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LIFTOFF!

Wow.

Go, baby, go

STS-130 lifted off at 4:14AM on 8 February 2010. The crew of the space shuttle Endeavor was strapped in for a second launch attempt after the previous morning’s attempt had been scrubbed for a low cloud ceiling. A few miles away, on a much emptier and slightly warmer causeway, the space tweeps gathered once again to see Endeavor lift into the sky.

The weather forecast was red for most of the night. Weather forecasters were, however, cautiously optimistic. We cheered as the forecast turned to green when the clouds broke up just before 4AM.

As the launch countdown came out of a hold and began counting down from the 9 minute mark, we raced to get our cameras, and ourselves, ready for the Big Moment. My little camera sat on a gorillapod, wrapped around a folding chair, ready for video. Aleya took some last video of us bouncing excitedly, and the guys and gals with fancy cameras got their last settings set. Tweets were sent, and we began the countdown. New Years Eve has nothing on this countdown!

At ignition start, the little white dot with the barely resolvable wings that we had been gazing at for two nights began to flare up. A cloud of smoke billowed up in front as the tiny, distant rocket began its ride up a column of fire into the sky. We screamed our little heads off. I swore I could feel the heat on my face, but maybe that was just the rush of excitement.

Unlike in all the pictures, the flames burned a bright yellow. We felt the rumble of takeoff and heard the crackling like fireworks. This was it. As the shuttle curved to our right, six astronauts were being launched into orbit.

With a cloud of smoke left behind, Endeavor became a bright star, fading slowly as it set off for the International Space Station. I almost missed the rapid brightening as the solid rocket boosters separated, as I was too busy hugging people and making sure I didn’t lose my camera. I finally started to cry, like I do for every launch I watch on tv. Only it wasn’t a quiet tear to myself, but a laughing cry! There was no time, as the voice over the speakers urged us to get away from the causeway as an acid rain cloud was on its way, and we had trekked pretty far from the car. I got my things, got back on Twitter, and kept hugging more Space Tweeps on the way.

This was my first live launch, and one of the last launches of the space shuttle program. I know that NASA’s manned spaceflight program is having a rough time, and I don’t know what to say about that. I am, however, optimistic that we’ll be reaching further and further away from our home planet, even if progress seems slow at the moment. It’s just part of our nature.

My launch video:

Aleya’s FANTASTIC video of the SDOisGO crew at both nights… plus the launch itself. With cool tunes!

So…. the launch of STS-130 was scrubbed last night. The crew of six was primed and ready to deliver the Tranquility module to the International Space Station, and the shuttle itself was all ready for liftoff! The weather, however, would not cooperate. We kept swinging between “go” and “no-go” due to a low cloud ceiling. We were out on the causeway in the 40-ish degree weather taking pictures, tweeting away, and drinking coffee and tea to stay warm and awake. We’ll be out there again tonight for the second attempt, so if you are staying/waking up, join the virtual party! (#STS130)

Endeavour

Pretty pretty shuttle pic by George. Also check out pretty pictures by Catherine. And my less pretty ones.

Also, as the shuttle gets bumped by 24 hours, so does the launch of the Solar Dynamics Observatory and all the #SDOisGO events! Stay tuned…

Thanks for the good times @privong, @blueskeyes207, @histella, @catherineq, @spacemanandy, @astrogerly, @johnmknight, @cmilesbaker, and probably more I’m forgetting! Also live-tweeting the launch were @Nancy_A, @moonrangerlaura, and @milesobrien.

I am such a happy girl right now. After some 13 hours in the car, (more for some!) George, Aleya, James and I made it to Titusville, Florida. We are here for the SDOisGO TweepUp event, and we’re catching the launch of STS-130 while we’re here! So what exactly is the SDO?

SDO stands for Solar Dynamics Observatory. This is the first mission of NASA’s Living With a Star program. We may think that Earth is the most important place in the solar system, but the Sun is the real powerhouse. We who live on this tiny rock in orbit about its fiery bulk must learn to live with what is, in its own way, a variable star.

The sun in extreme UV, as captured throughout one cycle by SOHO

The sun goes through a cycle of high and low activity. This manifests itself in a greater number of sunspots, solar flares, and coronal mass ejections about every eleven years. Sunspots are darkened, cooler areas of the sun, but they tell a tale of force and violence underneath. They are often linked with solar flares, which are explosions in the atmosphere of the sun that occur when magnetic energy is released. In an extremely energetic event, a coronal mass ejection can hurl electrons and protons away from the sun at incredible speeds, averaging 500 miles per hour kilometers per second! If a CME or flare is directed at Earth, these can cause power failures and disrupt satellites. As we become increasingly dependent on our power grids, cell phones, GPS, and yes, even your satellite radio, better forecasting is needed to predict such events. Enter SDO.

