HD 85945

HD 85945 (HR 3922) is a star in the constellation Ursa Major. It is a yellow giant star with a spectral type of G6III:Fe-0.5. Based on information from Gaia DR3, it is located 132.54 parsecs (432.3 ly) from Earth and is moving towards Earth at a velocity of 47 km/s. It has an apparent magnitude of 5.96, which makes it faintly visible to the naked eye.

HD 85945
Observation data
Epoch J2000      Equinox J2000
ConstellationUrsa Major[a]
Right ascension09h 57m 13.61s[1]
Declination+57° 25′ 05.54″[1]
Apparent magnitude (V)5.959±0.009[1]
Characteristics
Evolutionary stageHorizontal branch[2]
Spectral typeG6III:Fe-0.5[1]
Apparent magnitude (B)6.854±0.015[1]
Apparent magnitude (G)5.733[1]
Apparent magnitude (J)4.513±0.028[1]
Apparent magnitude (H)4.141±0.036[1]
Apparent magnitude (K)3.978±0.3[1]
B−V color index0.895[3]
Astrometry
Radial velocity (Rv)−46.55±0.12[4] km/s
Proper motion (μ) RA: 31.347 mas/yr[4]
Dec.: -61.766 mas/yr[4]
Parallax (π)7.4137 ± 0.024 mas[4]
Distance432.08 ly
(132.54 pc)[4]
Absolute magnitude (MV)0.32[5]
Details
Mass2.5[2] M
Radius10.28±0.14[6] R
Luminosity77.62[7][b] L
Surface gravity (log g)2.6866[4] cgs
Temperature5281±22[6] K
Metallicity [Fe/H]–0.4[7] dex
Rotational velocity (v sin i)7.53[3] km/s
Age660.7[2][c] Myr
Other designations
BD+58 1224, Gaia DR2 1046383298937140864, Gaia DR3 1046383298937140864, HIP 48802, HR 3922, PPM 32387, TIC 377368616, TYC 3817-1649-1, GSC 03817-01649, IRAS 09537+5739
Database references
SIMBADdata

Characteristics

It is an evolved G-type giant star, based on its spectral type of G6III:Fe-0.5, which also indicates that is has a [Fe/Hmetallicity of -0.5.[1] HD 85945 is 2.5 times more massive than the Sun and has expanded to 10.28 times the Sun's size.[2][6] It is emitting 78 times the solar luminosity from its photosphere at an effective temperature of 5,281 K.[7][6] Currently, the star is located in the horizontal branch stage of evolution.[2] The age of HD 85945 is estimated at 660 million years,[2] and it rotates under its axis at a speed of 7.53 km/s.[3] It is slightly metal-poor compared to the Sun, with an abundance of iron equivalent to 40% of the solar abundance.[7][d]

HD 85945 is located within the Ursa Major constellation, based on its celestial coordinates.[a] The distance to HD 85945 is of 132.54 parsecs (432.3 ly), based on spectra from Gaia DR3.[4] The apparent magnitude of the star is of 5.96,[1] which is brighter than the limiting magnitude for naked-eye vision (6.5m), making it faintly visible to the naked eye.[8] The absolute magnitude, i.e. the brightness of the star if it was seen at a distance of 10 parsecs (32.6 ly), is 0.32.[5] At the current distance, its brightness is diminished by 0.03 magnitudes due to interstellar extinction between Earth and the star.[6] HD 85945 is moving away from Earth at a velocity of 46.55 km/s.[4] It has a high proper motion in the sky.[6][1]

Notes

References