• Thumbnail for Cepheid variable
    A Cepheid variable (/ˈsɛfi.ɪd, ˈsiːfi-/) is a type of variable star that pulsates radially, varying in both diameter and temperature. It changes in brightness...
    38 KB (4,309 words) - 13:37, 26 March 2025
  • Thumbnail for Classical Cepheid variable
    Classical Cepheids are a type of Cepheid variable star. They are young, population I variable stars that exhibit regular radial pulsations with periods...
    40 KB (3,951 words) - 22:49, 28 April 2025
  • Thumbnail for Hubble's law
    the world's most powerful telescope at the time. His observations of Cepheid variable stars in "spiral nebulae" enabled him to calculate the distances to...
    132 KB (13,177 words) - 17:21, 2 May 2025
  • Thumbnail for Period-luminosity relation
    Period-luminosity relation (category Classical Cepheid variables)
    pulsating variable stars with their pulsation period. The best-known relation is the direct proportionality law holding for Classical Cepheid variables, sometimes...
    20 KB (2,319 words) - 00:25, 16 February 2025
  • not be confused with Cepheid variables, which are named after Delta Cephei and are luminous supergiant stars. Beta Cephei variables are somewhat evolved...
    27 KB (1,961 words) - 14:46, 17 July 2024
  • Thumbnail for Delta Scuti variable
    A Delta Scuti variable (sometimes termed dwarf cepheid when the V-band amplitude is larger than 0.3 mag.) is a class of pulsating star, comprising several...
    11 KB (913 words) - 16:07, 21 February 2025
  • Thumbnail for Polaris
    Polaris (category Classical Cepheid variables)
    in the Northern Sky makes it useful for navigation. As the closest Cepheid variable its distance is used as part of the cosmic distance ladder. The revised...
    53 KB (5,098 words) - 15:03, 30 April 2025
  • Thumbnail for Variable star
    numerous observations of variable stars, paying particular attention to Cepheid variables. Her analyses and observations of variable stars, carried out with...
    51 KB (6,578 words) - 14:46, 23 April 2025
  • Thumbnail for Cosmic distance ladder
    of bright stars beyond 50 parsecs and giant variable stars, including Cepheids and the RR Lyrae variables. The motion of the Sun through space provides...
    56 KB (8,113 words) - 20:40, 1 May 2025
  • Thumbnail for W Virginis variable
    W Virginis variables are a subclass of Type II Cepheids which exhibit pulsation periods between 10–20 days, and are of spectral class F6 – K2. They were...
    2 KB (202 words) - 21:12, 15 June 2024
  • Thumbnail for Henrietta Swan Leavitt
    Henrietta Swan Leavitt (category Cepheid variables)
    to discover the relation between the luminosity and the period of Cepheid variables. Leavitt's discovery provided astronomers with the first standard...
    29 KB (3,015 words) - 16:13, 16 April 2025
  • rate of pulsation of over a thousand cepheid variable stars in 25 galaxies. Theory suggests that the rate of cepheid pulsation in galaxies screened from...
    18 KB (2,154 words) - 05:22, 6 November 2024
  • Thumbnail for Crux
    Crux (section Variable stars)
    origins and motion across the southern Milky Way. Crux contains four Cepheid variables, each visible to the naked eye under optimum conditions. Crux also...
    45 KB (5,269 words) - 17:22, 6 May 2025
  • Thumbnail for RR Lyrae variable
    and BL Herculis variables, the type II Cepheids. Classical Cepheid variables are higher mass population I stars. RR Lyrae variables are much more common...
    20 KB (2,350 words) - 02:47, 18 April 2025
  • Thumbnail for Ursa Minor
    the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging in apparent magnitude from 1.97 to 2...
    53 KB (5,858 words) - 03:29, 9 April 2025
  • Thumbnail for Andromeda Galaxy
    Hubble settled the debate in 1925 when he identified extragalactic Cepheid variable stars for the first time on astronomical photos of Andromeda. These...
    113 KB (11,065 words) - 16:50, 6 May 2025
  • Thumbnail for Zeta Geminorum
    Zeta Geminorum (category Classical Cepheid variables)
    its south, on the left 'leg' of the twin Pollux. It is a classical Cepheid variable star, of which over 800 have been found in our galaxy. As such its...
    22 KB (2,222 words) - 19:15, 18 February 2025
  • Thumbnail for Oscillation
    periodic firing of nerve cells in the brain, and the periodic swelling of Cepheid variable stars in astronomy. The term vibration is precisely used to describe...
    21 KB (3,045 words) - 19:28, 24 April 2025
  • Thumbnail for Expansion of the universe
    Cluster more closely agree with subsequent and independent analyses of Cepheid variable calibrations of Type Ia supernova, which estimates a Hubble constant...
    37 KB (4,556 words) - 22:16, 22 March 2025
  • Thumbnail for Small Magellanic Cloud
    distance to any other Cepheid variable to be estimated in terms of the distance to the SMC. She hoped a few Cepheid variables could be found close enough...
    25 KB (2,694 words) - 16:24, 3 March 2025
  • galaxy was presented in 2015, based on the claimed discovery of four Cepheid variable stars by Sukanya Chakrabarti (RIT) and collaborators. Search for the...
    8 KB (665 words) - 00:11, 15 September 2024
  • Thumbnail for Delta Cephei
    Delta Cephei (category Classical Cepheid variables)
    the prototype of the Cepheid variable stars that undergo periodic changes in luminosity. Delta Cephei was discovered to be variable by John Goodricke during...
    21 KB (1,806 words) - 19:45, 27 April 2025
  • Thumbnail for Type II Cepheid
    Type II Cepheids are variable stars which pulsate with periods typically between 1 and 50 days. They are population II stars: old, typically metal-poor...
    13 KB (1,231 words) - 23:09, 28 April 2025
  • multigenre convention in the United States. Held annually since 1969 by Cepheid Variable at Texas A&M University's Memorial Student Center, it has grown to...
    16 KB (1,670 words) - 00:38, 29 March 2025
  • Thumbnail for Harlow Shapley
    political activist during the latter New Deal and Fair Deal. Shapley used Cepheid variable stars to estimate the size of the Milky Way Galaxy and the Sun's position...
    32 KB (3,257 words) - 16:50, 20 April 2025
  • A Cepheid is a type of pulsating variable star. It may also refer to: Cepheid (company), a molecular diagnostics company Cepheid, a fictional alien species...
    318 bytes (67 words) - 23:02, 8 December 2020
  • Thumbnail for Edwin Hubble
    Milky Way. He used the strong direct relationship between a classical Cepheid variable's luminosity and pulsation period (discovered in 1908 by Henrietta Swan...
    50 KB (5,132 words) - 18:49, 29 April 2025
  • Thumbnail for Large Magellanic Cloud
    Solar System. However, in 1986, Caldwell and Coulson found that field Cepheid variables in the northeast lie closer to the Milky Way than those in the southwest...
    36 KB (3,895 words) - 23:06, 5 May 2025
  • Thumbnail for Cepheus (constellation)
    Delta Cephei is the prototype of an important class of star known as a Cepheid variable. RW Cephei, an orange hypergiant, together with the red supergiants...
    21 KB (2,288 words) - 01:10, 3 March 2025
  • Thumbnail for Supergiant
    study of Cepheid variables". Popular Astronomy. 34: 493. Bibcode:1926PA.....34..493H. Shapley, Harlow (1925). "S Doradus, a Super-giant Variable Star"....
    39 KB (5,377 words) - 18:49, 20 July 2024