SDO has three instruments that will send back data on the Sun simultaneously and 24 hours a day. The Atmospheric Imaging Assembly (AIA) has four telescopes, looking at a total of ten bands, or colors, with super-high definition quality. Continually imaging the Sun’s surface and atmosphere, it will allow scientists to track the evolution of surface features and flares with a time resolution as small as 0.75 seconds. The Helioseismic and Magnetic Imager (HMI) will probe deeply into the sun and map the magnetic field structure. (How? Well, that’s so cool, I’ll devote a whole post to it later this week.) My favorite instrument of the bunch is the Extreme Ultraviolet Variability Experiment (EVE). This does just what the name says, measure the variability of the output of the sun at far-UV wavelengths. Why is that so important? UV light from the sun creates and shapes the ionosphere of the Earth. The ionosphere is the outermost layer of the Earth’s atmosphere, and although it has many beneficial effects on life, it’s a pain for low frequency radio astronomers such as myself. (So, let’s just say this will get a devoted post as well.)

SDO will sit in a geosynchronous orbit above Las Cruces, New Mexico, where a dedicated radio station will be ready to gobble up the 130 Mbps of data that this mission will send back. Project scientists are calling this an “avalanche of data.” This fits in with the trend of many modern telescopes, such as the EVLA and ALMA, producing much more data than astronomers have ever dealt with before. New techniques for handling and distributing these data are always needed.

But, don’t just take it from me. Here’s an official SDO video!

Want to get involved in solar research right now? The premier site for citizen science in astronomy, Zooniverse, has a project called Solar Stormwatch. You learn how to look for and identify solar flares, and then look at some real data from previous missions and discover solar flares better than any automated image recognition software can.

Stay tuned for more updates from KSC as we begin our adventure, and join in at a local or virtual TweetUp for the launch! I’ll be blogging here and posting pictures on Flickr. George is posting his gorgeous (and silly) photos as well!

And while we’re wrapped up in all this spacey goodness, won’t you also check out the most recent Carnival of Space at Mama Joules!

SDO Spacecraft Image

Anime USA After Thoughts

This post is brought to you by the letter “Tim” and the number “$Texas”

A few months ago, I attended Anime USA, my 4th anime convention.  This was the 2nd time I attended Anime USA and it was a great time as always.  I went to some interesting panels and enjoyed the dealer’s room and artist alley, and I got to sit down with one of the voice actors, J. Michael Tatum, and talk about various aspects of his job and the anime industry, as well as, a lot of other things.  Some things that intrigued me in the course of the weekend (panels, conversations, etc.) were the concept of classifying anime, the stigma surrounding anime, and the problems that these cause in marketing anime.

A lot of people seem to refer to anime as an all encompassing genre, similar to comedy, drama, romance, and action, but this classification isn’t really accurate.  It’s more complex than that.  Why?  Because you can find all of those genres in anime, too.  So, anime should fall into a different level of classification.  Maybe it should fall into a category such as television, movies, and books, but then again it doesn’t fit there too well either.  Why?  Because anime can be a TV show or movie.

Love Hina (Right Image) and Hellsing (Left Image)

So, it’s hard to classify anime just as anime.  I can’t say that because you like “Love Hina” you’ll most likely enjoy “Hellsing” because they are very different.  There’s anime that’s comedy, drama, science fiction, surreal, romantic… anime that focuses on robots and vampires… anime geared towards girls (Shojo), geared towards boys (Shonen), geared towards women (Josei), and geared towards men (Seinen).  There’s anime with real, in-depth, heartfelt stories and ones that are mostly action…there are musicals and shows that are just sickeningly cute and ones that are mind-blowingly absurd or just freaky and messed up.  There’s horror and suspense.  There are ones that are just epic.  Ones with morals and trying to make a social or political point.  There are ones that are just for fun.  Not to mention “adult” anime (Hentai) which has its own breakdown of types.  So it cannot be classified simply.

