Phi Capricorni
Phi Capricorni (φ Cap, φ Capricorni) is a solitary star in the southern constellation of Capricornus. It is visible to the naked eye with an apparent visual magnitude of +5.16. Based upon an annual parallax shift of 5.07 mas as seen from the Earth, the star is located about 640 light years from the Sun, give or take 30 light years.

This is an evolved, orange-hued K-type giant/bright giant star with a stellar classification of K0 II-III It shows an infrared excess, which may be due to leftover material from a mass-loss event. The star has an estimated 2.63 times the mass of the Sun, and radiates 447 times the solar luminosity from its photosphere at an effective temperature of 4,490 K. Phi Capricorni is around 1.24 billion years old and is spinning with a projected rotational velocity of 3.8 km/s.
Q523
star
Concept
Q8928
constellation
Concept
Q10535
Capricornus
CEL
Q124313
apparent visual magnitude
Concept
Q165074
parallax
Concept
Q12097402
mas
Concept
Q531
light year
Concept
Q525
Sun
CEL
Q6472
evolved
Concept
Q25377588
K-type
Concept
Q5875
giant
Concept
Q5881
bright giant
Concept
Q25377588
stellar classification
Concept
Q1396651
infrared excess
UNK
Q180892
mass of the Sun
Concept
Q843877
solar luminosity
Concept
Q6372
photosphere
Concept
Q854050
effective temperature
Concept
Q6464
projected rotational velocity
Concept
Q2404577
Phi Capricorni
CEL
Q2404577
Phi Capricorni
CEL
++5.16^^http://www.w3.org/2001/XMLSchema#decimal
+5.16
NUMBER
+5.07^^http://www.w3.org/2001/XMLSchema#decimal
5.07
NUMBER
+30^^http://www.w3.org/2001/XMLSchema#decimal
30
NUMBER
0^^http://www.w3.org/2001/XMLSchema#decimal
0
NUMBER
+2.63^^http://www.w3.org/2001/XMLSchema#decimal
2.63
NUMBER
+1.24^^http://www.w3.org/2001/XMLSchema#decimal
1.24
NUMBER
+3.8^^http://www.w3.org/2001/XMLSchema#decimal
3.8
NUMBER
instance of
constellation
mass
instance of
subclass of