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15 Leonis Minoris
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Star in the constellation Ursa Major
15 Leonis Minoris
Ursa Major constellation map.svg center 280 right Red circle.svg 8 15 LMi 793 600 Location of 15 Leo Minoris (circled)
J2000.0
Ursa Major
09 48 35.37135
+46 01 15.6266
5.08
subgiant
G0 IV-V
0.619 0.007
+0.175
5.20 0.09
+221.750
−92.356
53.1277
0.0773
3.75
1.15
1.62
2.80
4.04
5,859
1.25 AU
2.93 AU
0.01
3.97
9.3
15 LMi +46°1551 1255 368 84737 48113 3881 43046
15+LMi
15 Leonis Minoris is the Flamsteed designation for a single star in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 5.08, making it a fifth magnitude star that is visible to the naked eye. Based on parallax measurements, it is located at a distance of 61.7 light years from the Sun. The star has been examined for an infrared excess, but none was detected.
This star has a stellar classification of G0 IV-V with an age of about 9.3 billion years, which suggests that it is an older G-type main sequence star that may be evolving into a subgiant as the hydrogen at its core runs out. The estimated mass of the star is 15% greater than the Sun's mass, and it is larger in girth than the Sun by +52%. It is spinning with a projected rotational velocity of 4 km/s. The star is radiating nearly three times the luminosity of the Sun from its photosphere at an effective temperature of commas 5,859 K, giving it the yellow-hued glow of a G-type star.
15 Leonis Minoris presents a significantly difference on proper motion measurements taken by the Hipparcos and Gaia spacecraft, suggesting it may have an orbiting giant planet.
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collapsed
Category:Ursa Major
Leonis Minoris, 15
048113
3881
0368
084737
Category:G-type subgiants
BD+46 1551