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Bad Astronomy

Archive for the ‘Pretty pictures’ Category

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The Helix screams in infrared

About 700 light years away sits the expanding death cry of a star: the Helix Nebula, a four-light-year wide gas cloud blasted out when a star that was once like the Sun gave up its life.

A new image of it in colors just outside what the human eye can see shows just how much it does look like a screaming star:

[Click to ennebulenate, or download the huge 6600 x 600 pixel 35 Mb version.]

This image is in the near-infrared, taken using the European Southern Observatory’s Visible and Infrared Survey Telescope for Astronomy (VISTA), a 4.1 meter telescope in Chile. Equipped with a whopping 67 megapixel camera it can take pictures of large areas of the sky. The Helix nebula fits that bill: it’s close enough to us that it’s nearly the size of the full Moon in the sky.

This image is pretty nifty. It accentuates cooler gas than what we see in visible light. What’s colored red in the picture is actually infrared light coming from molecular hydrogen, and shows the sharp ring-like edge of the nebula. What you’re seeing here is not so much a ring as it is the walls of a barrel-like structure, and we happen to be seeing it nearly right down the tube (see Related posts below for all the info you could want on this amazing object).

It also accentuates the long, long streamers pointing directly away from the center. Those are comet-like tails coming from denser clumps of material boiling away as the fierce ultraviolet light of the central star floods out, their material flowing radially outward. This is seen in other nebulae as well.

And while it’s beautiful and scientifically very useful (I would’ve killed for data this nice when I was researching these nebulae in grad school), it’s also something of an existential reminder: someday, our own Sun will look a bit like this. Probably not quite this bright and well-defined; our local star doesn’t quite have the power needed to light up its surroundings this way. But for all intent and purpose, you’re seeing a snapshot of our solar system in seven or eight billion years.

Just in case you needed a little perspective this morning.

Image credit: ESO/VISTA/J. Emerson. Acknowledgment: Cambridge Astronomical Survey Unit


Related posts:

- The Helix’s dusty heart
- Top 10 Astronomy Pictures of 2007: Runners Up
- Down the throat of a dying star
- Thus spoked the Dumbbell

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January 19th, 2012 6:45 AM Tags: Helix Nebula, infrared, VISTA
by Phil Plait in Astronomy, Piece of mind, Pretty pictures | 19 Comments » | RSS feed | Trackback >

Incredible time lapse: Milky Way over Africa

This video is only 20 seconds long, but wow. Simply, wow.

[Note: I've noticed sometimes the video won't load and you get a black space. Try hitting refresh, or just click the link in the next sentence.]

This was created using a series of still images from the International Space Station on December 29, 2011, over the course of about 20 minutes. The ISS was orbiting over Africa at the time, as it passed from the center of the continent to Madagascar and then over the ocean. The flashes of light are from storms on our planet’s surface.

In the sky, though, the Milky Way steals the scene as it rises over the eastern horizon. Toward the end of the video, what I thought for a moment was a reflection of the Milky Way on the glass of the ISS turns out to actually be Comet Lovejoy, which was still visible at the time. You can also see the thin green arc of airglow over the Earth before the rising Sun ends the video.

If it weren’t copyrighted, I would’ve added Enya’s "Storms in Africa" track to this. It seems appropriate.

… and if there’s a metaphor here for overcoming adversity — whatever that may mean to you — well then, feel free to ruminate over it.

Credit: NASA


Related posts:
- JAW DROPPING Space Station time lapse!
- Time lapse: The spectacle of Comet Lovejoy
- INSANELY cool picture of Comet Lovejoy
- Time lapse video: ISS cometrise
- JAW DROPPING Space Station time lapse!

