BPM 37093 - Alchetron, The Free Social Encyclopedia

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ARICNS  data
Mass  2.188 × 10^30 kg (1.1 M☉)
Constellation  Centaurus
Surface temperature  11,730 K
Magnitude  14
Apparent magnitude (V)  14
BPM 37093 Astronomers Location of the quotdiamond starquot BPM 37093 Straight
Similar  Theta Centauri, Delta Centauri, Mu Centauri, 2M1207, Zeta Centauri

Najwi kszy diament we wszech wiecie lucy bpm 37093


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BPM 37093 (V886 Centauri) is a variable white dwarf star of the DAV, or ZZ Ceti, type, with a hydrogen atmosphere and an unusually high mass of approximately 1.1 times the Sun's. It is about 50 light-years from Earth, in the constellation Centaurus, and vibrates; these pulsations cause its luminosity to vary. Like other white dwarfs, BPM 37093 is thought to be composed primarily of carbon and oxygen, which are created by thermonuclear fusion of helium nuclei in the triple-alpha process.

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