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(of star contraction)

См. также в других словарях:

  • Star formation — is the process by which dense parts of molecular clouds collapse into a ball of plasma to form a star. As a branch of astronomy star formation includes the study of the interstellar medium and giant molecular clouds as precursors to the star… …   Wikipedia

  • Star — For other uses, see Star (disambiguation) …   Wikipedia

  • star — starless, adj. /stahr/, n., adj., v., starred, starring. n. 1. any of the heavenly bodies, except the moon, appearing as fixed luminous points in the sky at night. 2. Astron. any of the large, self luminous, heavenly bodies, as the sun, Polaris,… …   Universalium

  • star cluster — Astron. a number of stars of common origin held together as a group by gravitational attraction. Cf. globular cluster, open cluster, stellar association. * * * ▪ astronomy Introduction  either of two general types of stellar assemblages held… …   Universalium

  • white dwarf star — Any of a class of small, faint stars representing the end point of the evolution of stars without enough mass to become neutron stars or black holes. Named for the white colour of the first ones discovered, they actually occur in a variety of… …   Universalium

  • Variable star — A star is classified as variable if its apparent brightness as seen from Earth changes over time, whether the changes are due to variations in the star s actual luminosity, or to variations in the amount of the star s light that is blocked from… …   Wikipedia

  • T Tauri star — Drawing of a T Tauri star with a circumstellar accretion disc …   Wikipedia

  • De Sitter double star experiment — This article is about observing binary stars. For precession of orbiting bodies, see de Sitter precession. de Sitter s double star argument The de Sitter effect was described by de Sitter in 1913 and used to support the special theory of… …   Wikipedia

  • Brittle star — Temporal range: 488.2–0 Ma …   Wikipedia

  • Miri (Star Trek: The Original Series) — Miri Star Trek: The Original Series episode Miri befriends the landing party Episode no. Season 1 Episode 8 …   Wikipedia

  • Pre-main sequence star — A pre main sequence star (PMS star, or PMS object) is a star in the stage when it has not yet reached the main sequence. It can be a T Tauri star or FU Orionis star (0.5 Solar mass translates into a move along Hayashi tracks (almost vertically… …   Wikipedia

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