15 Leonis Minoris
{{short description|Star in the constellation Ursa Major}}
{{Starbox begin
| name = 15 Leonis Minoris
}}
{{Starbox image
| image=
{{Location mark
|image=Ursa Major constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=8|mark_link=15 LMi
|x=793|y=600
}}
|caption=Location of 15 Leo Minoris (circled)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Ursa Major
| dec = {{DEC|+46|01|15.6338}}
}}
{{Starbox character
| type =
| variable =
}}
{{Starbox astrometry
| radial_v = {{val|5.20|0.09}}
| parallax = 52.8994
| p_error = 0.1260
}}
{{Starbox detail
| luminosity = {{val|2.912|0.010}}
}}
{{Starbox catalog
| names = {{odlist | F=15 LMi | BD=+46°1551 | FK5=1255 | GJ=368 | HD=84737 | HIP=48113 | HR=3881 | SAO=43046 }}
}}
{{Starbox reference
| Simbad = 15+LMi
}}
{{Starbox end}}
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 almost three times the luminosity of the Sun from its photosphere at an effective temperature of 5,859 K, giving it the yellow-hued glow of a G-type star.
References
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| title=* 15 LMi
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}}
{{Stars of Ursa Major|state=collapsed}}