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Bad Astronomy

Posts Tagged ‘Mars’

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Rosetta’s stunning Mars

In 2007, the European Space Agency probe passed by Mars on its way to visit a comet. It used Mars for a gravity assist to help it on its way, and got close enough to take some very detailed pictures (it also passed by the asteroid Lutetia and returned amazing shots; see the gallery at the bottom of this post). That data wasn’t initially released by the mission leader (that’s fairly common in some missions), but they were finally made available late last year. My pal Emily Lakdawalla from the Planetary Society Blog grabbed a bunch of them and put together some simply amazing pictures from them, including this jaw-dropper:

Yeah. You really want to click that to Barsoomenate it. Holy dry ice polar caps!

In fact, you should go over to her blog where she gives all the details and has more incredibly cool pictures of the Red Planet as well. I don’t want to spoil her fun by giving it all away here. Go!

Credit: ESA / MPS / UPD / LAM / IAA / RSSD / INTA / UPM / DASP / IDA / processed by Emily Lakdawalla


Related posts:

- Rosetta’s cometary goal now in sight
- Lutetia may have witnessed the birth of the Earth
- Curiosity on its way to Mars!

<span>On July 10, 2010, the European Space Agency probe Rosetta passed just 3162 km (1960 miles) from the asteroid <a href="http://en.wikipedia.org/wiki/21_Lutetia" target="_blank">Lutetia</a>, a lumpy rock 130 km (81 miles) end-to-end. <br /><br />This image, taken at closest approach, shows how battered and worn Lutetia is. Craters pockmark the surface, including several that are many kilometers across. Like the Martian moon <a href="http://blogs.discovermagazine.com/badastronomy/2010/03/31/more-incredible-phobos-imagery/" target="_blank">Phobos</a>, grooves line the surface, which may be from boulders rolling around, perhaps ejected from some of the craters when they were formed. They may alternatively be stress fractures from impacts; there is still a lively debate over what causes these features in small bodies.<br /><br />Much of the surface appears smooth, indicating great age for this object. Over billions of years it's been assaulted by dust grains moving at incredible speeds, as well as the solar wind. This has essentially sandblasted the surface, taking - literally - the edge off of the rims of craters. <br /><em><br /></em>We have very few high-resolution images of asteroids, and the more we get, the more we learn about them. Given that every now and again <a href="http://www.amazon.com/Death-Skies-Science-Behind-World/dp/B0035G02BI/ref=sr_1_2?s=books&amp;ie=UTF8&amp;qid=1278972215&amp;sr=1-2" target="_blank">we get hit by them</a>, I'm a big fan of understanding them better. <br /><br /><em>Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span><p>This series of pictures was taken as Rosetta approached Lutetia.</p>
<p>The first image in the upper left was taken about 9.5 hours before closest  approach, when Rosetta was still 510,000 km (315,000 miles) from the asteroid - more distant than the Moon is from the Earth!</p>
<p>The last image (lower right) was obtained an hour and a half before the close encounter when the probe was still 81,000 km (50,000 miles) from Lutetia.</p>
<p>In the first image, details only about 20 km (12 miles) across can be seen, but that improves by almost a factor of 10 in the last image!</p>
<p><span><em>Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span></p><span>This is the final sequence of images taken right at closest approach. The bottom right image was taken just at the moment that Rosetta passed Lutetia.<em><br /><br /><br />Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span>For the first time ever, a spacecraft approached closely enough to  the asteroid Lutetia to see its surface clearly. Craters dot the surface, as well as grooves. Note the elongated crater near the bottom (left of center); was that from a nearly horizontal impact? It's curious that it points almost directly to the crater to the left. That may just be coincidence; the surface is so cratered that some are bound to be in patterns just randomly.<br /><span><em><br />Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span>Another closeup of Lutetia's surface provided by Rosetta. In this shot, you  can again see a variety of craters peppering the asteroid, as well as some  grooves that follow the landscape. Those curves give a relative age for  the grooves: they must have formed <em>after</em> the impact crater on the right,  which distorted the landscape. Also, had they formed before, the impact  would have eradicated them. Images like this can give scientists a vast amount of insight into the history of the asteroid.<br /><span><em><br />Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span><span>After Rosetta passed Lutetia, its cameras were pointed back to the rock, and therefore back toward the inner solar system. That geometry gives us an amazing, brooding, and lovely view we never get from Earth: a crescent asteroid.<em> <br /><br />Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span><span>When Rosetta was still 36,000 km (22,000 miles) from Lutetia, it snapped this jaw-dropping shot of the asteroid with Saturn in the distant background. This means the spacecraft, the asteroid, and Saturn were almost exactly along the same line, a configuration that probably only lasted for a few seconds. It's remarkable that controllers on the ground were able to take this picture at just the right moment to obtain this amazing picture!<br /><em><br /><br />Credit: ESA 2010 MPS for OSIRIS Team. MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA</em></span>

