[meteorite-list] Giant Remnants of Cosmic Collision Found Beyond Neptune
From: Sterling K. Webb <sterling_k_webb_at_meteoritecentral.com>
Date: Wed, 14 Mar 2007 20:39:42 -0500 Message-ID: <002d01c766a2$ce102c50$9948e146_at_ATARIENGINE> Hi, Yet another piece of pre-print puffery about tomorrow's Nature article, but (for the first time) it includes the details of the case: the existence of a collisional family from the Big Whack on 2003 EL61. One thing that is made clear is that the often repeated 4.5 billion year old date for the Big Whack is nothing but prejudicial guesswork, an unsupported assumption based on cherished desire not to have anything going on recently in the solar system. The collisional families in the Asteroid Belt were all assumed to be ancient. Every textbook and paper for decades has said so, that they must have originated in the first billion years of the solar system. With the advent of truly powerful computational technology a few brave souls suggested that the most recent "might" be less than a billion years old, perhaps only a few hundred million years. In the last decade, however, it has been demonstrated that these collisional families that we can closely observe are very recent, only a few million years old, Not billions, millions. This makes perfect sense, as such families are easily perturbed until they can only be identified with difficulty. Another source of the "ancient" rationale, is the amusing but universally held notion that the Kuiper Belt once had 100 to 1000 times its present mass, but lost it all. A truly whacky idea. Again, a few brave souls have called it a "missing mass" problem, and there are searches underway to see if it's really so. [The first one, a study of Sco1 Xray occultations, indicates that there's a lot more mass out there than was thought.] > the distant past, perhaps as far back as 4.5 billion > years ago, when the Kuiper Belt was much more > crowded than it is now... So we have the paradox of being told there's nothing there by the very people who keep finding things there. That's basically strange. And finally, we have a time line on 2003 EL61 leaving the Kuiper Belt and entering the inner solar system -- maybe a billion years or so in the future. Since even the best dynamic computations cannot be trusted for more 250 to 500 million years ahead, the billion year prediction sounds like... [politely] hot air. And we only have a fraction of one orbit observed of 2003 EL61 upon which to calculate the parameters of its orbit. Why don't you wait a century or so, Mike? Then we'll know what its orbit really is. Tomorrow, those with access to the journal Nature will get to see the actual data. Leaves me out. For now, this piece has more information that the previous ones posted to the List. Sterling K. Webb --------------------------------------------------------------------- http://www.space.com/scienceastronomy/070314_kuiper_family.html Giant Remnants of Cosmic Collision Found Beyond Neptune By Ker Than Staff Writer posted: 14 March 2007 1:00 pm ET Shiny, gray space boulders floating in the outskirts of the solar system are the remnants of an ancient fiery collision involving two massive objects, the larger of which was nearly the size of Pluto, scientists say. This rocky goliath could one day cross the orbit of Neptune and become one of the biggest comets ever known. The findings, detailed in the March 15 issue of the journal Nature, mark the first "collisional family" detected in the Kuiper Belt and provide new insights about the solar system's murky history. The Kuiper Belt is a vast expanse of space located beyond the orbit of Neptune. It is littered with rocky and icy bodies believed to be vestiges of the primordial disk from which the planets formed. A suburban family The parent body of the new collisional family is thought to be 2003 EL61, one of the largest objects in the Kuiper Belt. It currently is football-shaped [image], with a diameter of about 930 miles (1,500 kilometers), but was probably spherical and 20 percent larger before the collision, the researchers say. Pluto is about 1,400 miles (2,300 km) wide. 2003 EL61 is thought to have collided with an object in its distant past that was roughly half its size and traveling at nearly 7,000 mph. The amount of energy generated by the blast would have equaled about 10 billion nuclear bombs, said study team member Darin Ragozzine of Caltech. "In terms of collisions in the solar system, that's actually kind of mild," Ragozzine told SPACE.com. The impact blasted large icy chunks from 2003 EL61 into space and sent the parent body reeling, causing it to spin end-over-end every four hours. "It spins so fast that it has pulled itself into the shape of an American football, but one that's a bit deflated and stepped on," said Michael Brown, a Caltech planetary scientist who led the study. The impact spawned at least seven other rocky objects-and likely more-with diameters ranging from 6 to 250 miles (10 to 400 km). The researchers lumped the scattered objects into a family based on their matching gray color and evidence of surface water ice derived from spectral analyses. "None of the rest of the Kuiper Belt is as shiny and pristine" as these objects are, Ragozzine said. About 35 other collisional families are known, but they are all located in the asteroid belt, the rocky region of space between the orbits of Mars and Jupiter. A 'milestone' Alessandro Morbidelli, an astronomer at the Laboratoire Cassiopee in France, who was not involved in the study, called the discovery a "milestone in Kuiper Belt science." Writing in an accompanying Nature news article, Morbidelli said the discovery provides a physical model for astronomers to test their theories about the kinds of large-scale collisions thought to be behind the birth of our Moon and the Pluto- Charon system. Because such large collisions are relatively rare, scientists think the one involving 2003 EL61 occurred in the distant past, perhaps as far back as 4.5 billion years ago, when the Kuiper Belt was much more crowded than it is now and objects were more likely to bump into one another. If scientists can pin down when the collision occurred, they will have a unique glimpse into a specific time in the solar system's history and the evolution of the Kuiper Belt, Morbidelli said. To be a comet Some of the shards from the impact have made their way to the inner Solar system, the researchers say. "Probably, there are comets that we have seen that came from this collision," Brown said in a telephone interview. "In fact, there are probably chunks of that collision here on the ground." One day, EL2003 EL61 will cross the orbit of Neptune and become a comet itself. "That's going to be in about a billion years," Brown said. "It's a ways to wait." Received on Wed 14 Mar 2007 09:39:42 PM PDT |
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