Lambda Cancri

λ Cancri
Location of Piautos (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
Right ascension 08h 20m 32.13630s
Declination +24° 01′ 20.3198″
Apparent magnitude (V) +5.93
Characteristics
Evolutionary stage main sequence
Spectral type B9.5 V
B−V color index −0.039±0.004
Astrometry
Radial velocity (Rv)+23.0±4.3 km/s
Proper motion (μ) RA: −20.843 mas/yr
Dec.: −18.970 mas/yr
Parallax (π)5.7362±0.0582 mas
Distance569 ± 6 ly
(174 ± 2 pc)
Absolute magnitude (MV)+0.19
Details
λ Cnc A
Mass2.61±0.35 M
Radius3.69±0.13 R
Luminosity131±L
Surface gravity (log g)3.72±0.06 cgs
Temperature10,162±123 K
Rotational velocity (v sin i)188 km/s
Age105+287
−93
 Myr
λ Cnc B
Mass0.8 M
Temperature4,562±154 K
Metallicity [Fe/H]−0.5 dex
Rotational velocity (v sin i)10 km/s
Other designations
Piautos, λ Cnc, 19 Cancri, BD+24°1909, HD 70011, HIP 40881, HR 3268, SAO 80113
Database references
SIMBADdata

Lambda Cancri is a blue-white-hued spectroscopic binary star in the zodiac constellation of Cancer. Its name is a Bayer designation that is Latinized from λ Cancri, and abbreviated Lambda Cnc or λ Cnc. 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 approximately 569 light-years (174 pc) distant from the Sun. The system is drifting further away with a line of sight velocity of around +23 km/s.

The two components are designated Lambda Cancri A (formally named Piautos /piˈɔːtɒs/) and B. The position of this system near the ecliptic means it is subject to lunar occultation.