{"id":442037,"date":"2010-03-18T03:22:00","date_gmt":"2010-03-18T07:22:00","guid":{"rendered":"tag:blogger.com,1999:blog-1752027331714385066.post-9152444644644181436"},"modified":"2010-03-18T03:22:46","modified_gmt":"2010-03-18T07:22:46","slug":"wise-hunts-nemesis-the-death-star","status":"publish","type":"post","link":"https:\/\/mereja.media\/index\/442037","title":{"rendered":"WISE Hunts Nemesis the &#8216;Death Star&#8217;"},"content":{"rendered":"<div class=\"separator\" style=\"clear: both; text-align: center;\"><a href=\"http:\/\/1.bp.blogspot.com\/_Jx78YcF-F8U\/S6HUuxru85I\/AAAAAAAABQ8\/Ib4cRz36yN8\/s1600-h\/images.jpg\" imageanchor=\"1\" style=\"margin-left: 1em; margin-right: 1em;\"><img decoding=\"async\" border=\"0\" src=\"http:\/\/1.bp.blogspot.com\/_Jx78YcF-F8U\/S6HUuxru85I\/AAAAAAAABQ8\/Ib4cRz36yN8\/s320\/images.jpg\" \/><\/a><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\"><br \/><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\"><br \/><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">It is quite plausible that a large Jupiter sized object could be maintaining a distant orbit around the solar system<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>I would expect that such an orbit would be generally similar to that of the other planets although it could easily be tilted like that of Neptune. (I think that is right at seventeen degrees except that I do not know why I remember that)<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">I think associating it with a 26 million year cycle is not particularly plausible at all.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>The time frame allows any pass close to another star system to trigger a cascade of debris.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>Recall that we already appear to be orbiting the Sirius cluster on a one to two hundred year orbit and this does affect us.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>It would surely increase the probability of a close stellar encounter able to disturb the Oort belt.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">Close passes with unrelated stars is also a good possibility and may explain some events in the geological record and more believably that a particular orbit millions of years long.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">There is one remaining conjecture that could have spawned a legend like Nemesis which after all was close enough to be perceived by the naked eye.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>It is that Jupiter spat out Venus within the past few thousands of years and human legend has carried the story forward. First, it is enough to know that Jupiter is large enough and rotating fast enough to do this should it absorb a planet sized body.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>It is my conjecture that all the inner solar system and perhaps parts of the outer system were created this way.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">Velikovsky\u2019s contribution was to extract this story out of the cultural records available and actually tell it.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">Over many orbits, this new planet settled down into its present orbit while initially crossing Earth\u2019s orbit many times.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>It must have appeared many times in the sky approaching the size of the moon and made an exceptional impression on humanity.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">In the thousands of years since this happened, the surface of Venus maintains a high rock temperature that sustains an equally high atmospheric temperature.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>That would be impossible unless the rock itself was extremely hot.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>Venus is that recent a planet.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">Also Jupiter retains the scar from this event known as the red spot.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">I am inclined to accept this last as the source of ancient legends mainly because stellar events are simply too far distant in time.<span style=\"mso-spacerun: yes;\">&nbsp; <\/span>We are far from Sirius (we are heading in that direction against the flow of the galaxy in case you have any doubt) or any other star and have a quiet solar system presently around us.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">In the event we are soon to begin a deeper survey of near space and I expect plenty of surprises well beyond what we now conjecture.