HD 33875

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Right ascension05h 06m 09.2953s[1]
Declination−73° 02 15.6159[1]
Apparentmagnitude(V)6.26 ± 0.01[2]
HD 33875
Observation data
Epoch J2000      Equinox J2000
Constellation Mensa
Right ascension 05h 06m 09.2953s[1]
Declination −73° 02 15.6159[1]
Apparent magnitude (V) 6.26 ± 0.01[2]
Characteristics
Spectral type A1 V[3] or A0 V[4]
U−B color index −0.01[5]
B−V color index +0.01[5]
Astrometry
Radial velocity (Rv)8 ± 7.4[6] km/s
Proper motion (μ) RA: +17.783[1] mas/yr
Dec.: +63.090[1] mas/yr
Parallax (π)7.742±0.0276 mas[1]
Distance421 ± 2 ly
(129.2 ± 0.5 pc)
Absolute magnitude (MV)+0.7
Details
Mass2.31 ± 0.41[7] M
Radius2.84 ± 0.35[7] R
Luminosity49.2[8] L
Surface gravity (log g)4[9] cgs
Temperature9,392[10] K
Rotational velocity (v sin i)124 ± 6[10] km/s
Age411[11] Myr
Other designations
20 G. Mensae, CD−73°219, CPD−73°286, FK5 2388, GC 6313, HD 33875, HIP 23737, HR 1700, SAO 256160
Database references
SIMBADdata

HD 33875 (HR 1700) is a solitary star in the southern circumpolar constellation Mensa. With an apparent magnitude of 6.26,[2] it is barely visible to the naked eye under ideal conditions. The star is located at a distance of 421[1] light years but is receding at a rate of 8 km/s.[6]

HD 33875 is an ordinary A-type main-sequence star with a stellar classification of either A1 V[3] or A0 V[4] depending on the source. At present it has 2.38 times the mass of the Sun[7] and 2.84 times the radius of the Sun.[7] It shines at 49.2 times the Sun's luminosity[8] from its photosphere at an effective temperature of 9,392 K,[10] which gives it a white glow. HD 33875 is a fast rotator, spinning rapidly with a projected rotational velocity of 124 km/s.[10]

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