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HD 32188

Star in the constellation Auriga From Wikipedia, the free encyclopedia

HD 32188 is suspected variable star[5] in the northern constellation of Auriga, and is positioned roughly in between Eta and Zeta Aurigae. It has a white hue and is just barely visible to the naked eye with an apparent visual magnitude that fluctuates around 6.08.[3] The distance to this star is approximately 3,240 light years, based on parallax.[2] It has an absolute magnitude of −2.87.[4]

Quick facts Constellation, Right ascension ...
HD 32188
Location of HD 32188 (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Auriga[1]
Right ascension 05h 03m 18.63s[2]
Declination +41° 26′ 29.9″[2]
Apparent magnitude (V) 6.08[3]
Characteristics
Spectral type A2IIIshe[4]
U−B color index +0.22[3]
B−V color index +0.21[3]
Variable type Suspected[5]
Astrometry
Radial velocity (Rv)−0.7[6] km/s
Proper motion (μ) RA: −0.227[2] mas/yr
Dec.: −1.820[2] mas/yr
Parallax (π)1.0065±0.0294 mas[2]
Distance3,240 ± 90 ly
(990 ± 30 pc)
Absolute magnitude (MV)−2.87[4]
Details
Mass3.1[7] M☉
Radius40[2] R☉
Luminosity5,370[8] L☉
Surface gravity (log g)[7] cgs
Temperature8,665[7] K
Rotation0.41 days[8]
Rotational velocity (v sin i)23[9] km/s
Other designations
NSV 1810, BD+41°1044, HD 32188, HIP 23511, HR 1615, SAO 39979[10]
Database references
SIMBADdata
Close

This object is an A-type giant star with a stellar classification of A2IIIshe.[4] The suffix notation indicates this is a shell star,[11] which means it has a peculiar spectrum indicating there is a circumstellar disk of gas around the star's equator. While the spectral luminosity class is III, analysis of its colour and brightness suggest it more closely resembles a supergiant star.[4] HD 32188 has expanded to 40 times the radius of the Sun[2] and it is spinning with a projected rotational velocity of 23 km/s.[9] It is radiating 5,370 times the luminosity of the Sun[8] from its enlarged photosphere at an effective temperature of 8,665 K.[7]

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