42 Draconis b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | 42 Draconis | |
Constellation | Draco | |
Right ascension | (α) | 18h 25m 59.14s[1] |
Declination | (δ) | +65° 33′ 48.5″[1] |
Apparent magnitude | (mV) | 4.833 |
Distance | 315 ± 6[1] ly (97 ± 2[1] pc) | |
Spectral type | K1.5III | |
Orbital elements | ||
Semi-major axis | (a) | 1.19 ± 0.01 AU |
Periastron | (q) | 0.74 AU |
Apastron | (Q) | 1.64 AU |
Eccentricity | (e) | 0.38 ± 0.06 |
Orbital period | (P) | 479.1 ± 6.2 d (1.312 ± 0.017 y) |
Argument of periastron |
(ω) | 218.7 ± 10.6° |
Time of periastron | (T0) | 2452757.4 ± 3.7 JD |
Physical characteristics | ||
Minimum mass | (m sin i) | 3.88 ± 0.85 MJ |
Discovery information | ||
Discovery date | March 20, 2009 | |
Discoverer(s) | Doellinger et al. | |
Discovery method | radial velocity | |
Discovery site | TLS | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
42 Draconis b (abbreviated 42 Dra b), also named Orbitar, is an extrasolar planet located approximately 315 light years from Earth in the constellation of Draco. It orbits the 5th magnitude K-type giant star 42 Draconis with a period of 479 days and 38% orbital eccentricity.[2] The planet was discovered using the radial velocity method on March 20, 2009.[2]
Following its discovery the planet was designated 42 Draconis b. In July 2014 the International Astronomical Union launched 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 Orbitar for this planet.[5] The winning name was submitted by the Brevard Astronomical Society of Brevard County, Florida, United States.[6] Orbitar is a contrived word paying homage to the space launch and orbital operations of NASA.[7]
See also
References
- 1 2 3 4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- 1 2 Döllinger, M. P.; et al. (2009). "Planetary companion candidates around the K giant stars 42 Draconis and HD 139 357". Astronomy and Astrophysics 499 (3): 935–942. arXiv:0903.3593. Bibcode:2009A&A...499..935D. doi:10.1051/0004-6361/200810837.
- ↑ NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars. IAU.org. 9 July 2014
- ↑ NameExoWorlds The Process
- ↑ Final Results of NameExoWorlds Public Vote Released, International Astronomical Union, 15 December 2015.
- ↑ Website
- ↑ NameExoWorlds The Approved Names
- Jean Schneider (2011). "Notes for Planet 42 Dra b". Extrasolar Planets Encyclopaedia. Retrieved 3 October 2011.
Coordinates: 18h 25m 59.1381s, +65° 33′ 48.530″