25 Cancri

25 Cancri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cancer
Right ascension 08h 25m 49.87726s
Declination +17° 02 46.5717
Apparent magnitude (V) 6.11
Characteristics
Spectral type F6 V
B−V color index 0.448±0.005
Astrometry
Radial velocity (Rv)+37.56±0.13 km/s
Proper motion (μ) RA: −191.567 mas/yr
Dec.: −151.554 mas/yr
Parallax (π)21.9803±0.0321 mas
Distance148.4 ± 0.2 ly
(45.50 ± 0.07 pc)
Absolute magnitude (MV)2.85
Details
25 Cnc A
Mass1.51 M
Radius2.0 R
Luminosity6.60 L
Surface gravity (log g)4.01 cgs
Temperature6,487 K
Metallicity [Fe/H]−0.10 dex
Rotational velocity (v sin i)37.74±0.55 km/s
Age2.50 Gyr
25 Cnc B
Mass0.34 M
Other designations
d2 Cnc, 25 Cnc, BD+17°1842, HD 71030, HIP 41319, HR 3299, SAO 97806, WDS 08258+1703
Database references
SIMBADdata

25 Cancri is a common proper motion star system in the zodiac constellation of Cancer, located around 148 light-years away from the Sun. It has the Bayer designation d2 Cancri (d2 Cnc); 25 Cancri (25 Cnc) is the Flamsteed designation. It is near the lower limit of visibility to the naked eye in good viewing conditions, appearing as a dim, yellow-white-hued star with a combined apparent visual magnitude of 6.11. The pair have a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.245 per year. It is moving further from the Earth with a heliocentric radial velocity of +38 km/s.

Based upon a stellar classification of F6 V, the brighter component is an F-type main-sequence star that is generating energy through hydrogen fusion at its core. Cowley (1976) listed a class of F5 IIIm?, which suggests it may be an Am star. However, this has not been confirmed. It is about 2.5 billion years old with 1.51 times the mass of the Sun. The star is radiating 6.6 times the Sun's luminosity from its photosphere at an effective temperature of 6,487 K.

The companion is 4.19 magnitudes fainter than the primary, and lies at an angular separation of 16.798 along a position angle of 310°, as of 2013. If the pair are gravitationally bound, then they orbit each other with a period of around 4.05 million years.