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Protostar information


A protostar is a very young star that is still gathering mass from its parent molecular cloud. It is the earliest phase in the process of stellar evolution.[1] For a low-mass star (i.e. that of the Sun or lower), it lasts about 500,000 years.[2] The phase begins when a molecular cloud fragment first collapses under the force of self-gravity and an opaque, pressure-supported core forms inside the collapsing fragment. It ends when the infalling gas is depleted, leaving a pre-main-sequence star, which contracts to later become a main-sequence star at the onset of hydrogen fusion producing helium.

  1. ^ Stahler, S. W. & Palla, F. (2004). The Formation of Stars. Weinheim: Wiley-VCH. ISBN 3-527-40559-3.
  2. ^ Dunham, M. M.; et al. (2014). The Evolution of Protostars in Protostars and Planets VI. University of Arizona Press. arXiv:1401.1809. doi:10.2458/azu_uapress_9780816531240-ch009. ISBN 9780816598762. S2CID 89604015.

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Protostar

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A protostar is a very young star that is still gathering mass from its parent molecular cloud. It is the earliest phase in the process of stellar evolution...

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clouds (GMC) as precursors to the star formation process, and the study of protostars and young stellar objects as its immediate products. It is closely related...

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the USS Dauntless in Star Trek: Prodigy, searching for the missing USS Protostar which was being commanded by Captain Chakotay, her former first officer...

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383 is a Class 0 protostar. It is the first Class 0 protostar discovered to have had an outburst, and as of 2020, the youngest protostar known to have had...

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nebulae or molecular clouds. Over the course of millions of years, these protostars settle down into a state of equilibrium, becoming what is known as a main-sequence...

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core gradually grows in mass until it becomes a young hot protostar. At this stage, the protostar and its disk are heavily obscured by the infalling envelope...

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Solar System

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diameter of roughly 200 AU (30 billion km; 19 billion mi) and a hot, dense protostar at the center. The planets formed by accretion from this disc, in which...

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Young stellar object

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groups of objects: protostars and pre-main-sequence stars. A star forms by accumulation of material that falls in to a protostar from a circumstellar...

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Planet

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that an interstellar cloud collapses out of a nebula to create a young protostar orbited by a protoplanetary disk. Planets grow in this disk by the gradual...

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Astronomy

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(WISE) have been particularly effective at unveiling numerous galactic protostars and their host star clusters. With the exception of infrared wavelengths...

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Sun

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Formation Accretion Molecular cloud Bok globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track...

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starship USS Voyager, and later promoted to Captain in command of the USS Protostar in Star Trek: Prodigy. The character was suggested at an early stage of...

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Astronomical object

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Stellar evolution Variable star Compact star By luminosity / evolution Protostar Young stellar object Pre-main-sequence Main sequence Subdwarfs Subgiants...

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Formation and evolution of the Solar System

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might have been early in its formation a protostar system with Jupiter being the second but failed protostar, but Jupiter has far too little mass to trigger...

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Lists of planets

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that an interstellar cloud collapses out of a nebula to create a young protostar orbited by a protoplanetary disk. There are eight planets within the Solar...

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Bipolar outflow

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gas from the poles of a star. Bipolar outflows may be associated with protostars (young, forming stars), or with evolved post-AGB stars (often in the form...

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