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- Dynamical_parallax abstract "In astronomy, the distance to a visual binary star may be estimated from the masses of its two components, the size of their orbit, and the period of their revolution around one another. A dynamical parallax is an (annual) parallax which is computed from such an estimated distance.To calculate a dynamical parallax, the angular semi-major axis of the orbit of the stars around each other is observed, together with their apparent brightness. By using Newton's generalisation of Kepler's Third Law, which states that the total mass of a binary system multiplied by the square of its orbital period is proportional to the cube of its semi-major axis, together with the mass-luminosity relation, the distance to the binary star can then be determined.In this technique, the masses of the two stars in a binary system are estimated, usually as being the mass of the sun. Then, using Kepler's laws of celestial mechanics, the distance between the stars is calculated. Once this distance is found, the distance away can be found via the arc subtended in the sky, giving a preliminary distance measurement. From this measurement and the apparent magnitudes of both stars, the luminosities can be found, and by using the mass–luminosity relationship, the masses of each star. These masses are used to re-calculate the separation distance, and the process is repeated. The process is iterated many times, and accuracies as high as 5% can be achieved. The mass–luminosity relationship can also be used to determine the lifetime of stars by noting that lifetime is approximately proportional to M/L. One finds that more massive stars live shorter. A more sophisticated calculation factors in a star's loss of mass over time.".
- Dynamical_parallax wikiPageID "6008716".
- Dynamical_parallax wikiPageRevisionID "581625230".
- Dynamical_parallax hasPhotoCollection Dynamical_parallax.
- Dynamical_parallax subject Category:Astrometry.
- Dynamical_parallax subject Category:Binary_stars.
- Dynamical_parallax type BinaryStar109221070.
- Dynamical_parallax type BinaryStars.
- Dynamical_parallax type CelestialBody109239740.
- Dynamical_parallax type NaturalObject100019128.
- Dynamical_parallax type Object100002684.
- Dynamical_parallax type PhysicalEntity100001930.
- Dynamical_parallax type Star109444100.
- Dynamical_parallax type Whole100003553.
- Dynamical_parallax comment "In astronomy, the distance to a visual binary star may be estimated from the masses of its two components, the size of their orbit, and the period of their revolution around one another. A dynamical parallax is an (annual) parallax which is computed from such an estimated distance.To calculate a dynamical parallax, the angular semi-major axis of the orbit of the stars around each other is observed, together with their apparent brightness.".
- Dynamical_parallax label "Dynamical parallax".
- Dynamical_parallax label "Dynamische parallax".
- Dynamical_parallax label "Parallasse dinamica".
- Dynamical_parallax label "力學視差".
- Dynamical_parallax sameAs Parallasse_dinamica.
- Dynamical_parallax sameAs Dynamische_parallax.
- Dynamical_parallax sameAs m.0fkcwl.
- Dynamical_parallax sameAs Q2056396.
- Dynamical_parallax sameAs Q2056396.
- Dynamical_parallax sameAs Dynamical_parallax.
- Dynamical_parallax wasDerivedFrom Dynamical_parallax?oldid=581625230.
- Dynamical_parallax isPrimaryTopicOf Dynamical_parallax.