Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Microscopium |
Right ascension | 21h 12m 13.71281s[1] |
Declination | −40° 16′ 09.7010″[1] |
Apparent magnitude (V) | 5.83[2] (5.83 - 5.86)[3] |
Characteristics | |
Spectral type | F5 V[4][5] |
B−V color index | +0.45[2] |
Variable type | suspected[3] |
Astrometry | |
Radial velocity (Rv) | 4.5±0.9[6] km/s |
Proper motion (μ) | RA: +58.359 mas/yr[1] Dec.: −218.773 mas/yr[1] |
Parallax (π) | 31.4586 ± 0.0401 mas[1] |
Distance | 103.7 ± 0.1 ly (31.79 ± 0.04 pc) |
Absolute magnitude (MV) | +3.33[7] |
Details | |
Mass | 1.28[8] M☉ |
Radius | 1.47+0.07 −0.04[9] R☉ |
Luminosity | 3.79±0.01[1] L☉ |
Surface gravity (log g) | 4.21±0.01[10] cgs |
Temperature | 6,637±80[11] K |
Metallicity [Fe/H] | +0.06±0.01[12] dex |
Rotational velocity (v sin i) | 25.1±2.5[13] km/s |
Age | 916[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 201647 (HR 8100; Gliese 9726; LTT 8410) is a solitary star[16] located in the southern constellation Microscopium. It is faintly visible to the naked eye as a yellowish-white-hued star with an apparent magnitude of 5.83.[2] The object is located relatively close at a distance of light-years based on Gaia DR3 parallax measurements, but it is receding with a heliocentric radial velocity of 4.5 km/s.[6] At its current distance, HD 201647's brightness is diminished by 0.11 magnitudes due to interstellar extinction[17] and it has an absolute magnitude of +3.33.[7] It has a relatively high proper motion across the celestial sphere, moving at a rate of 226.331 mas/yr.[18]
HD 201647 has a stellar classification of F5 V,[5][4] indicating that it is an ordinary F-type main-sequence star that is generating energy via hydrogen fusion at its core. It has 1.28 times the mass of the Sun[8] and 1.47 times the radius of the Sun.[9] It radiates 3.79 times the luminosity of the Sun[1] from its photosphere at an effective temperature of 6,637 K.[11] HD 201647 is slightly metal enriched with an iron abundance of [Fe/H] = +0.06 or 115% of the Sun's.[12] It is estimated to be 916 million years old[8] and it spins modestly with a projected rotational velocity of 25.1 km/s.[13]
In the discovery paper for Lacaille 8760, HD 201647 was reported to be a variable star that varied between 5.83 and 5.86 in the visual passband.[3] As of 2004 however, it has not been confirmed to be variable.[19]
GaiaDR3
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