• Thumbnail for RR Lyrae variable
    RR Lyrae variables are periodic variable stars, commonly found in globular clusters. They are used as standard candles to measure (extra) galactic distances...
    20 KB (2,350 words) - 02:47, 18 April 2025
  • Thumbnail for RR Lyrae
    RR Lyrae is a variable star in the Lyra constellation, figuring in its west near to Cygnus. As the brightest star in its class, it became the eponym for...
    14 KB (1,178 words) - 19:31, 25 April 2025
  • Thumbnail for Lyra
    Lyra (redirect from Lyrae)
    famed Summer Triangle asterism. Beta Lyrae is the prototype of a class of binary stars known as Beta Lyrae variables. These binary stars are so close to...
    68 KB (7,584 words) - 22:17, 3 May 2025
  • Thumbnail for Horizontal branch
    pulsating horizontal-branch stars are known as RR Lyrae variable stars and they are obviously variable in brightness with periods of up to 1.2 days. It...
    15 KB (1,722 words) - 10:16, 3 January 2025
  • Thumbnail for Cepheid variable
    RR Lyrae variables have short periods and lie on the instability strip where it crosses the horizontal branch. Delta Scuti variables and RR Lyrae variables...
    38 KB (4,309 words) - 13:37, 26 March 2025
  • Thumbnail for Variable star
    1786, ten variable stars were known. John Goodricke himself discovered Delta Cephei and Beta Lyrae. Since 1850, the number of known variable stars has...
    51 KB (6,578 words) - 14:46, 23 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 Blue giant
    RR Lyrae variable stars, usually with spectral types of A, lie across the middle of the horizontal branch. Horizontal-branch stars hotter than the RR...
    11 KB (1,486 words) - 01:16, 3 March 2025
  • Blazhko effect (category RR Lyrae variables)
    long-period modulation, is a variation in period and amplitude in RR Lyrae type variable stars. Sergey Blazhko first reported its observation by Lidiya Tseraskaya...
    5 KB (542 words) - 21:19, 1 October 2024
  • Thumbnail for Messier 3
    Way. It contains 274 known variable stars, by far the most found in any globular cluster. These include 133 RR Lyrae variables, of which about a third display...
    11 KB (1,037 words) - 10:00, 5 May 2025
  • Thumbnail for Messier 92
    with longer period RR Lyrae variable stars. The 1997 Catalogue of Variable Stars in Globular Clusters listed 28 candidate variable stars in the cluster...
    14 KB (1,393 words) - 21:51, 15 May 2025
  • Thumbnail for Draco Dwarf
    discovered over 260 variables, of the 138 in the cluster's center, all but five were determined to be RR Lyrae variables. From this work a RR Lyrae derived distance...
    11 KB (1,161 words) - 19:36, 14 May 2025
  • Thumbnail for Galactic Center
    the distance to the Galactic Center as established from variable stars (e.g. RR Lyrae variables) or standard candles (e.g. red-clump stars) is hindered...
    48 KB (4,922 words) - 20:00, 7 May 2025
  • Thumbnail for Messier 107
    halo population. There are 22 known RR Lyrae variable stars in this cluster and a probable SX Phoenicis variable. The globular star cluster Messier 107...
    9 KB (738 words) - 23:31, 16 July 2024
  • Thumbnail for Messier 75
    yet. The mass density at the core is 7.9×104 M☉·pc−3. There are 38 RR Lyrae variable stars and the cluster appears to be Oosterhoff-intermediate in terms...
    8 KB (684 words) - 19:24, 25 April 2025
  • Thumbnail for Messier 62
    identified 245 variable stars in the cluster's field, of which 209 are RR Lyrae variables, four are Type II Cepheids, 25 are long period variables, and one...
    14 KB (1,290 words) - 15:37, 21 December 2024
  • Thumbnail for Virgo Stellar Stream
    Hato National Astronomical Observatory in Venezuela to search for RR Lyrae variable stars. Five were found in a clump with a right ascension near 12.4 hours...
    6 KB (762 words) - 19:32, 30 August 2022
  • Thumbnail for Messier 2
    of type ab RR Lyrae variable stars of the cluster. A cluster metallicity below −1.6, an age above 13 billion years, and an average RRab Lyrae pulsation...
    11 KB (1,083 words) - 03:02, 27 September 2024
  • 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 (8,092 words) - 18:42, 9 May 2025
  • Thumbnail for Serpens
    approximately 25,000 ly distant. Messier 5 contains a large number of known RR Lyrae variable stars, and is receding from us at over 50 km/s. The cluster contains...
    119 KB (11,800 words) - 06:08, 21 April 2025
  • Thumbnail for BL Boötis
    BL Boötis (category Objects with variable star designations)
    the variable star designation BL Boötis. However, he thought it was an eclipsing binary. It was subsequently thought to be an RR Lyrae variable by T...
    7 KB (778 words) - 18:17, 21 April 2025
  • MACHO 176.18833.411 (category RR Lyrae variables)
    MACHO 176.18833.411 (OGLE BLG-RRLYR-10353) is an RR Lyrae variable star located in the galactic bulge of our Milky Way Galaxy. However, it is not a galactic...
    3 KB (255 words) - 21:03, 24 February 2023
  • Thumbnail for Globular cluster
    scientific papers. He examined the clusters' RR Lyrae variables (stars which he assumed were Cepheid variables) and used their luminosity and period of variability...
    108 KB (12,119 words) - 23:51, 13 May 2025
  • Thumbnail for Leo IV (dwarf galaxy)
    giants, although a number of Horizontal branch stars including three RR Lyrae variable stars were also discovered. The stars of Leo IV were probably among...
    7 KB (756 words) - 10:25, 15 July 2024
  • Thumbnail for Messier 19
    stellar population includes four Cepheids and RV Tauri variables, plus at least one RR Lyrae variable for which a period is known. Observations made during...
    7 KB (645 words) - 06:52, 23 August 2024
  • Thumbnail for Classical Cepheid variable
    and whose present variability is approximately 0.05 of a magnitude. RR Lyrae variable Stellar pulsation Type II Cepheid Udalski, A.; Soszynski, I.; Szymanski...
    40 KB (3,951 words) - 22:49, 28 April 2025
  • Thumbnail for Instability strip
    pulsating variable stars: Delta Scuti variables, SX Phoenicis variables, and rapidly oscillating Ap stars (roAps) near the main sequence; RR Lyrae variables where...
    8 KB (961 words) - 05:39, 13 November 2023
  • Thumbnail for Ophiuchus
    multiple different types of variable stars. M62 is a globular cluster rich in variable stars such as RR Lyrae variables and has two generations of stars...
    49 KB (4,415 words) - 09:23, 6 May 2025
  • Thumbnail for R Lyrae
    R Lyrae, also known as its Flamsteed designation 13 Lyrae, is a 4th magnitude semiregular variable star in the constellation Lyra, approximately 350 light...
    8 KB (754 words) - 19:46, 4 May 2025
  • Thumbnail for Period-luminosity relation
    Period-luminosity relation (category Classical Cepheid variables)
    The cluster variables (RR Lyrae variables) were fainter still. Period-luminosity relations are known for several types of pulsating variable stars: type...
    20 KB (2,319 words) - 00:25, 16 February 2025