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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.[2] This object is located approximately 335 light years distant from the Sun, based on parallax, and is drifting further away with a radial velocity of +18 km/s.[2] It is circumpolar south of latitude 24°S.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Dorado |
Right ascension | 06h 06m 09.38154s[1] |
Declination | −66° 02′ 22.6304″[1] |
Apparent magnitude (V) | 5.72[2] |
Characteristics | |
Spectral type | A0V[3] |
U−B color index | −0.024±0.004[2] |
B−V color index | −0.03[4] |
Astrometry | |
Radial velocity (Rv) | +17.6±4.3[2] km/s |
Proper motion (μ) | RA: +13.656[1] mas/yr Dec.: +27.815[1] mas/yr |
Parallax (π) | 9.7251 ± 0.1094 mas[1] |
Distance | 335 ± 4 ly (103 ± 1 pc) |
Absolute magnitude (MV) | +0.75[2] |
Details | |
Mass | 2.46[5] M☉ |
Luminosity | 49[6] L☉ |
Surface gravity (log g) | 4.09±0.08[7] cgs |
Temperature | 10,325±240[7] K |
Rotational velocity (v sin i) | 149[5] km/s |
Age | 94[5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
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[6] times the Sun's luminosity from its photosphere at an effective temperature of 10,325 K.[7] It is the southern pole star of Venus.[9]
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