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California Institute of Technology
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Zeeman effet in which spectral lines are split into several components, in contrast to the normal Zeeman effect which results in only two distinct components.
Industry:Astronomy
(alpha Sco, HR 6134) A red M1 Ib supergiant. It has a B3 V companion, which is a radio source.
Industry:Astronomy
An old subgiant disk star (K2 IIIp, mv = 0.06) about 11 pc distant.
Industry:Astronomy
Second satellite of Uranus.
Industry:Astronomy
Physics as promulgated by Aristotle; includes the hypothesis that our world is comprised of four elements, and that the universe beyond the moon is made of a fifth element and so is fundamentally different from the mundane realm.
Industry:Astronomy
A radiationless quantum jump that occurs in the X-ray region. When a K-electron is removed from an atom and an L-electron drops into the vacancy in the K-shell, the energy released in the latter transition goes not into radiation, but into the liberation of one of the remaining L-electrons.
Industry:Astronomy
Runaway star which diverges from a comparatively small area in Orion.
Industry:Astronomy
A-type star with emission in one or several Balmer lines.
Industry:Astronomy
1) An eclipsing system of at least three components (B8 V, K0, Am). Period of components A and B is about 68.8 hours; period of components A, B, and C is about 1.9 years. Long term observations also indicate a massive, unseen fourth component with a period of about 190 years. Algol is also an erratic radio source of about 0.5 AU diameter. 2) The most famous eclipsing binary, Algol was probably the first variable star discovered. It lies in the constellation Perseus and consists of two stars that orbit each other every 2.87 days. When one star passes in front of the other, the light of the system dims.
Industry:Astronomy
A binary star whose components have G2 V and K5 V spectral types. The nearest star system to the Sun and the third brightest star in the night sky.
Industry:Astronomy