There is also a stigma that surrounds anime, similar to the stigma that surrounds science fiction.  Anime is looked as being childish and/or geeky.  People hear the name anime and immediately associate it with cartoons, geekiness, Pokémon, children’s shows, robots, etc.  Some of those things are correct.  If by cartoon, you mean it’s animated, then yes.  There is hand-drawn and computer-animated anime.  Is it geeky?  Well, it certainly does have that stigma and some of the fans are extremely hard-core and do dress up as characters (called Cosplay), so it is definitely something that appeals to geeks.  However, I don’t think there is anything instrinsically geeky about anime.  Pokémon and other such children’s show ideas are just one aspect of anime.  Some will argue that they are the parts that give anime a bad name and the stigma, but I disagree.  It is judged by the beliefs people have about it, and often these beliefs come from limited knowledge about it.  There is such a variety within anime that it is a shame it is not even given a chance by so many people.  As a young kid, I was into the anime that was available, though we didn’t think of it as “anime”, it was just another cartoon.  When I got older, I shunned it because I feared the ridicule of my peers and, at the time, I only knew one small sliver of what was available.  It was in college that I started to get back into it.  Yes, it started with Pokémon and it was everything I remembered as a kid.  It was silly and childish, but I now saw a message in the stories that I didn’t see as a kid.  I was then exposed to a hentai series, which was the complete opposite of everything I knew about anime.  So I started to explore other series and found a wide range of shows.  I liked some and I didn’t like others, but that’s when I started to realize a lot of people who shunned anime, like I did, could find something that interested them.  I just lucked out that I had friends who knew about anime and hadn’t shunned it like I had and they could walk me through it and help me find things I liked.  They helped me find where and how to look for series.

So not all anime is created equal.  So what?  Well the difficulty in classifying anime makes marketing it difficult.  The broad anime moniker means there is no target market because the age range, gender, sexual preference, race, etc. are all over the place since there is such variety.  Combine that with the stigma that surrounds anime and you’ve narrowed your market.  Even if you do take a broad approach at marketing, the stigma will keep a lot of people from even considering it, so you’re wasting lots of money for little results.  This is a major problem in the industry.  Without marketing and advertising, only the diehards are up-to-date on new releases.  It’s like a closed off genre because if you’re new you don’t know what is what and it’s hard to find out.  There isn’t a lot of marketing and advertising to even point you in the right direction or let you know new things are coming out.  People see Pokémon and Yu-Gi-Oh on television and for them that is anime.  So the consumer base is only growing very slowly, which is not good for the studios.  It’s expensive to purchase the titles, translate the story, adapt the story, record the new voices and then make & distribute the DVDs.  And since anime does not have as wide a consumer base as major television series and motion pictures, the prices are higher for each consumer.  That also results in people using the internet for downloading unlicensed “fansubbed” shows.  All of this combined really does hurt the industry.  Recently ADV, one of the few studios in the United States for dubbing anime, closed down.  Luckily, there are still others (like FUNimation) left to try to pick up all the titles once owned by ADV, but it was a major blow.  It’s getting harder and harder for these studios to operate and turn a profit.  Something needs to be done, marketing needs to improve, and the consumer base needs to increase.  How?  I am not sure, but social media networks such as Twitter and Facebook seem to be a good place to start.  Why?  Because compared to other forms of advertising, social media networks are relatively inexpensive.  There are definitely draw backs to social media networks.  With social media, consumers have to actively come to you for information, whereas with regular advertising information comes to the consumer.  But there are more and more people are joining Twitter and Facebook, and both are continuing to evolve.  Videos can be posted on Facebook and YouTube, so they are good places for trailers and teasers. Companies can search Twitter for certain terms and then send those people 140 characters of information.  Plus, fans and people who like what they see can repost the information or email it to their friends expanding the reach of the advertising.  For a tiny investment, it seems like a great place to start.

FUNimation is now on Twitter and Facebook

Spacey updates…

Okay, a slew of updates since I’ve been busy!

Last week, the very awesome Nancy Atkinson wrote up the Carnival of Space #138 over on her new blog. Check out news about Mars, Kepler’s findings, and more!

I’ve posted a draft of the Twitter poster I had at the AAS Meeting at the beginning of January. It includes some quotes from the survey I put out the week before, though I haven’t compiled all the numbers yet!

For some crazy reason that I’m not even fully aware of, I’ve started a Tumblr. It’ll probably be a dropping off place for random links and photos and things, whereas any actual writing I manage will stay here. Oh, it’ll probably feature some of my real-life potty mouth, which I keep tame here. ;-)

And finally, I’m going to Florida! George, Aleya, Aleya’s bro, and I are road-tripping down to Kennedy Space Center for the launch of the Solar Dynamics Observatory! We’ll be tweeting and blogging and posting pictures the whole way. Oh, and we’re also going to get to see the launch of STS-130… my first ever launch, and possibly the last shuttle night launch! Follow the SDO tweetup events with the #SDOisGO hashtag, and I’ll be posting here as well. UPDATED AGAIN: My photos will be uploaded to my new Flickr set.

