Lambda Cancri
Lambda Cancri (λ Cancri, abbreviated Lambda Cnc, λ Cnc) is a blue-white-hued spectroscopic binary star in the zodiac constellation of Cancer. With a combined apparent visual magnitude of +5.93, it is faintly visible to the naked eye. Based upon parallax measurements obtained during the Gaia mission, it is about 550 light-years distant from the Sun.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Cancer |
Right ascension | 08h 20m 32.13630s |
Declination | +24° 01′ 20.3198″ |
Apparent magnitude (V) | +5.93 |
Characteristics | |
Spectral type | B9.5 V |
Astrometry | |
Radial velocity (Rv) | +23.0±4.3 km/s |
Proper motion (μ) | RA: −20.29 mas/yr Dec.: −18.81 mas/yr |
Parallax (π) | 5.9490 ± 0.1482 mas |
Distance | 550 ± 10 ly (168 ± 4 pc) |
Absolute magnitude (MV) | +0.19 |
Details | |
λ Cnc A | |
Mass | 2.1+0.39 −0.32 M☉ |
Luminosity | 78 L☉ |
Surface gravity (log g) | 4.0±0.25 cgs |
Temperature | 9,500±1,000 K |
Rotational velocity (v sin i) | 188 km/s |
Age | 105+287 −93 Myr |
λ Cnc B | |
Mass | 0.8 M☉ |
Temperature | 4,562±154 K |
Metallicity [Fe/H] | −0.5 dex |
Rotational velocity (v sin i) | 10 km/s |
Other designations | |
Database references | |
SIMBAD | data |
The two components are designated Lambda Cancri A (formally named Piautos /piˈɔːtɒs/) and B.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.