Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Microscopium |
Right ascension | 20h 46m 20.06779s[1] |
Declination | −39° 11′ 57.3590″[1] |
Apparent magnitude (V) | 5.47±0.01[2] |
Characteristics | |
Evolutionary stage | main sequence star[3] |
Spectral type | B8/9 V[4] |
B−V color index | −0.10[5] |
Variable type | suspected SPB[6] |
Astrometry | |
Radial velocity (Rv) | −30±7.4[7] km/s |
Proper motion (μ) | RA: +50.451 mas/yr[1] Dec.: −27.196 mas/yr[1] |
Parallax (π) | 9.9354 ± 0.1022 mas[1] |
Distance | 328 ± 3 ly (101 ± 1 pc) |
Absolute magnitude (MV) | +0.49[8] |
Details | |
Mass | 2.83±0.04[3] M☉ |
Radius | 2.56±0.13[9] R☉ |
Luminosity | 73.5[10] L☉ |
Surface gravity (log g) | 4.11±0.14[11] cgs |
Temperature | 10,965+255 −250[12] K |
Metallicity | 59% solar |
Metallicity [Fe/H] | −0.23[13] dex |
Rotational velocity (v sin i) | 290[14] km/s |
Age | 113[11] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 197630, also known as HR 7933 or rarely 23 G. Microscopii, is a probable astrometric binary located in the southern constellation Microscopium. The visible component is a bluish-white hued star that is faintly visible to the naked eye with an apparent magnitude of 5.47.[2] Based on parallax measurements from the Gaia satellite, the system is estimated to be 328 light years away.[1] However, it is drifting closer with a heliocentric radial velocity of −30 km/s. At its current distance, HD 197630's brightness is diminished by 0.11 magnitudes due to interstellar dust.[17] A 2012 multiplicity survey failed to confirm the velocity variations.[18]
HD 197630 has a stellar classification of B8/9 V,[4] indicating that it is a B-type star with the characteristics of a B8 and B9 main sequence star. It has 2.83 times the mass of the Sun[3] and 2.56 times the Sun's radius. It radiates 73.5 times the luminosity of the Sun[10] from its photosphere at an effective temperature of 10,965 K.[12] The star is estimated to be 113 million years old,[11] having completed roughly half of its main sequence lifetime.[3] HD 19730 is spinning rapidly with a projected rotational velocity of 290 km/s.[14]
The object was in a 2002 Hipparcos variability survey and as a result,[20] the AAVSO cataloged HD 197630 as a suspected variable star that fluctuates by 0.005 magnitudes within 7.71 hours.[21] However, subsequent observations have not confirmed this. Further data from the Transiting Exoplanet Survey Satellite suggests that HD 197630 may be a slowly pulsating B-type star plus a variable star with rotation modulations.[6]
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