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Thread: A planet past Pluto? Astronomers redefine the solar system's edge

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    Default A planet past Pluto? Astronomers redefine the solar system's edge

    Nibiru found? LOL

    A planet past Pluto? Astronomers redefine the solar system's edge

    FoxNews.com





    • These are the discovery images of 2012 VP113, nicknamed Biden because of the VP in the provisional name. Three images of the night sky, each taken about two hours apart, were combined into one. The first image was artificially colored red, second green and third blue. 2012 VP113 moved between each image as seen by the red, green and blue dots. The background stars and galaxies did not move and thus their red, green and blue images combine to show up as white sources. (Scott Sheppard and Chad Trujillo)







    • The solar system is made up the sun, eight planets, 138 moons and many comets, asteroids and other space rocks. (NASA)







    • This is an orbit diagram for the outer solar system. The Sun and Terrestrial planets are at the center. The orbits of the four giant planets, Jupiter, Saturn, Uranus and Neptune, are shown by purple solid circles. The Kuiper Belt, including Pluto, is shown by the dotted light blue region just beyond the giant planets. Sedna's orbit is shown in orange while 2012 VP113's orbit is shown in red. Both objects are currently near their closest approach to the Sun (perihelion). (Scott Sheppard and Chad Trujillo)


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    Our little corner of the universe just got a little more crowded.


    Scientists at the Carnegie Carnegie Institution for Science announced Wednesday the discovery of a new cosmic neighbor -- a distant dwarf planet named 2012 VP113 that was found spinning in the depths of space well past Pluto. Its existence suggests there may be another actual planet out there, they said, a rogue giant ten times bigger than Earth orbiting in the distant blackness.


    One thing is clear: Astronomers will have to rethink the cosmic limits of our solar system.


    "This is an extraordinary result that redefines our understanding of our solar system," Linda Elkins-Tanton, director of Carnegie’s Department of Terrestrial Magnetism, said in a press release.
    'Some of these objects could rival the size of Mars or even Earth.'
    - Scott Sheppard of the Gemini Observatory

    The solar system as we know it today is divided into three parts: First come the rocky, Earth-like planets that are closest to the sun, next the gas giant planets like Jupiter and Saturn, and finally the frozen objects in the Kuiper Belt outside of Neptune's orbit.


    Pluto, which was demoted from planet status to dwarf planet in 2006, lives in the Kuiper Belt. And in it there appears to be a clear edge to the solar system 50 astronomical units out (AUs, a measure of the distance from the Earth to the sun) -- with the exception of the 2003 discovery of Sedna, one of those frozen objects that was believed until now to be the furthest known thing from the sun.


    Sedna lives in a region of space called the Oort cloud, a vast region of space that may be where many comets come from. Sedna lives in it, and the discovery of 2012 VP113 suggests that there may nearly 1,000 objects beyond that 50 AU "end" of the solar system.


    "The search for these distant inner Oort cloud objects beyond Sedna and 2012 VP113 should continue, as they could tell us a lot about how our solar system formed and evolved," Carnegie’s Scott Sheppard of the Gemini Observatory said in a press release.


    2012 VP113 is located 80 times the distance of the Earth from the sun (80 AUs), while Sedna is at 76 AU.


    Sheppard and fellow researcher Chadwick Trujillo determined that the Oort cloud is likely bigger than the Kuiper Belt and main asteroid belt. And the similarity in the orbits of Sedna, 2012 VP113 and a few other objects out there suggests that a massive planet may be shepherding them. Sheppard and Trujillo suggest a super Earth or an even larger object at hundreds of AU could create the shepherding effect seen in the orbits of these objects, which are too distant to be pulled on significantly by any of the known planets.


    "Some of these inner Oort cloud objects could rival the size of Mars or even Earth," said Sheppard. "This is because many of the inner Oort cloud objects are so distant that even very large ones would be too faint to detect with current technology."
    The findings are published in the March 27 edition of Nature.
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    Default Re: A planet past Pluto? Astronomers redefine the solar system's edge

    Dwarf Planet Discovery Could Help Show Life's Spread Through Solar System
    by Elizabeth Howell for Astrobiology Magazine
    Moffett Field CA (SPX) Apr 01, 2014

