Difference between revisions of "Terrestrial Planet"

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A '''Terrestrial Planet''' is a planet with a compact, rocky surface, like the Earth's, and a density greater than 3 grams per cubic cm.<ref>http://www.britannica.com/EBchecked/topic/553008/solar-system/242057/Planets-and-their-moons#ref515542</ref> By comparison, water has a density of 1 gram per cubic cm. They are composed primarily of rock and metal, have a slow rate of rotation, no rings and few satellites.<ref>http://www.nineplanets.org/overview.html</ref>  
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A '''Terrestrial Planet''' is a planet with a compact, rocky surface, like the Earth's, and a density greater than 3 grams per cubic cm.<ref>https://www.britannica.com/EBchecked/topic/553008/solar-system/242057/Planets-and-their-moons#ref515542</ref> By comparison, water has a density of 1 gram per cubic cm. They are composed primarily of rock and metal, have a slow rate of rotation, no rings and few satellites.<ref>http://www.nineplanets.org/overview.html</ref>  
  
 
Within our [[Solar System]] the four innermost planets, [[Mercury]], [[Venus]], [[Earth]] and [[Mars]] are all terrestrial planets.
 
Within our [[Solar System]] the four innermost planets, [[Mercury]], [[Venus]], [[Earth]] and [[Mars]] are all terrestrial planets.
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== See also ==
 
== See also ==
*[[Joavian Planet]]
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*[[Jovian Planet]]
  
 
==References==
 
==References==

Latest revision as of 20:40, September 26, 2018

A Terrestrial Planet is a planet with a compact, rocky surface, like the Earth's, and a density greater than 3 grams per cubic cm.[1] By comparison, water has a density of 1 gram per cubic cm. They are composed primarily of rock and metal, have a slow rate of rotation, no rings and few satellites.[2]

Within our Solar System the four innermost planets, Mercury, Venus, Earth and Mars are all terrestrial planets.


See also

References