy community, something he found “a little bit disturbing,” and the huge number of astronomy Ph.D.’s given in relation to the number of academic positions available in the United States (more than 4 times as many degrees as jobs). “This is not something to be depressed about,” he stressed. “You just need to be aware of the situation.” Individual astronomers and organizations need to do a better job of illuminating students on the variety of nonacademic positions out there, and to be more supportive of them.

Naturally, in a talk about demographics, Ulvestad also deplored the lack of minorities within the field of astronomy, calling the representation by women and racial minorities “abysmal.” It’s easy to forget in the 21st century how important it still is to be inclusive of these apparently marginalized folks, but diversity remains a key to innovation, he said, so astronomers need to work on this now. I found the call to arms rousing, but I noticed a guy in the row in front of me buying tickets to Boston’s Duck Tours during the talk, so perhaps Ulvestad has his work cut out for him.

The most complete map of the local universe in 3-D is, naturally, a beautiful sight by itself (purple dots are nearer galaxies, extending through the rainbow to red dots as the farthest galaxies). The gap in the middle is from the Milky Way’s stars and dust, which obscure farther galaxies. // Map by T. H. Jarrett (IPAC/SSC)Up next was a press conference featuring a variety of topics: “An astronomical assortment.” The legacy of former AAS President John Huchra again came up with the first topic, which concerned the newly released 2MASS Redshift Survey that has produced the most complete 3-D map of the local universe. “This is really John’s survey,” said Karen Masters of the University of Portsmouth in the United Kingdom; he was the driving force behind it and even wrote most of the upcoming journal paper describing the survey.

Following that, Farid Salama of NASA’s Ames Research Center in Moffett Field, California, spoke about the “Polycyclic Aromatic Hydrocarbons in Translucent Interstellar Clouds” — or, basically, the dirt between stars. For the first time, recent lab experiments have allowed astronomers to compare individual light profiles of these complex molecules in space to known ones in the lab, enabling them to better understand the makeup of this pervasive dust.

For the final “astronomical assortment,” Peter Foukal of Heliophysics, Inc., brought it all home with a metaphorical look at the Sun (which, remember, you should never do literally). Recent breakthroughs in solar brightness observations suggest our star may have been at least partially responsible for the “Little Ice Age” between roughly 1550 and 1850. Tuesday night’s final speaker, Hendrik Spruit, hinted at such a connection, but didn’t say much beyond how “controversial and political” a theory it was, so it was nice to hear a bit more about this interesting idea.

Debra Fischer of Yale University spoke about exoplanets past and present Wednesday at the 218th meeting of the American Astronomical Society (AAS). // Bill Andrews photoI then managed to squeeze in one more exoplanet talk for the week, and this one happened to feature a familiar face — or at least a familiar rhetorical style. Yale University’s Debra Fischer, who wrote Astronomy’s October 2010 cover story, “How astronomers will find another Earth,” gave a lecture titled “From Hot Jupiters to Habitable Worlds.” As she eyed the packed crowd, she said “This is a field that has exploded,” and the various exoplanet-related sessions (and their popularity) would seem to bear her out. She started with the history of exoplanet research and moved through to the present era, exploring the various methods of discovery, before getting to the current state of knowledge. Perhaps the most important recent development is the relative abundance of rocky, earthlike worlds out there, which until recently had been overshadowed by the bigger, gassier “hot Jupiter” type planets. “Earths are pretty common,” she said, with about 7 times as many super Earths as Jupiters. “That’s pretty exciting.”

Speaking of which, the next session I attended focused on ways to use astronomy to help make college physics classes more interesting. The speakers elaborated on various means, such as cosmology, planetary nebulae, and yes, even exoplanets, to teach the basic concepts of physics. As Harvard’s David Charbonneau put it, why use meaningless balls and frictionless planes to illustrate these ideas when you can use distant worlds and galaxies instead? The talks focused a little too heavily on specific teaching advice for my taste, but it was still interesting to learn new and creative ways this old science can be taught.

The final talk returned to one of my — and everyone else’s, it seems —favorite topics as Ryan Hickox of Durham University in the United Kingdom discussed “What Drives the Growth of Black Holes?” Beginning with the definitions of a black hole, their supermassive, super-bright, and galaxy-centering forms as Active Galactic Nuclei, and even their ultra-bright iterations as quasars, Hickox led the packed audience through what’s presently known about these enigmatic objects. In particular, he described the theory that quasar galaxies (perhaps brought on by galactic mergers) could be an intermediate step between younger star-forming bluer galaxies and older “dead” red galaxies. By switching between admittedly primitive cartoon models and cutting-edge visual simulations, Hickox did a great job explaining such a complex topic to the general audience.

The AAS tried something new this time around, holding a closing reception full of food, fun, and door prizes. Early judgments call it a success. // Elizabeth Zakszewski photoAnd then, once again, it was time to venture to the nearby Fairmont Copley Plaza, this time for the closing reception (the timing of which made me feel a little bad for Thursday’s presenters). It was actually the first time AAS has tried having a closing reception, and between the nine door prizes, the delicious free food (more crab cakes!), and the friendly atmosphere, I’d say it was a good idea (even if I didn’t win anything).

Well, that’s it! I don’t know how the week has gone by so quickly [insert relativity joke here], but my time in Boston is almost at an end. And just like last time, I’ll be sorry to leave. Yet I’m starting to get a little homesick for Wisconsin by now, so I’ll probably be all right.

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On the Road: American Astronomical Society May 2011 meeting, Tuesday recap

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On the Road: American Astronomical Society May 2011 meeting, Sunday recap


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On the Road: American Astronomical Society May 2011 meeting, Sunday recap

The 218th meeting of the American Astronomical Society (AAS) officially began Sunday, with the opening reception taking place in Boston’s Fairmont Copley Plaza (just a stone’s throw from the famous Boston Common, and right next door to the shapely Hancock tower). It’s a real thrill staying and, ostensibly, working so close to one of Beantown’s most famous landmarks, and really helps drive home that I’m back in familiar territory.

The crowds gathered for the opening reception of the 218th meeting of the American Astronomical Society in Boston, Massachusetts, at the Fairmont Copley Plaza’s Grand Ballroom. // Bill Andrews photoThe reception, as in years past, wasn’t so much a ceremony as just a chance for attendees to get together and mingle, chat, network, etc. No official bell marked the start of the conference, as I’d vaguely imagined last year before attending my first AAS meeting, and that’s fine. This crowd doesn’t seem overly concerned with formality, which makes sense because the AAS conference also meets with the American Association of Variable Star Observers (AAVSO), a group of almost professional-level amateur astronomers.

And so, the reception began slowly, in waves, as everyone entered the room and decided which food to eat first. This being Boston, we could smell the seafood selection before we saw it, and got to choose from crab cakes, lobster ravioli, cod and potato cakes, as well as traditional cocktail party fair like roast beef and an assortment of cold meats and cheeses. Hundreds of scientists, professors, students, amateurs, and even a few lucky members of the press crowded in and partook, enjoying the last night before the conference begins proper Monday morning.

