HD 98649

HD 98649
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Crater
Right ascension 11h 20m 51.76855s
Declination −23° 13 02.4295
Apparent magnitude (V) +8.00
Characteristics
Spectral type G3/5V
B−V color index +0.658
Astrometry
Radial velocity (Rv)4.25±0.12 km/s
Proper motion (μ) RA: −199.735±0.022 mas/yr
Dec.: −177.620±0.017 mas/yr
Parallax (π)23.7206±0.0216 mas
Distance137.5 ± 0.1 ly
(42.16 ± 0.04 pc)
Absolute magnitude (MV)+4.91
Details
Mass0.97±0.02 M
Radius1.01±0.02 R
Luminosity (bolometric)0.968±0.019 L
Luminosity (visual, LV)0.98±0.003 L
Surface gravity (log g)4.38±0.08 cgs
Temperature5,759±35 K
Metallicity [Fe/H]0.05±0.04 dex
Rotation27±4.0 days
Rotational velocity (v sin i)1.19 km/s
Age4.44+0.68
0.58
 Gyr
Other designations
BD−22°3121, HD 98649, HIP 55409, SAO 179793, LTT 4199
Database references
SIMBADdata
Exoplanet Archivedata

HD 98649 is a star with an orbiting exoplanet in the southern Crater constellation. Based on parallax measurements, it is situated at a distance of 137.5 light years from the Sun. The system is drifting further away with a heliocentric radial velocity of 4.3 km/s. With an apparent visual magnitude of +8.00, it is too faint to be viewed with the naked eye. The system has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.24·yr−1.

The spectrum of HD 98649 presents as an ordinary G-type main-sequence star with a stellar classification of G3/5V. It is around 4.4 billion years old and is spinning slowly with a rotation period of roughly 27 days. The star is similar to the Sun, having nearly the same size, mass, and luminosity. It is considered a solar analog. The level of magnetic activity in the chromosphere is minimal.