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Long period Jovian exoplanet orbiting HD 132406
HD 132406 b is a long-period, massive
gas giant
exoplanet orbiting the
Sun-like star
HD 132406. HD 132406 b has a
minimum mass 5.61 times the mass of
Jupiter. The
orbital distance from the star is almost twice that of from Earth to the Sun. The
orbital period is 2.7 years.
[1]
An
astrometric measurement of the planet's inclination and true mass was published in 2022 as part of
Gaia DR3,
[3] and this was updated in 2023.
[2]
References
- ^
a
b da Silva, Ronaldo; Udry, Stéphane; Bouchy, François; Moutou, Claire; Mayor, Michel; Beuzit, Jean-Luc; Bonfils, Xavier; Delfosse, Xavier; Desort, Morgan; Forveille, Thierry; Galland, Franck; Hébrard, Guillaume; Lagrange, Anne-Marie; Loeillet, Benoit; Lovis, Christophe; Pepe, Francesco; Perrier, Christian; Pont, Frédéric; Queloz, Didier; Santos, Nuno C.; Ségransan, Damien; Sivan, Jean-Pierre; Vidal-Madjar, Alfred; Zucker, Shay (October 2007).
"ELODIE metallicity-biased search for transiting Hot Jupiters IV. Intermediate period planets orbiting the stars HD 43691 and HD 132406".
Astronomy and Astrophysics. 473 (1): 323–328.
arXiv:
0707.0958.
Bibcode:
2007A&A...473..323D.
doi:
10.1051/0004-6361:20077314.
S2CID
18805775.
- ^
a
b
c Xiao, Guang-Yao; Liu, Yu-Juan; et al. (May 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements".
Research in Astronomy and Astrophysics. 23 (5): 055022.
arXiv:
2303.12409.
Bibcode:
2023RAA....23e5022X.
doi:
10.1088/1674-4527/accb7e.
-
^ Gaia Collaboration; et al. (2022). "Gaia Data Release 3: Stellar multiplicity, a teaser for the hidden treasure".
arXiv:
2206.05595 [
astro-ph.SR].
External links