Astronomy:HD 91312
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Ursa Major |
| Right ascension | 10h 33m 13.88880s[1] |
| Declination | 40° 25′ 32.0172″[1] |
| Apparent magnitude (V) | 4.72[2] (4.750 + 11.60)[3] |
| Characteristics | |
| Spectral type | A7IV-V[4] + M[5] |
| B−V color index | 0.222±0.013[2] |
| Astrometry | |
| Radial velocity (Rv) | 9.0±4.2[2] km/s |
| Proper motion (μ) | RA: −138.103[1] mas/yr Dec.: 3.172[1] mas/yr |
| Parallax (π) | 29.8168 ± 0.2283[1] mas |
| Distance | 109.4 ± 0.8 ly (33.5 ± 0.3 pc) |
| Absolute magnitude (MV) | 2.02[2] |
| Orbit[6] | |
| Period (P) | 292.56 d |
| Semi-major axis (a) | ≥1.56×107 km |
| Eccentricity (e) | 0.30 |
| Periastron epoch (T) | 2,419,108 JD |
| Argument of periastron (ω) (secondary) | 311° |
| Semi-amplitude (K1) (primary) | 14.5 km/s |
| Details | |
| A | |
| Mass | 1.83[7] M☉ |
| Radius | 1.97+0.07 −0.02[1] R☉ |
| Luminosity | 11.965+0.107 −0.088[1] L☉ |
| Surface gravity (log g) | 4.0[8] cgs |
| Temperature | 7,648+34 −472[1] K |
| Rotational velocity (v sin i) | 119[8] km/s |
| Age | ~200[7] Myr |
| B | |
| Mass | 0.337+0.042 −0.044[5] M☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 91312 is a multiple star system in the northern circumpolar constellation Ursa Major. Faintly visible to the naked eye, it is the brightest star of Ursa Major without Flamsteed designation with a combined apparent visual magnitude of 4.72.[2] The system is located at a distance of 109 light-years from the Sun based on parallax. The radial velocity is poorly constrained, but it appears to be drifting further away at a rate of ~9 km/s.[2]
This was identified as a visual binary by John Herschel in 1831.[3] The pair have an angular separation of 23″, equivalent to a linear projected separation of ~796 astronomical unit|AU. Variations in the radial velocity as well as direct imaging, indicate the presence of a low-mass stellar companion. This companion is an early-to-mid red dwarf, and orbits the primary on an edge-on orbit with a semi-major axis of 9.7 au.[5] This is a young system with an age of around 200 million years.[7] It display an infrared excess from a circumstellar disk of dusty debris.[10] It has a mean temperature of 35 K and is orbiting 218.1 AU from the inner pair.[11]
This star is relatively bright, but it was rarely included in old catalogues. Catalogues and atlases it was not included in are, for example, those by Ptolemy and all its derivatives and translations (by as-Sufi, al-Biruni, Ulugh Beg, Copernicus, Clavius, etc.), Tycho Brahe, de Houtman, Bayer, Kepler, Schiller, Halley, Flamsteed (as well as published by Carolina Herschel in 1798 catalogue of stars, observed by Flamsteed, but not inserted in his British Catalogue) and Bradley. Catalogues and atlases it was included in are those by Hevelius (1690) (65th in Ursa Major, designated In Ungula sinistri Pedis poster. trium sequens) and Bode (1801) (number 157 of Ursa Major). Bode used extended Bayer designations for some stars, and HD 91312 also was assigned designation "w", whereas original Bayer designations for Ursa Major stars are all Greek letters and Latin letters from "A" to "h".
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Mason, B. D. et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal 122 (6): 3466–3471, doi:10.1086/323920, Bibcode: 2001AJ....122.3466M.
- ↑ Gray, R. O.; Garrison, R. F. (1989), "The Late A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation", The Astrophysical Journal Supplement Series 70: 623, doi:10.1086/191349, Bibcode: 1989ApJS...70..623G.
- ↑ 5.0 5.1 5.2 Chilcote, Jeffrey; Tobin, Taylor; Currie, Thayne; Brandt, Timothy D.; Groff, Tyler D.; Kuzuhara, Masayuki; Guyon, Olivier; Lozi, Julien et al. (2021). "SCExAO/CHARIS Direct Imaging of a Low-mass Companion at a Saturn-like Separation from an Accelerating Young A7 Star". The Astronomical Journal 162 (6): 251. doi:10.3847/1538-3881/ac29ba. Bibcode: 2021AJ....162..251C.
- ↑ Batten, A. H. et al. (1978), "Seventh catalogue of the orbital elements of spectroscopic binary systems.", Publications of the Dominion Astrophysical Observatory Victoria 15: 121−295, Bibcode: 1978PDAO...15..121B. See No. 431
- ↑ 7.0 7.1 7.2 Borgniet, Simon; Lagrange, Anne-Marie; Meunier, Nadège; Galland, Franck; Arnold, Luc; Astudillo-Defru, Nicola; Beuzit, Jean-Luc; Boisse, Isabelle et al. (2019), "Extrasolar planets and brown dwarfs around AF-type stars. X. The SOPHIE northern sample. Combining the SOPHIE and HARPS surveys to compute the close giant planet mass-period distribution around AF-type stars", Astronomy & Astrophysics 621: A87, doi:10.1051/0004-6361/201833431
- ↑ 8.0 8.1 Draper, Zachary H. et al. (April 2018), "A-type Stellar Abundances: A Corollary to Herschel Observations of Debris Disks", The Astrophysical Journal 857 (2): 16, doi:10.3847/1538-4357/aab1fd, 93, Bibcode: 2018ApJ...857...93D.
- ↑ "HD 91312". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+91312.
- ↑ Sadakane, K.; Nishida, M. (July 1986), "Twelve additional "Vega-like" stars", Publications of the Astronomical Society of the Pacific 98: 685–689, doi:10.1086/131813, Bibcode: 1986PASP...98..685S.
- ↑ Cotten, Tara H.; Song, Inseok (July 2016), "A Comprehensive Census of Nearby Infrared Excess Stars", The Astrophysical Journal Supplement Series 225 (1): 24, doi:10.3847/0067-0049/225/1/15, 15, Bibcode: 2016ApJS..225...15C.
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