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January 26th, 2012 6:52 AM Tags: Emily Lakdawalla, ESA, Mars, Rosetta, The Planetary Society
by Phil Plait in Astronomy, Pretty pictures | 12 Comments » | RSS feed | Trackback >

Top 14 Solar System Pictures of 2011

<div style="background-image: initial; background-attachment: initial; background-origin: initial; background-clip: initial; margin: 8px;">A few days ago I posted <a href="http://blogs.discovermagazine.com/badastronomy/2011/12/06/top-16-pictures-from-space/" target="_blank">my favorite space pictures from 2011</a>, and said it was only Part 1. As promised, here is Part 2: my favorite pictures of solar system objects from the past year. <br /><br />Again, it was ridiculously hard to pick just a few. I had something like 70 to choose from. Our space probes keep sending back amazing shots of planets, moons, asteroids, and more, and we keep getting better at taking pictures of them from the ground as well. As an astronomer, I love it, but as a blogger it makes my fingers cramp. <br /><br />Still, it's not a terrible burden to bear. All of the pictures I chose are interesting for their beauty, their science, and their story.  <br /><br />To browse, just click the arrows or the next image in the filmstrip. Clicking the image will take you to my original blog post about it, with more information. <br /><br />... and there's still one more gallery to go! I've done space and now solar system, and that only leaves the rest of the Universe. So stay tuned, there's a whole cosmos coming your way in a few days.<br /><br /><strong>Related Posts:</strong><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/12/06/top-16-pictures-from-space/" target="_blank">Top 16 Space Pictures of 2011</a><br /><a href="http://blogs.discovermagazine.com/badastronomy/2010/12/20/top-ten-astronomy-pictures-of-2010-runners-up/" target="_blank"><br />Top 10 Astronomy Pictures of 2010 - Runners Up<br /><br /></a><a href="http://blogs.discovermagazine.com/badastronomy/2010/12/14/the-top-14-astronomy-pictures-of-2010/" target="_blank">The Top 14 Astronomy Pictures of 2010</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2009/12/15/top-ten-astronomy-pictures-of-2009/" target="_blank">Top Ten Astronomy Pictures of 2009<br /><br /></a><a href="http://blogs.discovermagazine.com/badastronomy/2008/12/17/top-ten-astronomy-pictures-of-2008/" target="_blank">Top Ten Astronomy Pictures of 2008</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2007/12/23/top-10-astronomy-pictures-of-2007-runners-up/" target="_blank">Top Ten Astronomy Pictures of 2007 - Runners Up</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2007/12/13/top-ten-astronomy-pictures-of-2007/" target="_blank">Top Ten Astronomy Pictures of 2007</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2006/12/27/the-top-ten-astronomy-images-of-2006/" target="_blank">Top Ten Astronomy Pictures of 2006</a></div>The Lunar Reconnaissance Orbiter has been circling the Moon since 2009, taking thousands of images in amazing resolution unseen since Apollo. Many of these pictures have been simply astonishing, including the one above taken in March 2011: an unnamed crater a few kilometers across (the image is 2.2 km or about 1.4 miles wide). Whatever smacked into the Moon all those eons ago blew out a lot of dust and other material that fell back to the surface, spreading out like the broad petals of a flower. In the crater floor you can barely see some boulders and other debris that must have gone straight up and back down after the impact. The Moon has no air, but formations like this erode after time anyway: countless meteorite impacts, the solar wind, and even thermal flexing during the Moon's day/night cycle take their toll. So we know that such craters must be young, but that's a relative term: this impact may have occurred when dinosaurs still walked the Earth.<br /><br /><em>Image credit: NASA/GSFC/Arizona State University</em><br /><br /><a href="http://lroc.sese.asu.edu/news/index.php?/archives/380-Action-Shot.html" target="_blank">Oriignal image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/05/11/a-flower-bloom-on-the-moon/" target="_blank">Original blog post</a><br />Solar eclipses are relatively rare events on the Earth's surface. The Moon's orbit around the Earth is tilted a bit with respect to the Earth's orbit around the Sun, so the Moon has to be at the right place at the right time to block the Sun. <br /><br />But what if you're in orbit around the Earth?  In that case, <em>the Earth itself</em> blocks the Sun all the time (of course, if you want to be pedantic, it happens to us on the surface every time the Sun sets). NASA's Solar Dynamics Observatory stares at the Sun 24/7/365, and was placed in an orbit to minimize the amount of time the Earth blocks its view. But it does happen twice a year, when the orbits all align.<br /><br /> The picture above is from late March 2011, during one of these eclipse seasons. The edge of the Earth cut right across the disk of the Sun, creating this odd view. This particular shot is in the ultraviolet, where Earth's atmosphere is almost opaque, completely cutting off the Sun's light... except for that one little curlicue on the left. That's an extremely bright filament of material, luminous enough to have some of its light get through, despite our atmosphere.