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| | Origin of Trans-Neptunian Asteroids |
 | | If the trans-Neptunian objects are debris from an exploded planet, as a great deal of evidence suggests is the case for main-belt asteroids, then their initial orbits would have to exhibit a wide range of eccentricities, inclinations, and mean distances from the Sun. |
 | | If the trans-Neptunian objects are from a parent body that exploded, the 35,000 number mentioned earlier can be combined with a mean diameter of, say, 150 km each to imply a parent body at least 5000 km in diameter, the size of Saturn’s moon Titan. |
 | | It therefore may be concluded with certainty that something fundamental is missing in conventional models suggesting accretion of these objects from a primeval solar nebula. |
| www.metaresearch.org /solar%20system/asteroids/trans-NeptunianAsteroids.asp (1533 words) |
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