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・ Stellar Astra
・ Stellar atmosphere
・ Stellar Awards
・ Stellar birthline
・ Stellar black hole
・ Stellar Charter School
・ Stellar chemistry
・ Stellar classification
・ Stellar collision
・ Stellar Conquest
・ Stellar constellations in fiction
・ Stellar Crests
・ Stellar Dawn
・ Stellar density
・ Stellar designation
Stellar drift
・ Stellar dynamics
・ Stellar engine
・ Stellar engineering
・ Stellar envelope
・ Stellar evolution
・ Stellar Group
・ Stellar Group (construction company)
・ Stellar II
・ Stellar isochrone
・ Stellar Kart
・ Stellar Kart discography
・ Stellar kinematics
・ Stellar magnetic field
・ Stellar mass


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Stellar drift : ウィキペディア英語版
Stellar drift

Stellar drift, or the motion of stars, is a necessary result of the lack of an absolute reference frame in special relativity. The term is used mainly in science fiction, however; in particular, the phenomenon affects stargates in the Stargate franchise.
Nothing in space stands still—more precisely, standing still is meaningless without defining what "still" means. Most galaxies have been moving away ever since the Big Bang, as explained by the metric expansion of space. Galaxy motion is also influenced by galaxy groups and clusters. Stars orbit moving galaxies, and they also orbit moving star clusters and companion stars. Planets orbit their moving stars.
Stellar drift is measured by two components: proper motion (multiplied by distance) and radial velocity. Proper motion is a star's motion across the sky, slowly changing the shapes of constellations over thousands of years. It can be measured using a telescope to detect small movements over long periods of time. Radial velocity is how fast a star approaches or recedes from us. It is measured using redshift. Both components are complicated by the Earth's orbit around the Sun, so the motions of stars are described relative to the Sun, not the Earth (kinematics of stars).
==See also==

*Big Bang
*Extinction event
*Gravitational wave
*Great dying
*Kinematics of stars
*metric expansion of space

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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