<br /><br />This is a weird and wonderful picture, accessible only from space, which is why I picked it for this year's list.<br /><br /> <em>Image credit: NASA/GSFC/SDO</em><br /><br /><a href="http://www.flickr.com/photos/gsfc/5576582865/sizes/l/" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/04/01/when-the-earth-takes-a-bite-out-of-the-sun/" target="_blank">Original blog post</a><div>When I was a kid (mumble mumble) years ago, asteroids were just points of light in even the biggest telescopes. That was true even just a few years ago, but in recent times we've seen quite  a few close up thanks to the space program. Vesta is the second largest asteroid, orbiting the Sun in the main belt between Mars and Jupiter. And despite its size (roughly 500 km or 300 miles across), until a few months ago we really didn't know much about it.</div>
<div><br />But then in July 2011, the spacecraft Dawn arrived. Orbiting the rock, it's been snapping away, revolutionizing our understanding of asteroids. Vesta's landscape is diverse, with <a href="http://blogs.discovermagazine.com/badastronomy/2011/08/16/vestas-double-whammy/" target="_blank">craters</a>, cliffs, mountains, and long, linear grooves (although, interestingly, no hints of vulcanism, when some were expected). Its south pole is an enormous impact basin; something <em>huge</em> hit Vesta <em>hard</em> a long time ago. Ejected material from that impact scattered across the solar system, and some of it has hit Earth as meteorites. We've found some of these, and<a href="http://blogs.discovermagazine.com/badastronomy/2011/09/18/invaders-from-vesta/" target="_blank"> through chemical analysis shown they are from Vesta</a>, which is truly amazing when you think about it. It took a lot of effort to get a spacecraft to the asteroid, and all that time we had pieces of it here already!</div>
<div><br />But that's OK. There's still plenty left to learn. And eventually Dawn will leave Vesta and head over to Ceres, the largest asteroid in the solar system. What will it find when it gets there?<br /><br /><em>Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA</em><br /><br /><a href="http://www.nasa.gov/images/content/576312main_pia14317-full_full.jpg" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/08/01/vesta-in-breathtaking-detail/" target="_blank">Original blog post</a><br /><br /></div><div>I really like pictures of Earth from space, but this is one only a mother could love. It's not actually a picture, but a map of Earth's gravity! It's a model created using data from the European Space Agency's orbiting GOCE satellite, which was used to very carefully map out the changing strength of Earth's gravity over our planet's surface. Essentially, this map tells you the direction of "down" over every point on the Earth. If you stand near a mountain, for example, then the gravity of that mountain pulls on you a little bit, and the direction you feel gravity pulling you changes a wee bit.</div>
<div>This kind of map - called a geoid - is a standard reference used by topographic maps, and also helps scientists understand how ocean currents flow, how ocean water circulates, and even better understand the dynamics of sea wave heights. It may make the Earth look lumpy and distorted and weird, but hey - nature calls 'em like it sees 'em.<br /><br />[Bonus: Nathanial Burton-Bradford took several  of these images <a href="http://blogs.discovermagazine.com/badastronomy/2011/04/21/the-lumpy-3d-earth/" target="_blank">and created red/green 3D images of them</a>!]</div>
<div><br />Image credit: ESA/HPF/DLR<br /><br /><a href="http://www.esa.int/esaCP/SEM1AK6UPLG_index_0.html" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/03/31/the-earths-lumpy-gravity/">Original blog post<br /> </a></div><div>This may look like a picture of the Moon taken through a small backyard telescope, but it's anything but: it's a huge mosaic of <em>1300 images</em> from the Lunar Reconnaissance Orbiter, painstakingly stitched together to make a huge high-res map of the Moon.<a href="http://lroc.sese.asu.edu/news/uploads/lroc_wac_nearside_noslew.png" target="_blank"> The bigger version</a> gives you a taste of what's in it (<a href="http://lroc.sese.asu.edu/news/uploads/lroc_wac_nearside_noslew_anot.png" target="_blank">a labeled one</a> is available as well) but even that pales in comparison to the massive 24,000 x 24,000 pixel <a href="http://lroc.sese.asu.edu/data/pr/tiff/wac_nearside.tif" target="_blank">full size version</a>, weighing in at an astonishing 550 megabytes, in case you needed to wallpaper your living room. If you prefer to interact a bit, then there's <a href="http://wms.lroc.asu.edu/lroc_browse/view/wac_nearside" target="_blank">a pan-and-scan version</a> where you can zoom in and have fun flying over the lunar surface.</div>