Because I just got off the plane Sunday, I didn’t have much time to do anything except attend the aforementioned festivities. Everyone seemed excited about the talks and announcements coming this week, and Monday’s schedule looks especially crowded (a full day of talks, press conferences, and meetings — including a rumored talk with a component delivered in song — plus a chance to visit the Boston Museum of Science’s Charles Hayden Planetarium, plus an open house at the Cambridge headquarters of the AAVSO). I’m sure Sunday will prove to be my lightest day here, which is just how I like it!

Keep checking back for more reports from the AAS meeting, and be sure to follow @AstronomyMag for live tweet updates (#AAS218).

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On the Road: American Astronomical Society May 2011 meeting, Monday recap

There was something for everyone Monday at the first full day of the 218th meeting of the American Astronomical Society (AAS) in Boston, Massachusetts, held jointly with the American Association of Variable Star Observers (AAVSO). Fittingly, both AAVSO Director Arne Henden and AAS President Debra Elmegreen handled the first talk, the Welcoming Address (which is about as close to the “official bell” I still naively expect at the opening reception). As it turned out, the scientist/amateur (not that Henden is any kind of amateur!) connection lasted almost all day.

American Association of Variable Star Observers (AAVSO) Director Arne Henden popped up numerous times throughout my first day of the American Astronomical Society’s 218th meeting in Boston, Massachusetts. Here, he’s in the midst of a press conference, explaining the AAVSO’s contribution to a NASA project to have the Hubble Space Telescope observe the star Hubble variable 1. // Elizabeth Andrews photoImmediately after the welcome, Elmegreen introduced Malcolm Longair of the Cavendish Laboratory in Cambridge, England, who discussed some of the subject’s long-term goals in his talk, “The 2050 Decadal Survey of Astronomy and Astrophysics.” He advised, “Be persistent and patient and never give up,” and keep trying to persuade the government of “the societal benefit of the astronomical enterprise.” He also gave a subtle shout-out to the importance of smaller and midscale telescopes, a perfect prelude to the next session I attended.

Led by the AAVSO, “Astrophysics with Small Telescopes” discussed, well, the astrophysics possible through small scopes. Many of Astronomy’s readers would have felt at home during these talks, which extolled amateur observers and their dedication, ingenuity, and even technical skills. Henden returned for the first science talk, “Contributions by Citizen Scientists to Astronomy,” which outlined the essential ways amateurs can help, including long-term deep-sky imaging, variable-star observing, and planetary monitoring (such as Australia’s Anthony Wesley’s numerous discoveries of odd phenomena on the gas giants). Henden also discussed some indirect ways the lay public can advance science, too, such as with the ever-popular Galaxy Zoo and as potential sources of visually pleasing simulations (after all, who better to get something to look nice than an experienced astroimager?). One particular project that garnered a lot of attention, and even its own talk, was the Epsilon (ε) Aurigae eclipse, which has relied on public participation to achieve fantastic results. “And the good news is, the eclipse is not over!” said the speaker, Robert E. Stencel of the University of Denver Observatories in Colorado, in a semi-call to action.

Not everything highlighted the importance of non-professional astronomers, though. The morning’s big talk, titled “Stars, Planets and The Weather: If You Don’t Like It Wait 5 Billion Years,” was not quite as public-friendly as the others. Luckily, presenter Jeremy Drake of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, as the title hints, was an amusing (and often amused) speaker. He regaled the crowds with a thorough look at how stellar weather (both of our Sun and the host stars of distant exoplanets) evolves and how it can affect the development of any nearby planets. For instance, the concept of a star’s habitable zone — where temperatures would be just right for liquid water, and thus life as we know it, to form — is but one factor to consider when judging the true habitability of any planet. Mars technically lies within our Sun’s habitable zone, but its small size and correspondingly weak magnetic field allowed the Sun’s emissions to strip the Red Planet of much of its water. Similarly, if an exoplanet lies within the habitable zone of a red-giant star, it will have a dramatically closer orbit than our world, leading to other potentially fatal stellar weather problems. He closed by mentioning some of the controversial research linking cosmic rays to cloud formation, and how such a relationship would interact with our Sun’s output to help explain some of the weather on Earth. After talking about our local star, our home planet, and the possible living worlds around other stars, Drake finished, “It literally doesn’t get any sexier than that.” How true.

The other fairly technical talk was by Ronald L. Gilliland of the Space Telescope Science Institute in Baltimore, Maryland, “Stellar Astrophysics from the Kepler Mission.” Yes, the famous exoplanet-hunting Kepler orbiting telescope has also produced “a real treasure-trove of results” in terms of stellar data, in particular for Sun-like stars and red giants. Before Kepler, astronomers had just about 25 good targets for this kind of research; now they have more than 500. Clearly, Kepler’s been pulling its weight.

The rest of the day’s events, however, did seem especially geared to non-practicing astronomers. First, a press conference titled “The most important object in the history of cosmology” discussed recent Hubble Space Telescope observations of the eponymous object: Hubble variable 1, a Cepheid variable star in the Andromeda Galaxy (M31). It was this star’s varying light that allowed Edwin Hubble to calculate a more accurate distance for Andromeda — and prove that it was not just another nebula in our Milky Way Galaxy, but a galaxy in its own right. As Hubble winds down its operations, it’s a fitting tribute that it observe this famous object for the first time, with the AAVSO’s help (Arne Henden showed up once more), this past winter.

Boston University’s Alan P. Marscher brought down the house with his original songs at an already-packed session discussing novel ways to raise interest in astronomy. // Bill Andrews photoHeartwarming as that is, it pales in comparison to perhaps the liveliest AAS session I’ve ever been to (in all my long year attending). “Astronomy Unexpected! Innovative Strategies for Reaching Non-Traditional Students” featured lively, animated speakers talking about fun, interesting ways to reach unwilling astronomy students, whether it’s actual college students, a fifth-grade class, or your neighbors. The “Galileo Impersonator" put on a great show, and poetry, personal simulations, and even science-fiction movies (yay!) all proved their worth as possible entry points for a good discussion on astronomy. But the final speaker, Alan P. Marscher of Boston University in Massachusetts, brought the house down with two of his original songs, “Relatively Weird” and “Another Planet.” (Check out these and others at http://www.bu.edu/blazars/songs/index.html.) As promised, he delivered interesting facts and ideas through the medium of rock ballad, and even got a few standing ovations. By the session’s end, the crowd was standing-room only.

In fact, that session’s moderator and first speaker, Noreen Grice, also has a book coming out about a different kind of astronomy outreach: making sure to include the disabled. After Astronomy honored the Santa Barbara Astronomical Unit for its similar efforts, it seems only fair to mention Grice’s work, Everyone’s Universe. She even had a special press reception highlighting the book, featuring chocolate chip cookies! Naturally, it was a crowded room — everyone enjoys indulging both their sweet tooth and their humanitarian side.

The day ended with a couple of field trips, or, at least, it was supposed to. Again, both were more about the importance of moving astronomy beyond practicing astronomers. The first, a press night at the Boston Museum of Science’s Charles Hayden Planetarium was just so much fun that I never made it to the second, an open house at the AAVSO’s headquarters. It’s too bad, because I was really curious to see the home of this century-old organization (especially because, as it turns out, I lived four blocks away from it for about a year). But that’s just a testament to the power of the planetarium, which recently finished some serious renovations.

