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14 Canis Minoris
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Star in the constellation Canis Minor
Canis Minor constellation map.svg center 280 right Red circle.svg 10 14 Canis Minoris 245 845 Location of 14 Canis Minoris (circled in red)
J2000
Canis Minor
07 58 20.6565
+02 13 29.156
+5.30
red clump
G8 IIIb
0.933 0.005
+42.61 0.20
−156.144
+98.798
13.50
0.34
0.95
2.54 0.11
8.66 0.70
48 12 10
3.10 0.06
5070 17 commas
0.02 0.04
550 60
+02°1833 65345 38962 3110 116182 J07583+0213A 10776 4361 07584+0213
14+CMi
14 Canis Minoris, also known as HD 65345, is a single star in the equatorial constellation of Canis Minor. It is faintly visible to the naked eye with an apparent visual magnitude of +5.30. The distance to this star, as determined from an annual parallax shift of 13.50 0.34 mas, is approximately 242 light years. 14 CMI has a relatively large proper motion, traversing the celestial sphere at the rate of 0.188 arcsecond/year. It is moving further from the Sun with heliocentric radial velocity of +42.6 km/s.
This is an evolved G-type giant star with a stellar classification of G8 IIIb. At the age of around 550 million years old, it is a red clump giant, which means it has already undergone helium flash and is generating energy through helium fusion at its core. The star has an estimated 2.5 times the mass of the Sun and has expanded to 8.7 times the Sun's radius. It is radiating roughly 48 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,070 K.
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Category:G-type giants
Category:Horizontal-branch stars
Category:Canis Minor
BD+02 1833
Canis Minoris, 14
065345
038962
3110