Boom, baby. STS-128 by cma3.

*NERDSQUEE!!*

I ranted a little while ago about the cheap, useless dowsing rods being used by Iraqi security forces to detect bombs. These units, being sold for tens of thousands of dollars each, were being manufactured by ATSC in the UK. It now seems that scumbag Jim McCormick, managing director of ATSC, may get what he deserves, as he’s been arrested on suspicion of fraud.

It is sickening and appalling that these people have made millions of dollars selling fake bomb detectors in a highly volatile area. People DIE when these dowsing rods ultimately fail. The news media is being far to generous is supposing that these detectors “may not work.” They are based on a pseudo-scientific concept that fails objective testing. James Randi, and later the JREF, has tested numerous dowsers under controlled conditions, and not one has succeeded better than chance. As can be expected, the JREF has responded to this story (twice). Rebecca over at Skepchick also weighs in on the harm of dowsing, including the following important investigative report on British TV:

I have little to add to the story except to say, score one for reason if these devices actually get recalled and if McCormick is properly punished. Seriously, these ATSC people have either completely bought into the myth of dowsing, or they are immoral jerks that have no place in decent society. And that’s being polite…

The first official day of the conference, my collaborator and I spent quite a bit of time hanging out at the poster group for the Allen Telescope Array. Although they work at a different frequency regime than we do (check out my PAPER episode at 365 Days of Astronomy for more about our project!), we do share some personnel and technology and, as it turns out, science goals.

The ATA is a centimeter-band array of 42 six-meter dishes with the central goal of pushing the Search for Extraterrestrial Intelligence further out into the galaxy. However, SETI is not the only goal for this array, as it is poised to become a general survey instrument and do all kinds of astrophysics along the way.

The SETI search has begun with a Galactic Center Survey. This survey looks for very narrowband signals, as one might expect to come from a non-natural source. Of course, there are intelligent beings emitting narrowband signals right from our own planet, so the initial survey picked up 421,432 signals! Scientists keep track of man-made radio frequency interference (called RFI) and can avoid obvious, known signals, dropping the count to 10,060 candidates. These move on to the second phase of processing. The ATA uses two beams on the sky (that is, it looks at two places at once.) If the signal is seen in both beams, then it must be local. This knocks out about 75% of these candidates. Further schemes involve immediate re-observation of candidates and a finer search for known, man-made signals. As you can expect, since we haven’t heard about it on the news, these methods knocked out all the remaining signals, so ET has not yet been found. But the survey has just begun!

ET signals are not the only time-dependent, or transient, signals of interest to astronomers. While naturally occurring signals are rejected from ET searches, they are scooped up for scientific study. Slow radio transients are sources that occasionally burst with emission, not as often or regularly as a normal pulsar (a rotating neutron star with “hotspots”). These were first detected serendipitously, but more systematic searches are underway as radio surveys become more standard. These sources can be intermittent pulsars, X-ray binaries, and other interesting astrophysical phenomena. Scientists at the ATA have already overcome a number of calibration hurdles in order to begin their science observations. (Just getting the data is only the first step… a lot needs to happen before the data can tell us anything interesting!)

The ATA can also be used to probe the Galactic magnetic field. Measuring magnetic fields is notoriously difficult in astronomy, as we can’t directly go out and probe various regions. One important tool is the polarization (or orientation of the EM fields) of radio emission. Quite roughly, as polarized light passes through a magnetic field, it is “spun around” or re-oriented, based on the frequency of the light in an effect called Faraday Rotation. By measuring the polarization of a source at multiple frequencies, information about the magnetic field can be extracted. A recent study using this technique with the Very Large Array significantly constrained models of our Galaxy’s magnetic field, and produced a very cool rotation measure map.

Taylor et al. 2009, ApJ, 702, 1230. The Galactic Plane goes through the center of the projection.

The astronomers at the ATA have been able to confirm some of these results and plan to extend them with the telescope’s multi-frequency capability. My collaborator, Danny, was especially excited about this since PAPER will have to deal with polarized emission from the Galaxy and beyond as well!

