Astronomy:HR 2096
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Short description: Star in the constellation Auriga
| Observation data {{#ifeq:J2000|J2000.0 (ICRS)|Epoch J2000.0 Equinox J2000.0 (ICRS)| Epoch J2000 [[Astronomy:Equinox (celestial coordinates)|Equinox J2000}} | |
|---|---|
| Constellation | Auriga[1] |
| A | |
| Right ascension | 06h 00m 18.8979s[2] |
| Declination | +44° 35′ 31.247″[2] |
| Apparent magnitude (V) | 6.20[3] |
| B | |
| Right ascension | 06h 00m 18.8991s[4] |
| Declination | +44° 35′ 31.246″[4] |
| Apparent magnitude (V) | 6.233 |
| Characteristics | |
| Spectral type | K2III[5] |
| Astrometry | |
| Radial velocity (Rv) | 1.7 km/s |
| Proper motion (μ) | RA: -31.17 mas/yr Dec.: -38.71 mas/yr |
| Parallax (π) | 8.94 ± 0.82 mas |
| Distance | 360 ± 30 ly (110 ± 10 pc) |
| Absolute magnitude (MV) | 7.388 |
| Details | |
| Mass | 0.8 M☉ |
| Radius | 0.9 R☉ |
| Luminosity | 0.4 L☉ |
| Temperature | 3,500–5,000 K |
| Other designations | |
| Database references | |
| SIMBAD | data |
HR 2096, also known as HD 40325 is a double star in the constellation Auriga. It is composed of two ageing orange giants of spectral types K0III and K2III.[6] It is not a member of any known moving group of stars.[7]
References
- ↑ 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.
- ↑ 2.0 2.1 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.
- ↑ Oja, T. (1991). "UBV photometry of stars whose positions are accurately known. VI.". Astronomy and Astrophysics Supplement Series 89: 415. Bibcode: 1991A&AS...89..415O.
- ↑ 4.0 4.1 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.
- ↑ Stephenson, C. B. (1960). "A study of visual binaries having primaries above the main sequence". The Astronomical Journal 65: 60. doi:10.1086/108191. Bibcode: 1960AJ.....65...60S.
- ↑ Stephenson, C. B. (1960). "A study of visual binaries having primaries above the main sequence". Astronomical Journal 65: 60–79. doi:10.1086/108191. Bibcode: 1960AJ.....65...60S.
- ↑ Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics 430: 165–186. doi:10.1051/0004-6361:20041272. Bibcode: 2005A&A...430..165F.
Components
| NAME | Right ascension | Declination | Apparent magnitude (V) | Spectral type | Database references |
|---|---|---|---|---|---|
| ADS 4576 C | 06h 00m 17.5327s | +44° 36' 03.07 | 10.2 | Simbad |
 |  |
