• Thumbnail for Red-giant branch
    The red-giant branch (RGB), sometimes called the first giant branch, is the portion of the giant branch before helium ignition occurs in the course of...
    32 KB (3,933 words) - 12:10, 8 June 2025
  • Thumbnail for Red giant
    most carbon stars. Red giants vary in the way by which they generate energy: most common red giants are stars on the red-giant branch (RGB) that are still...
    28 KB (3,497 words) - 14:13, 4 April 2025
  • Thumbnail for Tip of the red-giant branch
    Tip of the red-giant branch (TRGB) is a primary distance indicator used in astronomy. It uses the luminosity of the brightest red-giant-branch stars in...
    6 KB (645 words) - 10:29, 26 January 2025
  • Thumbnail for Asymptotic giant branch
    late in their lives. Observationally, an asymptotic-giant-branch star will appear as a bright red giant with a luminosity ranging up to thousands of times...
    26 KB (3,222 words) - 03:51, 24 June 2025
  • Thumbnail for Giant star
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    17 KB (2,383 words) - 04:05, 24 June 2025
  • Thumbnail for Stellar evolution
    the red-giant branch. When hydrogen shell burning finishes, these stars move directly off the red-giant branch like a post-asymptotic-giant-branch (AGB)...
    50 KB (6,439 words) - 09:11, 24 June 2025
  • Thumbnail for Subgiant
    Subgiant (redirect from Sub-giant)
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    29 KB (3,704 words) - 13:40, 20 June 2025
  • Thumbnail for Red clump
    slightly hotter than most red-giant-branch stars of the same luminosity. It is visible as a denser region of the red-giant branch or a bulge towards hotter...
    13 KB (1,733 words) - 15:54, 12 March 2025
  • Thumbnail for Blue loop
    place called the blue giant branch. Blue loops can occur for red supergiants, red-giant branch stars, or asymptotic giant branch stars. Some stars may...
    9 KB (1,092 words) - 06:00, 2 June 2025
  • stellar evolutionary phase when stars are giants. Giant branch may refer specifically to: Red-giant branch, the stellar evolutionary stage after the main...
    431 bytes (90 words) - 23:34, 28 April 2021
  • Thumbnail for Blue supergiant
    to the red giant branch for low-mass stars, this region is also called the blue giant branch. They are larger than the Sun but smaller than a red supergiant...
    21 KB (2,496 words) - 09:01, 10 June 2025
  • Thumbnail for Horizontal branch
    The horizontal branch (HB) is a stage of stellar evolution that immediately follows the red-giant branch in stars whose masses are similar to the Sun's...
    15 KB (1,722 words) - 09:22, 1 June 2025
  • Thumbnail for Sand 364
    Sand 364 (category K-type giants)
    Sand 364 is a K-type giant star on the red giant branch within the cluster Messier 67 (also called NGC 2682), which is located in the constellation Cancer...
    7 KB (740 words) - 13:57, 24 June 2025
  • Thumbnail for Stellar nucleosynthesis
    at the tip of the red giant branch with a helium flash from a degenerate helium core, and the star moves to the horizontal branch where it burns helium...
    38 KB (4,506 words) - 12:58, 23 June 2025
  • Thumbnail for Hubble's law
    Space Telescope and based on distances to red giant stars calculated using the tip of the red-giant branch (TRGB) distance indicator. Their measurement...
    132 KB (13,177 words) - 05:27, 15 June 2025
  • Thumbnail for Hertzsprung–Russell diagram
    turn-off in the main sequence can be used, but also the tip of the red giant branch stars. ESA's Gaia mission showed several features in the diagram that...
    23 KB (2,762 words) - 22:46, 23 April 2025
  • Thumbnail for Blue giant
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    11 KB (1,486 words) - 01:16, 3 March 2025
  • pressure is electron degeneracy pressure, and the star expands onto the red giant branch. Stars with higher masses have at least partially convective cores...
    15 KB (1,839 words) - 04:37, 6 June 2025
  • Thumbnail for Blue straggler
    Blue straggler (redirect from Red straggler)
    for the cluster, where ordinary stars begin to evolve towards the red giant branch. Blue stragglers were first discovered by Allan Sandage in 1953 while...
    13 KB (1,502 words) - 10:16, 8 November 2024
  • Thumbnail for Sun
    have higher mass loss on the red-giant branch produce smaller, less luminous stars at the tip of the asymptotic giant branch, perhaps only 2,000 times the...
    173 KB (19,378 words) - 13:02, 24 June 2025
  • Thumbnail for Arcturus
    Arcturus (category K-type giants)
    Arcturus is a red giant star in the northern constellation of Boötes, and the brightest star in the constellation. It has the Bayer designation α Boötis...
    56 KB (5,567 words) - 18:20, 23 June 2025
  • Thumbnail for Red supergiant
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    34 KB (4,293 words) - 21:26, 19 June 2025
  • HD 145250 (category K-type giants)
    shell around the core, being in the evolutionary stage known as the red-giant branch. HD 145250 displays photometric variability caused by seismic oscillations...
    8 KB (676 words) - 22:56, 16 June 2025
  • Thumbnail for Red dwarf
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    48 KB (5,552 words) - 00:37, 20 June 2025
  • dredge-up The first dredge-up occurs when a main-sequence star enters the red-giant branch. As a result of the convective mixing, the outer atmosphere will display...
    4 KB (416 words) - 14:59, 18 November 2024
  • Thumbnail for Starlight
    measured CP of q = 7 × 10 − 3 {\displaystyle q=7\times 10^{-3}} for the red supergiant NML Cygni and q = 2 × 10 − 3 {\displaystyle q=2\times 10^{-3}}...
    14 KB (1,695 words) - 21:03, 7 June 2025
  • Thumbnail for Formation and evolution of the Solar System
    temperature differences. When the Sun leaves the red-giant branch and enters the asymptotic giant branch, the habitable zone will abruptly shrink to roughly...
    113 KB (13,512 words) - 22:20, 21 June 2025
  • Thumbnail for Supergiant
    Supergiant (redirect from Super giant)
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    40 KB (5,378 words) - 22:07, 13 May 2025
  • Thumbnail for Sculptor Galaxy
    achieved in 2005. The Sculptor Galaxy is close enough that the tip of the red-giant branch (TRGB) method may also be used to estimate its distance. The estimated...
    20 KB (2,081 words) - 15:09, 22 June 2025
  • Thumbnail for Yellow supergiant
    dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants Bright giants Supergiants Red supergiant Hypergiants...
    20 KB (2,525 words) - 09:50, 30 April 2025