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January 18th, 2012 4:59 PM Tags: Comet Lovejoy, ISS, Milky Way, time lapse
by Phil Plait in Astronomy, Pretty pictures | 9 Comments » | RSS feed | Trackback >

Carcineidolia

If there is any definition of "ironic", it must be a smiley face seen in a cancerous cell:

Australian researchers at the Westmead Millennium Institute for Medical Research were investigating how the protein beta-catenin invades a cell’s nucleus and causes it to become cancerous, when they spotted the protein apparently mocking them. You can see this a bit more clearly in the video they made:

The circle is the cell’s nucleus as the protein moves in, and the dark spots are where the protein is blocked. The smiley face doesn’t surprise me; we’re hardwired to see faces and familiar shapes everywhere we look (click the tag marked "pareidolia" — the psych term for this — under this post to see lots of examples). Heck, I spotted one in a supernova once…

And I certainly hope this research yields insight into how to fight cancer. I’d love to see that smirk wiped off that nucleus’s face.

Tip o’ the gamma knife to Amos Zeeberg and Fark. Image credit: Westmead Millennium Institute for Medical Research

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January 17th, 2012 1:26 PM Tags: beta-catenin, cancer cell
by Phil Plait in Pareidolia, Pretty pictures | 15 Comments » | RSS feed | Trackback >

