Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cancer |
Right ascension | 08h 07m 45.85581s[1] |
Declination | +21° 34′ 54.5325″[1] |
Apparent magnitude (V) | +5.30[2] |
Characteristics | |
Evolutionary stage | Subgiant[3] |
Spectral type | G2 IV[4] |
U−B color index | +0.21[2] |
B−V color index | +0.63[2] |
Astrometry | |
Radial velocity (Rv) | −36.0±0.1[5] km/s |
Proper motion (μ) | RA: +23.610[1] mas/yr Dec.: −68.122[1] mas/yr |
Parallax (π) | 42.3605 ± 0.1251 mas[1] |
Distance | 77.0 ± 0.2 ly (23.61 ± 0.07 pc) |
Absolute magnitude (MV) | +3.46[6] |
Details | |
Mass | 1.192+0.017 −0.016[7] M☉ |
Radius | 1.82[8] R☉ |
Luminosity | 3.782±0.015[1] L☉ |
Surface gravity (log g) | 3.97±0.02[7] cgs |
Temperature | 5,809±59[7] K |
Metallicity [Fe/H] | 0.11[7] dex |
Rotational velocity (v sin i) | 3.7±0.3[6] km/s |
Age | 5.64+0.35 −0.14[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Mu2 Cancri is a solitary,[10] yellow-hued star in the zodiac constellation of Cancer. It is visible to the naked eye with an apparent visual magnitude of +5.30.[2] Based upon an annual parallax shift of 42.36 mas as seen from Earth,[1] this star is located 77 light-years from the Sun. It is drifting closer with a radial velocity of −36 km/s[5] and will make its closest approach in about 611,100 years when it passes at a distance of 16.8 light-years (5.2 parsecs).[11]
At the estimated age of 5.6 billion years,[7] Mu2 Cancri is an evolving G-type subgiant star[3] with a stellar classification of G2 IV.[4] It has 1.2[7] times the mass of the Sun and 1.8[8] times the Sun's radius. Mu2 Cancri has relatively high metallicity—what astronomers term the abundance of elements other than hydrogen and helium—having a 29% higher abundance compared to the Sun.[7] It is radiating 3.78[1] times the Sun's luminosity at an effective temperature of 5,809 K.[7] The star is spinning at a leisurely projected rotational velocity of 3.7 km/s.[6]
GaiaDR2
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