HD 35759
Observation data J2000.0
| |
---|---|
Constellation | Camelopardalis |
Right ascension | 05h 31m 33.349s[1] |
Declination | +64° 19′ 07.59″[1] |
Apparent magnitude (V) | 7.74±0.01[2] |
Characteristics | |
Spectral type | G0[3] or F9/G0V[citation needed] |
B−V color index | 0.602±0.015[4] |
Absolute magnitude (MV) | 3.45[4] |
Details | |
Gyr | |
Database references | |
Exoplanet Archive | data |
HD 35759 is a
light years based on parallax measurements,[1] and it is drifting closer with a heliocentric radial velocity of −12.6 km/s.[5]
This is a
projected rotational velocity
of 3 km/s.
Planetary System
In 2016, a super-jovian exoplanet was discovered orbiting the star on an eccentric orbit. Since the planet was discovered using doppler spectroscopy, its radius and true mass is unknown.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b
|
≥ 3.76±0.17 MJ | 0.389±0.09 | 82.467±0.019 | 0.389±0.006 | — | — |
References
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ISSN 0004-6361.
- Bibcode:1993yCat.3135....0C.
- ^ S2CID 119257644.
- ^ .
- PMID 33087913.
- S2CID 166227927.
- ^ S2CID 55138055.
- S2CID 11027621.
- S2CID 56118016.
- ^ "HD 35759". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-12-15.