The radial velocity of HD 104985 has been monitored since 2001 March, using HIDES at OAO. Check back here in December to find out. The International Astronomical Union has formally named this planet Orbitar, and its star is now named Fafnir. Tau Boötis b, did not receive a name, because, the IAU cryptically says, its winning entry “was judged not to conform with the IAU rules for naming exoplanets.” The very first confirmed exoplanetary system, announced in 1992, consists of three rocky worlds orbiting a stellar remnant, a millisecond pulsar ignominiously named PSR 1257+12. Star: HD 81688—Intercrus. Exoplanets are being discovered all the time so this might not be up to date. Currently, all exoplanets are named after their host star followed by a lower case letter, such as 51 Pegasi b. Trata-se definitivamente de um gigante gasoso, devido à sua massa que é 6 1 / 3 vezes maior que a de Júpiter. Planet: Fomalhaut b (alpha Piscis Austrini b)—Dagon. Tau Boötis b, did not receive a name, because, the IAU cryptically says, its winning entry “was judged not to conform with the IAU rules for naming exoplanets.” The very first confirmed exoplanetary system, announced in 1992, consists of three rocky worlds orbiting a stellar remnant, a millisecond pulsar ignominiously named PSR 1257+12. Dagon (Fomalhaut b, Planet) Tonatiuh (HD 104985, Star) Meztli (HD 104985 b, Planet) Ogma (HD 149026, Star) Smertrios (HD 149026 b, Planet) Intercrus (HD 81688, Star) Arkas (HD 81688b, Planet) 2003), by using the data collected during the past six years. Planeta yra 8,3 karto masyvesnė už Jupiterį (už Žemę – 2638 kartus), o jos spindulys – apytikriai 1,12 karto didesnis nei Jupiterio. The Astrophysical Journal Letters. 2003); HD 62509 (Reffert et al. Planet: HD 149026 b—Smertrios. Pages: 49. [4] In December 2015, the IAU announced the winning name was Meztli for this planet. - SIMBAD4 rel 1.7 - 2020.11.07CET06:42:40 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations . Explore the Archive Interactive Table Search and File Upload Statements. 2007); HD 142091 and HD 167042 (Johnson et al. With a mass 61/3 times Jupiter it is a gas giant. De magnitú aparente +5,80, nun tien denominación de Bayer nin de Flamsteed, siendo conocida davezu pol … Find more about your star on SIMBAD In its first bulletin of July 2016,[10] the WGSN explicitly recognized the names of exoplanets and their host stars approved by the Executive Committee Working Group Public Naming of Planets and Planetary Satellites, including the names of stars adopted during the 2015 NameExoWorlds campaign. Its host star is located in the constellation of The Giraffe. The radial velocity of HD 104985 has been monitored since 2001 March, using HIDES at OAO. Template:Planetbox begin Template:Planetbox star Template:Planetbox orbit Template:Planetbox character Template:Planetbox discovery Template:Planetbox reference Template:Planetbox end HD 104985 b is an extrasolar planet that takes 198 days to orbit at the distance of 0.78 AU. This is only an … , indicating that the enrichment may be attributed to the conversion of 3 He via 7 Be to 7 Li by the Cameron–Fowler mechanism. Jump to navigation Jump to search. A Planetary Companion to the G-Type Giant Star HD 104985. HD 104985 b is an extrasolar planet that takes 198 days to orbit at the distance of 0.78 AU. Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Planet: HD 104985 b—Meztli. HD 104985, also named Tonatiuh /toʊnəˈtiːuː/, is a helium-fusing yellow giant star located 97 parsecs (317 lys) from the Sun in the constellation of Camelopardalis. doi:10.1086/379967. Currently popular pronunciations. While this is useful for tracking these discoveries, the approach can make talking about some of these worlds a bit clumsy, as a name like HD 104985 b doesn't flow smoothly off the tongue in conversation. [8], In 2016, the IAU organized a Working Group on Star Names (WGSN)[9] to catalog and standardize proper names for stars. List of Extrasolar Planets in Cassiopeia. De Medeiros & Mayor (1999) determined the projected rotational velocity of the star to be km sv sin i p 2.7 1.1 1. Currently, all exoplanets are named after their host star followed by a lower case letter, such as 51 Pegasi b. HD 104985 (HR 4609 / HIP 58952 / SAO 7500) ye una estrella asitiada na constelación de Camelopardalis, la xirafa, a 333 años lluz de distancia del Sistema Solar. [1][2], Following its discovery in 2003[1] the planet was designated HD 104985 b. instance of. An extrasolar planet (designated HD 104985 b, later named Meztli /ˈmɛstli/) is believed to orbit the star. Planet: HD 149026 b—Smertrios. [2], Coordinates: 12h 05m 15.1178s, +76° 54′ 20.641″, For the pronunciation of a bilingual English–Spanish speaker, see, Duncan Tonatiuh: Audio Name Pronunciation, "A Planetary Companion to the G-Type Giant Star HD 104985", NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars, Final Results of NameExoWorlds Public Vote Released, "Bulletin of the IAU Working Group on Star Names, No. Exoplaneta okolo hvězdy HD 104985. (2008). 이 행성은 항성으로부터 0.78 천문단위 떨어져 있다. HD 104985 b (Q1073672) From Wikidata. ∗ Based on observations carried out at Okayama Astrophysical Observatory (Okayama, Japan). 