| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Indus |
| Right ascension | 20h 54m 48.60278s [1] |
| Declination | −58° 27′ 14.9618″ [1] |
| Apparent magnitude (V) | 3.67 [2] |
| Characteristics | |
| Spectral type | K1II [3] or K0III [4] |
| U−B color index | +1.23 [5] |
| B−V color index | +1.250±0.015 [2] |
| Astrometry | |
| Radial velocity (Rv) | −4.9±0.7 [2] km/s |
| Proper motion (μ) |
RA: 21.06
[1]
mas/
yr Dec.: −24.75 [1] mas/ yr |
| Parallax (π) | 5.41 ± 0.73 mas [1] |
| Distance | approx. 600
ly (approx. 180 pc) |
| Absolute magnitude (MV) | −2.664 [6] |
| Details | |
| Mass | 6.7±0.4 [7] M☉ |
| Radius | 55.58+9.35 −5.02 [8] R☉ |
| Luminosity | 1,183±58 [8] L☉ |
| Surface gravity (log g) | 0.800 [9] cgs |
| Temperature | 4,541+220 −334 [8] K |
| Metallicity [Fe/H] | −0.06 [9] dex |
| Age | 53.2±10.0 [7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Beta Indi, Latinized from β Indi, is the second brightest star in the southern constellation of Indus. [10] It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 3.67. [2] The star is located approximately 600 light years from the Sun, based on parallax, but is drifting closer with a radial velocity of −5 km/s. [2]
The stellar classification of this star is K1II, [3] matching an evolved bright giant. Earlier it had been categorized as an ordinary giant with a class of K0III. [4] It is a hybrid giant with both a hot stellar corona and cool stellar winds, and is a weak X-ray source with a flux measured at (11±1)×10−14 ergs cm−1 s−1. [11] Having consumed the supply of hydrogen at its core, this star has expanded off the main sequence and now has about 56 [8] times the girth of the Sun. It is 53 million years old with 6.7 times the mass of the Sun. [7] The star is radiating 1,183 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,541 K. [8]
β Indi has a visual companion, CCDM J20548-5827B, with an apparent visual magnitude of approximately 12.5. As of 2015, it lies at an angular separation of 17.2 ″ along a position angle of 100° from the brighter component. [12]
References
- ^ a b c d e 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 e Anderson, E.; Francis, Ch. (May 2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331–346, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1975mcts.book.....H.
- ^ a b Buscombe, W. (1962), "Spectral classification of Southern fundamental stars", Mount Stromlo Observatory Mimeogram, 4: 1, Bibcode: 1962MtSOM...4....1B.
- ^ Hoffleit, D.; Warren, Jr., W. H., "HR 7986, database entry", The Bright Star Catalogue (5th Revised Ed. (Preliminary Version) ed.), CDS. ID V/50. Accessed on line September 23, 2008.
- ^ Cassatella, A.; et al. (2001), "On the Wilson-Bappu relationship in the Mg II k line", Astronomy and Astrophysics, 374 (3): 1085–1091, arXiv: astro-ph/0106070, Bibcode: 2001A&A...374.1085C, doi: 10.1051/0004-6361:20010816, S2CID 16286422
- ^ a b c Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (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 c d e 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 Soubiran, C.; et al. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv: 1004.1069, Bibcode: 2010A&A...515A.111S, doi: 10.1051/0004-6361/201014247, S2CID 118362423.
- ^ a b "bet Ind". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-20.
- ^ Ayres, Thomas R. (January 2005), "X-Rays from Hybrid Stars", The Astrophysical Journal, 618 (1): 493–501, Bibcode: 2005ApJ...618..493A, doi: 10.1086/425891, S2CID 123363660
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Indus |
| Right ascension | 20h 54m 48.60278s [1] |
| Declination | −58° 27′ 14.9618″ [1] |
| Apparent magnitude (V) | 3.67 [2] |
| Characteristics | |
| Spectral type | K1II [3] or K0III [4] |
| U−B color index | +1.23 [5] |
| B−V color index | +1.250±0.015 [2] |
| Astrometry | |
| Radial velocity (Rv) | −4.9±0.7 [2] km/s |
| Proper motion (μ) |
RA: 21.06
[1]
mas/
yr Dec.: −24.75 [1] mas/ yr |
| Parallax (π) | 5.41 ± 0.73 mas [1] |
| Distance | approx. 600
ly (approx. 180 pc) |
| Absolute magnitude (MV) | −2.664 [6] |
| Details | |
| Mass | 6.7±0.4 [7] M☉ |
| Radius | 55.58+9.35 −5.02 [8] R☉ |
| Luminosity | 1,183±58 [8] L☉ |
| Surface gravity (log g) | 0.800 [9] cgs |
| Temperature | 4,541+220 −334 [8] K |
| Metallicity [Fe/H] | −0.06 [9] dex |
| Age | 53.2±10.0 [7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Beta Indi, Latinized from β Indi, is the second brightest star in the southern constellation of Indus. [10] It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 3.67. [2] The star is located approximately 600 light years from the Sun, based on parallax, but is drifting closer with a radial velocity of −5 km/s. [2]
The stellar classification of this star is K1II, [3] matching an evolved bright giant. Earlier it had been categorized as an ordinary giant with a class of K0III. [4] It is a hybrid giant with both a hot stellar corona and cool stellar winds, and is a weak X-ray source with a flux measured at (11±1)×10−14 ergs cm−1 s−1. [11] Having consumed the supply of hydrogen at its core, this star has expanded off the main sequence and now has about 56 [8] times the girth of the Sun. It is 53 million years old with 6.7 times the mass of the Sun. [7] The star is radiating 1,183 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,541 K. [8]
β Indi has a visual companion, CCDM J20548-5827B, with an apparent visual magnitude of approximately 12.5. As of 2015, it lies at an angular separation of 17.2 ″ along a position angle of 100° from the brighter component. [12]
References
- ^ a b c d e 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 e Anderson, E.; Francis, Ch. (May 2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331–346, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1975mcts.book.....H.
- ^ a b Buscombe, W. (1962), "Spectral classification of Southern fundamental stars", Mount Stromlo Observatory Mimeogram, 4: 1, Bibcode: 1962MtSOM...4....1B.
- ^ Hoffleit, D.; Warren, Jr., W. H., "HR 7986, database entry", The Bright Star Catalogue (5th Revised Ed. (Preliminary Version) ed.), CDS. ID V/50. Accessed on line September 23, 2008.
- ^ Cassatella, A.; et al. (2001), "On the Wilson-Bappu relationship in the Mg II k line", Astronomy and Astrophysics, 374 (3): 1085–1091, arXiv: astro-ph/0106070, Bibcode: 2001A&A...374.1085C, doi: 10.1051/0004-6361:20010816, S2CID 16286422
- ^ a b c Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (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 c d e 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 Soubiran, C.; et al. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv: 1004.1069, Bibcode: 2010A&A...515A.111S, doi: 10.1051/0004-6361/201014247, S2CID 118362423.
- ^ a b "bet Ind". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-20.
- ^ Ayres, Thomas R. (January 2005), "X-Rays from Hybrid Stars", The Astrophysical Journal, 618 (1): 493–501, Bibcode: 2005ApJ...618..493A, doi: 10.1086/425891, S2CID 123363660
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920