| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aries |
| Right ascension | 01h 50m 08.56984s [1] |
| Declination | +22° 16′ 31.2100″ [1] |
| Apparent magnitude (V) | 5.86 [2] (6.4/7.2) [3] |
| Characteristics | |
| Spectral type | K1 III + A6 V [3] |
| U−B color index | +0.5 [2] |
| B−V color index | +0.74 [2] |
| Astrometry | |
| Radial velocity (Rv) | 6.95±0.13 [4] km/s |
| Proper motion (μ) |
RA: –16.52
[1]
mas/
yr Dec.: –8.25 [1] mas/ yr |
| Parallax (π) | 5.57 ± 0.75 mas [1] |
| Distance | approx. 590
ly (approx. 180 pc) |
| Absolute magnitude (MV) | −0.39 [4] |
| Details | |
| Luminosity | 141.51 [4] L☉ |
| Other designations | |
| 1 Ari A: HD 11154. | |
| 1 Ari B: HD 11155. | |
| Database references | |
| SIMBAD | data |
1 Arietis is a double star [3] in the northern constellation of Aries. 1 Arietis is the Flamsteed designation. The pair have a combined visual magnitude of 5.86, [2] making it faintly visible to the naked eye. Based upon an annual parallax shift of 5.57 mas, [1] the distance to the two stars is approximately 590 light-years (180 parsecs). As of 2016, the secondary had an angular separation of 2.90 ″ along a position angle of 165° from the primary. [6] They are moving further from the Earth with a heliocentric radial velocity of +7 km/s. [4]
The brighter star, designated component A, is a magnitude 6.40 giant star with a stellar classification of K1 III. The companion star, component B, is a magnitude 7.20 A-type main sequence star with a classification of A6 V. [3] Helmut Abt (1985) had this star classified as A3 IV, [7] matching a more evolved subgiant.
- ^ a b c d e f van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID 18759600.
- ^ a b c d Nicolet, B. (1978). "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System". Astronomy and Astrophysics Supplement Series. 34: 1–49. Bibcode: 1978A&AS...34....1N.
- ^ a b c d Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
- ^ a b c d Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ "* 1 Ari". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-07-18.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920.
- ^ Abt, H. A. (September 1985), "Visual multiples. VIII - 1000 MK types", Astrophysical Journal Supplement Series, 59: 95–112, Bibcode: 1985ApJS...59...95A, doi: 10.1086/191064
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aries |
| Right ascension | 01h 50m 08.56984s [1] |
| Declination | +22° 16′ 31.2100″ [1] |
| Apparent magnitude (V) | 5.86 [2] (6.4/7.2) [3] |
| Characteristics | |
| Spectral type | K1 III + A6 V [3] |
| U−B color index | +0.5 [2] |
| B−V color index | +0.74 [2] |
| Astrometry | |
| Radial velocity (Rv) | 6.95±0.13 [4] km/s |
| Proper motion (μ) |
RA: –16.52
[1]
mas/
yr Dec.: –8.25 [1] mas/ yr |
| Parallax (π) | 5.57 ± 0.75 mas [1] |
| Distance | approx. 590
ly (approx. 180 pc) |
| Absolute magnitude (MV) | −0.39 [4] |
| Details | |
| Luminosity | 141.51 [4] L☉ |
| Other designations | |
| 1 Ari A: HD 11154. | |
| 1 Ari B: HD 11155. | |
| Database references | |
| SIMBAD | data |
1 Arietis is a double star [3] in the northern constellation of Aries. 1 Arietis is the Flamsteed designation. The pair have a combined visual magnitude of 5.86, [2] making it faintly visible to the naked eye. Based upon an annual parallax shift of 5.57 mas, [1] the distance to the two stars is approximately 590 light-years (180 parsecs). As of 2016, the secondary had an angular separation of 2.90 ″ along a position angle of 165° from the primary. [6] They are moving further from the Earth with a heliocentric radial velocity of +7 km/s. [4]
The brighter star, designated component A, is a magnitude 6.40 giant star with a stellar classification of K1 III. The companion star, component B, is a magnitude 7.20 A-type main sequence star with a classification of A6 V. [3] Helmut Abt (1985) had this star classified as A3 IV, [7] matching a more evolved subgiant.
- ^ a b c d e f van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID 18759600.
- ^ a b c d Nicolet, B. (1978). "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System". Astronomy and Astrophysics Supplement Series. 34: 1–49. Bibcode: 1978A&AS...34....1N.
- ^ a b c d Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv: 0806.2878. Bibcode: 2008MNRAS.389..869E. doi: 10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
- ^ a b c d Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ "* 1 Ari". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-07-18.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920.
- ^ Abt, H. A. (September 1985), "Visual multiples. VIII - 1000 MK types", Astrophysical Journal Supplement Series, 59: 95–112, Bibcode: 1985ApJS...59...95A, doi: 10.1086/191064