I recall seeing a few shows there in my collegiate youth, but the memories pale in comparison to the dizzying new visual heights the place is now capable of. Guided by the nimble hands of Astronomy Contributing Editor Martin Ratcliffe, we saw in unbelievable clarity the visual processes behind the Moon’s phases, the solar system’s orbital plane, a 3-D rendering of the constellations, and a powerful zoom-out that left the Milky Way Galaxy just a speck within a speck. Ratcliffe gave us a half-show/half-demo mix because so much of the audience was already aware of, say, how lunar eclipses work. If you happen to find yourself in Boston anytime soon, I definitely recommend you check out the newly opened planetarium.

And that was my first day at AAS! Whew! Again, it was a super-crowded and unusually full day, so don’t expect Tuesday’s and Wednesday’s recaps to be similarly extensive. Be sure to check those out right here, though, and remember to follow @AstronomyMag’s live coverage on Twitter (#AAS218).

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On the Road: American Astronomical Society May 2011 meeting preview

Once again the time has come for a meeting of the American Astronomical Society (AAS), and this time I’ll be the one heading out to cover it for Astronomy. Officially starting on Sunday, astronomers from all over the country will converge on Boston, the self-styled “Hub of the Universe," to discuss all the latest findings in planetary science, exoplanet research, high-energy astrophysics, cosmology, and so on.

I’ll be blogging and tweeting coverage, sporting the hashtag #AAS218, for the 218th meeting of the AAS. This year, the conference will also meet with the American Association of Variable Star Observers, which celebrates its 100th anniversary in the fall. Their headquarters, along with some of the many interesting science-y destinations in the Boston area, also serve as destinations for certain conference meetings and get-togethers, so it looks to be an extra-exciting year.

Not only am I excited to attend the conference, but it’ll be great to be back in the Boston area, where I spent some time going to school. I haven’t been there in 4 years, so it’ll be nice to visit a few of the old neighborhoods (and perhaps a certain college campus while I’m at it).

Be sure to keep up with the Blogs from the Local Group and @AstronomyMag to hear all about the conference, and if you happen to be attending, make sure to say hi!


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NEAF 2011: How did you get interested in astronomy?

I had a great time attending the 2011 Northeast Astronomy Forum (NEAF) held in Suffern, New York, April 16–17. During the event, I wandered from booth to booth with a small video camera in hand asking astronomy vendors, astroimagers, and one very happy Astronomy contest winner one simple question: “How did you get interested in astronomy?” Check out the three videos below to see the answers of people like NEAF Solar Star Party’s Barlow Bob, Meteorite Men’s Geoff Notkin, Astronomy Contributing Editor Mike Reynolds, representatives from Software Bisque, Celestron, Explore Scientific, and DayStar Filters, and many more. Hopefully, their answers will encourage you to reflect on how you first got into this great hobby. Then share your stories in the comments section below.

PART ONE: Barlow Bob, NEAF Solar Star Party; Steve Bisque, Software Bisque; Fred Bruenjes, Moonglow Observatory; Tom Davis, astroimager; Neil Fleming, astroimager

PART TWO: Carroll Iorg, Astronomical League; Imelda Joson, Writer and astrophotographer, Kevin Kawai, Celestron; Ruben Kier, astroimager; Geoff Notkin, Meteorite Men; Benjamin Palmer, Astronomy Youth Essay Contest winner 

PART THREE: Gary Palmer, astroimager; Greg Piepol, Solar imager; Mike Reynolds, Florida State College; Scott Roberts, Explore Scientific; Alan Traino, NEAF; Jen Winter, DayStar Filters 


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Weekend Observing Challenges – May 13-15, 2011

Greetings, fellow SkyWatchers!

I’m sure everyone has been enjoying following the morning planet show, but are you ready for something else? If you’ve got a telescope, then we’ve got some projects for you. While it’s definitely going to be a “moon light” weekend, that doesn’t mean that you can’t have fun! Let’s take a look at what the night has to offer… (…)
Read the rest of Weekend Observing Challenges – May 13-15, 2011 (525 words)


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NEAF 2011 Videos Are Here!

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On the road: IceCube and particle physics symposium, April 29–30, 2011

Hundreds of astrophysicists were in Madison, Wisconsin, Wednesday through Saturday of last week to celebrate the completion of the IceCube neutrino detector — on time and on budget. (This is a pretty awesome achievement in astronomy experiments.) While talks on Wednesday and Thursday were geared toward general science in Antarctica, the presentations on Friday and Saturday related to more-general particle astrophysics and cosmology.

Members of the IceCube team pose in front of the deployment tower after they complete the huge neutrino detector in Antarctica. They placed the last string December 18, 2010. // Photo by NSF/C. CarpenterFriday had a few sessions about the history of neutrino detectors and what processes create these “ghostly” particles. (Scientists refer to neutrinos as “ghosts” because they interact extremely weakly with matter and have tiny masses.) The first proposal to utilize water or ice for a neutrino detector was published in 1960. Nearly 2 decades later, the first underwater neutrino experiment began construction; however, it was never completed due to electronic problems. This project, DUMAND (Deep Underwater Muon And Neutrino Detector Project), was supposed to be located in the Pacific Ocean. While DUMAND didn’t work as planned, researchers did gain knowledge about how the detectors operate in water, or ice.

Scientists proposed the Antarctic Muon And Neutrino Detector Array (AMANDA) in 1988. This project, the precursor to IceCube, began construction in 1991, and was completed in 2000. AMANDA then became part of the next-generation neutrino ice detector: IceCube.

The National Science Foundation gave this 0.23-cubic-mile (1 cubic kilometer) neutrino experiment the go ahead in 2004. Scientists installed the first detector string of 60 digital optical modules (DOMs) in January 2005. They installed the 86th string — the last one — December 18, 2010. Scientists say 98 percent of the 5,160 optical detectors are working properly, which is a good thing, as all DOMs are now frozen within the Antarctic ice.

IceCube is looking for high-energy neutrinos. These particles are created in the same astrophysical processes that produce cosmic rays. Scientists, however, are unsure of what sources can create high-energy cosmic rays and neutrinos. Antarctic polar ice is an ideal medium for detecting neutrinos: It is pure, transparent, and has no radioactivity. So, the goal is to collect high-energy neutrinos and trace their paths back to their sources.

The talks both Friday and Saturday were filled with congratulatory remarks to the IceCube team. It took a lot of new technology and hard work to get this project up and running on time. Here’s hoping the huge experiment will do equally huge science in the next few years.

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On the road: The Antarctic Science Symposium, April 27, 2011

The Antarctic Science Symposium in Madison, Wisconsin, started off with a few presentations about drilling technology. It’s definitely an important topic because one of the reasons scientists utilize Antarctica as a lab is the ice — either used as a detection material, or a record of climate change. However, Astronomy magazine doesn’t cover drilling technologies, so on to what you, the readers, really want to know.

