• 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) - 20:55, 25 May 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 (3,964 words) - 10:05, 30 May 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) - 05:27, 15 June 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 (5,092 words) - 19:31, 2 July 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 (3,017 words) - 20:51, 21 June 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) - 22:03, 24 May 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 (2,155 words) - 23:12, 3 July 2025
  • Thumbnail for Cosmic distance ladder
    of distance measurements using Cepheid variables. In the 1950s, Walter Baade discovered that the nearby Cepheid variables used to calibrate the standard...
    56 KB (7,330 words) - 17:51, 3 July 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) - 01:34, 2 July 2025
  • 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 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) - 22:00, 30 June 2025
  • 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 (5,263 words) - 15:23, 28 June 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 (3,891 words) - 20:38, 27 June 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...
    52 KB (6,578 words) - 07:17, 4 July 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...
    116 KB (11,349 words) - 17:34, 3 July 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 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 Asteroseismology
    the pulsations in many of the longest-known variable stars, including the Cepheid and RR Lyrae variables. In stars with surface convection zones, turbulent...
    18 KB (2,290 words) - 07:53, 18 March 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) - 14:56, 25 June 2025
  • Thumbnail for Magellanic Clouds
    in 1913 using 1912 measurements of Cepheid variables in the SMC by Henrietta Leavitt. Recalibration of the Cepheid scales allowed Harlow Shapley to refine...
    26 KB (3,192 words) - 13:07, 19 June 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) - 15:18, 28 June 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...
    33 KB (3,260 words) - 14:32, 21 June 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"....
    40 KB (5,378 words) - 22:07, 13 May 2025
  • Thumbnail for Instability strip
    intersects the horizontal branch; and the Cepheid variables where it crosses the supergiants. RV Tauri variables are also often considered to lie on the...
    8 KB (959 words) - 06:09, 4 June 2025
  • Thumbnail for Yellow supergiant
    Delta Canis Majoris and Iota¹ Scorpii. Many of them are variable stars, mostly pulsating Cepheids such as δ Cephei itself. Yellow supergiants generally...
    20 KB (2,525 words) - 09:50, 30 April 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) - 16:20, 1 June 2025
  • Thumbnail for Messier 106
    contains Cepheid variables similar to both the metallicities of the Milky Way and other galaxies' Cepheids. By measuring the distance of the Cepheids with...
    12 KB (1,014 words) - 02:05, 25 April 2025
  • Thumbnail for Musca
    have been found to have planets. The constellation also contains two cepheid variables visible to the naked eye. Theta Muscae is a triple star system, the...
    44 KB (4,768 words) - 15:33, 28 June 2025
  • Thumbnail for Walter Baade
    same observations led him to discover that there are two types of Cepheid variable stars. Using this discovery he recalculated the size of the known universe...
    10 KB (835 words) - 21:09, 7 June 2025