red dwarf oor Masedonies

red dwarf

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(astronomy) A small, relatively cool star of the main sequence; most stars in the Milky Way are red dwarfs.

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type of small and relatively-cool star
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This star system consists of a dim red dwarf and a white dwarf.
Вукодлак? да. полачовек,пола волк. Следи меWikiMatrix WikiMatrix
The red dwarf, of magnitude 11, orbits the white dwarf every 250 years.
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11 Leonis Minoris has a red dwarf companion of spectral type M5V and apparent magnitude 13.0.
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EV Lacertae is a rapidly spinning magnitude 10 red dwarf with a strong magnetic field.
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Kruger 60 is an 11th-magnitude binary star consisting of two red dwarfs.
Вие двајцата сте одличен тимWikiMatrix WikiMatrix
In 1947, G. E. Kron proposed that starspots were the reason for periodic changes in brightness on red dwarfs.
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The companion is an old, active red dwarf that has a relatively high metallicity and is of spectral type M6.5.
Изненадување, изненадувањеWikiMatrix WikiMatrix
The system is composed of HD 188753A, a yellow dwarf; HD 188753B, an orange dwarf; and HD 188753C, a red dwarf.
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40 Eridani is a triple star system consisting of an orange main-sequence star, a white dwarf, and a red dwarf.
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If the orbit is almost face-on, especially for superjovians detected by radial velocity, then those objects may actually be brown dwarfs or even red dwarfs.
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Brandon Carter has shown that very much smaller changes in G would turn all stars into blue giants or red dwarfs, with equally dire consequences for life.”
Навистина чудно Мишел Ваилант не ја искористи шансатаjw2019 jw2019
Six star systems have been found to have planets: the red dwarf Gliese 832 is one of the closest stars to Earth to have a planetary system.
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Among the stars he discovered is Wolf 359, a dim red dwarf that was later found to be one of the nearest stars to our solar system.
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The system is a post-common-envelope binary and is losing angular momentum over time, which will eventually cause mass transfer from the red dwarf to the white dwarf.
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Kapteyn's Star, the nearest star in Pictor to Earth, is a red dwarf located 12.76 light-years away that was found to have two super-Earths in orbit in 2014.
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In 1984, Physicist Richard A. Muller postulated that the Sun has a heretofore undetected companion, either a brown dwarf or a red dwarf, in an elliptical orbit within the Oort cloud.
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By itself, this would be a quadruple hierarchy 2 system as in (d), but it is orbited by a fainter more distant component, which is also a close red dwarf binary.
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Although Jupiter would need to be about 75 times as massive to fuse hydrogen and become a star, the smallest red dwarf is only about 30 percent larger in radius than Jupiter.
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Gliese 832 is a red dwarf of spectral type M1.5V and apparent magnitude 8.66 located only 16.1 light-years distant; hence it is one of the nearest stars to the Solar System.
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Low mass main sequences of stars, such as red dwarfs below 0.35 solar masses, as well as pre-main sequence stars on the Hayashi track, are convective throughout and do not contain a radiation zone.
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The motion of halo stars does bring them through the disc on occasion, and a number of small red dwarfs close to the Sun are thought to belong to the galactic halo, for example Kapteyn's Star and Groombridge 1830.
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Small, relatively cold, low-mass red dwarfs fuse hydrogen slowly and will remain on the main sequence for hundreds of billions of years or longer, whereas massive, hot O-type stars will leave the main sequence after just a few million years.
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A star near the middle of the spectrum, such as the modest Sun or the giant Capella radiates more energy per unit of surface area than the feeble red dwarf stars or the bloated supergiants, but much less than such a white or blue star as Vega or Rigel.
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The primary is an orange dwarf of spectral type K1V orbited by a planet roughly 2.65 times the mass of Jupiter every 963 days, while the secondary is a red dwarf of spectral type M2V and orbited by a brown dwarf that is at least 19 times as massive as Jupiter.
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From the warmest surfaces to the coolest is the sequence of stellar classifications known as O, B, A, F, G, K, M. A red star could be a tiny red dwarf, a star of feeble energy production and a small surface or a bloated giant or even supergiant star such as Antares or Betelgeuse, either of which generates far greater energy but passes it through a surface so large that the star radiates little per unit of surface area.
За колку дена?WikiMatrix WikiMatrix
28 sinne gevind in 5 ms. Hulle kom uit baie bronne en word nie nagegaan nie.