<div><br />It's more than just fun: one big reason LRO is doing this is to make high-res maps of the Moon for future exploration. It is one of my most fervent hopes that one day, maps like this will be used by people who are trying to find their way from their dome to their in-laws' for dinner.<br /><br />And if you live on the Moon's far side, no worries: <a href="http://blogs.discovermagazine.com/badastronomy/2011/03/12/the-extraordinary-back-of-the-moon/" target="_blank">there's a map for that half</a>, too!<br /><br /><em>Image credit: NASA/GSFC/Arizona State University</em><br /><br /><a href="http://wms.lroc.asu.edu/lroc_browse/view/wac_nearside" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/02/22/the-extraordinary-face-of-the-moon/" target="_blank">Original blog post</a><br /><br /></div>We might like to think of the Sun as a steady, calm source of light and heat, but in reality it undergoes a cycle of violent activity driven by magnetic fields. This cycle peaks every 11 years or so, and we're due for the next maximum in 2013 or 2014. The previous minimum lasted an unusually long time, but things started ramping up again in 2011. Sunspots marring the Sun's face <a href="http://blogs.discovermagazine.com/badastronomy/2011/09/27/for-your-viewing-pleasure-active-region-1302/" target="_blank">started appearing in greater numbers</a>, and many of them were the source of incredible outbursts of energy called solar flares.<br /><br /> This picture shows a flare from August 2011, as seen in the ultraviolet by NASA's Solar Dynamics Observatory. When the subatomic particles spurted out by such flares interact with our own magnetic field, the result can be spectacular aurorae, which are also becoming a common sight. They can also cause blackouts (as a particularly large event did to Quebec in March 1989) and damage our satellites - including GPS and communication satellites. Studying the Sun is more than just science: our economy can literally depend on it.<br /><br /><em>Image credit: NASA/SDO/AIA</em><br /><br /><a href="http://www.flickr.com/photos/gsfc/6025628821/in/photostream" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/08/09/another-big-solar-flare/" target="_blank">Original blog post</a><div>Mars appears to be dead now, but a long time ago it was an active planet. Volcanoes roared, sending floods of lava across the plains of the planet. Sometimes those flows would solidify on top, forming a hollow tube through which the lava moved. Eventually, when the volcano died away, what was left was a hollow underground corridor, called a lava tube.</div>
<div>Sometimes, points along that tube will collapse, forming a hole in the ground above. Called <em>skylights</em>, we see these on Earth near volcanoes, but they're on Mars too! What you're seeing here is just such a skylight. Under this otherwise fairly featureless plain is a lava tube, and something - perhaps a meteorite - punched a hole in it. Sand flowed down, forming the collapse pit, which is about 175 meters (600 feet) across. The hole itself is 35 meters (115 feet) across, the size of a decent back yard. You can even see the rim of the hole casting a shadow on the lava tube floor, 20 meters (60 feet) down!<br /><br />Skylights on Mars are pretty cool, but they may eventually be useful. The lava tubes are big enough to support a decent size exploration base, and the ground above would protect astronauts from solar radiation. What you're looking at here might very well one day be called "home" by your descendents!<br /><br /><em>Image credit: NASA/JPL/University of Arizona</em><br /><br /><a href="http://hirise.lpl.arizona.edu/images/wallpaper/2560/ESP_023531_1840.jpg" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/08/18/spectacular-sand-pit-found-on-mars/" target="_blank">Original blog post</a></div><div>Since Pluto's demotion from the brotherhood of planets a few years back, Neptune has taken on the mantle of responsibility of most distant planet in the solar system. It's big, about 4 times the diameter of Earth, but so far away - 4.4 billion kilometers (2.7 billion miles) away at its closest - that even in big telescopes it's hard to see detail. Astronomer Mike Brown used one of the biggest telescopes on Earth, the monster 10-meter Keck eye in Hawaii, to observe Neptune in September 2011, getting this lovely infrared picture of it. The bright bands around Neptune are high-altitude clouds, similar to the cloud patterns we see on Jupiter and Saturn.</div>
<div><br />And oh, did I say he was observing Neptune? Actually, Mike studies the giant frozen iceballs that orbit the Sun out past Neptune, so really he was more interested in Neptune's moon Triton, seen to the lower right in that picture. Triton is so similar to those other objects that it may actually have once been one, captured eons ago by Neptune's gravity. It's unclear how something like that could've happened, so observations of these distant denizens of the outer solar system are important for us to understand the history and evolution of our local neighborhood.<br /><br /><em>Image credit: Mike Brown</em><br /><br /><a href="http://web.gps.caltech.edu/~mbrown/out/triton.png" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/09/19/neptune-is-really-far-away/" target="_blank">Original blog post</a></div>The MESSENGER spacecraft was launched in 2004 and spent <em>seven years</em> getting to Mercury; it's not all that easy dropping a probe down into the inner solar system. It swung by Mercury twice (not to mention the Earth once and Venus twice!) before finally settling into orbit in March 2011, and then beginning its scientific mission of analyzing the overheated world.  