| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lupus |
| Right ascension | 15h 14m 37.32104s [1] |
| Declination | −31° 31′ 08.8434″ [1] |
| Apparent magnitude (V) | 4.90 [2] |
| Characteristics | |
| Spectral type | F1 III [3] or F0 Ib-II [4] |
| U−B color index | +0.26 [2] |
| B−V color index | 0.37 [5] |
| Astrometry | |
| Radial velocity (Rv) | −22.80 [6] km/s |
| Proper motion (μ) |
RA: −9.873
[1]
mas/
yr Dec.: –0.892 [1] mas/ yr |
| Parallax (π) | 1.8055 ± 0.1876 mas [1] |
| Distance | approx. 1,800
ly (approx. 550 pc) |
| Absolute magnitude (MV) | −3.93 [7] |
| Details | |
| Mass | 6.9±0.1 [8] M☉ |
| Radius | 41.3+2.2 −1.7 [1] R☉ |
| Luminosity | 2,900 [9] L☉ |
| Temperature | 6,867 [6] K |
| Rotational velocity (v sin i) | 3.9±0.2 [5] km/s |
| Age | 47.1±3.8 [8] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
1 Lupi is a solitary [11] giant star in the southern constellation of Lupus. It has the Bayer designation i Lupi; 1 Lupi is the Flamsteed designation. The apparent visual magnitude is 4.90, [2] which indicates it is faintly visible to the naked eye. Based on parallax measurements, this star is approximately 1,800 light-years from the Sun. [1] It is moving closer to the Earth with a heliocentric radial velocity of −23 km/s. [6]
Houk (1978) assigned the spectral classification of this star as F1III, [3] which suggests it is an F-type (yellow-white) star that has evolved away from the main sequence and expanded into a giant. However, Gray et al. (2001) found a class of F0 Ib-II, [4] matching a supergiant/ bright giant star. It has a mass around seven times that of the Sun [8] and has expanded to 41 [1] times the Sun's radius. The star is radiating 2,900 [9] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 6,867 K. [6] The estimated age of the star is around 47 million years. [8]
- ^ a b c d e f g h Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode: 1986EgUBV........0M.
- ^ a b Houk, N. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ^ a b Gray, R. O.; et al. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal, 121 (4): 2148–2158, Bibcode: 2001AJ....121.2148G, doi: 10.1086/319956.
- ^ a b Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv: 1204.2459, Bibcode: 2012A&A...542A.116A, doi: 10.1051/0004-6361/201118724, S2CID 53666672.
- ^ a b c d Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv: 1606.08053, Bibcode: 2006AstL...32..759G, doi: 10.1134/S1063773706110065, S2CID 119231169.
- ^ 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.
- ^ a b c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv: 1007.4883, Bibcode: 2011MNRAS.410..190T, doi: 10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ "i Lup -- Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2016-03-07.
- ^ Eggleton, P. P.; Tokovinin, A. A. (September 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.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lupus |
| Right ascension | 15h 14m 37.32104s [1] |
| Declination | −31° 31′ 08.8434″ [1] |
| Apparent magnitude (V) | 4.90 [2] |
| Characteristics | |
| Spectral type | F1 III [3] or F0 Ib-II [4] |
| U−B color index | +0.26 [2] |
| B−V color index | 0.37 [5] |
| Astrometry | |
| Radial velocity (Rv) | −22.80 [6] km/s |
| Proper motion (μ) |
RA: −9.873
[1]
mas/
yr Dec.: –0.892 [1] mas/ yr |
| Parallax (π) | 1.8055 ± 0.1876 mas [1] |
| Distance | approx. 1,800
ly (approx. 550 pc) |
| Absolute magnitude (MV) | −3.93 [7] |
| Details | |
| Mass | 6.9±0.1 [8] M☉ |
| Radius | 41.3+2.2 −1.7 [1] R☉ |
| Luminosity | 2,900 [9] L☉ |
| Temperature | 6,867 [6] K |
| Rotational velocity (v sin i) | 3.9±0.2 [5] km/s |
| Age | 47.1±3.8 [8] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
1 Lupi is a solitary [11] giant star in the southern constellation of Lupus. It has the Bayer designation i Lupi; 1 Lupi is the Flamsteed designation. The apparent visual magnitude is 4.90, [2] which indicates it is faintly visible to the naked eye. Based on parallax measurements, this star is approximately 1,800 light-years from the Sun. [1] It is moving closer to the Earth with a heliocentric radial velocity of −23 km/s. [6]
Houk (1978) assigned the spectral classification of this star as F1III, [3] which suggests it is an F-type (yellow-white) star that has evolved away from the main sequence and expanded into a giant. However, Gray et al. (2001) found a class of F0 Ib-II, [4] matching a supergiant/ bright giant star. It has a mass around seven times that of the Sun [8] and has expanded to 41 [1] times the Sun's radius. The star is radiating 2,900 [9] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 6,867 K. [6] The estimated age of the star is around 47 million years. [8]
- ^ a b c d e f g h Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode: 1986EgUBV........0M.
- ^ a b Houk, N. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ^ a b Gray, R. O.; et al. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal, 121 (4): 2148–2158, Bibcode: 2001AJ....121.2148G, doi: 10.1086/319956.
- ^ a b Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv: 1204.2459, Bibcode: 2012A&A...542A.116A, doi: 10.1051/0004-6361/201118724, S2CID 53666672.
- ^ a b c d Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv: 1606.08053, Bibcode: 2006AstL...32..759G, doi: 10.1134/S1063773706110065, S2CID 119231169.
- ^ 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.
- ^ a b c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv: 1007.4883, Bibcode: 2011MNRAS.410..190T, doi: 10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ "i Lup -- Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2016-03-07.
- ^ Eggleton, P. P.; Tokovinin, A. A. (September 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.