<o:p><\/o:p><\/span><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><b><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">Getting WISE About Nemesis<o:p><\/o:p><\/span><\/i><\/b><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">by Leslie Mullen<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/>for&nbsp;<a href=\"http:\/\/www.astrobio.net\/\">Astrobiology Magazine<\/a><o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><st1:place w:st=\"on\"><st1:city w:st=\"on\">Moffett Field<\/st1:city> <st1:state w:st=\"on\">CA<\/st1:state><\/st1:place> (SPX) Mar 12, 2010<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"letter-spacing: 0pt;\"><a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html\">http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html<\/a><o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><a href=\"http:\/\/www.spacedaily.com\/images-lg\/sun-lowmass-browndwarf-jupiter-earth-chart-lg.jpg\">http:\/\/www.spacedaily.com\/images-lg\/sun-lowmass-browndwarf-jupiter-earth-chart-lg.jpg<\/a><o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: windowtext; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Size comparison of our Sun, a low mass star, a brown dwarf, Jupiter, and Earth. Stars with less mass than the Sun are smaller and cooler, and hence much fainter in visible light. Brown dwarfs have less than eight percent of the mass of the Sun, which is not enough to sustain the fusion reaction that keeps the Sun hot. These cool orbs are nearly impossible to see in visible light, but stand out when viewed in infrared. Their diameters are about the same as Jupiter&#8217;s, but they can have up to 80 times more mass and are thought to have planetary systems of their own. Image credit: NASA<\/span><\/i><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/>A dark object may be lurking near our&nbsp;<a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html##\" >solar&nbsp;system<\/a>, occasionally kicking comets in our direction.<\/span><\/i><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: windowtext; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Nicknamed &#8220;Nemesis&#8221; or &#8220;The Death Star,&#8221; this undetected object could be a red or brown dwarf star, or an even darker presence several times the mass of Jupiter.<\/span><\/i><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: windowtext; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Why do scientists think something could be hidden beyond the edge of our solar system? Originally, Nemesis was suggested as a way to explain a cycle of mass extinctions on Earth.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">The paleontologists David Raup and Jack Sepkoski claim that, over the last 250 million years, life on Earth has faced extinction in a 26-million-year cycle. Astronomers proposed comet impacts as a possible cause for these catastrophes.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Our solar system is surrounded by a vast collection of icy bodies called the Oort Cloud. If our Sun were part of a binary system in which two gravitationally-bound stars orbit a common center of mass, this interaction could disturb the Oort Cloud on a periodic basis, sending comets whizzing towards us.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">An asteroid impact is famously responsible for the extinction of the dinosaurs 65 million years ago, but large comet impacts may be equally deadly. A comet may have been the cause of the Tunguska event in <st1:country-region w:st=\"on\"><st1:place w:st=\"on\">Russia<\/st1:place><\/st1:country-region> in 1908. That explosion had about a thousand times the power of the atomic bomb dropped on <st1:city w:st=\"on\"><st1:place w:st=\"on\">Hiroshima<\/st1:place><\/st1:city>, and it flattened an estimated 80 million trees over an 830 square mile area.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">While there&#8217;s little doubt about the destructive power of cosmic impacts, there is no evidence that comets have periodically caused mass extinctions on our planet. The theory of periodic extinctions itself is still debated, with many insisting that more proof is needed. Even if the scientific consensus is that extinction events don&#8217;t occur in a predictable cycle, there are now other reasons to suspect a dark companion to the Sun.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><b><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">The Footprint of Nemesis<o:p><\/o:p><\/span><\/i><\/b><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><b><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/b><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">A recently-discovered dwarf planet, named Sedna, has an extra-long and usual elliptical orbit around the Sun. Sedna is one of the most distant objects yet observed, with an orbit ranging between 76 and 975 AU (where 1 AU is the distance between the Earth and the Sun). Sedna&#8217;s orbit is estimated to last between 10.5 to 12 thousand years. Sedna&#8217;s discoverer, Mike Brown of Caltech, noted in a Discover magazine article that Sedna&#8217;s location doesn&#8217;t make sense.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">&#8220;Sedna shouldn&#8217;t be there,&#8221; said Brown. &#8220;There&#8217;s no way to put Sedna where it is. It never comes close enough to be affected by the Sun, but it never goes far enough away from the Sun to be affected by other stars.