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11 Persei
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Star in the constellation Perseus
J2000.0 (ICRS)
Perseus
02 43 02.83826
+55 06 21.6700
5.76
main sequence
B7 III(p?) (Hg?)
−0.110 0.003
−0.7 1.0
+34.859
−21.955
7.8022
0.0874
0.16
3.77 0.06
3.2
210.4 21.9 19.9
14,550
+0.09
4.19
4.50
25–70 d
50.9 12.2
11 Per +54°598 2188 16727 12692 785 23555
11+Per
11 Persei is a single star in the constellation of Perseus, located about 418 light years away from the Sun. It is visible to the naked eye as a dim, blue-white hued star with an apparent visual magnitude of 5.76.
This is a chemically peculiar mercury-manganese star. Cowley (1972) found a stellar classification of B7 III(p?) (Hg?), while Hube (1970) had B8 IV, and Appenzeller (1967) showed B6 V. Stellar models indicate this is a young B-type main sequence star with an estimated age of around 51 million years. It has a low rotation rate, showing a projected rotational velocity of 4.50 km/s. The star has 3.8 times the mass of the Sun and is radiating 210 times the Sun's luminosity from its photosphere at an effective temperature of 14,550 K.
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Category:B-type main-sequence stars
Category:Mercury-manganese stars
Category:Perseus (constellation)
Category:Durchmusterung objects
Persei, 11
016727
012692
0785
Category:Population I stars