HD 95086

HD 95086 / Aiolos

HD 95086 system. g and g2 are background galaxies, s is a background star
Credit: NASA/ESA/CSA JWST, modified work by Mâlin et al. 2024[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 10h 57m 03.02157s[2]
Declination −68° 40′ 02.4492″[2]
Apparent magnitude (V) 7.36
Characteristics
Evolutionary stage Pre-main-sequence star[3]
Spectral type A8[4]
Astrometry
Radial velocity (Rv)18.04±0.16[2] km/s
Proper motion (μ) RA: −41.128 mas/yr[2]
Dec.: 12.861 mas/yr[2]
Parallax (π)11.5659 ± 0.0187 mas[2]
Distance282.0 ± 0.5 ly
(86.5 ± 0.1 pc)
Details[4]
Mass1.6±0.1 M☉
Luminosity5.7±1.7 L☉
Surface gravity (log g)4.0±0.5 cgs
Temperature7750±250 K
Metallicity [Fe/H]−0.25±0.5 dex
Rotational velocity (v sin i)20 ± 10 km/s
Age13.3+1.1
−0.6[5] Myr
Other designations
Aiolos, CD−68 847, Gaia DR2 5231963962676292224, HD 95086, HIP 53524, TYC 9212-4675-1, GSC 09212-04675, 2MASS J10570301-6840023[6]
Database references
SIMBADdata

HD 95086, formally named Aiolos,[7] is a pre-main-sequence star[3] about 282 light-years (86 parsecs) away. Its surface temperature is 7,750±250 K. HD 95086 is somewhat metal-deficient in comparison to the Sun, with a metallicity Fe/H index of −0.25±0.5 (~55%), and is much younger at an age of 13.3 million years.[5] It was originally thought to be part of the Lower Centaurus-Crux association, until it was found using Gaia data that the star may be instead part of the Carina association.[5]

Multiplicity surveys did not detect any stellar companions to HD 95086 as of 2013.[8]

  1. ^ Cite error: The named reference Mâlin2024 was invoked but never defined (see the help page).
  2. ^ a b c d e Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  3. ^ a b Meshkat, T.; Bailey, V.; Rameau, J.; Bonnefoy, M.; Boccaletti, A.; Mamajek, E. E.; Kenworthy, M.; Chauvin, G.; Lagrange, A. -M.; Su, K. Y. L.; Currie, T. (October 2013). "Further Evidence of the Planetary Nature of HD 95086 b from Gemini/NICI H-band Data". The Astrophysical Journal Letters. 775 (2): L40. arXiv:1309.0543. Bibcode:2013ApJ...775L..40M. doi:10.1088/2041-8205/775/2/L40. L40.
  4. ^ a b Cite error: The named reference Ghauvin2018 was invoked but never defined (see the help page).
  5. ^ a b c Cite error: The named reference Desgrange was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference NEW2022 was invoked but never defined (see the help page).
  8. ^ De Rosa, R. J.; Patience, J.; Wilson, P. A.; Schneider, A.; Wiktorowicz, S. J.; Vigan, A.; Marois, C.; Song, I.; Macintosh, B.; Graham, J. R.; Doyon, R.; Bessell, M. S.; Thomas, S.; Lai, O. (2013), "The VAST Survey – III. The multiplicity of A-type stars within 75 pc", Monthly Notices of the Royal Astronomical Society, 437 (2): 1216–1240, arXiv:1311.7141, Bibcode:2014MNRAS.437.1216D, doi:10.1093/mnras/stt1932