&#8221;<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Perhaps a massive unseen object is responsible for Sedna&#8217;s mystifying orbit, its gravitational influence keeping Sedna fixed in that far-distant portion of space.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">&#8220;My surveys have always looked for objects closer and thus moving faster,&#8221; Brown told Astrobiology Magazine. &#8220;I would have easily overlooked something so distant and slow moving as Nemesis.&#8221;<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">John Matese, Emeritus Professor of Physics at the University of Louisiana at Lafayette, suspects Nemesis exists for another reason. The comets in the inner solar system seem to mostly come from the same region of the Oort Cloud, and Matese thinks the gravitational influence of a solar companion is disrupting that part of the cloud, scattering comets in its wake.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">His calculations suggest Nemesis is between 3 to 5 times the mass of Jupiter, rather than the 13 Jupiter masses or greater that some scientists think is a necessary quality of a brown dwarf. Even at this smaller mass, however, many astronomers would still classify it as a low mass star rather than a planet, since the circumstances of birth for stars and&nbsp;<a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html##\" >planets<\/a>&nbsp;differ.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">The Oort Cloud is thought to extend about 1 light year from the Sun. Matese estimates Nemesis is 25,000 AU away (or about one-third of a light year). The next-closest known star to the Sun is Proxima Centauri, located 4.2 light years away.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Richard Muller of the University of <st1:state w:st=\"on\">California<\/st1:state> <st1:city w:st=\"on\"><st1:place w:st=\"on\">Berkeley<\/st1:place><\/st1:city> first suggested the Nemesis theory, and even wrote a popular science book on the topic. He thinks Nemesis is a red dwarf star 1.5 light years away.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Many scientists counter that such a wide orbit is inherently unstable and could not have lasted long &#8211; certainly not long enough to have caused the extinctions seen in Earth&#8217;s fossil record. But Muller says this instability has resulted in an orbit that has changed greatly over billions of years, and in the next billion years Nemesis will be thrown free of the solar system.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Binary star systems are common in the&nbsp;<a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html##\" >galaxy<\/a>. It is estimated that one-third of the stars in the Milky Way are either binary or part of a multiple-star system.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Red dwarfs are also common &#8211; in fact, astronomers say they are the most common type of star in the galaxy. Brown dwarfs are also thought to be common, but there are only a few hundred known at this time because they are so difficult to see. Red and brown dwarfs are smaller and cooler than our Sun, and do not shine brightly.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">If red dwarfs can be compared to the red embers of a dying fire, then brown dwarfs would be the smoldering ash. Because they are so dim, it is plausible that the Sun could have a secret companion even though we&#8217;ve searched the sky for many years with a variety of instruments.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html##\" >NASA&#8217;s<\/a>&nbsp;newest telescope, the Wide-field Infrared Survey Explorer (WISE), may be able to answer the question about Nemesis once and for all.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><b><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\">Finding Dwarfs in the Dark<o:p><\/o:p><\/span><\/i><\/b><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><b><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/b><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">WISE looks at our universe in the infrared part of the spectrum. Like the Spitzer space telescope, WISE is hunting for heat. The difference is that WISE has a much wider field of view, and so is able to scan a greater portion of the sky for distant objects.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">WISE began scanning the sky on January 14, and NASA recently released the mission&#8217;s first images. The mission will map the entire sky until October, when the <a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html##\" >spacecraft&#8217;s<\/a>&nbsp;coolant runs out.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Part of the WISE mission is to search for brown dwarfs, and NASA expects it could find one thousand of the dim stellar objects within 25 light years of our solar system.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Davy Kirkpatrick at NASA&#8217;s Infrared Processing and <st1:place w:st=\"on\"><st1:placename w:st=\"on\">Analysis<\/st1:placename> <st1:placetype w:st=\"on\">Center<\/st1:placetype><\/st1:place> at Caltech found nothing when he searched for Nemesis using data from the Two Micron All Sky Survey (2MASS). Now Kirkpatrick is part of the WISE science team, ready to search again for any signs of a companion to our Sun.