Gliese 146

From Wikipedia, the free encyclopedia
Gliese 146
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Horologium
Right ascension 03h 35m 00.93995s[1]
Declination −48° 25′ 08.9046″[1]
Apparent magnitude (V) 8.64[2]
Characteristics
Evolutionary stage Main Sequence[3]
Spectral type K6.5V[3]
U−B color index +1.24[2]
B−V color index +1.30[2]
Variable type suspected, range 8.57 to 8.7 mag, NSV 1203[4][5]
Astrometry
Radial velocity (Rv)+19.5[6] km/s
Proper motion (μ) RA: 404.71[1] mas/yr
Dec.: 308.13[1] mas/yr
Parallax (π)73.520 ± 0.016[7] mas
Distance44.363 ± 0.010 ly
(13.602 ± 0.003 pc)
Details[7]
Mass0.684±0.013 M
Radius0.674±0.020 R
Luminosity0.121[8] L
Surface gravity (log g)4.69±0.05 cgs
Temperature4385±21 K
Metallicity [Fe/H]-0.08±0.02 dex
Rotation34.99+0.58
−0.53
Age970[9] Myr
Other designations
CD−48° 1011, GJ 146, HD 22496, HIP 16711, LTT 1698, SAO 85397, 2MASS J03350093-4825089[4]
Database references
SIMBADdata
ARICNSdata

Gliese 146 is a K5V class star located in the constellation Horologium. At 44.4 light years, GJ 146 has an apparent magnitude of +8.57. Gliese 146 is also known as HD 22496, HIP 16711, SAO-216392, and LHS 1563.[10]

Its speed relative to the sun is 38.1 km/second, and its galactic orbit ranges between 20,800 and 25,400 light years from the center of the Galaxy, placing it within a thin disk.[7] It is a suspected variable star.[4][5] It belongs to the Hyades supercluster of stars[11] It is one of 155 K-type stars within 50 light years.[10]

Gliese 146 is a flare star, with average flare frequency 0.23 flares per day.[12]

Planetary system[]

It is one of 500 stars selected in 2009 for the SCUBA-2 All Sky Survey for stars with debris disks.[13] The debris disk was not detected by any survey as in 2015 though.[8]

In 2021, a Sub-Neptune planet HD 22496b was discovered utilizing a Doppler spectroscopy method.[7]

The HD 22496 planetary system[7]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
HD 22496b >5.57+0.73
−0.68
, <16 M
WIKI