Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydrus |
Right ascension | 00h 16m 12.6791s[1] |
Declination | −79° 51′ 04.2447″[1] |
Apparent magnitude (V) | 6.59 |
Characteristics | |
HD 1237 A | |
Spectral type | G6 V |
B−V color index | 0.749 |
HD 1237 B | |
Spectral type | M4 V[2] |
Astrometry | |
Radial velocity (Rv) | −5.2±0.2[3] km/s |
Proper motion (μ) | RA: 433.908±0.044[1] mas/yr Dec.: −56.322±0.039[1] mas/yr |
Parallax (π) | 56.9319 ± 0.0235 mas[1] |
Distance | 57.29 ± 0.02 ly (17.565 ± 0.007 pc) |
Absolute magnitude (MV) | 5.37 ± 0.01[4] |
Details | |
HD 1237 A | |
Mass | 1.00 ± 0.10[5] M☉ |
Radius | 0.86 ± 0.07[5] R☉ |
Luminosity | 0.64[5] L☉ |
Surface gravity (log g) | 4.58 ± 0.09[5] cgs |
Temperature | 5,572 ± 40[5] K |
Metallicity [Fe/H] | 0.12 ± 0.04[5] dex |
Rotation | 7.0±0.7 d[3] |
Rotational velocity (v sin i) | 5.3±1.0[3] km/s |
Age | 800[6] Myr |
HD 1237 B | |
Mass | 0.13[2] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
HD 1237 is a binary star system approximately 57 light-years away in the constellation of Hydrus (the Water Snake).
The visible star in the system, A, is considered to be a solar analog due close mass to the sun. HD 1237 differs from the sun in that HD 1237 is much younger, has high metallicity, has much cooler temperature and is in a binary system. As of 2000, it has been confirmed that an extrasolar planet orbits the star. It is of note for being a relatively Sun-like star not very far from the Sun that is home to an extrasolar planet.[7]
Gaia DR2
was invoked but never defined (see the help page).Chauvin2007
was invoked but never defined (see the help page).Alvarado-Gómez2015
was invoked but never defined (see the help page).Holmberg2009
was invoked but never defined (see the help page).apj720_2_1290
was invoked but never defined (see the help page).Saffe2005
was invoked but never defined (see the help page).Naef2001
was invoked but never defined (see the help page).