For IceCube, scientists drill  8,040-foot (2,450 meters) holes into Antarctic ice and lower a string of 60 detectors into each hole. When a neutrino triggers a reaction with an atom in the ice, the newly created particle produces flashes of light, which detector modules record. // Mark Krasberg/NSF photoScientists are planning to install a lot of detectors in Antarctica. They’re utilizing the open skies, minimal TV and cellphone frequencies, dry air, and pristine ice. The IceCube project is an extension of a previous neutrino observatory near the South Pole called AMANDA. IceCube is on schedule for at least 3 years of operation, and after that, scientists want to build off this project by possibly creating an even larger neutrino detector. Such a plan is in the very early stages, however.

A project that is a bit further along is a radio-frequency detector in Antarctica. So, instead of detecting blue flashes of light (called Cerenkov radiation) from high-energy neutrinos — which is a simplified description of what IceCube does — this detector will look for lower-energy radio signals. Lower-energy photons have longer wavelengths, so the detectors can be spaced farther from each other. This project — the Askaryan Radio Array  (ARA) — will be huge. How huge? Some 80 square kilometers — that’s 31 square miles. The ARA collaboration hopes to detect about 1,000 high-energy neutrino events each year. Right now, scientists expect to detect about two such events with IceCube. Making a bigger array means they can reach higher energies.

Why are these experiments important? Neutrinos originate in the same processes that generate cosmic rays — high-energy protons and other atomic nuclei. Scientists don’t yet know what methods create these particles. Because cosmic rays have an electromagnetic charge, they interact with galactic magnetic fields and thus change direction. Neutrinos, on the other hand, are chargeless and interact extremely weakly with matter. So, by detecting high-energy neutrinos, scientists can learn about the processes that generate cosmic rays. And bigger experiments will capture more particles.

It seems “bigger is better” isn’t just for optical telescopes, but all detectors.


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On the Road: Northeast Astro Imaging Conference, April 15, 2011

Friday, April 15, the second and final day of the 2011 Northeast Astro Imaging Conference (NEAIC), proved to be even better than the first. NEAIC occurs at the Crowne Plaza Conference Center in Suffern, New York.

This is a new facility for NEAIC, which, until this year, was held at Rockland Community College, the site of the Northeast Astronomy Forum (NEAF). One of the conference organizers told me that they had to limit the attendance of prior NEAICs to 120 attendees because of the limitations of the college's adjacent rooms. The new facility is larger and has more rooms, so attendance this year is all the way up to 175.

Many of these would-be astroimagers are new to the hobby, which really pleased all the speakers I talked to. Probably the most popular was retired software engineer Dave Snay. He conducted a four-part series yesterday and today for beginners. He outlined main points about telescopes and astroimaging, and attendees packed every talk. A NEAIC organizer told me that he'll put such talks in the big room next year. (One of the rooms holds approximately 25 percent more than the others.)

Like yesterday, I chatted with some old friends. Contributing Editor Mike D. Reynolds and I shared a nice supper and chatted about new products, possible upcoming reviews and stories, and what each of us was most looking forward to at NEAF.

Vic Maris of Stellarvue Telescopes promised to send Astronomy magazine one of his new 105mm refractors so we can conduct a review of it. Likewise, Tim Puckett of Apogee Instruments will be sending us one of the company's latest CCD cameras and filter wheels. And I'm sure more products will turn up.

Because NEAF starts tomorrow!

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On the Road: Northeast Astro Imaging Conference, April 14, 2011

The Northeast Astro Imaging Conference (NEAIC) kicked off Thursday, April 14. This meeting of astroimagers occurs during the 2 days preceding the Northeast Astronomy Forum (NEAF). Both are held in Suffern, New York — NEAIC at the Crowne Plaza Conference Center, and NEAF at Rockland Community College.

NEAIC is a much more focused event than NEAF, which caters to skygazers of all levels, and even to those with only a passing interest in the hobby. NEAIC blends imaging talks from professional and amateur astronomers with vendors eager to sell tthe latest equipment to those who pursue photons from distant celestial sources.

As I ambled from room to room to sample the talks, I heard a wide array of subjects. After NEAIC organizers made some introductory remarks, Steve Howell of NASA's Ames Research Center kicked off the conference by speaking about the current Kepler mission and how images are collected and analyzed. Then the concurrent sessions began.

At 10:45 a.m., professional photographer Jerry Lodriguss revealed secrets of DSLR astrophotography, while software developer Tom Field talked about real-time spectroscopy. At the same time, retired software engineer Dave Snay was introducing beginners to telescopes and astroimaging.

Between talks, I wandered the vendor area. NEAF is known for having a huge college gymnasium filled with manufacturers displaying their latest and greatest. Not so much with NEAIC … until this year, that is. In fact, the number of vendors who set up displays amazed me.

Among them were some old friends. Brian Deis of Vixen Optics showed me a brand-new tripod-mounted drive you can attach to a DSLR that I predict is going to revolutionize wide-field imaging. And the price won't scare anyone, either. He only had a prototype with him (and he wouldn't give it to me!), but look for a full review in Astronomy magazine — probably early in 2012.

Al Nagler of Tele Vue Optics demonstrated an eyepiece that the company just announced Wednesday. It has a 72° apparent field of view with a comfortable 20mm of eye relief. He had prototypes of the 6mm and 10mm models.

In other words, manufacturers are producing new products. This is a great sign for amateur astronomy.

And here's another encouraging sign from one of the talks: A speaker asked the crowd, "How many of you are attending your first imaging conference?" Ninety percent in attendance raised their hands! It shows that the hobby we all love is, indeed, reaching new people.

More tomorrow!

 


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S&T’s Audio Sky Tour for April 2011

Look out! Jupiter is no longer ruling the evening sky, and sky critters are on the march in the north, east, and south.
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Saturday, March 26, 2011 – Lights Out for Earth Hour!

At 8:30 PM on Saturday 26th March 2011, lights will switch off around the globe for Earth Hour and people will commit to actions that go beyond the hour. We need you… (…)
Read the rest of Saturday, March 26, 2011 – Lights Out for Earth Hour! (340 words)


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Focusing on astroimagers in 2011

The Bates College Museum of Art in Lewiston, Maine, is mounting the exhibition “Starstruck: The Fine Art of Astrophotography” in the latter half of 2012. The exhibition will include a juried section and is open to imagers from around the world.

Jurors include Weston Naef, curator emeritus of photographs, J. Paul Getty Museum; Jerry T. Bonnell, one of the masterminds behind the popular “Astronomy Picture of the Day” website; and Dennis diCicco, senior editor of Sky & Telescope. The museum staff believes this will be the first art museum exhibition to focus on astrophotography.

Astrophotographers must submit works to the juried portion of the exhibition by the end of August 2011. For more information, visit the exhibition website or contact Anthony Shostak, Lead Curator-Starstruck, Bates College Museum of Art, 75 Russell Street, Lewiston, ME 04240.