Among the first pictures it took was this one, showing the crater named <a href="denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:denied:link to:http://blogs.discovermagazine.com/badastronomy/2011/09/30/clair-de-mercury/" target="_blank">Debussy</a> (after the composer). The crater is 80 km (50 miles) wide, but reaching much farther are those streaks called <em>rays</em>; collapsed plumes of ejected material when whatever hit Mercury hit Mercury. Many craters on the Moon show rays, and in some cases pictures of the two objects look very similar.<br /><br /> Since March, MESSENGER has taken huge amounts of data of the planet, increasing our knowledge of what makes it tick - and it's returned not just images but also laser altimetry data, spectroscopy, and mineralogical maps. Mercury isn't much like Earth at all, but sometimes it's the contrasts that aid our understanding. The planets in the solar system are a diverse lot, and it's only by studying all of them that we can come to understand the one we live on.<br /><br /> <em>Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington</em><br /><br /><a href="http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&amp;image_id=432" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/03/29/messengers-first-picture-from-mercury-orbit/" target="_blank">Original blog post</a><div>In late 2010, an amateur astronomer noticed an odd white spot in Saturn's northern hemisphere. It was a storm, like a gigantic hurricane, which quickly grew in size to thousands of kilometers across and rapidly surpassed the diameter of our own planet. And yet it continued to grow, and in February 2011 the Cassini spacecraft orbiting Saturn took this incredible picture showing the storm had grown so long <em>it had literally wrapped its way around the entire planet!</em> At this point, it was a staggering 300,000 km (180,000 miles) in length - <strong>the same distance as 3/4 of the way from the Earth to the Moon!<br /> </strong></div>
<div><br />Pictures taken in late 2010 and early January <a href="http://blogs.discovermagazine.com/badastronomy/2011/11/17/psychedelic-saturn-storm/" target="_blank">also show details of the storm in psychedelic false color</a>, where the whorls and vortices of the raging weather are clear. Saturn's face is usually far more subtle and calm than this - look at the nice, smooth southern hemisphere for comparison - so the eruption of this storm was a surprise to astronomers... but surprises are good, because in many cases that's how we learn things. And I'm glad Cassini was there to get these amazing close-up shots.<br /><br /><em>Image credit: NASA/JPL-Caltech/SSI</em><br /><br /><a href="http://www.ciclops.org/view/6738/Catching_Its_Tail" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2010/12/28/a-saturnian-storm-larger-than-worlds/" target="_blank">Original blog post </a></div>In March of 2011, the spacecraft MESSENGER became the first ever moon of Mercury, taking unprecedented high-resolution images of the solar system's smallest official planet. But while it was on its tortuous path to Mercury, engineers back home programmed the spacecraft to take a series of snapshots, pointing the cameras painstakingly across the solar system. The result is what you see above: every planet in the solar system, a sort of cosmic family portrait.<br /><br />
<div>Uranus and Neptune are there, but too faint to see (you should grab <a href="http://www.nasa.gov/mission_pages/messenger/media/SolarSytemPortrait.html" target="_blank">the bigger version of this</a> to see the details). Venus was relatively close to MESSENGER at the time, and so is very bright. My favorite part of this, though, is being able to see the Earth and Moon together. There's something eerie about seeing them both in pictures at the same time, nearly lost in the black (the Jupiter-bound spacecraft Juno <a href="http://blogs.discovermagazine.com/badastronomy/2011/08/31/home-from-the-start-of-a-long-long-journey/" target="_blank">took a similar shot of our world</a> this year as well). <br /><br />It really brings home - well, so to speak - the fact that we are a speck of dust floating in space, tiny to the point of insignificance when seen like this. And yet, never forget that we <em>are</em> significant: after all, <strong>we created the machine that took this picture!</strong> I think it says a lot about us humans that not only do we send spacecraft to other worlds, but we take the time to make pictures like this. Sometimes, just sometimes, people are pretty cool. <br /> <br /><em>Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington</em></div>
