HD 101581

HD 101581
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 11h 41m 02.46847s
Declination −44° 24 18.6867
Apparent magnitude (V) 7.762
Characteristics
Evolutionary stage main sequence
Spectral type K4.5Vk:
Astrometry
Radial velocity (Rv)13.55±0.13 km/s
Proper motion (μ) RA: −660.634 mas/yr
Dec.: 242.096 mas/yr
Parallax (π)78.2268±0.0182 mas
Distance41.694 ± 0.010 ly
(12.783 ± 0.003 pc)
Absolute magnitude (MV)+7.30
Details
Mass0.653±0.028 M
Radius0.630±0.027 R
Luminosity (bolometric)0.18332±0.00059 L
Surface gravity (log g)4.654±0.057 cgs
Temperature4675±53 K
Metallicity [Fe/H]−0.505±0.027 dex
Rotation~30 days
Rotational velocity (v sin i)2.47±0.30 km/s
Age6.88±4.27 Gyr
Other designations
CD−43 7228, GJ 435, HD 101581, HIP 56998, SAO 222956, LHS 2441, TOI-6276, TIC 397362481
Database references
SIMBADdata
Exoplanet Archivedata

HD 101581 (TOI-6276, Gliese 435) is a nearby K-type main-sequence star located in the constellation Centaurus, approximately 41.7 light-years (12.8 parsecs) away, based on a parallax of 78.227 mas. At an apparent magnitude of 7.8, it is too faint to be seen with the naked eye, although it can be viewed with a small telescope.

HD 101581 has a spectral type of K5V, which classifies it as a main sequence star (similar to the Sun) having the core hydrogen converted into helium. It has 0.65 times the Solar mass and 0.63 times the Solar radius while its age is estimated to be about 6.9 billion years old. Its surface has an effective temperature of 4633 K giving it the typical orange hue of a K-type star. The metallicity index of it is −0.344±0.059, indicating an iron-to-hydrogen ratio 45% that of the Sun.