Share on Facebook Share on Twitter Email
Answers.com

Ocean planet

 
Wikipedia: Ocean planet
Illustration of a hypothetical ocean planet with a terrestrial atmosphere and two satellites

An ocean planet is a hypothetical type of planet whose surface is completely covered with an ocean of water.

Planetary objects that form in the outer solar system begin as a comet-like mixture of roughly 50% water and 50% rock by weight. Simulations of solar system formation have shown that planets are likely to migrate inward or outward as they form, presenting the possibility that icy planets could move to orbits where their ice melts into liquid form, turning them into ocean planets. This possibility was first discussed in the professional astronomical literature by Marc Kuchner [1] and Alain Léger[2] in 2003. Such planets could theoretically support life.

The oceans on such planets could be hundreds of kilometers deep, much deeper than the oceans of Earth. The immense pressures in the lower regions of these oceans could lead to the formation of a mantle of exotic forms of ice. This ice would not necessarily be as cold as conventional ice. If the planet is close enough to its sun that the water's temperature reaches the boiling point, the water will become supercritical and lack a well-defined surface.[2]

The extrasolar planet GJ 1214 b is currently the most likely candidate for an ocean planet, with data-fitting mass and radius values that are consistent with a modeled composition of 75% H2O (and 22% Si, 3% Fe).[3][4]

Fictional ocean planets

Fictional ocean planets have been used as story motifs:

References

  1. ^ "Volatile-rich Earth-Mass Planets in the Habitable Zone". Astrophysical Journal. 2003-10-10. http://www.journals.uchicago.edu/doi/full/10.1086/378397. 
  2. ^ a b "Ocean Planets on the Brink of Detection". Physorg.com. 2007-02-02. http://www.physorg.com/news89627725.html. Retrieved 2007-02-02. 
  3. ^ Charbonneau, David; Zachory K. Berta, Jonathan Irwin, Christopher J. Burke, Philip Nutzman, Lars A. Buchhave, Christophe Lovis, Xavier Bonfils, David W. Latham, Stéphane Udry, Ruth A. Murray-Clay, Matthew J. Holman, Emilio E. Falco, Joshua N. Winn, Didier Queloz, Francesco Pepe, Michel Mayor, Xavier Delfosse, Thierry Forveille (2009). "A super-Earth transiting a nearby low-mass star". Nature 462 (17 December 2009): 891-894. doi:10.1038/nature08679. http://www.nature.com/nature/journal/v462/n7275/full/nature08679.html. Retrieved 2009-12-15. 
  4. ^ Kuchner, Seager; M., Hier-Majumder, C. A., Militzer (2007). "Mass–radius relationships for solid exoplanets". The Astrophysical Journal 669: 1279–1297. doi:10.1086/521346. http://www.iop.org/EJ/abstract/0004-637X/669/2/1279/. 
  5. ^ Adam Charles Roberts. Science Fiction. http://books.google.com/books?id=RAvM9els2acC&pg=PA17&dq=solaris+%22ocean+planet%22&lr=&hl=it&cd=11#v=onepage&q=solaris%20%22ocean%20planet%22&f=false. 
  6. ^ a b c www.daviddarling.info Ocean Planet

External links


Search unanswered questions...
Enter a question here...
Search: All sources Community Q&A Reference topics
 
 

 

Copyrights:

Wikipedia. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article "Ocean planet" Read more