<br /><a href="http://www.nasa.gov/mission_pages/messenger/media/SolarSytemPortrait.html" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/02/18/messengers-family-portrait/" target="_blank">Original blog post</a><br /><div>The twisted magnetic fields inside of sunspots have as much or more effect on the Sun's outer layers as the gravity of our star itself. As <a href="http://blogs.discovermagazine.com/badastronomy/2011/11/10/the-face-of-our-star/" target="_blank">the field lines tangle up</a>, vast towers of ionized gas (called plasma) can erupt, sometimes collapsing back onto the solar surface, and sometimes blasting off into space. These are called <em>prominences</em>, and can take on all sorts of fantastic shapes, usually in the form of plumes or arcs.<br /><br /> Solar photographer Alan Friedman took these two shots of two different prominences, both of which made me laugh when I saw them: the top one looks like a cat nuzzling the Sun, and the bottom one like a dragon!</div>
<div><br />Expect to see more pictures like this over the coming years, as the Sun's activity gets even more common. Hopefully, we'll also see a dog, and perhaps St. George.<br /><br /><em>Image credit: Alan Friedman</em><br /><br />Original images: <a href="http://alanfriedman.tumblr.com/post/11279675645/cat-on-a-hot-hydrogen-roof-i-found-this-prowling" target="_blank">Cat</a> and <a href="http://www.avertedimagination.com/img_pages/delicato.html" target="_blank">Dragon</a></div>
<div><br />Original blog post: <a href="http://blogs.discovermagazine.com/badastronomy/2011/10/11/solar-purrominence/" target="_blank">Cat</a> and <a href="http://blogs.discovermagazine.com/badastronomy/2011/09/02/the-delicate-tendrils-of-a-solar-dragon/" target="_blank">Dragon</a></div>Saturn <a href="http://blogs.discovermagazine.com/badastronomy/2011/10/24/a-panoply-of-moons-and-rings/" target="_blank">and its rings</a> are a continuously-playing show of beauty and grace, but the giant planet also has a vast retinue of moons,<a href="http://blogs.discovermagazine.com/badastronomy/2011/06/20/a-moody-moon-turns-its-face/" target="_blank"> each as different from each other</a> as any family of siblings (which make it very hard to pick my favorite from ones like <a href="http://blogs.discovermagazine.com/badastronomy/2011/10/24/a-panoply-of-moons-and-rings/" target="_blank">this</a> or <a href="http://blogs.discovermagazine.com/badastronomy/2011/02/28/peeking-past-rhea/" target="_blank">this</a>). The biggest, the aptly-named Titan, is a monster, bigger than the planet Mercury and possessing an atmosphere of nitrogen that's twice as thick as Earth's! The atmosphere is so thick and opaque that it blocks our view of the ground in visible light. Infrared light can penetrate that gloom, though, and it's not by coincidence that the Cassini spacecraft is equipped with filters and detectors designed to look in those wavelengths.<br /><br /> Using that equipment, astronomers created the first-ever multicolor map of the surface of Titan (<a href="http://blogs.discovermagazine.com/badastronomy/2011/10/14/a-window-into-titan/" target="_blank">a map using a single color</a> was created in 2009).  This false-color map shows elevated regions (white areas), lakes of liquid methane and ethane near the north pole of the moon, and what's most amazing to me, vast areas of wind-blown dunes (shown in brown)! Those aren't grains of sand in the dunes, but grains of frozen hydrocarbons, blown across the plains by Titan's thick air. Detailed radar observations by Cassini show them to be much like dunes on Earth, but a bit chillier: the temperature on the surface of Titan is a numbing (or perhaps I should say "shattering") -180°C (-300°F). <br /><br />And yet, it's a world not so different than ours: atmosphere, liquid lakes, wind... and at those temperatures, the chemistry of methane is similar to that of water at room temperature on Earth. It's not crazy to wonder if there's life on Titan...<br /><br /><em>Image credit: NASA/JPL/University of Arizona/CNRS/LPGNant</em><br /><br /><a href="http://www.ciclops.org/view/5492/Map_of_Titan_February_2009" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/10/12/a-hidden-world-revealed-titan/" target="_blank">Original blog post</a>Of all these pictures of our planetary neighbors, I think I might love this one the most. That's us: it's home. Blue, with feathered white, the only planet to really look this way (Uranus and Neptune are both blue, but for different reasons; we have water, they have methane). This picture is from Terra, a NASA Earth-observing satellite, designed to look down and investigate our environment.<br /><br />But that's not why this picture really amazes me. Look at it more carefully: almost all you see is water! If you look to the upper right you'll see the west coast of the US, Baja California, and Mexico. <em>Everything else you see is ocean.</em> The satellite was over the Pacific when this was taken, and that expanse of water is vast, covering nearly an entire hemisphere of the planet. It's a coincidence that this is the way things are right now; continental drift changes the sizes of the oceans over geologic time scales. But still, it's a sharp reminder of just how much water we have here on Earth, and why we look for it so steadfastly on other worlds, and why we need to take our job as planetary caretakers more seriously.<br /><br /><em>Image credit: NASA</em><br /><br /><a href="http://www.nasa.gov/multimedia/imagegallery/image_feature_1925.html" target="_blank">Original image</a><br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/04/22/happy-earth-day/" target="_blank">Original blog post</a>