Both an art exhibition by the Bates College Museum of Art and a special issue by Astronomy magazine will highlight the work of astroimagers this year.Incidentally, Astronomy magazine will publish Spectacular Universe in May. This special issue will feature more than 200 incredible images taken by amateur astroimagers from around the world. If you preorder Spectacular Universe, you’ll save $ 1 off the cover price and receive free shipping.


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Videos from the 2011 Tucson Gem and Mineral Show

The annual Tucson Gem and Mineral show is a huge event that draws more than 100,000 to the city each year to look at hundreds of thousands of minerals, gems, meteorites, beads, pieces of jewelry, and other items that rock and gem folks just love — and all of it’s for sale. The show is the biggest event within the meteorite world and brings together hundreds of dealers and collectors. This year, Editor David J. Eicher spent 5 days checking out the “satellite shows” and the main show, talking to collectors and shooting video.

While at the 2011 Tucson Gem and Mineral Show, Editor Dave Eicher had the chance to interview Geoff Notkin and Steve Arnold, better-known as the Meteorite Men, as well as Anne Black, a world-renowned meteorite collector. Click on the image to go to the videos. David J. Eicher photo First, Dave had the chance to spend a half-hour with collectors Geoff Notkin and Steve Arnold, better known as the Science Channel’s Meteorite Men. In a five-part interview, Geoff and Steve share memories from the show and plans for upcoming episodes, as well as discuss amateur involvement in meteoritics and the different paths of specialization in collecting.

Then, Geoff spent some time taking Dave through the Aerolite Meteorites room (Geoff's company). While in Tucson, Geoff displayed a large Moon rock, a variety of historic pieces, and a 328-pound Nantan iron meteorite, among other treasures.

And finally, Dave visited Anne Black of Impactika and took a tour of her room, as well. Anne is well-known for her vast collection of thin sections, which she had on hand — all 275 of them!

To see all of Dave’s videos, check out the 2011 Tucson Gem and Mineral Show page in the Trips & Tours area of Astronomy.com. Be sure to check out his blog entries and photos from the show, as well.


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S&T’s Audio Sky Tour for March 2011

This will be a month of transition, celestially speaking: spring and daylight-saving time arrive for northern skywatchers, Jupiter makes an exit, and Saturn is waiting in the wings.
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Tucson Gem and Mineral Show: February 11, 2011

Here goes, the final report from the Tucson Gem and Mineral Show this year. Tomorrow I will head home with my Dad, John Eicher, who once again tagged along with me to the biggest show centered on meteorites and minerals in the world. Before I provide today’s report, however, I would ask you to think about a favorite saying: Earth is a planet, too. As astronomy enthusiasts, we often think about the cosmos that is “out there” and our 2-D world on the surface of our planet as separate things. However, by holding Earth minerals in our hands, we are looking at the best examples of planetary geology we can get. And because chemistry is the same throughout the universe, Earth minerals give us a look at what exoplanets may be like throughout the universe. Consider the following background:

One portion of the exhibition floor of the Tucson Gem and Mineral Show prepares to open for another day, February 11, 2011. David J. Eicher photoMost people tend to think of rocks and minerals as pretty much the same. In reality, however, they are very different. Minerals are the basic forms in which nature crystallizes matter, in its purest form. In other words, because of the chemistry of matter in the universe, certain substances combine with others in a very precise way, forming crystals of specific types.

Atoms of various kinds — carbon, oxygen, silicon, etc. — link together in ways that are determined by their chemistry and their electrical properties. This systematic process of nature, combined with varying conditions of temperatures, pressures, geography, and other factors, produce minerals inside Earth over greatly varying timescales. Some mineral crystals form quickly, as with evaporates in salt lakes, and other crystals form over thousands or even millions of years.

So minerals are the pure chemical products of atoms being assembled the way nature likes it into what scientists call crystal lattices, the framework that produces the arrangement of atoms that nature prefers. Rocks, on the other hand, are the jumbled, mixed up remains of minerals whose structure is blended by geological processes and whose atomic arrangements were taken from order to disorder. Imagine throwing a huge batch of minerals into a giant blender — rocks would be what you get out afterward.

The
“Empress of China,” a giant rhodochrosite specimen on display at
Tucson, is reportedly worth some $ 5 million. David J. Eicher
photoAlthough we have only one sample of a living planet, Earth, minerals also tell us a great deal about the universe as a whole. For decades, astronomers have used spectroscopy as a means of studying stars, galaxies, and other objects throughout the cosmos. Because of this, we know that chemistry is the same everywhere in the universe. Samples returned from the Moon and studied on Mars and other planets also show us that minerals are remarkably similar on worlds other than Earth. And as of now, scientists know of more than 500 planets outside the solar system.

While local conditions such as temperatures and pressures would vary greatly on other worlds, the fact that chemical bonds and processes are the same everywhere suggests that holding a nice mineral in your hands on Earth gives you a pretty fair estimate of what minerals might look like on other worlds. That’s an exciting prospect that ties astronomy and mineralogy together as the closely related sciences they are.

The specific composition of minerals on Earth varies greatly from mineral to mineral, of course. At present, some 4,000 minerals are known, and mineralogists are discovering more every year. Of these, about 100 are very common and easily recognizable. They are chemical compounds, solids, that generally have several elements combined in a specific way — although native elements such as copper, gold, and silver consist of just one element. And each mineral describes the exact way the elements come together in a chemical formula. For example, two elements, iron and sulfide, can combine in more than one way. Pyrite, iron sulfide with the formula FeS2, has a cubic crystallization. Marcasite, on the other hand, has the same formula, FeS

2, but crystallizes in the orthorhombic system. So the two substances, made out of the same stuff, are considered two different minerals.

The manner in which minerals crystallize is controlled by electrical charges. That a mineral compound exists at all is because the matter comes together and is electrically balanced as it combines. Charged particles known as ions, which are simply atoms with a positive or negative electrical charge, form the units that make up minerals. In some minerals, the positively charged ions, or cations, are metals. Ions called anions often group together in minerals to carry the negative charge. These ions with unpaired electrons are looking to bind with their opposites and are often called radicals. Taking pyrite as an example again, the negatively charged sulfur, S2, balances the positively charged iron, Fe. This precarious balance keeps the mineral crystal together and allows these little units, consisting of one positively charged iron atom and two negatively charged sulfur atoms, to build large crystals made of many such units. This is how minerals come together and stay together.

So with that background, I present a set of photos of things I encountered during the final day of the 2011 Tucson Gem and Mineral Show. Enjoy!

 

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Tucson Gem and Mineral Show: February 10, 2011

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Tucson Gem and Mineral Show: February 10, 2011

Yesterday was a big day for the Tucson Gem and Mineral Show, the world’s biggest event for gem and mineral collectors, meteorite enthusiasts, jewelry buyers, and beaders. The so-called “main show,” held at the Hotel Tucson Convention Center and in its 57th incarnation, cranked up Thursday morning at 10. Long lines twisted around the entrances to the show, and with the opening bell, hundreds of attendees streamed into the show, encountering an enormous mass of dealers with thousands of items for sale. Meteorites were everywhere, and I will report on the main show in greater detail later.