Gallery: Cosmic pictures from the AAS

Twice a year, the American Astronomical Society holds a big meeting where thousands of professional astronomers get together to talk about the latest results and ongoing work in the field. The January meeting is traditionally very well-attended, and is also when a lot of big news is released. <br /><br />The January 2012 meeting was in Austin, Texas. Even though I couldn't make it this year, I was inundated with news from the event, so much so that I couldn't really keep up. So I figured it would be fun to take some of the best pictures from news items and write up a brief description for a gallery.<br /><br />At the bottom of each picture is a link labeled "Original Source"; click that to get the full story with all the gory and glorious technical details of the news. You can use the arrows to navigate the pictures, or click them to go to the next in the series. Enjoy!<div>The Large Magellanic Cloud is a dwarf galaxy that orbits our Milky Way at distance of roughly 160,000 light years. It can be seen by the naked eye from the southern hemisphere... but not like this! Combining images from ESA's Herschel observatory with NASA's Spitzer Space Telescope, this image shows the incredibly complex system of dust in the galaxy glowing in the far infrared.</div>
<br />
<div>Bright clumps are where stars are forming; the big one on the left is the Tarantula Nebula, one of the largest and most active stellar nurseries known. However, there are many places where stars are being churned out in the LMC, which is one of the reasons astronomers study it so intently.<br /><br /><a href="http://www.nasa.gov/mission_pages/herschel/multimedia/pia15254.html" target="_blank">Original Source</a><br /><br /><em>Credit:  ESA/NASA/JPL-Caltech/STScI</em></div><div>A combination of observations using the orbiting Chandra X-Ray Observatory and the ground-based Very Large Telescope and Atacama Cosmology Telescope has found the largest galaxy cluster ever seen in the distant Universe. They've nicknamed it <em>El Gordo</em>, meaning<em> the fat man</em> in Spanish.</div>
<br />
<div>It's actually the result of two clusters colliding. <a href="http://www.eso.org/public/archives/images/screen/eso1203a.jpg" target="_blank">The image</a> is dominated by X-rays (colored blue in the picture) being emitted by gas heated to millions of degrees by the collision. The cluster was found in a survey of how matter distorts the light from the far more distant background glow of the sky emitted by the Big Bang itself. They knew the cluster was big, and when they pointed Chandra at it they knew it was terribly hot from the collision as well. The most amazing thing is its distance: seven billion light years! Knowing how clusters behave at such huge distances helps astronomers understand how the Universe has changed over time, and how the largest structures in the cosmos came to be.<br /><br /><a href="http://www.eso.org/public/news/eso1203/" target="_blank">Original Source</a> <br /><br /><em>Credit:  ESO/SOAR/NASA</em></div><div>The kind of light we see is called optical light. It's actually rather low energy, emitted by hot things like the Sun, gas clouds, and so on. But what if we could see light that had energies millions of times higher? <strong>Billions?<br /> </strong></div>
<br />
<div>Then the sky would look like this: <a href="http://www.nasa.gov/images/content/614826main_Fermi-3-year.jpg" target="_blank">a map from NASA's Fermi telescope</a>, which sees in gamma rays. Sources of gamma rays are among the most violent in the Universe: exploding stars, fiercely magnetic neutron stars, black holes gobbling down matter. Fermi just completed its third year in space, surveying the entire sky and building up a large and sensitive database of this highest-energy form of light. While many of the individual sources are identified, as many as one third of all the objects in this map cannot be determined.</div>
<div><br />And that line across the middle? That's our own galaxy, the Milky Way. It's a flat disk, and we're inside it, so we see it as a broad line across the sky. It takes a dark night to see the faint milky band of the galaxy to the naked eye, giving no real hint of the vast and terrible forces at play there. Only by examining the sky in other energies do we start to unveil the true nature of the Universe.<br /><br /><a href="http://www.nasa.gov/mission_pages/GLAST/news/energy-extremes.html" target="_blank">Original Source</a><br /><br /><em>Credit:  NASA/DOE/Fermi LAT Collaboration</em></div>4500 light years away in the direction of the constellation of the swan, Cygnus X is a sprawling star-forming region. This infrared image by NASA's Spitzer Space Telescope shows huge, complex structures carved by the fierce winds and light of newborn massive stars. Cavities are dug out, long finger-like tendrils formed, and filaments compressed by these forces, which glow in the IR. Eventually, many of the stars born here will explode, compressing the gas and dust further, in turn creating even more stars. It's the cycle of life, written in cosmic material dozens of light years across.