{"id":266854,"date":"2010-02-02T17:33:30","date_gmt":"2010-02-02T22:33:30","guid":{"rendered":"http:\/\/davidkirkpatrick.wordpress.com\/?p=6607"},"modified":"2010-02-02T17:33:30","modified_gmt":"2010-02-02T22:33:30","slug":"head-on-asteroid-crash-%e2%80%94-cool-space-image","status":"publish","type":"post","link":"https:\/\/mereja.media\/index\/266854","title":{"rendered":"Head-on asteroid crash \u2014 cool space image"},"content":{"rendered":"<p><\/p>\n<p>This bit of interesting news is from this morning&#8217;s inbox. Very cool image<\/p>\n<blockquote>\n<p>Suspected Asteroid Collision Leaves Trailing Debris<\/p>\n<p>WASHINGTON, Feb. 2  \/PRNewswire-USNewswire\/ &#8212; NASA&#8217;s Hubble Space Telescope has observed a  mysterious X-shaped debris pattern and trailing streamers of dust that suggest a  head-on collision between two asteroids. Astronomers have long thought the  asteroid belt is being ground down through collisions, but such a smashup has  never been seen before.<\/p>\n<p>(Logo:\u00a0 <a href=\"http:\/\/www.newscom.com\/cgi-bin\/prnh\/20081007\/38461LOGO\">http:\/\/www.newscom.com\/cgi-bin\/prnh\/20081007\/38461LOGO<\/a>)<\/p>\n<p>Asteroid  collisions are energetic, with an average impact speed of more than 11,000 miles  per hour, or five times faster than a rifle bullet. The comet-like object imaged  by Hubble, called P\/2010 A2, was first discovered by the Lincoln Near-Earth  Asteroid Research, or LINEAR, program sky survey on Jan. 6. New Hubble images  taken on Jan. 25 and 29 show a complex X-pattern of filamentary structures near  the nucleus.<\/p>\n<p>&#8220;This is quite different from the smooth dust envelopes of  normal comets,&#8221; said principal investigator David Jewitt of the University of  California at Los Angeles. &#8220;The filaments are made of dust and gravel,  presumably recently thrown out of the nucleus. Some are swept back by radiation  pressure from sunlight to create straight dust streaks. Embedded in the  filaments are co-moving blobs of dust that likely originated from tiny unseen  parent bodies.&#8221;<\/p>\n<p>Hubble shows the main nucleus of P\/2010 A2 lies outside  its own halo of dust. This has never been seen before in a comet-like object.  The nucleus is estimated to be 460 feet in diameter.<\/p>\n<p>Normal comets fall  into the inner regions of the solar system from icy reservoirs in the Kuiper  belt and Oort cloud. As comets near the sun and warm up, ice near the surface  vaporizes and ejects material from the solid comet nucleus via jets. But P\/2010  A2 may have a different origin. It orbits in the warm, inner regions of the  asteroid belt where its nearest neighbors are dry rocky bodies lacking volatile  materials.<\/p>\n<p>This leaves open the possibility that the complex debris tail  is the result of an impact between two bodies, rather than ice simply melting  from a parent body.<\/p>\n<p>&#8220;If this interpretation is correct, two small and  previously unknown asteroids recently collided, creating a shower of debris that  is being swept back into a tail from the collision site by the pressure of  sunlight,&#8221; Jewitt said.<\/p>\n<p>The main nucleus of P\/2010 A2 would be the  surviving remnant of this so-called hypervelocity collision.<\/p>\n<p>&#8220;The  filamentary appearance of P\/2010 A2 is different from anything seen in Hubble  images of normal comets, consistent with the action of a different process,&#8221;  Jewitt said. An impact origin also would be consistent with the absence of gas  in spectra recorded using ground-based telescopes.<\/p>\n<p>The asteroid belt  contains abundant evidence of ancient collisions that have shattered precursor  bodies into fragments. The orbit of P\/2010 A2 is consistent with membership in  the Flora asteroid family, produced by collisional shattering more than 100  million years ago. One fragment of that ancient smashup may have struck Earth 65  million years ago, triggering a mass extinction that wiped out the dinosaurs.  But, until now, no such asteroid-asteroid collision has been caught &#8220;in the  act.