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Stellar drift

Stellar drift, or the motion of stars, is a necessary result of the lack of an absolute reference frame in special relativity.

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, in connection with the expansion of the universe. 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).

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stellar, drift, this, article, needs, additional, citations, verification, please, help, improve, this, article, adding, citations, reliable, sources, this, article, unsourced, material, challenged, removed, find, sources, news, newspapers, books, scholar, jst. This article needs additional citations for verification Please help improve this article by adding citations to reliable sources in this article Unsourced material may be challenged and removed Find sources Stellar drift news newspapers books scholar JSTOR November 2009 Learn how and when to remove this message Stellar drift or the motion of stars is a necessary result of the lack of an absolute reference frame in special relativity 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 in connection with the expansion of the universe 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 editGravitational wave nbsp This article about stellar astronomy is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title Stellar drift amp oldid 1170881335, wikipedia, wiki, book, books, library,

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