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December 8th, 2011 6:30 AM Tags: Earth, Mars, Mercury, Moon, Neptune, prominence, Saturn, solar flare, Sun, Titan, Triton, Vesta
by Phil Plait in Astronomy, Cool stuff, Pretty pictures, Top Post | 17 Comments » | RSS feed | Trackback >

Curiosity on its way to Mars!

Yesterday morning, NASA successfully launched the Mars Science Laboratory — named Curiosity — toward the fourth planet. If, like me, you missed the launch itself (^%$#@&! sinuses) why then, here’s some pretty dramatic video of the liftoff:

[Make sure to set it to 720p resolution!]

The cool parts to watch are: about 2 minutes in when the booster rockets fall by the wayside; 3:42 when the payload fairing is jettisoned, exposing the Curiosity spacecraft — as seen by the camera onboard the rocket, which is way cool; 4:38 when the entire rocket starts to slowly spin up, providing stabilization and allowing the Sun to heat the assembly evenly; then a few seconds later when the upper stage Centaur rocket ignites, leaving the booster behind (also extremely cool).

But wait! There’s more!

(more…)

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November 27th, 2011 7:05 AM Tags: Curiosity, Mars
by Phil Plait in Cool stuff, NASA, Space | 77 Comments » | RSS feed | Trackback >

Curiosity launches to Mars on Saturday

[UPDATE: SUCCESS! The launch was just about perfect, and Curiosity is now on its way to Mars, scheduled to land in August 2012. Congrats to everyone on the mission!]

Tomorrow, Saturday, November 26 at 10:02 Eastern (US) time (15:02 UTC), an Atlas V rocket carrying the Curiosity Mars rover will blast off from Florida, sending the sophisticated rolling lab to the Red Planet.

You can watch the launch live at NASA TV, or I recommend on the NASA/JPL UStream channel. I imagine I’ll be up and tweeting about it, as will my pal Emily Lakdawalla.

It is no exaggeration to say that Curiosity is a huge leap forward for Mars exploration. Designed to last for nearly two years, it’s 3 meters long — the size of a hefty golf cart — and its scientific payload is ten times more massive than its predecessors. It has instruments (PDF) that can sample and taste the air and surface, imagers to provide high resolution stereo pictures, a laser to zap rocks and get their spectra (which yields their composition), and even a camera that will take video of the last two minutes of its descent to the surface to provide aerial context for its cameras once it lands.

If you thought Spirit and Opportunity were cool — and you’d be right — Curiosity will up the ante considerably. I’m very excited by the prospect of the science this rover will do, and the exploration it’s capable of as a precursor, eventually, to a human being stepping foot on this odd, dry, and cold neighboring world.

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November 25th, 2011 11:55 AM Tags: Curiosity, Mars, rover
by Phil Plait in Astronomy, Cool stuff, NASA, Space | 61 Comments » | RSS feed | Trackback >

Phobos-Grunt scheduled to launch at 20:16 UT

[Update (20:30 UT): The mission launched on time, and everything looks good so far! As I write this, the probe's orbiting the Earth. In a few hours (a little after 01:00 UT) it will make its burn to send it on its way to the Red Planet. Congrats to everyone involved in this mission!]

[UPDATE 2 (05:00 UT): There are problems, potentially serious ones, with the mission. As I write this what happened is not clear, but Emily is keeping up with the news.]

[UPDATE 3 (Nov 9, 16:00 UT): It looks like the spacecraft is in safe mode, meaning it shut itself off to prevent damage due to an unforeseen problem. The burn to move it out of Earth orbit and no to Mars did not occur, which means it still has all its fuel. This is very bad, but perhaps not catastrophic. Emily has the details.]

The Russian Mars probe Phobos-Grunt — which will land on the Martian moon Phobos and return a sample to Earth! — is scheduled to launch today at 20:16 UT (15:16 Eastern US time). As usual with planetary missions, Emily Lakdawalla has the details. The launch will be streamed live on SpaceflightNow.

phobos_hires

Grunt means "soil" in Russian; the name is a little misleading since soil technically is rock and other material broken down in part by bacterial processes. A better term is regolith, but I’m just being pedantic. The important thing to note is that if all goes well this probe will return a sample of the surface of another planet’s moon back to Earth!

That’s awesome.

We still don’t understand Phobos all that well; it may be a captured asteroid orbiting Mars, and its surface is weird, as you can see in the picture above. It’s lined with grooves, which may have formed when asteroid impacts on Mars below blasted up material, which the tiny rock then plowed through. That’s still being argued about. A sample return might help resolve issues like that (for example, finding clear evidence of Martian minerals in Phobos samples). I’m not a geologist, or an asteroid expert, so I’m just excited that a) this probe is going to get intense images of Phobos, 2) we’re going to expand the boundaries of science once again, and γ) there will be even more new mysteries to solve once the material is studied, too.

And it all starts today, in a few hours.

Credits: ESA/DLR/FU Berlin (G. Neukum)


Related posts:

- More *incredible* Phobos imagery
- Phobos, closeup of fear
- It’s rabbit^h^h^h Phobos season!

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November 8th, 2011 9:05 AM Tags: Mars, Phobos, Phobos-Grunt
by Phil Plait in Astronomy, Cool stuff | 40 Comments » | RSS feed | Trackback >

Happy first day of spring… Mars!

Today, September 14, 2011, is the vernal equinox for the northern hemisphere of Mars!

If you want to be technical, it’s the time when the axis of Martian rotation is perpendicular to the direction of the Sun, and the northern hemisphere is headed into summer (making it the autumnal equinox for the southern hemisphere). When this happens here on Earth, it’s called the first day of spring (here in the US at least, in other countries it’s considered the middle of the season — a tradition with which I agree).

Mars, like Earth, is tilted with respect to its orbit around the Sun; Earth is canted at an angle of roughly 23°, while Mars is at 25°. That’s why we (and Mars) have seasons! Over the course of the year, the angle of sunlight hitting the surface of the planet changes, heating it more efficiently in the summer and less in the winter. Boom! Seasons.

