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Star in the constellation of Mensa From Wikipedia, the free encyclopedia
YY Mensae, also known as HD 32918, is a variable star located in the southern circumpolar constellation Mensa. It has an apparent magnitude that fluctuates between 8.6 and 8.9,[3] which is within the visibility of binoculars. Based on parallax measurements from Gaia DR3, it is estimated to be 715 light years distant.[2] It appears to be approaching the Solar System with a heliocentric radial velocity of −8.5 km/s.[6]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Mensa |
Right ascension | 04h 58m 17.93697s[2] |
Declination | −75° 16′ 37.9879″[2] |
Apparent magnitude (V) | 8.60 - 8.89[3] |
Characteristics | |
Spectral type | K1 III/IVe[4] |
U−B color index | +0.70[5] |
B−V color index | +1.04[5] |
Variable type | FK Com[3] |
Astrometry | |
Radial velocity (Rv) | −8.5±2.5[6] km/s |
Proper motion (μ) | RA: −4.149 mas/yr[2] Dec.: −3.077 mas/yr[2] |
Parallax (π) | 4.5587 ± 0.0161 mas[2] |
Distance | 715 ± 3 ly (219.4 ± 0.8 pc) |
Absolute magnitude (MV) | +0.81[7] |
Details | |
Mass | 0.983[8] M☉ |
Radius | 12.3[9] R☉ |
Luminosity | 68.5[10] L☉ |
Surface gravity (log g) | 1.63[11] cgs |
Temperature | 4,691±128[12] K |
Metallicity [Fe/H] | −0.59[11] dex |
Rotational velocity (v sin i) | 45±2[13] km/s |
Other designations | |
Database references | |
SIMBAD | data |
This star was known to have an unusual spectrum since the 1970's, but its variability wasn't observed until the 1980's. Collier (1982) found it to be a FK Comae Berenices variable, a class of rapidly rotating giant stars.[15] After a few additional years of observations, HD 32918 was given the variable star designation YY Mensae.[16] A paper in 1987 observed a long and powerful flare coming from the star.[17] X-ray emissions from YY Mensa have been detected in its corona, which may be a result of its fast rotation.[18]
YY Mensae has a stellar classification of K1 III/IVe,[4] indicating an evolved red giant with the blended luminosity class of a giant star and a subgiant. It is chromospherically active and emission lines are also present in its spectra. It has 98% the mass of the Sun[8] but has expanded to 12.3 times its girth.[9] It radiates 68.5 times the luminosity of the Sun[10] from its photosphere at an effective temperature of 4,691 K,[12] giving it an orange hue. Typical for stars its type, YY Mensae spins rapidly, having a projected rotational velocity of 45 km/s.[13] The star is metal deficient, having an iron abundance only 26% that of the Sun.[11]
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