Discovery | |
---|---|
Discovered by | Doellinger et al. |
Discovery site | TLS |
Discovery date | March 20, 2009 |
radial velocity | |
Orbital characteristics | |
Apastron | 1.64 AU (245,000,000 km) |
Periastron | 0.74 AU (111,000,000 km) |
1.19 ± 0.01 AU (178,000,000 ± 1,500,000 km) | |
Eccentricity | 0.38 ± 0.06 |
479.1 ± 6.2d 1.312 ± 0.017y | |
2452757.4 ± 3.7 | |
218.7 ± 10.6 | |
Star | 42 Draconis |
Physical characteristics | |
Mass | ≥3.88±0.85 MJ |
42 Draconis b (abbreviated42 Dra b), formally namedOrbitar/ˈɔːrbɪtɑːr/, is a candidateextrasolar planet located approximately 315light years from Earth in theconstellation ofDraco. It orbits the 5thmagnitudeK-typegiantstar42 Draconis with aperiod of 479 days and 38%orbital eccentricity.[1] The planet was discovered using theradial velocity method on March 20, 2009.[1]
Following its discovery the planet was designated 42 Draconis b. In July 2014 theInternational Astronomical Union launchedNameExoWorlds, a process for giving proper names to certain exoplanets and their host stars.[2] The process involved public nomination and voting for the new names.[3] In December 2015, the IAU announced the winning name was Orbitar for this planet.[4] The winning name was submitted by the Brevard Astronomical Society ofBrevard County, Florida,United States.[5] Orbitar is a contrived word paying homage to the space launch and orbital operations ofNASA.[6]
A 2021 study found that more recentradial velocity measurements of 42 Draconis were inconsistent with the proposed planetary orbit, casting serious doubt on 42 Draconis b's existence, but with a two-planet solution still being a possibility. The study suggests that the radial velocity signal is likely caused by a yet unknown stellar phenomenon, which might be common ingiant stars.[7]
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