HIP 11915

HIP 11915 is a G-type main-sequence star located about 190 light-years from Earth in the constellation Cetus. It is best known for its characteristics, which are very similar to those of the Sun, including the mass, radius, temperature, metallicity and age, which means that it is almost a solar twin, being just 500 million years younger than the Sun and with a lower metallicity. It is also known for its planetary companion, HIP 11915 b, which has a mass and orbital distance very similar to that of Jupiter, but probably with a slightly higher orbital eccentricity.

HIP 11915
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 02h 33m 49.026s
Declination –19° 36 42.500
Apparent magnitude (V) 8.58
Characteristics
Evolutionary stage Main sequence
Spectral type G5V
Astrometry
Radial velocity (Rv)+14.1 ± 0.5 km/s
Proper motion (μ) RA: 225.590±0.082 mas/yr
Dec.: 35.400±0.090 mas/yr
Parallax (π)18.63 ± 0.29 mas
Distance175 ± 3 ly
(53.7 ± 0.8 pc)
Absolute magnitude (MV)4.83
Details
Mass0.991±0.003 M
Radius~1.01 R
Luminosity1.0+0.13
−0.12
 L
Surface gravity (log g)4.47±0.008 cgs
Temperature5773±2 K
Metallicity [Fe/H]−0.057±0.003 dex
Rotational velocity (v sin i)0.99 ± 0.15 km/s
Age3.87±0.39 Gyr
Other designations
HD 16008, HIP 11915, SAO 148468, BD-20°481
Database references
SIMBADdata

This star is entry number 11915 in the Hipparcos Catalogue. The star is located at 02:33:49.02495 right ascension, −19° 36' 42.5032" dec. Too faint to be seen with the unaided eye, the star can be spotted with good binoculars.

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