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HD 72337

Star in the constellation Volans From Wikipedia, the free encyclopedia

HD 72337, also known as HR 3370, is a solitary,[13] bluish-white hued star located in the southern constellation Volans. With an apparent magnitude of 5.51,[3] it is faintly visible to the unaided eye but only under ideal conditions.

Right ascension08h 27m 16.7555s[2]
Declination−70° 05′ 36.541″[2]
Quick facts Constellation, Right ascension ...
HD 72337
Observation data
Epoch J2000      Equinox ICRS
Constellation Volans[1]
Right ascension 08h 27m 16.7555s[2]
Declination −70° 05′ 36.541″[2]
Apparent magnitude (V) 5.51±0.01[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A0 V[4]
U−B color index −0.04[5]
B−V color index −0.03[5]
Astrometry
Radial velocity (Rv)13±7.4[6] km/s
Proper motion (μ) RA: −18.630 mas/yr[2]
Dec.: +45.723 mas/yr[2]
Parallax (π)11.3465±0.0387 mas[2]
Distance287.5 ± 1.0 ly
(88.1 ± 0.3 pc)
Absolute magnitude (MV)+0.85[1]
Details
Mass2.51±0.07[7] M☉
Radius2.26±0.06[8] R☉
Luminosity42.5[9] L☉
Surface gravity (log g)4.15[10] cgs
Temperature10,251±384[11] K
Rotational velocity (v sin i)149[10] km/s
Age265[10] Myr
Other designations
30 G. Volantis, CPD−69°919, GC 11620, HD 72337, HIP 41451, HR 3370, SAO 250235[12]
Database references
SIMBADdata
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Velocity

Based on recent parallax measurements from the Gaia spacecraft, HD 72337 is currently located at a distance of 287 light years.[2] The object made its closest approach 1.914 million years ago when it was 234 light years distant.[1] At that distance, it brightened slightly to an apparent magnitude of 5.13.[1] Currently, HR 3370 is receding with a heliocentric radial velocity of 10.7 km/s.[6]

Properties

The stellar classification of HD 72337 is A0 V,[4] indicating that it is an ordinary A-type main-sequence star. It has 2.25 times the radius of the Sun[8] and a mass of 2.51 M☉.[7] It radiates at 42.5 times the luminosity of the Sun[9] from its photosphere at an effective temperature of 10,251 K.[11] Like many hot stars, HD 72337 rotates rapidly with a projected rotational velocity of 149 km/s, and is estimated to be 265 million years old.[10]

References

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