HD 45364
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Canis Major |
Right ascension | 06h 25m 38.48s[1] |
Declination | −31° 28′ 51.4″[1] |
Apparent magnitude (V) | 8.07 |
Characteristics | |
Spectral type | G8V |
B−V color index | 0.719 |
V−R color index | 0.01 |
Astrometry | |
Radial velocity (Rv) | 15.9 km/s |
Proper motion (μ) | RA: 53.22 ± 0.48 [1] mas/yr Dec.: −13.20 ± 0.77 [1] mas/yr |
Parallax (π) | 30.59 ± 0.68[1] mas |
Distance | 107 ± 2 ly (32.7 ± 0.7 pc) |
Absolute magnitude (MV) | +5.50 |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Extrasolar Planets Encyclopaedia | data |
HD 45364 is a star approximately 107 light years away from Earth in the constellation of Canis Major. As of August 2008 there are two confirmed extrasolar planets orbiting around it.[2]
Planetary system
HD 45364 is one of only a relative few systems that have had more than one exoplanet discovered in its orbit. The two planets, HD 45364 b and HD 45364 c respectively, were both discovered in August 2008.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥0.1872 MJ | 0.6813 | 226.93 ± 0.37 | 0.1684 ± 0.190 | — | — |
c | ≥0.6579 MJ | 0.8972 | 342.85 ± 0.28 | 0.0974 ± 0.012 | — | — |
Formation scenario
A detailed analysis of the formation scenario revealed that the previously reported orbital configuration might not be correct.[3] The eccentricities are a factor of 4-5 too large to be consistent with standard planet formation theories. This is the first time that planet formation theory was able to predict new orbital parameters of a planetary system.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 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
- ↑ 2.0 2.1 Correia, A. C. M. et al. (2009). "The HARPS search for southern extra-solar planets XVI. HD 45364, a pair of planets in a 3:2 mean motion resonance". Astronomy and Astrophysics 496 (2): 521–526. arXiv:0902.0597. Bibcode:2009A&A...496..521C. doi:10.1051/0004-6361:200810774.
- ↑ Rein et al. (2010). "The dynamical origin of the multi-planetary system HD 45364" (abstract). Astronomy and Astrophysics 510 (1). arXiv:0910.5082. Bibcode:2010A&A...510A...4R. doi:10.1051/0004-6361/200913208. (web preprint)
Coordinates: 06h 25m 38s, −31° 28′ 51″
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