There were a bunch more posters in the ATA section, so be sure to browse their abstracts and the official websites at the SETI Institute and Berkeley’s Radio Astronomy Laboratory.

Related: AAS Wrap-up: Personal Perspective and the Big Stories

Carnival of Space #137

The Carnival of Space has finally made it’s appearance this week.

When the carnival players first showed up, I was lost in a beautiful, idyllic world called Pandora, inhabited by those tall, blue Na’vi and lots of fantastic (and fluorescent) creatures. But as I stepped out of the theatre labeled “Avatar”, leaving my 3-D glasses at the door, I came back to the real world (and my inbox) to remember that our universe is pretty wonderful as well. And this is exactly the point made at Martian Chronicles, our first stop at the carnival, who tells us How to Cure the Avatar Blues; so head there to take some time to wonder at Earth’s own beauty to start.

Our planet itself is by far not the only source of wonder. Go outside on a clear night and just gaze up at the treasures of the universe. The objects may be distant, but the beauty can be experienced first-hand. How big is space, really? Get a bit of a feel for it at Astroblog, where you can see The Southern Cross in Stereo and find out what it would look like if you “hopped over” to Alpha Centauri.

Humans have begun to reach out into this vast ocean of space. Kentucky Space takes us to a new center at Morehead State University which is Creating Kentucky’s Future in Space”. As NASA’s space shuttle approaches retirement, you can celebrate its achievements by participating in a Fan’s Choice Poll for Space Shuttle Commemorative Patch at collectSPACE. The lovely Astropixie celebrates human spaceflight as well as we wait for Hubble in 3-D to obliterate Avatar 3-D’s box office performance. (Well, we can hope!) But in order to get the public in general to care as much about spaceflight as we do here at the carnival, it’ll take some marketing savvy, as discussed in TED Friday: Rebranding Space and Education at Habitation Intention. We should just be sure to avoid any Risks of Manmade Sun Explosions as described at Next Big Future as we move along.

There is one man that we have been celebrating pretty specifically for a year now who realized the beauty and grandeur of our solar system: Galileo Galilei. Revisit Galileo’s Discovery of the Moons of Jupiter at Steve’s Astro Corner. Today, we know much more about those tiny points of light as they are extreme, and sometimes violent, worlds of their own. Visit volcanic Io in great detail with a paper on Verifying a new model of Io’s atmosphere by simulating multi-spectral observations at the Gish Bar Times. And once you are bowled over by that, check out Another dose of Martian awesomeness by the Bad Astronomer, with some truly breathtaking, high-resolution images of sand dunes from a neighboring world. Go explore Mars from the ground through the camera of Opportunity with The Road to Endeavor as she says Farewell, Marquette. Don’t forget to break out your red/blue 3-D glasses for the full experience!

Like the characters of Avatar, let us take our journey through our fantastic and awe-inspiring universe to the stars. You can fly to Messier 80 with Simostronomy, where we re-discover T Scorpii, Our Long Lost Friend. Just watch out for supernovae on your journey, as We Are All in the Gutter tells us about
A new, bigger kind of boom. Nevertheless, a supernova is still a pretty thing from a safe distance. We’re reminded that the universe is truly large enough to entertain us for a very long time as the Spacewriter shows us A Cosmos of Galactic Content. Our universe can be entirely bizzare with even just A Simple Look at Black Holes and Their Affect on Light and Mass at Weirdwarp. But it’s not so weird, as the Q & A of the Day at ChandraBlog reassures us that we’re not actually inside a black hole.

Don’t forget to share the wonders of the universe with those around you. One great way to do this is through astrophotography. WillGator.com tells us about the Astronomy Photographer of the Year 2010 contest, which is sure to serve up even more wonderous astronomical goodness. Another way to share the cosmos is actually with humor! The Angry Astronomer is starting a series on Astronomer Humor, so do check that out. (Are you taking submissions, Jon?) And finally, get a chuckle at an amusing out-take from next week’s Cheap Astronomy podcast. Someone with audio skills really needs to auto-tune/remix that for some real fun.

I hope you enjoyed this week’s tour of the cosmos and realize just a bit that the real world is often more marvelous than anything we can dream up with our fiction.

Photo credits: The Suss-Man on Flickr, Kara Allyson on Flickr, Hubblesite.org, saturn.jpl.nasa.gov, NRAO/AUI, Space Ritual on Flickr

First, as I mentioned earlier, check out the Carnival of Space #136 at Simostronomy. There’s an update on Spirit, more news from the AAS, and the usual spaceflight goodness.

