Kepler's third law of planetary motion
GPTKB entity
Statements (14)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:legislation
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:Astronomia_nova
gptkb:Harmonices_Mundi |
| gptkbp:applies_to |
all planets in the solar system
|
| gptkbp:distance |
the distance of planets from the sun
|
| https://www.w3.org/2000/01/rdf-schema#label |
Kepler's third law of planetary motion
|
| gptkbp:is_described_as |
T^2 ∝ a^3
the relationship between the orbital period and the radius of orbit of a planet |
| gptkbp:is_part_of |
gptkb:Kepler's_laws_of_planetary_motion
|
| gptkbp:is_used_in |
astrophysics
|
| gptkbp:named_after |
gptkb:Johannes_Kepler
|
| gptkbp:published_by |
1609
|
| gptkbp:state |
the square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit
|