The Aerolite Meteorites and Impactika Meteorites rooms at the Hotel Tucson City Center (formerly the InnSuites), Tucson Gem and Mineral Show, February 10, 2011. David J. Eicher photoEarly Thursday afternoon, I had a date with the Meteorite Men, Steve Arnold and Geoff Notkin, popularizers of meteorite hunting on the Science Channel. Their show was just picked up for a third season, and we celebrated by creating a series of videos in the sales room of Aerolite Meteorites (Geoff”s company) highlighting a vast number of meteorite specimens. You’ll see these videos once I arrive back in Wisconsin early next week.

Next door, Anne Black of Impactika Meteorites also gave me an extensive tour of “goodies” in her room in the form of a video blog. I expect that if you have any interest in meteorites, you’ll want to see the latest from their rooms when the videos are posted next week.

Stay tuned for more from the main show and elsewhere. I leave you today with more images of spectacular meteorites in our ever-growing online picture gallery.

Related blog:
2011 Tucson Gem and Mineral Show: February 8–9, 2011


Astronomy.com blog

Tucson Gem and Mineral Show: February 8–9, 2011

My father John and I bid farewell to the Granite Gap dedication and to dark-sky observing in New Mexico and, on Tuesday, February 8, 2011, drove northwest to Tucson, Arizona, for the annual Gem and Mineral Show. This huge event draws more than 100,000 to the city each year to look at hundreds of thousands of minerals, gems, meteorites, beads, pieces of jewelry, and other items that rock and gem folks just love — and all of it’s for sale. The show is the big event for the meteorite world and brings together hundreds of dealers and collectors. Yet it’s actually many shows: The so-called satellite shows are set up at numerous hotels throughout the city for several weeks, and as I write, these are coming to an end. Conversely, the “main show” at the Tucson Convention Center starts today. I’ll bring you coverage of the show and its meteorites on Astronomy.com and also in a feature story in Astronomy magazine a little ways down the road.

The gang at Aerolite Meteorites relaxes during one of many discussions about meteorite hunting on Wednesday, February 9, 2011. Geoff Notkin, co-star of TV’s Meteorite Men is at right. David J. Eicher photo The center of activity for the past 2 days has been the Hotel Tucson City Center, known for years until 2010 as the InnSuites. This biggest and most active of the satellite shows hosts numerous meteorite dealers, including Aerolite Meteorites, centrally located and always a hub of activity. Its owner, Geoff Notkin, is the-well recognized star of the Science Channel’s Meteorite Men. We stopped by and talked all things meteoritic with Geoff for a considerable time, learning of his show’s success and the many hot topics that now pervade meteorite collecting. Among them is Geoff’s new book, Meteorite Hunting: How to Find Treasure from Space (84 pp., paperback, Aerolite Meteorites, Tucson, 2011; see www.aerolite.org to order). This great guide will be a must on the bookshelves of meteorite collectors for years to come. Geoff’s inventory is substantial and widely varied, including artifacts and finds from the TV episodes and lots of spectacular meteorites of all types, ranging from those for beginners up to sophisticated and extremely rare lunar and martian meteorites.

Anne Black of Impactika Meteorites showed an incredible meteorite in her room — a Sikhote-Alin from Russia lodged in a tree stump since 1947. The meteorite sold while I was in the room. David J. Eicher photoNext door to Aerolite stands the room of Anne Black, who owns Impactika Meteorites in Denver, Colorado. Anne has some of the most incredible space rocks around, including the biggest thin secton collection on the planet. As I entered her room Wednesday, she was in the process of selling an astonishing artifact — a Sikhote-Alin meteorite that fell in Russia and struck a tree trunk, having been lodged there since 1947. It’s now headed for an Australian museum. It was a breathtaking display of nature!

Numerous other meteorite dealers are here, including France’s Luc Labenne, Mike Farmer, the Comet Meteorite Shop from Russia, ELKK Meteorites, ET Meteorites, H. K. Meteorites, K. D. Meteorites, Meteorite Collection from Prague, Meteorite Caravan from Tunisia, Pani Meteorites from Vienna, and others. I also ran into celebrated mineral photographer Jeff Scovil, whose images grace the best publications in mineral collecting, such as the Mineralogical Record, and discovered that he is the son of Charles Scovil, the well-known astronomer — something I hadn’t known! I hope that you will see some of Jeff’s meteorite images in Astronomy over the coming months.

There is so much going on here, and much more to report tomorrow!  

Find more photos from the 2011 Tucson Gem and Mineral Show in our Online Reader Gallery


Astronomy.com blog

Videos: Two Different Satellite Views of the Big Snowstorm of 2011

To speak in the vernacular of the peasantry, this storm was a whopper. Heavy snow, ice, freezing rain, and frigid wind battered about two thirds of the United States, making it “a winter storm of historic proportions,” said the National Weather Service. This animation—made with images from the NOAA-NASA GOES 13 satellite—shows the giant storm developing and moving across the country between January 31 and February 2. Below is another video view from GOES-East satellite, which includes infrared water vapor imagery from January 29 -February 1, 2011.

And there’s also an update on Cyclone Yasi.
(…)
Read the rest of Videos: Two Different Satellite Views of the Big Snowstorm of 2011 (131 words)


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2011 Tucson Gem and Mineral Show preview

Outside my office today, a lake-effect snowstorm is dropping flakes the size of small birds into the Kalmbach Publishing Co. parking lot west of Milwaukee. But if the giant storm that’s set to pound much of the United States tomorrow doesn’t derail my plans, I’ll be heading to the Tucson Gem and Mineral Show (TGMS) on Friday, February 4. The TGMS is the premier event for meteorite and mineral collectors (it’s actually a conglomeration of many shows spread throughout the city). I’ll be blogging, shooting photos, and collecting videos of what’s happening in the world of meteorites for future articles in Astronomy magazine and online.

Before heading to the show, I’ll spend a couple days at Granite Gap and Rancho Hidalgo, the astronomy development southeast of Tucson that is gearing up to be an amateur astronomy mecca. There, developer Gene Turner is creating a “24/7 star party” with new observatories, RV and house sites for dark-sky observing, and imaging facilities that are transforming the area of Animas, New Mexico, into a center of amateur astronomy. Dark-sky observing at the site next week will also fuel new stories about observing over the coming year in Astronomy magazine.

At the show, I’ll report on the whole spectrum of meteorites and meteorite collecting. You’ll see video reports from dealers and what’s hot in the world of meteorite collecting.

That’s if I can make it out of the snowy Midwest on a western-bound aircraft. Stay tuned!


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S&T’s Audio Sky Tour for February 2011

February brings into view Orion and his faithful hunting dogs, a set of constellations that sparkle with bright, colorful stars.
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American Astronomical Society meeting: January 13, 2011

Thursday was my last day (or really hour) at the American Astronomical Society (AAS) meeting. I went to the morning invited talk, which is usually a great way to figure out what theories, and what scientists, are big in the field right now.

A simplified “longitudinal” map of Earth gives a rough estimate for where landmasses are on our planet. Scientists hope to create such maps from data of earthlike planets, and thus learn if these worlds harbor land. Liz Kruesi photoEric Agol of the University of Washington spoke about exoplanets. He focused on one type of detection method, transits, which occur when a planet crosses in front of its star and thus blocks light according to our view. In particular, Agol talked about what astronomers can do with the information they glean through transiting exoplanets.