<br /><br /><a href="http://www.nasa.gov/mission_pages/spitzer/multimedia/pia15253.html" target="_blank">Original Source</a><br /><br /><em>Credit: NASA/JPL-Caltech/Harvard-Smithsonian CfA</em><div>Looking at random parts of the sky with Hubble, astronomers have found what appears to be the most distant protocluster ever seen: five galaxies in the process of growth, forming a cosmic collection that may grow into a massive cluster. The project, called the Brightest of Reionizing Galaxies (BoRG! ha!) survey, examined many images from Hubble. The galaxies are incredibly faint to the eye -- you'd have a hard time seeing them in the image without their locations marked -- but are intrinsically incredibly bright. They're located at a distance of something like 13.1 billion light years away! That means they were forming shortly after the Universe itself did, 13.7 billion years ago!</div>
<br />
<div>It's not yet confirmed if the five galaxies are bound together by gravity; the method used to get their distances isn't accurate enough. They'll need to follow up with spectroscopic observations to find that out. If they are connected gravitationally, then they will eventually form the core of a massive cluster of galaxies like the nearby Virgo Cluster, which boasts 2000 members. But as we see them back then, when the Universe itself was so young, they are still just in the process of initial growth (each is smaller than the Milky Way).</div>
<br />
<div>And how do they grow? <em>By assimilating material around them.</em> This is how<strong> the BORG</strong> cluster grows.</div>
<br />
<div><a href="http://en.wikipedia.org/wiki/Borg_(Star_Trek)" target="_blank">Hmmm</a>.<br /><br /><br /><br /><a href="http://hubblesite.org/newscenter/archive/releases/2012/05/full/" target="_blank">Original Source</a><br /><br /><em>Credit:  NASA, ESA, M. Trenti (University of Colorado, Boulder, and Institute of Astronomy, University of Cambridge, UK), L. Bradley (STScI), and the BoRG team</em></div><div>The Andromeda Galaxy is a big, splashy spiral galaxy, the largest one nearby (less than 3 million light years away - that's close as galaxies go). Like every major galaxy, it has a supermassive black hole in its core -- specifically, Andromeda's has a hefty 100 million times the mass of the Sun, making it far larger than our own Milky Way's 4 million mass central black hole.</div>
<div><br />You'd think such a place would be anathema for anything else, but in fact there is not one but two populations of stars there! Seen in this Hubble image, there is a large cluster of bright blue stars surrounding the galaxy's black hole, which apparently formed there about 200 million years ago.<br /> Surrounding that is a ring of older, redder stars, appearing to give Andromeda two nuclei. Stars orbiting black holes are not too surprising - we see that in our own galaxy - but it's not at all clear how those blue stars could've formed so close to that monster in the middle. Hubble observations like this one will hopefully help us understand and eventually solve that mystery.<br /><br /><a href="http://hubblesite.org/newscenter/archive/releases/2012/04/image/a/format/web_print/" target="_blank">Original Source</a><br /><br /><em>Credit: NASA, ESA, and T. Lauer (National Optical Astronomy Observatory)/T. Rector and B. Wolpa, NOAO</em></div><div>Dark matter is a substance about which we know very little. We know more about what it isn't: it can't be dead stars, rogue planets, or wandering black holes, for example. For various reasons, every kind of normal matter has been eliminated from the list, leaving some form of exotic matter that isn't well understood.</div>
<br />
<div>But that doesn't mean we know nothing: we actually can map its location on the sky! As light from distant galaxies passes through dark matter, the gravity of the invisible material bends that light, distorting it - this is called a gravitational lens. The bigger the warp, the more dark matter must be there. The Canada-France-Hawaii Telescope Lensing Survey observed over 10 million galaxies, looking for that subtle distortion, and made dark matter maps of four regions on the sky. The result is the image above. For comparison, it includes the full Moon for scale, as well as <a href="http://blogs.discovermagazine.com/badastronomy/2007/01/07/aas-report-2-dark-matter-and-large-scale-structure/" target="_blank">the largest dark matter map previously made</a>.</div>
<br />
<div>Large scale maps of dark matter like this are critical for understanding its distribution, and for figuring out what the heck this stuff is. As it happens, detectors on board the Fermi spacecraft as well as underground in the Large Hadron Collider are on the hunt for the weird particle constituents of dark matter. Very soon, we may know quite a bit more about it.</div>
<div><br /><a href="http://www.cfht.hawaii.edu/en/news/CFHTLens/" target="_blank">Original Source</a><br /><br /><em>Credit:  Van Waerbeke, Heymans, and CFHTLens collaboration</em></div><div>The Sloan Digital Sky Survey is an amazing project: map out the positions and colors of objects in the sky to high precision. In the case of galaxies, the colors can be use to get a decent estimate of the distance; galaxies moving away from us as the Universe expands get their colors subtly changed versus distance.</div>
