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Specific angular momentum

In celestial mechanics, the specific relative angular momentum (often denoted h → {\displaystyle {\vec {h}}} or h {\displaystyle \mathbf {h} } ) of a body is the angular momentum of that body divided by its mass. In the case of two orbiting bodies it is the vector product of their relative position and relative linear momentum, divided by the mass of the…

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Definition

Proof of constancy in the two body case

Kepler's laws of planetary motion

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Specific angular momentum

Nodes31
Edges30
Triples6
Avg. degree1.94
Density0.064516
Components1

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Specific angular momentum

Top relations

related to Proof of constancy in the two body case · 4
Specific angular momentum → Each, No, The, Under
see also · 2
Specific angular momentum → Classical, Specific

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Important terminology

momentum specific displaystyle angular mathbf relative vector constant mass frac two second body times product position orbital time one equation

Entity relationships Subject–Predicate–Object triples

SubjectPredicateObjectConfidenceSrc
Specific angular momentumrelated to Proof of constancy in the two body caseUnder0.60section
Specific angular momentumrelated to Proof of constancy in the two body caseThe0.60section
Specific angular momentumrelated to Proof of constancy in the two body caseEach0.60section
Specific angular momentumrelated to Proof of constancy in the two body caseNo0.60section
Specific angular momentumsee alsoSpecific0.60section
Specific angular momentumsee alsoClassical0.60section

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