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Eta1 Doradus

Star in the constellation Dorado From Wikipedia, the free encyclopedia

Eta1 Doradus, Latinized from η1 Doradus, is a star in the southern constellation of Dorado. It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.72.[1] This object is located approximately 342 light years distant from the Sun, based on parallax, and is drifting further away with a radial velocity of +18 km/s.[1] It is circumpolar south of latitude 24°S.

Right ascension06h 06m 09.38177s[2]
Declination−66° 02′ 22.6352″[2]
Quick facts Constellation, Right ascension ...
Eta1 Doradus
Observation data
Epoch J2000      Equinox ICRS
Constellation Dorado[1]
Right ascension 06h 06m 09.38177s[2]
Declination −66° 02′ 22.6352″[2]
Apparent magnitude (V) 5.72[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A0V[3]
U−B color index −0.024±0.004[1]
B−V color index −0.03[4]
Astrometry
Radial velocity (Rv)+17.6±4.3[1] km/s
Proper motion (μ) RA: +13.575[2] mas/yr
Dec.: +28.139[2] mas/yr
Parallax (π)9.5464±0.0474 mas[2]
Distance342 ± 2 ly
(104.8 ± 0.5 pc)
Absolute magnitude (MV)+0.75[1]
Details
Mass2.46[5] M☉
Radius2.5[6] R☉
Luminosity49[7] L☉
Surface gravity (log g)4.09±0.08[8] cgs
Temperature10,325±240[8] K
Rotational velocity (v sin i)149[5] km/s
Age94[5] Myr
Other designations
η1 Dor, CPD−66°493, GC 7813, HD 42525, HIP 28909, HR 2194, SAO 249448, PPM 355182, TYC 8905-1950-1[9]
Database references
SIMBADdata
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This object is an A-type main-sequence star with a stellar classification of A0V.[3] It is 94[5] million years old with a high rotation rate, showing a projected rotational velocity of 149.[5] The star has 2.46[5] times the mass of the Sun and is radiating 49[7] times the Sun's luminosity from its photosphere at an effective temperature of 10,325 K.[8] It is the northern pole star of Venus.[10]

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