
BABY GIANT PLANET swoops up gas from the disk around a newborn star.
Image: Illustration by Don Dixon
In Brief
- Barely a decade ago scientists who study how planets form had to base their theory on a single example—our solar system. Now they have dozens of mature systems and dozens more in birth throes. No two are alike.
- The basic idea behind the leading theory of planetary formation—tiny grains stick together and swoop up gas—conceals many levels of intricacy. A chaotic interplay among competing mechanisms leads to a huge diversity of outcomes.
More In This Article
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Photo Album
Slideshow: Genesis of Planets
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Infographic
Stage 2: Cosmic dust bunnies
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Stage 3: The rise of the oligarchs
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Infographic
Stage 4: One giant leap for planetkind
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Infographic
Stage 5: How to hug a star
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Stage 6: Enlarging the family
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Stage 7: Noncircular reasoning
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Sidebar
Meteorites: Emissaries from the Past
Although they are, in cosmic terms, mere scraps—insignificant to the grand narrative of heavenly expansion—planets are the most diverse and intricate class of object in the universe. No other celestial bodies support such a complex interplay of astronomical, geologic, and chemical and biological processes. No other places in the cosmos could support life as we know it. The worlds of our solar system come in a tremendous variety, and even they hardly prepared us for the discoveries of the past decade, during which astronomers have found more than 200 planets.
The sheer diversity of these bodies’ masses, sizes, compositions and orbits challenges those of us trying to fathom their origins. When I was in graduate school in the 1970s, we tended to think of planet formation as a well-ordered, deterministic process—an assembly line that turns amorphous disks of gas and dust into copies of our solar system. Now we are realizing that the process is chaotic, with distinct outcomes for each system. The worlds that emerge are the survivors of a hurly-burly of competing mechanisms of creation and destruction. Many are blasted apart, fed into the fires of their system’s newborn star or ejected into interstellar space. Our own Earth may have long-lost siblings that wander through the lightless void.
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6 Comments
Add CommentRubbish.
Reply | Report Abuse | Link to thisIn the light of observational and theoretical constraints the Solar Nebula model is untenable. At almost every stage of the proposed mechanism there are difficulties either with formation timescales or with basic theoretical problems. As an example, at the distance of the Earth a planetary embryo of 0.1 Earth mass would plunge into the Sun in less than the time for the embryo to grow to terrestrial mass. This is due to what is called Type 1 migration. There are other and even more severe difficulties - detailed by those that work with the theory. For details read 'The Formation of the Solar System; Theories Old and New' by M M Woolfson. This also describes an alternative model without any presently-known theoretical or observational difficulties.
Reply | Report Abuse | Link to thisMany questions arise from this article.
Reply | Report Abuse | Link to thisWhere does the energy for heat transfer come from -during planet growth via collisions of all these particles can a planet really outshine its star? That's a lot of energy -it would need to be nuclear. Can the nuclear decay at the core of planets be explained with this evolution process?
Why should an increased gravity decrase the number of collisions by stirring up things? Is this correct according to standard gravitational theory, i.e. Einstein's
Reply | Report Abuse | Link to thisWhy should an increased gravity decrase the number of collisions by stirring up things? Is this correct according to standard gravitational theory, i.e. Einstein's
Reply | Report Abuse | Link to thisSee my blog on the Origin of thee Solar System:
Reply | Report Abuse | Link to thishttp://acksblog.firmament-chaos.com/2008/01/25/the-origin-of-the-solar-system/