• Thumbnail for Iota Horologii
    Iota Horologii, Latinized from ι Horologii, is a yellow-hued star approximately 56.5 light-years away in the Horologium constellation. The star is classified...
    14 KB (1,008 words) - 06:31, 21 August 2024
  • Thumbnail for Iota Horologii b
    Iota Horologii b (ι Hor b / ι Horologii b), often catalogued HR 810 b, is an extrasolar planet approximately 56.5 light-years away in the constellation...
    7 KB (580 words) - 00:58, 12 December 2023
  • Thumbnail for Horologium (constellation)
    TW Horologii is a semiregular variable red giant star that is classified as a carbon star, and is 1,370 (± 70) light-years from Earth. Iota Horologii is...
    28 KB (3,162 words) - 01:57, 18 July 2024
  • the remaining members of the Hyades Stream, the exoplanet host star Iota Horologii has recently been proposed as an escaped member of the primordial Hyades...
    4 KB (450 words) - 00:22, 13 January 2023
  • Thumbnail for Hyades (star cluster)
    the remaining members of the Hyades Stream, the exoplanet host star Iota Horologii has recently been proposed as an escaped member of the primordial Hyades...
    40 KB (4,643 words) - 20:51, 20 August 2024
  • proper-motion Star, database entry, SIMBAD. Accessed on line January 20, 2011. "Iota Horologii". SolStation. Retrieved May 28, 2008. Zechmeister, M.; et al. (2013)...
    36 KB (1,514 words) - 14:19, 6 October 2024
  • 599.1383H. doi:10.1086/379281. S2CID 11506537. "The planet-host star Iota Horologii". Kiefer, Flavien (17 October 2019). "Determining the mass of the planetary...
    7 KB (438 words) - 20:25, 27 November 2023
  • Thumbnail for Gamma Cephei Ab
    revealed the true mass of γ Cephei Ab to be 9.4 MJ. Dimidium HD 114762 b Iota Horologii b Poltergeist Phobetor "ESA Science & Technology - A brief introduction...
    9 KB (811 words) - 08:18, 5 October 2024
  • Thumbnail for Sylvie Vauclair
    the star Mu Arae. She is responsible for the discovery that the star Iota Horologii in the middle of the Hyades star cluster, observed in the Southern Hemisphere...
    10 KB (810 words) - 10:11, 19 June 2024
  • Thumbnail for Gliese 570
    this multiple star system thus far. Epsilon Indi Gliese 229 HD 188753 Iota Horologii Phi2 Pavonis From L=4πR2σTeff4, where L is the luminosity, R is the...
    16 KB (1,203 words) - 14:49, 29 September 2024
  • a mass 6 times that of Jupiter, comparable to HD 28185 b. 51 Pegasi Iota Horologii Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release...
    12 KB (1,010 words) - 15:26, 11 October 2024
  • Thumbnail for 94 Ceti b
    is about 65 or 115, yielding a mass of about 1.85 that of Jupiter. Iota Horologii b 79 Ceti b 94 Ceti Plávalová, Eva; Solovaya, Nina A. (2013). "Analysis...
    5 KB (161 words) - 13:55, 27 October 2023
  • Thumbnail for HD 80606 and HD 80607
    difference is very interesting and hard to explain. Gliese 752 HD 20782 Iota Horologii Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data...
    11 KB (982 words) - 11:59, 24 August 2024
  • Thumbnail for HD 28185 b
    likely than if the planet was about Jupiter's mass or less. 51 Pegasi b Iota Horologii b Gliese 876 b Yavin Habitable exomoons From f f ⊕ = ( R ∗ R ⊙ ) 2 (...
    10 KB (944 words) - 10:14, 25 September 2023
  • 21 confirmed and 139 candidates. The most massive confirmed exoplanet is Iota Draconis b, which masses 9.40 MJ (i.e. 9.4 times the mass of Jupiter); the...
    36 KB (286 words) - 20:08, 22 December 2023
  • Thumbnail for Mira variable
    stars found that 75% of the Mira stars which could be resolved using the IOTA telescope are not spherically symmetric, a result which is consistent with...
    24 KB (1,621 words) - 10:51, 29 July 2024