Observation data Epoch J2000.0[1] Equinox J2000.0[1] | |
---|---|
Constellation | Fornax |
Right ascension | 02h 27m 28.37813s |
Declination | −27° 38′ 06.7368″ |
Apparent magnitude (V) | 9.09[2] |
Characteristics | |
Spectral type | K1V[3] |
B−V color index | 0.86[4] |
J−H color index | 0.338[4] |
J−K color index | 0.509[4] |
Astrometry | |
Radial velocity (Rv) | −3.882[5] km/s |
Proper motion (μ) | RA: -73.581[1] mas/yr Dec.: −211.935[1] mas/yr |
Parallax (π) | 22.2922 ± 0.016 mas[1] |
Distance | 146.3 ± 0.1 ly (44.86 ± 0.03 pc) |
Absolute magnitude (MV) | 5.56+0.05 −0.06[a] |
Details[6] | |
Mass | 0.829±0.038 M☉ |
Radius | 0.855±0.008 R☉ |
Luminosity | 0.472+0.023 −0.024[7] L☉ |
Surface gravity (log g) | 4.37±0.08 cgs |
Temperature | 5131±74 K |
Metallicity [Fe/H] | 0.03±0.04 dex |
Rotation | 36.55 d |
Age | 9.6+3.8 −3.9 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 15337 (TOI-402) is a star with two orbiting exoplanets in the southern constellation of Fornax. It has an apparent magnitude of 9.09, making it too faint to be observed by the naked eye from Earth, but readily visible using a small telescope.[8] It is located 146 light-years (45 parsecs) distant based on stellar parallax, and is currently heading towards the Solar System with a radial velocity of −3.9 km/s.
The star is about 15% smaller than the Sun in both mass and radius and radiates slightly less than half the Sun's luminosity from its photosphere. It has a spectral type of K1V and an effective temperature of 5,131 K (4,858 °C; 8,776 °F), giving the star an orange hue. It is 9.6+3.8
−3.9 billion years old, making it much older than the Solar System. The star has a solar-like metallicity and displays similar amounts of stellar activity to the Sun,[7] though when the star was only 150 million years old, it may have emitted between 3.7 and 127 times the high-energy luminosity of the Sun in the present day.[3]
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