On Earth, that’s most dramatically seen as polar ice shrinks and grows over the year. Same with Mars! The picture above is from the European Space Agency’s Mars Express orbiter, and shows the northern polar cap in May 2010, during the last summer. The north pole of Mars is icy, but it’s actually two kinds of ice: water, and frozen carbon dioxide. CO2 turns directly from a solid into a gas (a process called sublimation), and does so at much lower temperature than water ice melts. This means the CO2 goes away first as temperatures rise in the northern hemisphere, leaving the water ice behind. In that picture, the ice is essentially all water.

In other words: the north pole of Mars is sublime*.

Where does the CO2 go? Into the atmosphere! So much of it adds to the air there that the atmospheric pressure on the planet increases measurably, by about 30%. That much extra carbon dioxide adds a small but significant greenhouse effect to the planet as well, warming the surface. Estimates vary, but I’ve seen quotes of a few degrees Celsius for the effect.

The change of seasons also kicks up winds on Mars, and that can cause everything from dust devils which leave incredibly beautiful scrollwork on the surface to planet-wide dust storms.

I’ll note that the year on Mars is about twice the length of an Earth year, so all the seasons are about twice as long as well. May 2010 is when summer started on Mars (in the northern hemisphere), and here we are 17 months later with the start of spring. The Planetary Society has a page listing the next few seasonal dates on Mars if you’re curious.

So anyway, happy first day of spring, Martians! Don’t forget to try to stand up malagor eggs today.

Image credits: Earth/Mars tilts: from Calvin J. Hamilton’s fantastic Solar views website; Mars polar cap: ESA/DLR/FU Berlin (G. Neukum.)


* Hahahahahaha! Man, that’s funny. Also, <McBain>ice to see you.</McBain>

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September 14th, 2011 6:53 AM Tags: carbon dioxide, Mars, seasons, tilt
by Phil Plait in Astronomy, Cool stuff, Pretty pictures | 26 Comments » | RSS feed | Trackback >

Spectacular sand pit found on Mars!

Check. This. Out: a perfectly-formed collapse pit on Mars that leads to an underground cavern!

Amazing! [Click to barsoomenate.]

This was taken by the Mars Reconnaissance Orbiter in July 2011. See the hole in the bottom? You can tell from the lighting that this is an underground opening to a cavern — a skylight. Quite a few of these have been found on Mars, actually. We see them on Earth and even on the Moon. Given the angle of the shadows, the vertical distance from the bottom of the pit to the floor of the cavern is about 20 meters (65 feet). Watch your step!

Here’s how we think skylights like this form. In the distant past, Mars was geologically active. Rivers of lava ran across the surface. If the surface of the lava hardens it can form a roof, allowing the lava underneath to continue flowing; these are called lava tubes and there are bazillions of them in Hawaii, for example. Eventually, the source of the lava chokes off and the lava flows away, leaving the empty tube underground. If the roof is thin in one spot it can collapse. Sometimes that just leaves a hole, but apparently in this case it was under a sand field. Some of the sand must have fallen into the chamber below and eventually blown away, leaving the pit and the hole. The pit is located not too far from Pavonis Mons, a known (long-dead) Martian volcano.

The hole is about 35 meters (115 feet) across, so the pit is about 175 meters (nearly 600 feet) across the rim. I love how it sits in an otherwise nearly featureless sand field; the contrast is beautiful. In the high-res image you can see boulders perched on the pit wall, having rolled part of the way down as well. The inside of the pit has lines and furrows that are instantly recognizable to anyone who has tried to dig a hole at the beach and had sand continually flow down from the rim.

It would be incredible to see something like this up close. It’s possible eventually someone will: such lava tubes would make good homes for future Mars explorers; they’d be protected from sand storms, temperature swings, and solar radiation (which is worse than for us on Earth because Mars doesn’t have a strong magnetic field to protect it).

… but you couldn’t pay me enough to go inside one of those. I have no desire to be slowly digested over ten thousand years.

Image credit: NASA/JPL/University of Arizona. Tip o’ the light saber to reddit.


Related posts:

- More Mars caves found
- There’s a hole in the Moon!
- Spelunking the lunar landscape
- Martian dunes under the microscope

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August 18th, 2011 12:50 PM Tags: cavern, collapse pit, lava tube, Mars, Mars Reconnaissance Orbiter, Sarlacc, skylight
by Phil Plait in Astronomy, Pretty pictures, SciFi, Space | 69 Comments » | RSS feed | Trackback >

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      Phil Plait, the creator of Bad Astronomy, is an astronomer, lecturer, and author. After ten years working on Hubble Space Telescope and six more working on astronomy education, he struck out on his own as a writer. He's written two books, dozens of magazine articles, and 12 bazillion blog articles. He is a skeptic and fights the abuse of science, but his true love is praising the wonders of real science.


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