orbital speed
(speed of an orbiting body around the barycenter of a system)
Orbital speed is the speed of an orbiting body around the center of
gravity of the system, i.e., around its barycenter.
For a given pair, the further apart, the lower the orbital speed.
Earth's orbital speed as it orbits the Sun is
about 30 km/second, while Jupiter's is about 13 km/second.
The Moon's orbital speed around the Earth is about 1 km/second.
Artificial satellites around Earth vary from around 7 km/second
for a low orbit to 3 km/second for a geostationary orbit.
With eccentricity, an orbiting object's
speed cyclically varies, fastest when it is nearest its host body.
(orbits,celestial mechanics,measure)
Further reading:
https://en.wikipedia.org/wiki/Orbital_speed
https://www.nagwa.com/en/explainers/142168516704/
http://hyperphysics.phy-astr.gsu.edu/hbase/Solar/soldata.html
Referenced by pages:
astronomical quantities
broad line region (BLR)
CMB anisotropies
corotation resonance
Earth
epicycle
gravity assist
Kepler radius
Kepler's laws
Keplerian orbit
Lagrangian point
Lindblad resonance
minimum mass (m sin i)
moon
Poynting-Robertson effect
rotation curve
semi-major axis (a)
stellar parameter determination
tidal migration
wide binaries (WB)
Index