Astronomy:HD 95086
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Carina[2] |
| Right ascension | 10h 57m 03.02157s[3] |
| Declination | −68° 40′ 02.4492″[3] |
| Apparent magnitude (V) | 7.36[4] |
| Characteristics | |
| Evolutionary stage | Pre-main-sequence star[5] |
| Spectral type | A8[6] |
| Astrometry | |
| Radial velocity (Rv) | 18.04±0.16[3] km/s |
| Proper motion (μ) | RA: −41.128[3] mas/yr Dec.: 12.861[3] mas/yr |
| Parallax (π) | 11.5659 ± 0.0187[3] mas |
| Distance | 282.0 ± 0.5 ly (86.5 ± 0.1 pc) |
| Absolute magnitude (MV) | +2.58[7] |
| Details[6] | |
| Mass | 1.6±0.1 M☉ |
| Luminosity | 5.7±1.7 L☉ |
| Surface gravity (log g) | 4.0±0.5 cgs |
| Temperature | 7750±250 K |
| Metallicity [Fe/H] | −0.25±0.5 dex |
| Rotational velocity (v sin i) | 20 ± 10 km/s |
| Age | 13.3+1.1−0.6[8] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 95086, formally named Aiolos,[10] is a pre-main-sequence star[5] 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.[8] 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.[8]
Multiplicity surveys did not detect any stellar companions to HD 95086 as of 2013.[11]
Nomenclature
The designation HD 95086 comes from the Henry Draper Catalogue.
In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project.[12] The approved names, proposed by a team from Greece, were announced in June 2023. HD 95086 is named Aiolos after a Greek mythological figure, and its planet is named Levantes, from a modern Greek word referring to easterly Mediterranean winds.[10]
Planetary system
In 2013, one planet, named HD 95086 b, was discovered on a wide orbit by direct imaging.[13] The discovery was confirmed in 2014.[14]
Besides the planet, the star is surrounded by a complex, relatively massive (0.5±0.2 M⊕) debris disk, which may consist of up to four belts (Hot, Warm, Cold and Halo) separated by gaps.[6] A small amount (1.4–13)×10−6 M⊕ of gaseous carbon monoxide was detected in the outer disk, implying a recent collisional cascade followed by cometary activity of fresh debris.[15]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (years) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| Warm debris disk | 7–10[6] AU | — | — | |||
| b / Levantes | 4.5±0.5 MJ | 51.45±4.66 | 70.98±55.01 | 0.16±0.09 | 106±49° | — |
| Cold debris disk | 106–320[6] AU | 90±3[6]° | — | |||
References
- ↑ Mâlin, Mathilde; Boccaletti, Anthony; Perrot, Clément; Baudoz, Pierre; Rouan, Daniel; Lagage, Pierre-Olivier; Waters, Rens; Güdel, Manuel et al. (2024-08-01). "Unveiling the HD 95086 system at mid-infrared wavelengths with JWST/MIRI". Astronomy & Astrophysics 690: A316. doi:10.1051/0004-6361/202450470. Bibcode: 2024A&A...690A.316M.
- ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode: 1987PASP...99..695R Constellation record for this object at VizieR.
- ↑ 3.0 3.1 3.2 3.3 3.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355. Bibcode: 2000A&A...355L..27H.
- ↑ 5.0 5.1 Meshkat, T.; Bailey, V.; Rameau, J.; Bonnefoy, M.; Boccaletti, A.; Mamajek, E. E.; Kenworthy, M.; Chauvin, G. et al. (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. doi:10.1088/2041-8205/775/2/L40. L40. Bibcode: 2013ApJ...775L..40M.
- ↑ 6.0 6.1 6.2 6.3 6.4 6.5 Chauvin, G.; Gratton, R.; Bonnefoy, M.; Lagrange, A. -M.; de Boer, J.; Vigan, A.; Beust, H.; Lazzoni, C. et al. (2018). "Investigating the young Solar System analog HD 95086 A combined HARPS and SPHERE exploration". Astronomy and Astrophysics 617. doi:10.1051/0004-6361/201732077. Bibcode: 2018A&A...617A..76C.
- ↑ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A XHIP record for this object at VizieR.
- ↑ 8.0 8.1 8.2 Desgrange, C. et al. (2022). "In-depth direct imaging and spectroscopic characterization of the young Solar System analog HD 95086". Astronomy & Astrophysics 664: A139. doi:10.1051/0004-6361/202243097. Bibcode: 2022A&A...664A.139D.
- ↑ "HD 95086". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+95086.
- ↑ 10.0 10.1 "2022 Approved Names". IAU. https://www.nameexoworlds.iau.org/2022approved-names.
- ↑ De Rosa, R. J.; Patience, J.; Wilson, P. A.; Schneider, A.; Wiktorowicz, S. J.; Vigan, A.; Marois, C.; Song, I. et al. (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, doi:10.1093/mnras/stt1932, Bibcode: 2014MNRAS.437.1216D
- ↑ "List of ExoWorlds 2022". IAU. 8 August 2022. https://www.nameexoworlds.iau.org/2022exoworlds.
- ↑ Rameau, J.; Chauvin, G.; Lagrange, A.-M.; Boccaletti, A.; Quanz, S. P.; Bonnefoy, M.; Girard, J. H.; Delorme, P. et al. (2013), "Discovery of a probable 4 − 5 Jupiter-mass exoplanet to HD 95086 by direct-imaging", The Astrophysical Journal 772 (2): L15, doi:10.1088/2041-8205/772/2/L15, Bibcode: 2013ApJ...772L..15R
- ↑ Galicher, Raphael; Rameau, Julien; Bonnefoy, Mickael; Baudino, Jean-Loup; Currie, Thayne; Boccaletti, Anthony; Chauvin, Gael; Lagrange, Anne-Marie et al. (2014), "Near-infrared detection and characterization of the exoplanet HD 95086 b with the Gemini Planet Imager", Astronomy and Astrophysics 565: L4, doi:10.1051/0004-6361/201423839, Bibcode: 2014A&A...565L...4G
- ↑ Booth, Mark; Matrà, Luca; Su, Kate Y L.; Kral, Quentin; Hales, Antonio S.; Dent, William R F.; Hughes, A Meredith; MacGregor, Meredith A. et al. (2019). "Deep ALMA Search for CO Gas in the HD 95086 Debris Disc". Monthly Notices of the Royal Astronomical Society 482 (3): 3443–3452. doi:10.1093/mnras/sty2993.
- ↑ Le Coroller, H.; Nowak, M.; Delorme, P.; Chauvin, G.; Gratton, R.; Devinat, M.; Bec-Canet, J.; Schneeberger, A. et al. (2020), "K-Stacker, an algorithm to hack the orbital parameters of planets hidden in high-contrast imaging First applications to VLT/SPHERE multi-epoch observations", Astronomy & Astrophysics A113: 639, doi:10.1051/0004-6361/202037605, Bibcode: 2020A&A...639A.113L
Coordinates:
10h 57m 03.0216s, −68° 40′ 02.4469″
