Examples of using Variable star in English and their translations into Swedish
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Colloquial
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Official
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Medicine
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Ecclesiastic
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Ecclesiastic
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Official/political
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Computer
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Programming
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Political
This is a suspected variable star with an apparent magnitude that may rise as high as 2.76.
The American Association of Variable Star Observers collects such observations from participants around the world and shares the data with the scientific community.
It is a variable star with a magnitude that varies between 2.76m and 2.90m.
The designation"IK Pegasi" follows the expanded form of the variable star nomenclature introduced by Friedrich W. Argelander.
Epsilon Apodis is classified as a Gamma Cassiopeiae type variable star and its brightness varies between magnitudes 4.99 and 5.04.
which allows you to download a light curve for any variable star from the American Association of Variable Star Observers.
The pulsing of a variable star could be used to calculate its distance from Earth.
lower instability strip and is classified as a Delta Scuti type variable star.
which he's labelled as VAR, or variable star.
This was the second variable star of this type, with eta Aquilae being discovered just a few weeks earlier, on September 10, 1784.
The International Variable Star Index lists Eta Centauri as both a Gamma Cassiopeiae variable
The American Association of Variable Star Observers collects such observations from participants around the world and shares the data with the scientific community.
But because the stars eclipse one another during their orbits, it is classified as a variable star, and its brightness varies from magnitude +3.70 to +3.79.
1997A&A… 323L… 49P"lam Her-- Variable Star.
in 1931 he joined the American Association of Variable Star Observers AAVSO.
Mira variables are popular targets for amateur astronomers interested in variable star observations, because of their dramatic changes in brightness.
It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +4.73 to +4.78 with a stable period of 38 minutes.
It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +5.43 to +5.61.
was originally thought to be an irregular variable star in the Milky Way galaxy and so was given a variable star designation.
proved to everyone that this was not a supernova or a foreground variable star, but was something quite remarkable.”.