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Kirkpatrick doesn&#8217;t think Nemesis will be the red dwarf star with an enormous orbit described by Muller. In his view, Matese&#8217;s description of Nemesis as a low mass object closer to home is more plausible.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">&#8220;I think the possibility that the Sun could harbor a companion of another sort is not a crazy idea,&#8221; said Kirkpatrick. &#8220;There might be a distant object in a more stable, more circular orbit that has gone unnoticed so far.&#8221;<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Ned Wright, professor of&nbsp;<a href=\"http:\/\/www.spacedaily.com\/reports\/Getting_WISE_About_Nemesis_999.html##\" >astronomy<\/a>&nbsp;and physics at UCLA and the principal investigator for the WISE mission, said that WISE will easily see an object with a mass a few times that of Jupiter and located 25,000 AU away, as suggested by Matese.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">&#8220;This is because Jupiter is self-luminous like a brown dwarf,&#8221; said Wright. &#8220;But for planets less massive than Jupiter in the far outer solar system, WISE will be less sensitive.&#8221;<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Neither Kirkpatrick nor Wright think Nemesis is disrupting the Oort cloud and sending comets towards Earth, however. Because they envision a more benign orbit, they prefer the name &#8220;Tyche&#8221; (the good sister).<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Regardless of what they expect to find, the WISE search won&#8217;t focus on one particular region of the sky.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">&#8220;The great thing about WISE, as was also true of 2MASS, is that it&#8217;s an all-sky survey,&#8221; said Kirkpatrick. &#8220;There will be some regions such as the Galactic Plane where the observations are less sensitive or fields more crowded, but we&#8217;ll search those areas too. So we&#8217;re not preferentially targeting certain directions.&#8221;<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">We may not have an answer to the Nemesis question until mid-2013. WISE needs to scan the sky twice in order to generate the time-lapsed images astronomers use to detect objects in the outer solar system. The change in location of an object between the time of the first scan and the second tells astronomers about the object&#8217;s location and orbit.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">&#8220;I don&#8217;t suspect we&#8217;ll have completed the search for candidate objects until mid-2012, and then we may need up to a year of time to complete telescopic follow-up of those objects,&#8221; said Kirkpatrick.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\"><br \/><\/span><\/i><\/div>\n<div class=\"MsoNormal\" style=\"mso-margin-bottom-alt: auto; mso-margin-top-alt: auto; text-align: justify;\"><i style=\"mso-bidi-font-style: normal;\"><span style=\"color: black; letter-spacing: 0pt; mso-bidi-font-weight: normal; mso-font-kerning: 0pt;\">Even if Nemesis is not found, the WISE telescope will help shed light on the darkest corners of the solar system. The telescope can be used to search for dwarf planets like Pluto that orbit the Sun off the solar system&#8217;s ecliptic plane. The objects that make up the Oort Cloud are too small and far away for WISE to see, but it will be able to track potentially dangerous comets and asteroids closer to home.<o:p><\/o:p><\/span><\/i><\/div>\n<div class=\"MsoNormal\"><\/div>\n<div class=\"blogger-post-footer\"><img width='1' height='1' src='https:\/\/blogger.googleusercontent.com\/tracker\/1752027331714385066-9152444644644181436?l=globalwarming-arclein.blogspot.com' alt='' \/><\/div>\n","protected":false},"excerpt":{"rendered":"<p>It is quite plausible that a large Jupiter sized object could be maintaining a distant orbit around the solar system&nbsp; I would expect that such an orbit would be generally similar to that of the other planets although it could easily be tilted like that of Neptune. (I think that is right at seventeen degrees [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[],"class_list":["post-442037","post","type-post","status-publish","format-standard","hentry","category-news"],"_links":{"self":[{"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/posts\/442037","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\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/comments?post=442037"}],"version-history":[{"count":0,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/posts\/442037\/revisions"}],"wp:attachment":[{"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/media?parent=442037"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/categories?post=442037"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/mereja.media\/index\/wp-json\/wp\/v2\/tags?post=442037"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}