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・ Gliese 208
・ Gliese 22
・ Gliese 221
・ Gliese 229
・ Gliese 229 Ab
・ Gliese 229 B
・ Gliese 251
・ Gliese 268
・ Gliese 282
・ Gliese 299
・ Gliese 3021 b
・ Gliese 317
・ Gliese 317 b
・ Gliese 318
・ Gliese 3470 b
Gliese 3634
・ Gliese 3634 b
・ Gliese 3685 A
・ Gliese 393
・ Gliese 402
・ Gliese 408
・ Gliese 412
・ Gliese 42
・ Gliese 422 b
・ Gliese 433
・ Gliese 436
・ Gliese 436 b
・ Gliese 445
・ Gliese 504 b
・ Gliese 521


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Gliese 3634 : ウィキペディア英語版
Gliese 3634


Gliese 3634 (Often shortened to GJ 3634) is a red dwarf star in the Hydra constellation. One planet has been discovered in its orbit, Gliese 3634 b. GJ 3634 is under half the mass and size of the Sun, and is estimated to be at least a billion years younger, and lies near to Earth, with a distance of 19.8 parsecs (64.6 light years). It was targeted by astronomers during an over six-year survey of red dwarfs. The astronomers had recently changed their strategy to search for planets with extremely short orbits so they could narrow down candidates that transited, or crossed in front of, their host stars as seen from the Earth. The Super-Earth GJ 3634 b was the first planet discovered using this new strategy.〔 The planet was confirmed using Doppler spectroscopy, or the observation and extrapolation of data from a recorded Doppler effect in the star's light, but later observations found no transiting pattern.〔 The planet was published by its discoverers on February 8, 2011.
==Naming and discovery==

GJ 3634 is named for its location in the Gliese Catalogue of Nearby Stars; a later expansion of the original catalogue was compiled jointly by Gliese and Hartmut Jahreiß. The Third Catalogue, the most recent catalogue, was formed to tag all then-known stars within 25 parsecs of Earth (81.54 light years).〔 GJ 3634 was first catalogued in 1987.〔 The discoverers of GJ 3634 b worked through the High Accuracy Radial Velocity Planet Searcher (HARPS) at the European Southern Observatory's La Silla Observatory in Chile for over six years in search of planets that orbited low-mass red dwarfs. After the discoveries of eleven prior planets, the researchers changed their strategy to search for planets with extremely short orbits. They would first discover the system using the radial velocity method, in which an observed Doppler shift in the star's light would be measured and interpreted; and would then follow up with a search for transits, in which the planet crosses in front of and dims its star as seen from Earth. Radial velocity measurements would help determine the most efficient and time-effective means of observing potential planetary transits.〔
Radial velocity measurements revealed the existence of a planet with a mass of at least 7 Earths. This planet, GJ 3634 b, became the first planet to be discovered under the new strategy.〔 The team of astronomers then followed up with transit measurements using instruments on the Spitzer Space Telescope; they found that there was most likely no transit event present at the star, but they were able to discover its true mass.〔 GJ 3634 b was published to the journal ''Astronomy and Astrophysics'' on February 8, 2011.〔

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