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On the road: January 2012 AAS meeting, Wednesday recap

Even though the American Astronomical Society (AAS) meeting still has another day of research presentations and invited talks, today was the last day of press conferences – and the organizers made sure it was a good one.

Virginia Trimble, Eric Mamajek, John Johnson, and William Welsh (left to right) presented during the extrasolar planet press conference at AAS. // Photo by Liz Kruesi.Members of the Kepler mission to discover extrasolar planets revealed some exciting new finds. William Welsh of San Diego State University in California announced two more cases of an exoplanet orbiting a double star system — the “Tatooine” situation. Each of these worlds (Kepler-34b and Kepler-35b) are roughly Saturn-sized, and in the first example, the exoplanet orbits two stars similar to the Sun. While the planet in the previous announcement (Kepler-16b, in September) was just outside its stellar habitable zone (HZ), Kepler-34b is a bit too close to its stars to be within the HZ. Welsh added that he and colleagues expect there to be millions more of these cases, where a planet orbits a double star, and that in the next few dozen discoveries he expects to find one in its system’s HZ.

At the same press conference, John Johnson of the Kepler team announced a planetary system containing three worlds smaller than Earth, and orbiting a red dwarf star about 13 percent the size of the Sun. The innermost planet orbits its star (KOI 961) in about 10.8 hours, and astronomers haven’t yet determined the orbital period of the other two planets, but they know both are less than two days.

After a third exoplanet announcement of an extrasolar dusty disk (with a ring system) more than 400 light-years away, Virginia Trimble, an astronomer and science historian at the University of California, Irvine, spoke about how astronomy is changing due to recent discoveries. (She specifically spoke of “paradigm shifts.” While at college, all freshmen were required to read Thomas Kuhn’s The Structure of Scientific Revolutions, and so I felt that I really got what Trimble was saying.) 

Newly discovered Kepler-34b, shown in this illustration, orbits binary stars that are similar to the Sun. // Photo by David A. Aguilar (CfA)While the topic of exoplanets seems to dominate this blog post, it certainly wasn’t the only research area discussed at today’s meeting. Steven Rodney of Johns Hopkins University in Baltimore, Maryland, announced the discovery of the most distant type 1a supernova yet. It exploded when the universe was just about 4.2 billion years old, and its light has redshifted out of visible and into infrared due to the universe’s expansion. The star that evolved into this supernova was younger than the Sun is currently (which is about 4.5 billion years) when it exploded. Astronomers expect to find supernovae in data from when the universe was just 3 billion years old.

So those were some of the science highlights of my third full day at the AAS meeting in Austin, Texas. And today, I also finally got to enjoy some tasty Texas BBQ.

Read about my Tuesday at AAS and Monday at AAS here.


Astronomy.com blog

On the road: January 2012 AAS meeting, Tuesday recap

Today was another packed day — but that seems to be the norm at the American Astronomical Society (AAS) meeting. The first invited talk echoed a topic that one of today’s press conferences covered: the status of the Fermi Gamma-ray Space Telescope. After three years in orbit, the observatory has identified more than 1,870 gamma-ray objects, including many types that hadn't been discovered before.

The Fermi Gamma-ray Space Observatory's data at its highest energies reveal the outline of the giant gamma-ray bubbles discovered in 2010. // Photo byNASA/DOE/Fermi LAT CollaborationThe Fermi team also released its view of a largely unexplored region of high-energy astrophysics. These energies are greater than 10 billion electronvolts and extend up to about 300 billion electron volts (visible light has an energy of about 2 or 3 electronvolts). At these energies, the Fermi all-sky map also shows signatures of the giant gamma-ray bubbles quite clearly. The observatory has found 496 objects in this energy region, and 168 are unidentified. Dave Thompson, Fermi deputy project scientist, added that multiwavelength observations of these unknown objects are crucial to figuring out what they are.

A later press conference focused on (pun intended) the lower end of the electromagnetic spectrum — infrared radiation. Astronomers from four projects released gorgeous images that are also jam-packed with information about star formation. Scientists can observe dust and thus trace the cold raw material that eventually becomes hot stars, and observe young stars forming behind dust clouds, using infrared light.