The newly discovered worlds Kepler-9b and 9c were two main examples of the talk. These planets are in nearly resonant orbits, with one completing two orbits in the time it takes for the other to complete one. But to figure this out, scientists had to carefully analyze the brightness dips caused whenever the planets passed in front of their star.

He also covered ways to analyze atmospheres, and thus weather, on massive exoplanets called “hot Jupiters.” Years ago, astronomers had begun to figure out general information about one such world, HD 189733b — meaning, they could determine that one part of the atmosphere is hotter than another part, and that this is likely due to high-speed winds. (OK, it’s more complicated than that. See February 2010’s article in Astronomy magazine about weather on exoplanets for more information.)

Agol also showed how this research could extend into analysis of earthlike planets. So, to simulate what such a world’s atmosphere might look like, scientists took images in seven filters of our planet using the Deep Impact spacecraft. They then simulated an extremely basic map to provide an idea of landmasses versus oceans (and thus an estimate of the percent of land). Pretty neat.

After this talk was over, I had to head out of the meeting. Today was the last day, so I’m hopeful I didn’t miss too much. AAS meetings are always packed with information — between press conferences, oral presentations, and posters (not to mention the “town hall” meetings and just running into familiar people). You’ll definitely see some articles in future issues of the magazine from topics that came out of this meeting.

Related blogs:
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AAS meeting: January 11, 2011

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AAS meeting: January 9, 2011


Astronomy.com blog

American Astronomical Society meeting: January 12, 2011

Wednesday was another busy day at the American Astronomical Society (AAS) meeting. I ran into a few contributors to Astronomy magazine (it’s always great to meet the people I talk to on the phone) and my roommate from a summer research internship I did nearly a decade ago.

Wednesday was a big day for the Crab Nebula at the AAS meeting. NASA/ESA photoOK, back to the science. At the first press conference of the day, scientists announced all sorts of crazy stuff happening within the Crab Nebula (aka M1). Actually, they focused on the Crab’s pulsar — a stellar remnant left over from the supernova explosion that created the beautiful nebula. This pulsar emits radiation over broad wavelengths, and astronomers had long considered the pulsar stable in X-rays. So much so that scientists would calibrate their X-ray detectors using the Crab pulsar. It turns out, however, that’s probably not a good idea.

Colleen Wilson of NASA’s Marshall Space Flight Center announced that her team has seen the Crab’s energy emission decrease by 7 percent since 2008. And this wasn’t just using one detector — they looked at data from the Fermi Gamma-ray Observatory, the Swift satellite, the Rossi X-ray Timing Explorer, and the INTEGRAL gamma-ray observatory. And this wasn’t the only oddity discovered about the Crab.

The Italian high-energy satellite AGILE detected a gamma-ray flare from the nebula in October 2007. After the observatory saw another flash in September 2010, it became apparent there was some sort of repetition to this signal. AGILE researchers informed the rest of the high-energy astronomy community, and Fermi confirmed the flare just a few days later. The scientists imaged the Crab Nebula’s central region with the Hubble Space Telescope and the Chandra X-ray Observatory to see if there were any sources that could have caused the flares. They aren’t sure if the flares originated from the star’s wind, a shock wave around the pulsar, one of the jets, or the gaseous wind structure around the pulsar. The team did see (in both Hubble and Chandra data) several knots of material within one of the pulsar’s jets (and very close to the object itself) that might be related to the gamma-ray signal. They expect another flare within the year, and they hope to have Chandra and Hubble monitor the pulsar when that happens. (You can read even more about the Crab Nebula in the March issue of Astronomy, on newsstands February 1.)

Later in the day, I attended a press conference about black holes. Karl Gebhardt of the University of Texas announced that his team had made the most precise measurement yet of the supermassive black hole within elliptical galaxy M87. This black hole tips the scales at 6.6 billion solar masses. (For comparison, the Milky Way’s central black hole is around 4 million solar masses — more than 1,000 times less massive). This measurement confirms that M87’s black hole is the most massive one in the nearby universe. (Distant quasars are likely closer to 10 billion solar masses, but astronomers can’t directly measure those yet.)

Gebhardt also mentioned that the black hole’s theoretical event horizon (the radius where nothing can escape from) might be 12 billion miles (20 billion kilometers) wide, which is some 3 times the size of Pluto’s orbit. So of the black holes presently known, the one in M87 offers the best chance for astronomers to actually image its event horizon. This is important because, as Gebhardt said, astronomers don’t know if black holes are actually “black holes.” There’s no proof yet of an event horizon. There’s been talk of virtually connecting many sub-millimeter telescopes across the globe in order to essentially create a detector with a diameter of Earth’s radius. This facility could provide the resolution to directly image the event horizon of M87’s supermassive black hole. And that would be awesome.

Related blogs:
AAS meeting: January 11, 2011

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Astronomy.com blog

American Astronomical Society meeting: January 11, 2011

The Planck science team released their early results today. While the mission’s main purpose is to study the Big Bang’s “light echo” (the cosmic microwave background, or CMB), it hasn’t yet compiled and analyzed enough data to report on CMB findings. However, as the satellite surveys the radio sky looking for leftover radiation from the Big Bang, it also observes the “stuff” between the CMB and us. On Tuesday the team announced discoveries found in that “stuff” at the January American Astronomical Society (AAS) meeting. 

The microwave sky as seen by Planck. ESA imageFirst, George Helou of the California Institute of Technology talked about really cold objects that are the precursors to baby stars. These “cores” are between 7 and 17 kelvin (that’s between about –447° and –429° Fahrenheit). When combining data from Planck and the earlier Infrared Astronomy Satellite (IRAS, from some 2 decades prior), the scientists found about 10,000 cold cores. The Planck team performed follow-up observations on a number of these objects and found that they aren’t so much “cores” as they are “clumps” — the objects aren’t spherical.

The smallest of these cores measure about 1 light-year in size, which is comparable to the extent of the solar system’s Oort Cloud of icy bodies. These cores come before protostars in the star formation process. When asked what stage of human birth these objects can be compared to, Helou responded that they’re equivalent to the mother’s womb before anything has started to form … they’re early on in the star creation process. (As a side note, isn’t that a lovely comparison? I laughed when this question was posed.)

Another result from Planck is on the opposite end of the temperature spectrum. Elena Pierpaoli of the University of Southern California announced the discovery of a whole bunch of galaxy clusters (containing gas with temperatures of tens to hundreds of millions of degrees). The Planck sky survey detected 189 galaxy clusters, 12 of which have been confirmed as newly discovered clusters (and another 8 possible). The other 169 had been observed mainly in X-rays and optical radiation; this was the first time they were seen in radio.

The Planck researchers also gave AAS attendees a timeline for the mission’s CMB findings — we’ll have to wait another 2 years.

Midday, I attended a town hall meeting as a follow-up to the Astro2010 Decadal Survey. A panel of astronomers released this report in August; it provides recommendations for which projects should be the main focus of astronomers in the coming decade. This was a 2-year effort, which the survey panel clearly didn’t take lightly.