<br />
<div>Using this data covering an incredible 1/4 of the entire sky, astronomers created the map above of 900,000 luminous galaxies: ones that are brighter than usual. By choosing these overachievers they can see them at great distances, and make a complete map. This map, the largest ever compiled, shows each galaxy as a single green dot, and stretches out to a distance of 6 billion light years -- halfway across the Universe. The galaxies can be seen to cluster in some spots, and this tells us about conditions in the early cosmos when these clusters formed. Astronomers using these data have constrained limits on such disparate things as dark energy and neutrino mass!</div>
<br />
<div>They also put together <a href="http://www.youtube.com/watch?v=NvbKfucv3cM&amp;feature=player_embedded" target="_blank">a very cool video</a> where they move the data around in 3D. It's mesmerizing... especially when you think that to do this in real life you'd have to travel at trillions of times the speed of light!<br /><br /><a href="http://www.sdss3.org/press/20120111.sloanguide.php" target="_blank">Original Source</a><br /><br /><em>Credit:  David Kirkby (University of California, Irvine) and the SDSS-III Collaboration</em></div><div>Hubble has bagged the most distant Type Ia supernova ever to have its distance confirmed: dubbed SN Primo, the light we see left it a staggering 9 billion years ago!</div>
<br />
<div>It was found as part of an ambitious project using Hubble to look for such distant explosions in the near infrared, and is the first one found in the three-year survey. The project is being led by my old pal (yes, I'm bragging) and <a href="http://blogs.discovermagazine.com/badastronomy/2011/10/04/discovery-of-dark-energy-nabs-nobel-prize-for-three-astronomers/" target="_blank">Nobel Prize winner</a> Adam Riess, who has long been working with supernova to understand the expansion of the Universe. These types of exploding stars tend to explode in a manner that makes their distance relatively simple to calculate (well, once you've solved a host of problems first, which Adam did, which is why he won the Prize). And since they can be seen at vast distances, this makes them very useful <a href="http://blogs.discovermagazine.com/badastronomy/2006/09/26/what-astronomers-do/" target="_blank">for determining the overall shape and evolution of the Universe</a>.</div>
<br />
<div>The top pictures shows the Hubble Ultra Deep Field; nearly everything you see in it is a far-flung galaxy. The boxed region is expanded on the bottom; on the left is one image of it and on the right another taken at a later time. The supernova wasn't there in the first image, but can be seen in the second. Adam's team will continue to use Hubble to look at this region over and again, looking for the tell-tale bright spot that marks the location of a new supernova.</div>
<div><br />By doing this they will improve our measurements of how the Universe is expanding, including the bizarre acceleration of the expansion discovered - in part by Adam - in 1998. I'll be very interested to see what else they find over the next few years of this project. <br /><br /><a href="http://hubblesite.org/newscenter/archive/releases/2012/02/full/" target="_blank">Original Source</a><br /><br /><em>Credit: NASA, ESA, A. Riess (Space Telescope Science Institute and The Johns Hopkins University), and S. Rodney (The Johns Hopkins University) </em></div><div>NASA’s Wide-field Infrared Survey Explorer (WISE) mapped out the entire sky in the far-infrared for about a year. Since it was a survey instrument, it didn't take pictures per se, instead counting infrared photons, noting their position, time, and energy. This allows astronomers to make a mosaic image of any size... so they created this astonishing map of the constellations Cassiopeia (the Queen) and Cepheus (the king), covering over 1000 square degrees of sky! For comparison, the full Moon is about 1/5 of a square degree: this map covers the equivalent of 5000 full Moons!</div>
<div><br />There is no way I can convey the sheer depth and breadth of this image in the 610 pixel width of this blog, so you should download <a href="http://wise.ssl.berkeley.edu/gallery_images/WISE2012-001-xl.jpg" target="_blank">the crazy huge 70 Mb 13530 x 4609 pixel version</a>. You can then sweep over the dust, gas, stars, cavities, shells, supernova remnants, and everything else littering this picture. It's breath-taking. <a href="http://blogs.discovermagazine.com/badastronomy/2011/04/15/orions-wise-head/" target="_blank">To give you a hand</a>, red colors are from very cool dust, green tends to come from complex organic molecules, and blue from warmer dust and gas.<br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/03/24/wise-shuts-its-eye/" target="_blank">WISE shut its eye in February 2011</a>, but the data it complied will keep astronomers busy for many years to come.<br /><br /><a href="http://wise.ssl.berkeley.edu/gallery_fireworks.html" target="_blank">Original Source</a><br /><br /><em>Credit: Image Credit: NASA/JPL-Caltech/WISE Team</em></div>