These four projects look at slightly different wavelengths, and so astronomers can combine data from different telescopes to see great detail. One of the observations presented today did just that: Data from both the European Space Agency’s Herschel satellite and NASA’s Spitzer telescope show current and potential sites of star formation in the Large and Small Magellanic Clouds. The images show detail about 5 light-years across.

Tuesday's second press conference focused on infrared radiation. // Photo by Liz Kruesi.Another project used Spitzer to survey the Cygnus X star-formation region, which contains all phases of star creation. The released image covers about 25 square degrees (100 times the size of the Full Moon) and contains some 4 million stars. Astronomers with the project specifically were looking for stellar objects in the early stages of formation.

In the same press conference, Xavier Koenig of the Wide-field Infrared Survey Explorer (WISE) released new findings about how massive stars form. His team selected a sample of regions in a 1,000-square-degree mosaic of WISE data, and mapped the distributions of young stars in those regions. The data indicate that stars form in a chain reaction once nearby massive star formation begins.

Tuesday included many other highlights — such as a great talk by Gaspar Bakos of Princeton University. He gave an overview of the extrasolar planet search project HATNet, which has been searching for nearly 10 years for planets passing in front of their stars. It’s found about 30 so far. This project is just one case of small telescopes doing big science. (The automated telescope system is made up of 4-inch and 8-inch scopes across the globe.)

Tomorrow promises another exciting day filled with announcements, poster presentations, and interesting talks.

Read about my recap of Monday at AAS here.


Astronomy.com blog

On the road: January 2012 AAS meeting, Monday recap

I’ve successfully survived the first full day of the American Astronomical Society (AAS) meeting. I managed to attend all three press conferences, two invited talks, a session on extrasolar planets, a few science education presentations, and the poster exhibition hall. Plus, I caught up with a few fellow science journalists and met with an associate editor of our sister publication, Discover magazine.

The LOFAR project has begun taking data, and will be completely installed later this year. // Photo by Liz KruesiAt the first press conference of the day, astronomers released the largest dark matter maps yet. They combined five years of observations from the Canada-France-Hawaii Telescope showing how the invisible dark matter in massive galaxy clusters warps background radiation. Each map is comparable to the size of the palm of your hand. The team released two-dimensional maps today, but they’ve also collected three-dimensional data and plan on incorporating this later.

After the dark matter announcement, I listened in on a few presentations about extrasolar planets. A major theme was how important it is to understand the star when investigating the planets orbiting it. The star is the system’s prime energy and gravity source, and its characteristics (especially temperature) define the system’s habitable zone — where water could possibly exist on a world’s surface. Along those lines, a talk by Billy Quarles of the University of Texas at Arlington described the habitability of the Kepler-16 system. His team suggested astronomers look to see if a moon is orbiting the Saturn-sized Kepler-16b, because if so, it could be habitable.

After lunch, we reconvened for another press conference — this one about the LOFAR radio telescope. This project is located in the Netherlands, a seemingly unusual place for a radio observatory. However, with advanced computer processing, it has so far been successful at filtering out background radio sound (although the motion of windmill blades seems to cause some problems). The LOFAR team announced today that the project’s hardware will be fully installed and online later this year, and LOFAR has already begun taking data in two bands: the low band looks at frequencies between 30 and 75 Megahertz (MHz), and the high band observes between 115 and 185 MHz. There’s a gap between 75 and 115 MHz because of FM radio signals.

Nobel laureate Steven Weinberg gave the last talk of the evening on Monday January 9. // Photo by Liz KruesiThe last session of the night — a public talk by Steven Weinberg, Nobel laureate of physics — was great, but also a bit depressing. Titled “Big science in crisis,” he focused on how difficult it is for huge science projects (such as particle accelerators and space observatories) to get funding. The current financial climate, combined with the requirement to cut 8 percent of the federal non-defense budget at the end of the year, means it will only get harder.

So spread your excitement for science, and get others interested in it. Until the public perception changes and people realize that science is important, and that it leads to incredible technology, funding will continue to decrease.


Astronomy.com blog

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).

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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


Astronomy.com blog

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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Astronomy.com blog

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).

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

On the Road: American Astronomical Society May 2011 meeting preview


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