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BD−17 63 b

Coordinates:Sky map00h 28m 34.3061s, −16° 13′ 34.839″
From Wikipedia, the free encyclopedia
Extrasolar planet in the constellation Cetus
BD-17°63 b / Finlay
Discovery[1]
Discovered byMoutouet al.
Discovery siteLa Silla Observatory
Discovery dateOctober 26, 2008
Doppler spectroscopy
(HARPS)
Designations
Finlay
Orbital characteristics[2]
1.361±0.021 AU
Eccentricity0.5455±0.0025
655.641+0.070
−0.076
 d
Inclination82.4°+2.8°
−2.0°
127.0°+5.1°
−3.6°
2,457,249.6+0.36
−0.32
 JD
112.41°±0.43°
Semi-amplitude173.35+0.76
−0.69
 m/s
StarBD−17 63
Physical characteristics[2]
Mass5.325±0.036 MJ

BD-17°63 b, formally namedFinlay, is anexoplanet located approximately 112.5light-years away in theconstellation ofCetus, orbiting the 10thmagnitudeK-typemain sequencestarBD−17 63. Thisplanet has aminimum mass of 5.1MJ and orbits at a distance of 1.34astronomical units from the star. The distance ranges from 0.62 AU to 2.06 AU, corresponding to theeccentricity of 0.54. One revolution takes about 656 days.[1]

This planet was discovered on October 26, 2008 by Moutouet al. using theHARPS spectrograph on ESO’s 3.6 meter telescope installed atLa Silla Observatory inAtacama Desert,Chile.

The planet BD-17 63 b is namedFinlay. The name was selected in theNameExoWorlds campaign byCuba, during the 100th anniversary of theIAU.Carlos Juan Finlay (1833–1915) was an epidemiologist recognized as a pioneer in the research of yellow fever.[3][4]

Anastrometric measurement of the planet's inclination and true mass was published in 2022 as part ofGaia DR3,[5][6] with another astrometric orbital solution published in 2023.[2]

See also

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References

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  1. ^abMoutou, C.; et al. (2009)."The HARPS search for southern extra-solar planets XVII. Six long-period giant planets around BD -17 0063, HD 20868, HD 73267, HD 131664, HD 145377, HD 153950".Astronomy and Astrophysics.496 (2):513–519.arXiv:0810.4662.Bibcode:2009A&A...496..513M.doi:10.1051/0004-6361:200810941.S2CID 116707055.
  2. ^abcUnger, N.; Ségransan, D.; et al. (December 2023). "Exploring the brown dwarf desert with precision radial velocities and Gaia DR3 astrometric orbits".Astronomy & Astrophysics.680: A16.arXiv:2310.02758.Bibcode:2023A&A...680A..16U.doi:10.1051/0004-6361/202347578.
  3. ^"Approved names".NameExoworlds. Retrieved2020-01-02.
  4. ^"International Astronomical Union | IAU".www.iau.org. Archived fromthe original on 2022-12-05. Retrieved2020-01-02.
  5. ^Gaia Collaboration; et al. (June 2023). "Gaia Data Release 3: Stellar multiplicity, a teaser for the hidden treasure".Astronomy & Astrophysics.674: A34.arXiv:2206.05595.Bibcode:2023A&A...674A..34G.doi:10.1051/0004-6361/202243782.
  6. ^Winn, Joshua N. (September 2022)."Joint Constraints on Exoplanetary Orbits from Gaia DR3 and Doppler Data".The Astronomical Journal.164 (5): 196.arXiv:2209.05516.Bibcode:2022AJ....164..196W.doi:10.3847/1538-3881/ac9126.S2CID 252211643.

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