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Pages Related to Stellar properties, Pages using the word stellar in a physics context. Stellar aberration; Stellar age estimation; Stellar archaeology; Stellar ...
Artist's concept of an "uneven ring of dust" orbiting KIC 8462852, also known as Tabby's Star. This list of stars that have unusual dimming periods is a table of stars that have been observed to darken and brighten and do not appear to be eclipsing binaries or intrinsic variables.
An OB association is a young stellar association containing 10 to 100 massive stars of spectral classes O and B, i.e., blue and very hot; they form together in giant molecular clouds, whose residual gas, once the stars are formed, is blown away by the strong stellar wind. [31]
44 Aquarii is a single [10] star located 336 [1] light years away from the Sun in the equatorial constellation of Aquarius. 44 Aquarii is its Flamsteed designation. [9] It is visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of 5.75. [2]
Stellar structure models describe the internal structure of a star in detail and make predictions about the luminosity, the color and the future evolution of the star. Different classes and ages of stars have different internal structures, reflecting their elemental makeup and energy transport mechanisms.
Gliese 876 is a red dwarf star 15.2 light-years (4.7 parsecs) away from Earth in the constellation of Aquarius.It is one of the closest known stars to the Sun confirmed to possess a planetary system with more than two planets, after GJ 1061, YZ Ceti, Tau Ceti, and Wolf 1061; as of 2018, four extrasolar planets have been found to orbit the star.