2 references. The star and the planet both need names, and YOU may be able to name them! Language Label Description Also known as; English: HD 104985 b. extrasolar planet in the constellation Camelopardalis. In July 2014 the International Astronomical Union launched a process for giving proper names to certain exoplanets and their host stars. {{Camelopardalis}} is a {{}}-based template to be used at the bottom of articles about astronomical objects beyond the Solar System, located in the constellation of Camelopardalis.The template is divided into categories of stars, star clusters, nebulae, galaxies, galaxy clusters, and a miscellaneous "other" category.. Red links. HD 104985: HD 104985 b/Meztli: 6.33: 198: 2003: Superjovian: 1 Current IAU guidelines use a plus sign (+) for northern constellations and a minus sign (−) for southern ones. for HD 104985, which is located in the clump region. HD 104985 b, also named Meztli /ˈmɛstli/, is an extrasolar planet approximately 97 parsecs (317 lys) from the SunThe 198-day period planet orbits the yellow giant star HD 104985 (Tonatiuh) at a distance of 0.78 AU. 2003 SATO B., ANDO H., KAMBE E., TAKEDA Y., IZUMIURA H., MASUDA S., WATANABE E., NOGUCHI K., WADA S., OKADA N., KOYANO H., MAEHARA H., NORIMOTO Y., OKADA T., SHIMIZU Y., URAGUCHI F., YANAGISAWA K. & YOSHIDA M. HD 104985 b – egzoplaneta, skriejanti apie G9 III spektrinės klasės žvaigždę HD 104985. HD 104985 b, nomeado de Meztli, é um planeta extrassolar orbitando a estrela HD 104985 a uma distância de 0.78 UA, completando uma revolução em 198 dias. A waveband of 5000– Thank you for helping build the largest language community on the internet. De Meztli (oder HD 104985 b) ass en Exoplanéit.Hie kreest an 199,5 Deeg ëm de giele Ris Tonatiuh am Stärebild Camelopardalis.Wéinst senger héijer Mass gëtt ugeholl, datt et sech ëm e Gasplanéit handelt.. Dës Säit gouf de(n) 24. HD 104985, also named Tonatiuh / t oʊ n ə ˈ t iː uː /, is a helium-fusing [citation needed] yellow giant star located 97 parsecs (317 lys) from the Sun in the constellation of Camelopardalis.An extrasolar planet (designated HD 104985 b, later named Meztli / ˈ m ɛ s t l i /) is believed to orbit the star. The stellar parameters described above are summarized in Table 1. We also update orbital parameters of HD 104985 b, the first planet discovered around G giants from our survey (Sato et al. HD 104985: HD 104985 b/Meztli: 6.33: 198: 2003: Superjovian: 1 Current IAU guidelines use a plus sign (+) for northern constellations and a minus sign (−) for southern ones. The Astrophysical Journal Letters 597 (2): L157-L160. Sign in to disable ALL ads. While this is useful for tracking these discoveries, the approach can make talking about some of these worlds a bit clumsy, as a name like HD 104985 b doesn't flow smoothly off the tongue in conversation. With a mass 6 /3 times Jupiter it is a gas giant. mass G and K giants (18 Del, ξ Aql, HD 81688)from the Okayama Planet Search Program (Sato et al. [6], Coordinates: 12h 05m 15.1178s, +76° 54′ 20.641″, "A Planetary Companion to the G-Type Giant Star HD 104985", "Planetary Companions around Three Intermediate-Mass G and K Giants: 18 Delphini, ξ Aquilae and HD 81688", NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars, Final Results of NameExoWorlds Public Vote Released, https://en.wikipedia.org/w/index.php?title=HD_104985_b&oldid=951447953, Creative Commons Attribution-ShareAlike License, This page was last edited on 17 April 2020, at 06:29. HD 104985の惑星; 名称 （恒星に近い順） 質量 軌道長半径 （天文単位） 公転周期 軌道離心率 軌道傾斜角 半径; b (Meztli) >8.3 M J: 0.95 199.505 ± 0.085 0.090 ± 0.009 — — HD 104985 b HD 104985 b is a gas giant exoplanet that orbits a K-type star. [5] The winning name was submitted by the Sociedad Astronomica Urania of Morelos, Mexico. Full table display Database search. for HD 104985, which is located in the clump region. Explore the Archive Interactive Table Search and File Upload stated in. Star: HD 81688—Intercrus. Language Label Description Also known as; English: HD 104985 b. extrasolar planet in the constellation Camelopardalis. As indicated in the last column of table 1, we regard in this paper 10 specific stars (out of 322 objects) as stars hosting planets: HD 104985 (Sato et al. Pluto Mercury Mars Venus Earth Neptune Uranus Saturn Jupiter HD 104985 b Habitable zone. The planet 42 Draconis b, discovered in 2008 and rendered here by an artist, has 1,233 times Earth's mass and orbits its host star in 479 days. World's most comprehensive interactive database of extrasolar planets updated daily since 1995. 2 Pronounced 'ka-mel-o-PAR-da-lis', camelopardalis is the Latin word for 'giraffe'. Sato et al. On October 31, the IAU is closing voting on NameExoWorlds.org.So make sure to case your vote. The properties of the variations in these 3 stars have been, and will be, extensively discussed in separate papers. [3] The process involved public nomination and voting for the new names. Jump to navigation Jump to search. HD 194937 and HD 214995 are K giants, which had been studied in Kumar et al. The star and the planet both need names, and YOU may be able to name them! The planet 42 Draconis b, discovered in 2008 and rendered here by an artist, has 1,233 times Earth's mass and orbits its host star in 479 days. extrasolar planet in the constellation Camelopardalis. The planetary system HD 104985 hosts at least one planet. The last votes are nearly cast, get in before it is too late! Relatively large, but not apparently periodic, radial-velocity variations of σ > 30 m s-1 are found in 4 stars (HD 41597, HD 134190, HD 161178, and HD 176598). Was designated HD 104985 b, later named Meztli /ˈmɛstli/ ) is believed to orbit the star and planet! 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