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1 References  





2 See also  














Protoplanet: Difference between revisions






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Often compared to such groups as; Joe Satriani, Steve Vai, Planet X, Rush, and Dream Theater, Protoplanet is paving the way for the next generation of instrumental guitar rock.

Often compared to such groups as; Joe Satriani, Steve Vai, Planet X, Rush, and Dream Theater, Protoplanet is paving the way for the next generation of instrumental guitar rock.



[[www.protoplanetband.com]]

'[www.protoplanetband.com]'



[[www.reverbnation.com/protoplanet]]

'[www.reverbnation.com/protoplanet]'



[[www.myspace.com/protoplanet]]

'[www.myspace.com/protoplanet]'



'''Protoplanets''' are moon-sized or larger planetary embryos within [[protoplanetary disc]]s that have undergone internal melting to produce differentiated interiors. They are believed to form out of kilometer-sized [[planetesimal]]s that attract each other gravitationally and collide. According to [[solar nebula|planet formation theory]], protoplanets perturb each other's orbits slightly and thus collide in giant impacts to gradually form the dominant [[planet]]s.

'''Protoplanets''' are moon-sized or larger planetary embryos within [[protoplanetary disc]]s that have undergone internal melting to produce differentiated interiors. They are believed to form out of kilometer-sized [[planetesimal]]s that attract each other gravitationally and collide. According to [[solar nebula|planet formation theory]], protoplanets perturb each other's orbits slightly and thus collide in giant impacts to gradually form the dominant [[planet]]s.


Revision as of 18:01, 21 February 2011

Protoplanet is an instrumental progressive rock band from Portland, OR.

Often compared to such groups as; Joe Satriani, Steve Vai, Planet X, Rush, and Dream Theater, Protoplanet is paving the way for the next generation of instrumental guitar rock.

'[www.protoplanetband.com]'

'[www.reverbnation.com/protoplanet]'

'[www.myspace.com/protoplanet]'

Protoplanets are moon-sized or larger planetary embryos within protoplanetary discs that have undergone internal melting to produce differentiated interiors. They are believed to form out of kilometer-sized planetesimals that attract each other gravitationally and collide. According to planet formation theory, protoplanets perturb each other's orbits slightly and thus collide in giant impacts to gradually form the dominant planets.

In the case of the Solar System it is thought that the collisions of planetesimals created a few hundred planetary embryos. Such embryos were similar to Pluto with masses of about 1022 to 1023 kg and were a few thousand kilometres in diameter. Over the course of about 100 Ma they were involved in giant impacts with one another. The exact sequence whereby planetary embryos collided to assemble the planets is not known, but it is thought that initial collisions would have replaced the first "generation" of embryos with a second generation consisting of fewer but larger embryos. These in their turn would have collided to create a third generation of fewer but even larger embryos. Eventually only a handful of embryos were left, which collided to complete the assembly of the planets proper.[1]

Early protoplanets had more radioactive elements, the quantity of which has been reduced over time due to radioactive decay. Heating due to radioactivity, impact, and gravitational pressure melted parts of protoplanets as they grew toward being planets. In melted zones their heavier elements sank to the center; while lighter elements rose to the surface; such a process is known as planetary differentiation. Composition of some meteorites show that differentiation took place in some asteroids.

The giant impact theory proposes that Earth's Moon formed from a colossal impact of a hypothetical protoplanet, named Theia, with Earth, early in the solar system's history.

In the inner Solar System, the three protoplanets to survive more-or-less intact are the dwarf planet 1 Ceres and the asteroids 2 Pallas, and 4 Vesta.[2] Kuiper Belt dwarf planets have been referred to as protoplanets also.[3]

References

  1. ^ McBride, Neil (2004). An Introduction to the Solar System. Cambridge: Cambridge University Press. p. 56. ISBN 978052183735. {{cite book}}: Check |isbn= value: length (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  • ^ "BIG PIC: 2 Pallas, the Asteroid with Protoplanetary Attitude". Discovery Space. Discovery Communications. 2009-10-08. Retrieved 2009-10-08. {{cite web}}: Cite has empty unknown parameter: |coauthors= (help)
  • ^ Alan Boyle (2009-10-08). "Protoplanet frozen in time". MSNBC. Retrieved 2009-09-12.
  • See also


    Retrieved from "https://en.wikipedia.org/w/index.php?title=Protoplanet&oldid=415166860"

    Category: 
    Types of planet
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    CS1 errors: unsupported parameter
    CS1 errors: ISBN
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    This page was last edited on 21 February 2011, at 18:01 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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