&#8221;<\/p>\n<p>At the time of the Hubble observations, the object was  approximately 180 million miles from the sun and 90 million miles from Earth.  The Hubble images were recorded with the new Wide Field Camera 3 (WFC3), which  is capable of detecting house-sized fragments at the distance of the asteroid  belt.<\/p>\n<p>For Hubble images and more information, visit:<\/p>\n<p><a href=\"http:\/\/www.nasa.gov\/hubble\">http:\/\/www.nasa.gov\/hubble<\/a><\/p>\n<p>Photo:\u00a0  <a href=\"http:\/\/www.newscom.com\/cgi-bin\/prnh\/20081007\/38461LOGO\">http:\/\/www.newscom.com\/cgi-bin\/prnh\/20081007\/38461LOGO<\/a><br \/>\nAP  Archive:\u00a0 <a href=\"http:\/\/photoarchive.ap.org\/\">http:\/\/photoarchive.ap.org\/<\/a><br \/>\nPRN Photo  Desk <a href=\"mailto:photodesk@prnewswire.com\">photodesk@prnewswire.com<\/a><br \/>\nSource:  NASA<\/p>\n<p>Web Site:\u00a0 <a href=\"http:\/\/www.nasa.gov\/\">http:\/\/www.nasa.gov\/<\/a><\/p>\n<\/blockquote>\n<p>And to save a trip to the Hubble site, here&#8217;s the image:<\/p>\n<blockquote>\n<p><img decoding=\"async\" src=\"http:\/\/www.nasa.gov\/images\/content\/421558main_hs-2010-07-a-print-540.jpg\" alt=\"Hubble image of comet-like object P\/2010 A2\" \/><\/p>\n<p>Credit: NASA, ESA, and D. Jewitt (University of California, Los Angeles). Photo No. STScI-2010-07<\/p>\n<\/blockquote>\n<p>  <a rel=\"nofollow\" href=\"http:\/\/feeds.wordpress.com\/1.0\/gocomments\/davidkirkpatrick.wordpress.com\/6607\/\"><img decoding=\"async\" alt=\"\" border=\"0\" src=\"http:\/\/feeds.wordpress.com\/1.0\/comments\/davidkirkpatrick.wordpress.com\/6607\/\" \/><\/a> <a rel=\"nofollow\" href=\"http:\/\/feeds.wordpress.com\/1.0\/godelicious\/davidkirkpatrick.wordpress.com\/6607\/\"><img decoding=\"async\" alt=\"\" border=\"0\" src=\"http:\/\/feeds.wordpress.com\/1.0\/delicious\/davidkirkpatrick.wordpress.com\/6607\/\" \/><\/a> <a rel=\"nofollow\" href=\"http:\/\/feeds.wordpress.com\/1.0\/gostumble\/davidkirkpatrick.wordpress.com\/6607\/\"><img decoding=\"async\" alt=\"\" border=\"0\" src=\"http:\/\/feeds.wordpress.com\/1.0\/stumble\/davidkirkpatrick.wordpress.com\/6607\/\" \/><\/a> <a rel=\"nofollow\" href=\"http:\/\/feeds.wordpress.com\/1.0\/godigg\/davidkirkpatrick.wordpress.com\/6607\/\"><img decoding=\"async\" alt=\"\" border=\"0\" src=\"http:\/\/feeds.wordpress.com\/1.0\/digg\/davidkirkpatrick.wordpress.com\/6607\/\" \/><\/a> <a rel=\"nofollow\" href=\"http:\/\/feeds.wordpress.com\/1.0\/goreddit\/davidkirkpatrick.wordpress.com\/6607\/\"><img decoding=\"async\" alt=\"\" border=\"0\" src=\"http:\/\/feeds.wordpress.com\/1.0\/reddit\/davidkirkpatrick.wordpress.com\/6607\/\" \/><\/a> <img decoding=\"async\" alt=\"\" border=\"0\" src=\"http:\/\/stats.wordpress.com\/b.gif?host=davidkirkpatrick.wordpress.com&#038;blog=2464417&#038;post=6607&#038;subd=davidkirkpatrick&#038;ref=&#038;feed=1\" \/><\/p>\n","protected":false},"excerpt":{"rendered":"<p>This bit of interesting news is from this morning&#8217;s inbox. Very cool image Suspected Asteroid Collision Leaves Trailing Debris WASHINGTON, Feb. 2 \/PRNewswire-USNewswire\/ &#8212; NASA&#8217;s Hubble Space Telescope has observed a mysterious X-shaped debris pattern and trailing streamers of dust that suggest a head-on collision between two asteroids. Astronomers have long thought the asteroid belt [&hellip;]<\/p>\n","protected":false},"author":4050,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[],"class_list":["post-266854","post","type-post","status-publish","format-standard","hentry","category-news"],"_links":{"self":[{"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/posts\/266854","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/users\/4050"}],"replies":[{"embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/comments?post=266854"}],"version-history":[{"count":0,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/posts\/266854\/revisions"}],"wp:attachment":[{"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/media?parent=266854"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/categories?post=266854"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/tags?post=266854"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}