http://www.space.com/scienceastronomy/rare_earth_040803.htmlEarth is Rare, New Study Suggests
By Robert Roy Britt Senior Science Writer SPACE.com
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http://www.space.com/scienceastronomy/rare_earth_1_020715.html <snip> Theorists involved in the new study acknowledge the distinct possibility that there could be many solar systems similar to ours, as others have suggested
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http://www.space.com/scienceastronomy/astronomy/jupiter_typical_020128.html , and that we haven't seen them because technology has yet to allow their detection. But they raise an interesting counter-argument: All known extrasolar planets are roughly as massive as Jupiter or much more so. In studying about 100 of these, the scientists found most are similar to one another in terms of orbital characteristics, and that Jupiter is the oddball. The results are 98 percent on track by a scientific measure known as the significance level. It follows that perhaps the known extrasolar planets formed in a different manner, one by which rocky, Earth-like planets would not be created. "We have shown that the solar system, as represented by Jupiter, is formally not part of the distribution of observed extrasolar planetary systems," Martin Beer of the UK's University of Leicester told SPACE.com. "From this result we suggest that we may be looking at two different methods of planet formation." <snip>
The leading model of planet formation -- conjured before anyone knew there were planets around other stars -- is called core accretion. A rocky core develops first, then an object either becomes a terrestrial planet (like Mercury, Venus, Earth or Mars) or it attracts huge amounts of gas and grows into something like Jupiter or Saturn. An alternative method
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http://www.space.com/scienceastronomy/solarsystem/planet_formation_020709-1.html forms a gas giant planet via the gravitational collapse of a knot of material.
Scientists disagree which way the outer planets of our solar system were born. The core accretion model has shortcomings. For one thing, when run on a computer, Neptune and Uranus typically don't show up. Further, observations reveal that Saturn has a solid core but Jupiter does not
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http://www.space.com/scienceastronomy/planet_formation_040720.html .
The gravitational collapse model has been invoked to explain some these discrepancies. It is also appealing as a method for making the gargantuan gaseous planets found around other stars. Most are a few to several times the mass of Jupiter and orbit incredibly near to their host stars on wildly non-circular orbits.
In all but a handful
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http://www.space.com/scienceastronomy/astronomy/planet_discovery_020613.html of these setups, rocky inner planets are not possible because they'd be consumed by a giant or gravitationally booted out of the "habitable zone," a comfortable region that can support life, Beer explained. Earth and Mars both orbit stabily in just such a temperate area, thanks to the fact that the outer planets are far away and on nearly circular orbits.
If gravitational collapse formed the known extrasolar planets, then there's no need for rocky cores. "Without these rocky cores, terrestrial planets (that is, Earth-like) do not form," Beer points out.<snip>
A firmer answer to our uniqueness will likely come around the end of this decade from NASA (news - web sites)'s space-based Kepler mission, due to launch in 2007. It is designed to detect Earth-sized planets by searching 100,000 stars for four years, looking for tiny dips in stellar brightness that would indicate an orbiting object.<snip>
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