HD 43691
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Observation data Epoch J2000.0 |
|
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Constellation (pronunciation) |
Auriga |
Right ascension | 06h 19m 34.68s |
Declination | +41º 05' 32.3" |
Apparent magnitude (V) | +8.03 |
Distance | 304 ly (93.2 pc) |
Spectral type | G0IV-V |
Other designations | |
HD 43691 is a star with magnitude +8.03 in the constellation Auriga. This yellow star is about to stop thermonuclear hydrogen-fusion in its core and eventually expand to become a red giant.
In 2007, the star is found to have a giant planet in orbit around it.
[edit] HD 43691 b
Extrasolar planet | List of extrasolar planets | |
---|---|---|
Orbital elements | ||
Semimajor axis | (a) | 0.24 AU |
Eccentricity | (e) | 0.14±0.02 |
Orbital period | (P) | 36.96±0.02 d |
Angular distance | (θ) | 2.575 mas |
Longitude of periastron |
(ω) | 290±5° |
Time of periastron | (T0) | 2454046.6 JD |
Semi-amplitude | (K) | 90.15 m/s |
Physical characteristics | ||
Mass | (m) | >2.49 MJ |
Discovery information | ||
Discovery date | 2007 | |
Discoverer(s) | Da Silva et al. | |
Detection method | Doppler spectroscopy | |
Discovery site | Geneva observatory | |
Discovery status | Published |
HD 43691 b is a massive jovian planet, though only the minimum mass is known. It might be found to be a superjovian planet when its true mass is known. The planet orbits close to the star, closer than Mercury to the Sun.
[edit] References
- Da Silva R., Udry S., Bouchy F., Moutou C., Mayor M., Beuzit J.-L., Bonfils X., Delfosse X., Desort M., Forveille T., Galland F., Hebrard G., Lagrange A.-M., Loeillet B., Lovis C., Pepe F., Perrier C., Pont F., Queloz D., Santos N., Segresan D., Sivan J.-P., Vidal-Madjar A. (2007). "Elodie metallicity-biased search for transiting Hot Jupiters. IV. Intermediate period planets orbiting the stars HD43691 and HD132406". Astron & Astrophys.