Examples of using Variable star in English and their translations into Vietnamese
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Colloquial
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Ecclesiastic
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Computer
Arcavi was so sure, he said,“I would have bet my car that that was a variable star.”.
Gamma Cassiopeiae is a Be star, a variable star, and a binary star system.
Aludra is classified as an Alpha Cygni type variable star and its brightness varies from magnitude +2.38 to +2.48 over a period of 4.7 days.
If the source is the luminous blue variable star, it is the first time that gamma-ray emission has been linked to such a massive star.”.
The Sun is not considered a variable star, but it does undergo periodic changes in activity known as the sunspot cycle.
The shapes of variable star light curves give valuable information about the underlying physical processes producing the brightness changes.
Luyten-726-8A was found to be a variable star and given the variable star designation BL Ceti.[3] It is a red dwarf
It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +3.35 to +3.42 with a period of 1.82 hours.[1]
Bonfils noted in 2005 that Gliese 581"has been classified as a variable star(HO Lib), but its variability(Weis 1994) is only marginally significant.
It contains NGC 2363-V1, a Luminous Blue Variable star which is 6,300,000 times more luminous than the Sun and one of the most luminous stars known.
Andromedae is the Flamsteed designation, while its variable star designation is V340 And.[3]
several hundred thousand stars, the brightest of which is the variable star V11 with an apparent magnitude of 11.95.
It is a suspected variable star with an average apparent visual magnitude of 3.20,[1] making it visible to the naked eye
AA is the first variable star in a constellation, then AB;
the brightest of which is a red giant, the variable star V11, with an apparent visual magnitude of 11.95.
Today similar flare stars are classified as UV Ceti type variable stars(using the abbreviation UV) in variable star catalogs such as the General Catalogue of Variable Stars. .
period of 40.44 days.[2] HD 183143 was formally announced as a variable star, probably of the α Cygni type, in 1979 and given the variable star designation HT Sagittae.[3].
has been given the variable star designation KV Ursae Majoris.[1].
Being a new variable star, it was designated V838 Monocerotis, the 838th variable star of Monoceros.
Barnard's Star has the variable star designation V2500 Ophiuchi.