Our website is made possible by displaying online advertisements to our visitors.
Please consider supporting us by disabling your ad blocker.

Responsive image


15 Leonis Minoris

15 Leonis Minoris
Location of 15 Leo Minoris (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ursa Major[1]
Right ascension 09h 48m 35.37130s[2]
Declination +46° 01′ 15.6338″[2]
Apparent magnitude (V) 5.08[3]
Characteristics
Spectral type G0 IV-V[4]
U−B color index +0.175[5]
B−V color index 0.619±0.007[3]
Astrometry
Radial velocity (Rv)5.20±0.09[6] km/s
Proper motion (μ) RA: 221.788[2] mas/yr
Dec.: −92.816[2] mas/yr
Parallax (π)52.8994 ± 0.1260 mas[2]
Distance61.7 ± 0.1 ly
(18.90 ± 0.05 pc)
Absolute magnitude (MV)3.75[7]
Details
Mass1.15[8] M
Radius1.52[9] R
Luminosity2.912±0.010[2] L
Surface gravity (log g)4.04[4] cgs
Temperature5,859[4] K
Metallicity [Fe/H]0.01[4] dex
Rotational velocity (v sin i)3.97[10] km/s
Age9.3[11] Gyr
Other designations
15 LMi, BD+46°1551, FK5 1255, GJ 368, HD 84737, HIP 48113, HR 3881, SAO 43046[12]
Database references
SIMBADdata

15 Leonis Minoris is the Flamsteed designation for a single[13] star in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 5.08,[3] 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.[14]

This star has a stellar classification of G0 IV-V[4] with an age of about 9.3 billion years,[11] 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,[8] and it is larger in girth than the Sun by +52%.[9] It is spinning with a projected rotational velocity of 4 km/s.[10] The star is radiating almost three[2] times the luminosity of the Sun from its photosphere at an effective temperature of 5,859 K,[4] giving it the yellow-hued glow of a G-type star.[15]

  1. ^ Cite error: The named reference discordances was invoked but never defined (see the help page).
  2. ^ a b c d e f g Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  3. ^ a b c Cite error: The named reference Anderson_Francis_2012 was invoked but never defined (see the help page).
  4. ^ a b c d e f Cite error: The named reference aj132_1_161 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Mermilliod1986 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference apjss141 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference apj131 was invoked but never defined (see the help page).
  8. ^ a b Cite error: The named reference apj756_1_46 was invoked but never defined (see the help page).
  9. ^ a b Cite error: The named reference takeda was invoked but never defined (see the help page).
  10. ^ a b Cite error: The named reference MartínezArnáiz2010 was invoked but never defined (see the help page).
  11. ^ a b Cite error: The named reference Ballering2013 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference mnras389_2_869 was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference apj801_2_143 was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference csiro was invoked but never defined (see the help page).

Previous Page Next Page






15 Leonis Minoris AST 15 Leonis Minoris Spanish 15 Малого Льва Russian 15 Leonis Minoris Swedish HD 84737 Chinese

Responsive image

Responsive image