Alpha Indi
| |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Indus |
| Right ascension | 20h 37m 34.03201s[1] |
| Declination | –47° 17′ 29.4026″[1] |
| Apparent magnitude (V) | 3.11[2] |
| Astrometry | |
| Radial velocity (Rv) | −1.3[3] km/s |
| Proper motion (μ) | RA: +49.24[1] mas/yr Dec.: +66.53[1] mas/yr |
| Parallax (π) | 33.17 ± 0.18[1] mas |
| Distance | 98.3 ± 0.5 ly (30.1 ± 0.2 pc) |
| Absolute magnitude (MV) | 0.65[4] |
| Characteristics | |
| Spectral type | K0 III–IV[5] |
| U−B color index | +0.79[2] |
| B−V color index | +1.00[2] |
| Details | |
| Mass | 2.0[4] M☉ |
| Radius | 12[6] R☉ |
| Surface gravity (log g) | 3.00[7] cgs |
| Temperature | 4,893[7] K |
| Metallicity [Fe/H] | +0.03[7] dex |
| Age | 1[4] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Alpha Indi (α Ind, α Indi) is a third magnitude giant star in the constellation Indus, located about 98 light years from the Earth.[1] The stellar classification of this star is K0 III-IV,[5] so it has exhausted the hydrogen at its core and evolved away from the main sequence. It has about double the mass of the Sun and is an estimated billion years old.[4] As a giant star it has expanded to about 12 times the radius of the Sun.[6] The effective temperature of the photosphere is 4,893 K,[7] giving it the characteristic orange hue of a K-type star.[9] It may have two nearby M-type companion stars, which are located at least 2,000 Astronomical Units from the primary.[10]
In China, this star is called Pe Sze where it also was known as the Persian, a title from the Jesuit missionaries.[11] The term Pe Sze is from the name of asterism 波斯 (Bō Sī, English: Persia). In Chinese astronomy, consequently, α Indi itself is known as 波斯二 (Bō Sī èr, English: the Second Star of Persia)[12]
References
- 1 2 3 4 5 6 van Leeuwen, F. (November 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.
- 1 2 3 Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99), Bibcode:1966CoLPL...4...99J
- ↑ Evans, D. S. (June 20–24, 1966), "The revision of the general catalogue of radial velocities", in Batten, Alan Henry; Heard, John Frederick, Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30 30, University of Toronto: International Astronomical Union, p. 57, Bibcode:1967IAUS...30...57E
- 1 2 3 4 Thorén, P.; Edvardsson, B.; Gustafsson, B. (October 2004), "Subgiants as probes of galactic chemical evolution", Astronomy and Astrophysics 425: 187–206, arXiv:astro-ph/0407260, Bibcode:2004A&A...425..187T, doi:10.1051/0004-6361:20040421
- 1 2 Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I", The Astronomical Journal 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637
- 1 2 Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics 367: 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451
- 1 2 3 4 Gratton, R. G.; Ortolani, S. (November 1986), "The forbidden O/Fe ratio in metal-poor late-type stars", Astronomy and Astrophysics 169 (1-2): 201–207, Bibcode:1986A&A...169..201G
- ↑ "alf Ind -- Star in double system", SIMBAD (Centre de Données astronomiques de Strasbourg), retrieved 2011-12-12
- ↑ "The Colour of Stars", Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004, retrieved 2012-01-16
- ↑ Kaler, James B., "THE PERSIAN (Alpha Indi)", Stars (University of Illinois), retrieved 2011-12-23
- ↑ Star Name - R.H.Allen p. 246
- ↑ (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 30 日)
| ||||||||||||||||||||||||||||||