Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

42 Draconis b

Coordinates:Sky map18h 25m 59.1381s, +65° 33′ 48.530″
From Wikipedia, the free encyclopedia
Extrasolar planet in the constellation Draco
"Orbitar" redirects here. For the video game weapon, seeKid Icarus: Uprising.
42 Draconis b / Orbitar
Discovery
Discovered byDoellinger et al.
Discovery siteTLS
Discovery dateMarch 20, 2009
radial velocity
Orbital characteristics
Apastron1.64 AU (245,000,000 km)
Periastron0.74 AU (111,000,000 km)
1.19 ± 0.01 AU (178,000,000 ± 1,500,000 km)
Eccentricity0.38 ± 0.06
479.1 ± 6.2d
1.312 ± 0.017y
2452757.4 ± 3.7
218.7 ± 10.6
Star42 Draconis
Physical characteristics
Mass3.88±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]

See also

[edit]

References

[edit]
  1. ^abDöllinger, M. P.; et al. (2009)."Planetary companion candidates around the K giant stars 42 Draconis and HD 139357".Astronomy and Astrophysics.499 (3):935–942.arXiv:0903.3593.Bibcode:2009A&A...499..935D.doi:10.1051/0004-6361/200810837.S2CID 15677079.
  2. ^NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars. IAU.org. 9 July 2014
  3. ^"NameExoWorlds". Archived fromthe original on 2015-08-15. Retrieved2015-09-05.
  4. ^Final Results of NameExoWorlds Public Vote Released, International Astronomical Union, 15 December 2015.
  5. ^Website
  6. ^"NameExoWorlds". Archived fromthe original on 2018-02-01. Retrieved2015-12-18.
  7. ^Döllinger, M. P.; Hartmann, M. (September 2021)."A Sanity Check for Planets around Evolved Stars".The Astrophysical Journal Supplement Series.256 (1): 10.Bibcode:2021ApJS..256...10D.doi:10.3847/1538-4365/ac081a.S2CID 237369556.

External links

[edit]


Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
NGC
Other
Galaxy clusters
Astronomical events


Stub icon

This extrasolar-planet-related article is astub. You can help Wikipedia byexpanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=42_Draconis_b&oldid=1194519031"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp