59 Aurigae

Star in the constellation Auriga From Wikipedia, the free encyclopedia

59 Aurigae, often abbreviated as 59 Aur, is a star in the constellation Auriga. Its baseline apparent magnitude is 6.1,[3] meaning it can just barely be seen with the naked eye as a dim, yellow-white hued star. Based on parallax measurements, it is located about 482 light-years (148 parsecs) away from the Sun.[2]

Right ascension06h 53m 01.41097s[2]
Declination+38° 52 08.9322[2]
Quick facts Constellation, Right ascension ...
59 Aurigae

Four visual band light curves for 59 Aurigae, adapted from Zhiping (2000)[1]
Observation data
Epoch J2000      Equinox ICRS
Constellation Auriga
Right ascension 06h 53m 01.41097s[2]
Declination +38° 52 08.9322[2]
Apparent magnitude (V) 6.099[3]
Characteristics
Evolutionary stage subgiant[2]
Spectral type F2V[4]
U−B color index +0.14[5]
B−V color index +0.38[5]
Variable type δ Sct[6]
Astrometry
Radial velocity (Rv)1.0±4.3[7] km/s
Proper motion (μ) RA: −3.916[2] mas/yr
Dec.: +6.659[2] mas/yr
Parallax (π)6.7702±0.0476 mas[2]
Distance482 ± 3 ly
(148 ± 1 pc)
Absolute magnitude (MV)0.23±0.12[8]
Details
Mass2.37[9] M
Radius5.7[10] R
Luminosity62[2] L
Surface gravity (log g)3.23[9] cgs
Temperature6,848[10] K
Metallicity [Fe/H]0.18[8] dex
Rotational velocity (v sin i)165[11] km/s
Age530[12] Myr
Other designations
59 Aur, OX Aur, BD+39°1771, GC 8993, HD 50018, HIP 33041, HR 2539, SAO 59571, PPM 72197, ADS 5534, CCDM J06530+3852, WDS J06530+3852, TYC 2942-2005-1, GSC 02942-02005
Database references
SIMBADdata
Close

In 1966, Ivan John Danziger and Robert John Dickens discovered that 59 Aurigae star is a variable star.[13] This object is a Delta Scuti variable, meaning it varies in luminosity due to pulsations on its surface, ranging in magnitude from 5.94 down to 6.14 with a period of 0.154412 days (3.7 h).[6] For that reason, in 1975, it was given the variable star designation OX Aurigae.[14] The star's spectrum matches that of an F-type main-sequence star and it has a spectral type of F2V.[4] It has 2.4 times the mass of the Sun[9] and 5.7 times the Sun's radius.[10] 59 Aurigae is thought to be around 530 million years old,[12] and is radiating 62 times the Sun's luminosity[2] from its photosphere an effective temperature of 6,848 K.[10]

References

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