Second, I had a great conversation with Mister Payne for the Religion of Curiosity podcast, and the episode has just posted. This is a really great show that genuinely, curiously explores many questions about religion, so check out all of his shows! I haven’t listened to this episode yet*, but we talk about my beefs with Catholicism, why I consider myself to be pretty laid-back about my atheism these days, astronomy, bellydancing, etc. It was a really fun conversation so I hope you enjoy listening in.

*And I probably won’t… I hate how I sound, or my accent, or my word choice or something… so once something is published, I can’t go back and listen to it without cringing!

What a crazy ride!

I am finally recovered, mostly, from the big American Astronomical Society meeting in Washington, DC, that occurred last week.  What a ride!

For me, the conference started off with a teaching workshop put on by the Center for Astronomy Education on interactive learning methods in “Astro 101.” As I start to sort through those notes, I’ll be able to write more about it. Suffice to say, it was wonderful to see that many interactive methods which were used in some of my favorite humanities classes are applicable to the large, lecture-hall-filling introductory astronomy classes.  Some of the exercises brought more questions out of me than they answered, but I have yet to even teach my first class… so time will tell.

The conference itself was just a whirlwind of activity. I made it to a number of the main talks, but very few of the small talks. I made it around to many, but not all, of the posters that I wanted to see.  A typical meeting has maybe a hundred posters each day, and maybe a dozen or so 5-minute talks going on at any one time.  You can’t do it all.  Walking around the poster session, I found myself having lengthy conversations with presenters or running into and having conversations with people on the floor at random. This is great for my research, for my education, and for networking, but absolutely terrible for keeping a schedule! But that is what made this conference great. Even at my own poster (the research one) I spent at least half an hour poring over the details with my collaborators, and we probably scared off at least one of the judges that was supposed to come by for the student competition. (Sorry!)

I also hardly slept. The conversations spilled out of the conference and around the dinner tables at nearby restaurants, then to the bars! I found myself out every night with such wonderful people, then had to drag my butt up to make the 8:30am talks. But who needs sleep when you are surrounded by so many great people?  I managed to work in some quality pub time with Phil Plait, a mini-reunion of 2004 Socorro summer students, a tweet-up with Pamela Gay and friends, a night of finishing the DSBK website while at the bar, and a particularly entertaining evening at the hotel bar with my friends and Neil deGrasse Tyson. And that was before the “real” party on Wednesday night which was, as the kids say, “off the hook.”

Check out my Flickr page for some visuals!

The Big Stories

Some of the big topics were already covered quite well by the science news sites and blogs, so I’ll do a quick roundup here before I delve into my own notes later.

Kepler

The Kepler mission made a splash with its first science results.  With just a few weeks of preliminary data, the team has discovered 5 exoplanets, studied variable stars, detected weird planet-sized hot objects, and identified many candidate planets. Read up with Universe Today, Star Stryder, and Astroengine.

Magellanic Clouds

The Spitzer Space Telescope released a gorgeous image of starbirth in the Small Magellanic Cloud, as covered by Bad Astronomy. UVa’s David Nidever and Steve Majewski used the Green Bank Telescope to show that the streams of gas being pulled away from the Magellanic Clouds by the Milky Way are longer than was previously thought. Galactic cannibalism at it’s best can be found over at Universe Today.

Bolden’s NASA

NASA Administrator Charlie Bolden made a big splash with his talk, which I missed, but I was able to catch up via Twitter. I can’t comment since I wasn’t there, but Phil Plait and Pamela Gay give excellent summaries and reactions. (My first response to Bolden’s call to get children to look through telescopes would be, look over here!)

Gravity Waves

NANOGrav, a method for detecting gravitational waves by timing millisecond pulsars (MSPs), got some good press that was picked up by Astroengine. I love seeing this story, but I’m biased since a) it involves radio telescopes and b) I know a few of the team members and they are super brilliant people. Although this particular collaboration is relatively new, these people have been crunching away on pulsar timing for years now and have been perfecting their techniques, just waiting for a great chance such as Fermi and its ability to detect new MSPs.

The stories don’t end there…

And there was so much more! I’m sure the upcoming Carnival of Space will include a smorgasbord of new discoveries that were announced at the AAS, and I’ll be following up with my own notes on topics that didn’t quite make it to press. Til then… cheers! To honor… ;-)

Part of the 2004 Socorro Summer crowd, the coolest REU ever: Kirstin, Chun, me, Yancy, Kelley, and Ben.

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