Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Canis Major |
Right ascension | 06h 54m 11.399s[1] |
Declination | −12° 02′ 19.061″[1] |
Apparent magnitude (V) | 4.08[2] |
Characteristics | |
Evolutionary stage | Red giant |
Spectral type | K4 III[2] |
U−B color index | +1.69[3] |
B−V color index | +1.43[3] |
Astrometry | |
Radial velocity (Rv) | +96.2±0.1[4] km/s |
Proper motion (μ) | RA: −136.454 mas/yr[1] Dec.: −14.322 mas/yr[1] |
Parallax (π) | 12.0676 ± 0.62 mas[1] |
Distance | 270 ± 10 ly (83 ± 4 pc)[1] |
Absolute magnitude (MV) | −0.36±0.15[5] |
Details[4] | |
Mass | 0.95±0.03 M☉ |
Radius | 33.01±0.75[6] R☉ |
Luminosity | 304.9±7[6] L☉ |
Surface gravity (log g) | 1.67±0.08 cgs |
Temperature | 4196±43[6] K |
Metallicity [Fe/H] | −0.52±0.04 dex |
Rotational velocity (v sin i) | 2.72±0.40 km/s |
Age | 10.41±1.31 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Theta Canis Majoris (θ Canis Majoris) is a solitary,[8] orange-hued star near the northern edge[9] of the constellation Canis Major, forming the nose of the "dog".[10] The star is visible to the naked eye with an apparent visual magnitude of 4.08.[2] Based upon an annual parallax shift of 12.07 mas as seen from Earth,[1] it is located about 270 light years from the Sun. The star is moving away from Earth with a radial velocity of +96.2 km/s.[4]
This is a evolved K-type giant star with a stellar classification of K4 III.[2] Theta Canis Majoris is 5% less massive than the Sun,[4] but has expanded to 33 times the Sun's size.[6] This old star, around ten billion years old,[4] is over two times older than the Solar System.[11] It irradiates 305 times the Sun's luminosity from its expanded photosphere at an effective temperature of 4,200 K.[6] This temperature gives it the cool orange hue of a K-type star.[12]
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