Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Dorado |
Right ascension | 05h 26m 19.26577s[1] |
Declination | −58° 54′ 45.06402″[1] |
Apparent magnitude (V) | 5.13±0.01[2] |
Characteristics | |
Evolutionary stage | red giant branch[3] |
Spectral type | G6 III[4] or G8 III[5] |
B−V color index | +1.00[6] |
Astrometry | |
Radial velocity (Rv) | 10±0.07[7] km/s |
Proper motion (μ) | RA: −9.792 mas/yr[1] Dec.: +33.350 mas/yr[1] |
Parallax (π) | 5.9209 ± 0.0712 mas[1] |
Distance | 551 ± 7 ly (169 ± 2 pc) |
Absolute magnitude (MV) | −0.6[8] |
Details[9] | |
Mass | 3.82±0.16 M☉ |
Radius | 21.1±0.5 R☉ |
Luminosity | 252±9 L☉ |
Surface gravity (log g) | 2.41±0.12 cgs |
Temperature | 5,009±43 K |
Metallicity [Fe/H] | −0.06±0.04 dex |
Rotational velocity (v sin i) | 5.2±1[10] km/s |
Age | 258[11] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Lambda Doradus (Lambda Dor), Latinized from λ Doradus, is a solitary[14] yellow hued star located in the southern constellation Dorado. It has an apparent magnitude of 5.13,[2] making it faintly visible to the naked eye if viewed under ideal conditions. Parallax measurements place the star at a distance of 551 light years,[1] and it is currently receding with a heliocentric radial velocity of 10 km/s.[7]
Lambda Dor has a stellar classification of either G6[4] or G8 III,[5] depending on the source. Nevertheless, both indicate that it is a red giant, and it is currently on the red giant branch fusing hydrogen in a shell outside a helium core.[3] At present it has 3.82 times the mass of the Sun[9] and at an age of 258 million years, it has expanded to a radius of 21.2 R☉.[9] It radiates at over 250 times the luminosity of the Sun from its photosphere at an effective temperature of 5,009 K.[9] Lambda Dor is slightly metal deficient, with an iron abundance 12% below solar levels.[9] It currently spins with a projected rotational velocity of 5.2 km/s.[10]
GaiaDR3
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