    Comparisons of some of the dwarf planets with the Earth and the moon. Image courtesy NASA.
    On March 26, researchers announced the discovery of 2012 VP133, an estimated 280-mile wide (450-kilometer) object that lies just beyond the Kuiper Belt of icy objects that swarm outside of Neptune's orbit. The new object is nicknamed "Biden" after the vice-president of the United States, because both Joe Biden and 2012 VP133 are "VPs." It is one of only two dwarf planets discovered beyond the Kuiper Belt, with Sedna (a decade ago) being the other one.
    The paper, "A Sedna-like body with a perihelion of 80 astronomical units," was published in the journal Nature. Mapping tiny worlds at the Solar System's edge could one day show scientists how life arose on Earth. That's because many of these objects could contain organics, carbon-based material that are ingredients for life.
    As the scientists continue their search, they expect that 2012 VP133 will be the first of a series of discoveries of such objects. Finding such a world has a value of its own, but the team is also thinking of a greater astrobiological question as they study 2012 VP133. Are the possible organics -which show up as ultra-red material in telescopes - a possible source for life on Earth? And could be this be true of other planetary systems as well?
    "One of the questions I've had is trying to map out what is this ultra-red material in the Kuiper Belt," said Scott Sheppard, a faculty member at the Carnegie Institution for Science, Department of Terrestrial Magnetism (DTM) in Washington, D.C.
    Sheppard co-discovered the object along with the Gemini Observatory's Chadwick Trujillo.
    Curiously enough, 2012 VP133 has none of this material on it, but Sedna does. It will take more discoveries of such objects to figure out if ultra-red material is common outside of the Kuiper Belt, and how organics could have been transported to Earth early in our Solar System's history.
    A treasure trove of possible organics
    Most dwarf planets found to date - including Pluto, which was once considered a planet - reside in the Kuiper Belt, a vast collection of frozen objects that orbit our Sun about 30 to 50 astronomical units (AUs) away. One astronomical unit is the distance between the Earth and the Sun, about 150 million kilometers.
    There are millions of objects in the Kuiper Belt, but the ones that interest Sheppard and his colleagues are those that have "resonances" with Neptune. An orbital resonance occurs when two bodies - like a planet and a moon, or a planet and an asteroid - exert gravitational influences on each other that put them into closely related orbits.
    In a 2012 paper in the Astronomical Journal, "The Color Differences of Kuiper Belt Objects in Resonance with Neptune," Sheppard examined 58 Kuiper Belt objects that have a resonance with the gas giant.
    He found that those resonant objects that are embedded in the Kuiper Belt are full of this ultra-red material, indicating likely organics. On the edge of the belt, some of those objects also still have the material, showing that it is somehow leaking into the inner Solar System. Those that are quite far away, however, show none of the material.
    Sedna and 2012 VP133 are well beyond the boundaries of the Kuiper Belt. Sheppard's new paper argues that they are part of the edges of the Oort Cloud, a theorized icy collection of objects extending thousands of AUs away from Earth. (The Oort Cloud is perhaps best known for being the supposed source of many comets that fly into the inner solar system.)
    It's difficult to envision how dwarf planets such as Sedna and 2012 VP133 could receive ultra-red material from the Kuiper Belt because they are so far away from it. Further, it's unclear why only Sedna (of the two dwarf planets known in that region) has the material. They're too far away for Neptune to have any influence on them. So what happened? "Determining what resonants have and do not have ultra-red material helps us understand how the ultra-red material has moved around the outer Solar System," said Sheppard.
    A big jolt
    Looking at other objects, it becomes clear that something big likely disturbed some of them. For example, Sedna's weird orbit got the attention of researchers because it is so eccentric. The dwarf planet ranges between 80 AU and 940 AU - meaning that one orbit takes about 11,400 years to complete. It's by far the most eccentric orbit in the Solar System.
    "It probably formed much further in and somehow got scattered out there and captured into the no-man land area," Sheppard said.
    Sheppard and Trujillo then compared Sedna's and 2012 VP133's orbits with 10 representative Kuiper Belt objects that have eccentric orbits. To their surprise, they found that all 12 of them had almost identical "arguments of perihelion." That's an orbital parameter that measures the angle between two points in each object's orbit: the closest approach to the Sun, and the location where the objects cross the plane of the Solar System.
    "They should just have random arguments of perihelion," Sheppard said.
    The similarities point to a giant disturbance causing chaos. There are three theories for this. Perhaps a rogue planet (Earth's size or smaller) was ejected out of the Solar System, throwing smaller objects aside as it passed into the outer Solar System.
    "That rogue planet could have been ejected or it could be out there today," Sheppard said.
    He said it would be too dim to show up in surveys, such as NASA's Wide-field Infrared Survey Explorer (WISE), a spacecraft more suited to finding gas giant planets, which emit their own heat.
    Another theory - the leading one - says a passing star about 200 AU from our own caused huge gravitational disturbances. It seems easy to explain a star tugging on the wandering Sedna, but VP113 has a more circular orbit that only goes as far as 266 AU.
    "That makes VP113 more tightly bound to the Sun, and it's harder to form that from a stellar encounter," Sheppard said. "It would have to be stronger or a bigger object, so it's less likely to have happened."
    The third - Sheppard termed it the "dark horse" theory - suggests the Sun captured extrasolar planets from another star early in the Sun's history, while it was forming in a cloud of gas and young stars.
    Hundreds of objects waiting for discovery
    As Sheppard wrestles with the question of how the ultra-red material moved around, he's also interested in learning more about the nature of the material itself. Researchers suspect it's organics, but what sort of organics is of great interest. Luckily, there's a chance to take a closer look.
    NASA's New Horizons probe is currently sailing to the outer Solar System. It's expected to make a pass by Pluto and its moons in 2015 before zooming toward the Kuiper Belt. After the Pluto encounter is finished, perhaps the spacecraft could turn its observations to an ultra-red object. No candidates have been identified yet, but this is a possibility, Sheppard said.
    Sheppard's search of the outer Solar System will continue. He and his collaborators have some suspected new objects that need confirmation, and better yet, his research estimates that there could be at least 900 objects in the Oort Cloud's fringes that are at least 621 miles (1,000 km) in diameter - a little less than half of Pluto's size.
    "There are for sure some bigger than Pluto, and there might be some bigger than Earth or Mars," Sheppard said. "We think there's a lot of these objects out there."
    Libertatem Prius!


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