Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cancer |
Right ascension | 08h 28m 36.78530s[2] |
Declination | +24° 08′ 41.7179″[2] |
Apparent magnitude (V) | 6.05[3] |
Characteristics | |
Spectral type | F0 Vn[4] |
U−B color index | +0.13[3] |
B−V color index | +0.22[3] |
Variable type | δ Sct[5] |
Astrometry | |
Radial velocity (Rv) | +9.0±4.3[6] km/s |
Proper motion (μ) | RA: −30.946[2] mas/yr Dec.: −39.719[2] mas/yr |
Parallax (π) | 8.4885 ± 0.1539 mas[2] |
Distance | 384 ± 7 ly (118 ± 2 pc) |
Absolute magnitude (MV) | 0.41[7] |
Details | |
Mass | 2.36±0.11[8] M☉ |
Radius | 3.7[2] R☉ |
Luminosity | 44[2] L☉ |
Surface gravity (log g) | 3.61[2] cgs |
Temperature | 7,516+52 −103[8] K |
Metallicity [Fe/H] | +0.16[9] dex |
Rotational velocity (v sin i) | 133[8] km/s |
Age | 737[2] Myr |
Other designations | |
Database references | |
SIMBAD | data |
28 Cancri is a star system in the zodiac constellation of Cancer. It is a variable star with the designation CX Cancri, and is close to the lower limit of visibility with the naked eye, having a mean apparent visual magnitude of 6.05.[3] The annual parallax shift seen from Earth's orbit is 8.5 mas, which provides a distance estimate of about 384 light years. It is moving away from the Sun with a radial velocity of around +9 km/s.[6]
Based upon proper motion variation, this is an astrometric binary system with high likelihood (99.8%).[11] The visible component has a stellar classification of F0 Vn,[4] indicating it is a F-type main-sequence star with "nebulous" lines due to rapid rotation. It is a Delta Scuti variable star with a period of 0.0960 days and an amplitude of 0.020 in magnitude.[12] With 2.4 times the mass of the Sun it is spinning with a high projected rotational velocity of 133 km/s. 28 Cancri is radiating roughly 44 times the Sun's luminosity from its photosphere at an effective temperature of around 7,516 K.
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