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January 17th, 2012 7:00 AM Tags: American Astronomical Society, Andromeda galaxy, CFHT, Chandra X-Ray Observatory, Cygnus, Fermi, galaxy, Herschel, Hubble Space Telescope, nebula, SDSS, Spitzer Space Telescope, VLT, WISE
by Phil Plait in Astronomy, Cool stuff, Pretty pictures, Top Post | 13 Comments » | RSS feed | Trackback >

Time lapse: Chinese rocket caught on video

Not that any time lapse video of the Very Large Telescope complex at Paranal in Chile would be normal, but this one by Farid Char caught something pretty unusual: what appears to be a Chinese rocket boosting a satellite to orbit!

Did you catch it? From 14 – 18 seconds in, you can see it as a bright object moving against the setting stars to the west. If you pause the video, you can see what look like two plumes of gas coming from the object (though I wonder; a cone-shaped plume might look like this too seen from the side due to limb-brightening). Given the time, it was most likely the Chinese satellite FengYun 2-F moving into its transfer orbit (or possibly just venting some fuel), and it will slowly boost itself to a final geosynchronous orbit over the next few weeks.

These time lapse videos are always pretty cool, but they’re even better when they get a surprise like this!

Tip o’ the lens cap to eundas on Twitter.


Related posts:

- Time lapse: The Aurora
- Time lapse: The spectacle of Comet Lovejoy
- Time lapse video: ISS cometrise
- Lunar eclipse time lapse

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January 16th, 2012 7:00 AM Tags: FengYun 2-F, time lapse, VLT
by Phil Plait in Cool stuff, Pretty pictures, Space | 6 Comments » | RSS feed | Trackback >

Rapturday

[Just a note: if you're not a fan of nature documentaries because they sometimes show nature being natural -- specifically, predators eating prey -- then you might want to skip this post.]

This morning I was at my computer, just settling down with my coffee and a ton of emails to get through, when the dogs started barking upstairs. It wasn’t their usual "Alert! Alert! The neighbors are outside!" or "Wake up! A truck drove by!" bark — it was urgent and non-stop. Wondering what it could be, I got up, walked over to the back door, and HOLY CRAP THERE’S A HAWK EATING ANOTHER BIRD THREE METERS FROM MY DOOR!

I grabbed the dogs, threw them in the bedroom, hastily told my wife what was happening, ran back to my office to grab the camera, and took about a hundred shots.

[Click to accipiterenate.]

I have some software that helps identify birds, and it turns out to be surprisingly difficult to figure out what kind of hawk is what. My best guess is that this is a Sharp-shinned hawk, judging from the tail coloration and the plumage. The software says they can have blue-gray upper parts, but all the pictures I see look like this fierce raptor, with red-brown striped feathers. It’s definitely not a Red-tailed hawk. [UPDATE: in the comments a lot of folks seem to be converging on it being a Cooper's hawk. I looked at some photos, and it does match.]

The bird it was eating was also hard to identify from a distance (especially given the circumstances). At first I thought it was a gull; we get them around here at dumps and reservoirs. However, once the hawk left and I got the privilege of cleaning up (yuck; there were feathers everywhere) I could see it was a common white pigeon.

Here are a couple of more shots, which I’ll put after the jump just in case some folks are squeamish. They aren’t horribly gruesome, but might disturb more empathetic readers.

(more…)

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January 14th, 2012 11:41 AM Tags: hawk, pigeon
by Phil Plait in Caturday, Cool stuff, Pretty pictures | 90 Comments » | RSS feed | Trackback >

Stunning view of a bloom from space

Almost exactly one year ago, I posted a beautiful picture of a phytoplankton bloom as seen from space. And here’s another one, and it’s way, way more spectacular!

Holy wow! [Click to enalgaenate.]

This shot of a bloom in the southern Atlantic Ocean was taken by the ESA’s Envirosat, which — duh — is designed to observe our environment. In this case, scientists keep a keen eye on phytoplankton blooms: while this bloom is breathtaking and gorgeous, many can be hazardous. Besides producing toxins that can harm sea life, they can also consume more oxygen in the water than usual, which is obviously tough on any life in the area. The color of the bloom can be found quickly using satellite imagery like this, and the algae species determined. Also, phytoplankton are sensitive to some climate changes, so observing them can act as a "canary in the coal mine" for climate change.

Sometimes, the best view of the Earth around us is from above. And sometimes that view is amazing, but a reminder that our ecosystem is a dynamic balance… and it’s best that we understand all the forces that can upset that equilibrium.

Tip o’ the petri dish to Alan Boyle on Google+. Image credit: ESA

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January 14th, 2012 7:00 AM Tags: Envisat, ESA, phytoplankton
by Phil Plait in Cool stuff, Pretty pictures, Space | 21 Comments » | RSS feed | Trackback >

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