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. With a mass 61/3 times Jupiter it is a gas giant.[1][2]
| Discovery | |
|---|---|
| Discovered by | Sato et al.[1] |
| Discovery site | Okayama Planet Search Program |
| Discovery date | June 26, 2003 |
Detection method | radial velocity |
| Orbital characteristics | |
| Apastron | 0.80 AU (120,000,000 km) |
| Periastron | 0.76 AU (114,000,000 km) |
Semi-major axis | 0.78 AU (117,000,000 km) |
| Eccentricity | 0.03 ± 0.02 |
Orbital period (sidereal) | 198.2 ± 0.3 d 0.5426 ± 0.0008 y |
Average orbital speed | 43 |
Time of periastron | 2451990 ± 20 |
Argument of periastron | 310 ± 30 |
| Semi-amplitude | 161 ± 2 |
| Star | HD 104985 |
Following its discovery in 2003[1] the planet was designated HD 104985 b. In July 2014 the International Astronomical Union launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars.[3] The process involved public nomination and voting for the new names.[4] In December 2015, the IAU announced the winning name was Meztli for this planet.[5] The winning name was submitted by the Sociedad Astronomica Urania of Morelos, Mexico. 'Meztli' was the Aztec goddess of the Moon.[6]
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