Glossary term: Protostar

Description: A protostar is a large mass formed as a result of the contraction of the gas of a giant molecular cloud in the interstellar medium. The protostar is an early stage of star formation. This phase may take anywhere from 10⁵ to 10⁷ years, depending on the mass of the star. It begins with an increase in density in the molecular cloud core and ends with the formation of the T-Tauri star, which will later evolve into the main sequence star.

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Term and definition status: This term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

Related Media

A dark cloud blocks out background stars. Infront, two jets of material shoot in opposite directions from a central object

Witnessing the birth of a star

Caption: A combination of radio and visible light imaged with the Atacama Large Millimeter/submillimeter Array (ALMA) and European Southern Observatory's New Technology Telescope (NTT) revealing birth of a star forming the Herbig-Haro object HH 46/47. ALMA observations shown in orange and green unveil the energetic jet from the central protostar otherwise hidden at visible wavelength due to dust obscuration and dense gas. NTT observations in pink and purple highlight the visible light from the jet emitted towards the observer.
Credit: ESO/ALMA (ESO/NAOJ/NRAO)/H. Arce. Acknowledgements: Bo Reipurth credit link
License: CC-BY-3.0 Creative Comments Attribution 3.0 Unported icons
Young stars form along a ribbon of gas

Stellar birth environment

Caption: Snapshot of the formation of multiple protostars in the Orion Molecular Clouds with a closer look at each of them with the Atacama Large Millimeter/submillimeter Array and Very Large Array. Such an image provides unique insights of the process and early stages of star formation as well as the influence of the parent cloud in which they form.
Credit: ALMA (ESO/NAOJ/NRAO), J. Tobin; NRAO/AUI/NSF, S. Dagnello; Herschel/ESA credit link
License: CC-BY-3.0 Creative Comments Attribution 3.0 Unported icons