• Thumbnail for Stellar evolution
    Stellar evolution is the process by which a star changes over the course of time. Depending on the mass of the star, its lifetime can range from a few...
    50 KB (6,437 words) - 20:53, 17 May 2025
  • Thumbnail for Star
    Star (redirect from Stellar radius)
     21–25. ISBN 978-1466584617. Bisnovatyi-Kogan, G. S. (2013). Stellar Physics: Stellar Evolution and Stability. Translated by Blinov, A. Y.; Romanova, M. Springer...
    148 KB (16,418 words) - 01:39, 18 May 2025
  • Compact objects are often the endpoints of stellar evolution and, in this respect, are also called stellar remnants. They can also be called dead stars...
    20 KB (2,589 words) - 22:40, 1 March 2025
  • for a particular mass, and a particular stage of evolution, it is necessary to use a numerical stellar model computed with computer algorithms. Such models...
    14 KB (1,675 words) - 11:34, 8 May 2025
  • Thumbnail for Subgiant
    Salaris, Maurizio; Cassisi, Santi (2005). "Evolution of Stars and Stellar Populations". Evolution of Stars and Stellar Populations: 400. Bibcode:2005essp.book...
    29 KB (3,704 words) - 21:57, 18 February 2025
  • Thumbnail for Stellar structure
    Grids of Stellar Evolution Models (some of them including rotational induced mixing) The BaSTI database of stellar evolution tracks Stellar atmospheres:...
    15 KB (2,089 words) - 21:20, 1 October 2024
  • Thumbnail for Planetary nebula
    few tens of millennia, compared to considerably longer phases of stellar evolution. Once all of the red giant's atmosphere has been dissipated, energetic...
    55 KB (5,922 words) - 02:49, 19 April 2025
  • Thumbnail for Stellar mass loss
    varies widely based on numerous factors. Stellar mass loss plays a very important role in stellar evolution, the composition of the interstellar medium...
    12 KB (1,347 words) - 21:20, 1 October 2024
  • Thumbnail for Stellar nucleosynthesis
    In astrophysics, stellar nucleosynthesis is the creation of chemical elements by nuclear fusion reactions within stars. Stellar nucleosynthesis has occurred...
    38 KB (4,497 words) - 17:04, 5 May 2025
  • mass to fuse hydrogen and helium, hence do not undergo the usual stellar evolution that limits the lifetime of stars. A substellar object with a mass...
    7 KB (881 words) - 13:21, 9 December 2024
  • Thumbnail for Galaxy formation and evolution
    In cosmology, the study of galaxy formation and evolution is concerned with the processes that formed a heterogeneous universe from a homogeneous beginning...
    46 KB (5,623 words) - 04:13, 13 May 2025
  • Thumbnail for Stars in fiction
    light of their emanating radiation or superpowers. Certain stages of stellar evolution have received particular attention: supernovae, neutron stars, and...
    43 KB (3,669 words) - 13:13, 18 May 2025
  • Thumbnail for Habitable zone
    habitable zone in the outer parts of stellar systems may exist during the pre-main-sequence phase of stellar evolution, especially around M-dwarfs, potentially...
    139 KB (13,879 words) - 19:12, 24 April 2025
  • Thumbnail for Formation and evolution of the Solar System
    survival – Idea that spacefaring is necessary for long-term human survival Stellar evolution – Changes to stars over their lifespans Structure formation – Formation...
    113 KB (13,512 words) - 19:49, 17 May 2025
  • The stellar birthline is a predicted line on the Hertzsprung–Russell diagram that relates the effective temperature and luminosity of pre-main-sequence...
    2 KB (201 words) - 07:39, 3 February 2025
  • A stellar core is the extremely hot, dense region at the center of a star. For an ordinary main sequence star, the core region is the volume where the...
    15 KB (1,839 words) - 01:34, 28 January 2025
  • Thumbnail for Main sequence
    Main sequence (category Stellar evolution)
    the main sequence is a classification of stars which appear on plots of stellar color versus brightness as a continuous and distinctive band. Stars on...
    61 KB (6,825 words) - 06:23, 3 May 2025
  • Thumbnail for Hertzsprung–Russell diagram
    Hertzsprung–Russell diagram (category Stellar evolution)
    in 1913, and represented a major step towards an understanding of stellar evolution. In the nineteenth century large-scale photographic spectroscopic...
    23 KB (2,762 words) - 22:46, 23 April 2025
  • Thumbnail for Stellar isochrone
    In stellar evolution, an isochrone is a curve on the Hertzsprung-Russell diagram, representing a population of stars of the same age but with different...
    3 KB (369 words) - 04:39, 18 June 2024
  • Stellar Blade (Korean: 스텔라 블레이드) is a 2024 action-adventure game developed by Shift Up and published by Sony Interactive Entertainment. Players take control...
    42 KB (4,062 words) - 20:05, 12 May 2025
  • Thumbnail for Astrophysics
    Astrophysics (redirect from Stellar physics)
    astrophysicists include Solar System formation and evolution; stellar dynamics and evolution; galaxy formation and evolution; magnetohydrodynamics; large-scale structure...
    30 KB (3,285 words) - 20:06, 9 May 2025
  • Thumbnail for Open cluster
    rest of the gas away. Open clusters are key objects in the study of stellar evolution. Because the cluster members are of similar age and chemical composition...
    52 KB (6,310 words) - 13:36, 18 April 2025
  • luminous supergiant star of intermediate mass in a very late phase of stellar evolution. The post-AGB stage occurs after the asymptotic giant branch (AGB...
    4 KB (461 words) - 10:29, 5 January 2024
  • still exist above 150–200 M☉ they would challenge current theories of stellar evolution. Studying the Arches Cluster, which is currently the densest known...
    167 KB (9,043 words) - 06:42, 11 May 2025
  • Thumbnail for Sun
    Bloecker, T. (1995). "Stellar evolution of low and intermediate-mass stars. I. Mass loss on the AGB and its consequences for stellar evolution". Astronomy and...
    176 KB (19,925 words) - 20:56, 15 May 2025
  • Thumbnail for Star formation
    within molecular clouds in interstellar space—sometimes referred to as "stellar nurseries" or "star-forming regions"—collapse and form stars. As a branch...
    49 KB (5,712 words) - 03:32, 5 May 2025
  • Circumstellar envelope (category Stellar evolution)
    around young stellar objects Circumstellar dust Common envelopes Stellar evolution Leao; Patrick De Laverny; Mekarnia; De Medeiros; Benoit Vandame (2007)...
    2 KB (198 words) - 07:50, 1 October 2023
  • Thumbnail for Stellar pulsation
    stars into which they gradually morph as their periods get longer. Stellar evolution and pulsation theories suggest that these irregular stars have a much...
    25 KB (3,258 words) - 21:55, 8 July 2024
  • He is best known for his contributions to theoretical star models, stellar evolution theory, concerning the production of planetary nebulae, red giant...
    3 KB (328 words) - 22:38, 31 July 2023
  • Thumbnail for Stellar wind
    the high temperature of the corona. Stellar winds from main-sequence stars do not strongly influence the evolution of lower-mass stars such as the Sun...
    5 KB (591 words) - 21:02, 18 November 2024