Downhill creep: Difference between revisions

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{{Refimprove|date=December 2009}}
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In [[astrodynamics]], an '''orbiting body''' (<math>m_2</math>) is a body that [[orbit]]s a [[central body|primary body]] (<math>m_1</math>).
 
The orbiting body is properly referred to as the '''secondary body'''.<ref>NASA "Dictionary of Technical Terms for Aerospace Use" http://er.jsc.nasa.gov/SEH/s.html, retrieved 5/11/2010</ref>
 
It is less massive than the primary body (i.e. <math>m_1>m_2</math>).
 
Under standard assumptions in astrodynamics the [[barycenter]] of the two bodies is a [[Focus (geometry)|focus]] of both [[orbit]]s.
 
Pertaining to Astronomy, an Orbiting Body (sometimes seen as OB) is any object smaller than the body it orbits. These may include, but are not limited to, comets, planets, dwarf planets, moons, and asteroids.
 
==See also==
*[[Central body|Primary body]]
 
==References==
 
{{Reflist}}
 
{{DEFAULTSORT:Orbiting Body}}
[[Category:Orbits]]
 
{{Astronomy-stub}}
{{physics-stub}}

Latest revision as of 04:07, 10 November 2014

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