Much of the discussion in the town hall meeting focused on funding issues, especially given the current economy. And a number of undergraduate and graduate students asked about career options (how funding shortfalls might affect their futures). I actually found the meeting quite sobering. But, at the same time, it reminded me why what we at Astronomy magazine do is so important: We need to show why astronomy is so awesome, and why the public should care (and thus should pay for astronomical research). Actually, a student brought up the fact that science communication seems to be lacking.

So, dear readers, what do astronomy enthusiasts need to do better? What will help invigorate the field? How can we (the science journalists) explain the science clearer, what other modes/media do we need to involve? I’m interested to read your comments, which you can post below.

Related blogs:
AAS meeting: January 10, 2011
AAS meeting: January 9, 2011


Astronomy.com blog

American Astronomical Society meeting: January 10, 2011

A few exoplanet discoveries kicked off the press conference portion of the American Astronomical Society (AAS) meeting. (Worlds around other stars is a hot topic.) The first presentation came from a study that didn’t find what it was supposed to find. Edward Guinan of Villanova University announced that an undergraduate research project to determine the age of planet-hosting stars turned into quite the discovery. The team found out that there’s a lot of magnetic interaction between one particular star and its planet. (They were looking at the “famous” hot Jupiter HD 189733b and its star HD 189733A.) The star is taking material from the planet and is “spinning up.” This causes it to look much younger than the other star in the system, HD 189733B (that’s an uppercase B).

Kepler-10b is a rocky exoplanet that measures 1.4 times the size of Earth and 4.6 times its mass. NASA imageLater in the same press conference, we learned about a Kepler find. This mission is expected to haul in hundreds of exoplanets (back in June, scientists with the mission revealed they already had some 706 exoplanet candidates). Kepler researcher Natalie Batalha announced that the Kepler team had discovered a planet just 1.4 times the diameter of Earth. The planet (Kepler-10b) isn’t exactly habitable — it’s so close to its star that it orbits in 0.84 Earth day, and its sun-facing side has a temperature of 2500° Fahrenheit (1370° Celsius). Scientists used the planet’s mass and radius to determine its density, which is higher than Earth’s. They think this world contains more iron and nickel than our planet.

Kepler-10b dimmed the light from its star by just 1.5 parts in 10,000. This sensitivity is what makes the Kepler mission (and this discovery) so awesome. At the press conference, scientists talked about the possibility of this super-Earth being the stripped-down core of a hot Jupiter. Whatever it is, the astronomers agreed that it’s a pretty awesome discovery.

The rest of the day’s topics shifted gears — to the high-energy world and black holes. I’m a sucker for particle astrophysics, so the press conference for the Fermi Gamma-ray Space Telescope had me hooked. But no one could deny how cool their discovery was: Fermi scientists detected positrons (the electron’s antiparticle) associated with thunderstorms.

In December 14, 2009, there was an intense thunderstorm above southern Africa. The lightening produced gamma rays, which then interacted with air particles to create electrons and positrons. These charged particles traveled along Earth’s magnetic field lines to where Fermi detected them, some 2,800 miles (4,500 kilometers) away. So, gamma-ray astrophysicists discovered an Earth-science phenomenon — it’s great when findings can reach multiple areas of science. Fermi has actually observed about 130 terrestrial gamma-ray flares, but this was the first where it detected antimatter.

The day involved a number of other announcements (many of which have been posted to the Astronomy magazine news page) and a few invited talks. Interestingly, the afternoon ones had much higher attendance rates than the 8:00 a.m. talk. Astronomers don’t seem to like the mornings — who would’ve thought. It was a busy day, and I’m sure today will be just as crazy.

Related blog:
American Astronomical Society meeting: January 9, 2011


Astronomy.com blog

American Astronomical Society meeting: January 9, 2011

After arriving in Seattle Sunday, I went to the conference center to get my American Astronomical Society (AAS) meeting badge and the giant book of abstracts for the next few days. (And I ran into a friend from grad school!) Since then, I’ve been paging through the press meetings, talks, and posters to figure out which ones to attend today.

It’s insane how much research scientists present each day at AAS. To give you an idea, the poster abstracts take up 22 pages with some 15 on each page — that’s 330, just for Monday.

And yes, it’s raining in Seattle. Actually, on the shuttle ride from the airport to my hotel we encountered rain, then sleet, and finally snow!


Astronomy.com blog

American Astronomical Society January 2011 meeting preview

On Sunday the 9th, I’ll head out to Seattle, Washington, to represent Astronomy magazine at the 217th meeting of the American Astronomical Society. I haven’t been to one since 2009, so I’m pretty psyched (plus, Seattle is a wonderful city).

More than 2,700 astronomers will attend the meeting, which will cover topics ranging from planetary science to the history of astronomy to high-energy astrophysics. There are nearly three dozen press announcements scheduled, so expect to see lots of news on www.Astronomy.com/news. I’ll also blog and tweet about the conference, so keep an eye out for my updates.


Astronomy.com blog

Eclipses in 2011

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Upcoming Solar Eclipse on January 4, 2011

Williams astronomer Jay Pasachoff during the partial phase of the March 29, 2006, solar eclipse. Photo by Anna Tsykalova.

Some of the world will be able to greet the first part of the new year with a solar eclipse. On the morning of Tuesday, January 4, 2011, an eclipse of the Sun will be widely visible across Europe and as far east as India. The eclipse won’t be visible in North and South America, however. Jay Pasachoff of Williams College in the US is the Chair of the International Astronomical Union’s Working Group on Eclipses, and says that even at a maximum, this eclipse will be only partial, with some of the Sun always visible. Because the Sun is too bright to look at safely, Pasachoff stresses that special solar filters or projection methods should always be used to protect the eyes.
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NASA Budget Uncertainties Will Continue Well into 2011

The Constellation Program, still on the books for now. Credit: NASA

A temporary spending measure signed by President Obama on December 22 means NASA and other government agencies will stay at 2010 funding levels until March 4, 2011. This means, according to Jeff Foust at Space Politics, that among other items, the prohibition in the FY10 appropriations bill that prevents NASA from terminating any Constellation programs remains in effect, despite the human spaceflight plan enacted in the NASA authorization act signed into law in October.
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Shuttle Launch Delayed to February of 2011

Discovery on the launchpad. Credit: Alan Walters (awaltersphoto.com) for Universe Today

NASA announced today that the launch of space shuttle Discovery for the STS-133 mission has been pushed back to no earlier than Feb. 3, 2011, to allow for more testing on the external tank stringers. Cracks on the stringers were found after the tank was loaded with cryogenic fuel for a subsequently scrubbed launch attempt in November.

“We’ve hit a point where there is no obvious answer for what has occurred,” said shuttle program manger John Shannon at a press briefing today, “so we have to take the next step and understand to very fine level the stress on the stringers and to find if that is a root cause of what happened to the STS-133 tank. I need to better understand the conditions to fly that fly tank confidently. It’s unfortunate we are not making the December launch window. But we want to make sure that we do this exactly right.”
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