Fomalhaut
Appearance
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Piscis Austrinus (Fomalhaut A+B), Aquarius (Fomalhaut C) |
| Fomalhaut | |
| Richt ascension | 22h 57m 39.0465s[1] |
| Declination | −29° 37′ 20.050″[1] |
| Apparent magnitude (V) | 1.16 |
| TW Piscis Austrini | |
| Richt ascension | 22h 56m 24.05327s[1] |
| Declination | −31° 33′ 56.0351″[1] |
| Apparent magnitude (V) | 6.48[2] |
| LP 876-10 | |
| Richt ascension | 22h 48m 04.47s[3] |
| Declination | −24° 22′ 07.5″[3] |
| Apparent magnitude (V) | 12.618[3] |
| Chairactereestics | |
| Spectral type | A3 V / K5Vp / M4V[3][4] |
| U−B colour index | 0.08 / 1.02 / ?[5] |
| B−V colour index | 0.09 / 1.10 / 1.683[3][5] |
| Variable teep | None / BY Draconis / ? |
| Astrometry | |
| Fomalhaut | |
| Radial velocity (Rv) | +6.5 km/s |
| Proper motion (μ) | RA: +328.95[1] mas/yr Dec.: −164.67[1] mas/yr |
| Parallax (π) | 129.81 ± 0.47[1] mas |
| Distance | 25.13 ± 0.09 ly (7.70 ± 0.03 pc) |
| Absolute magnitude (MV) | 1.72[6] |
| TW Piscis Austrini | |
| Radial velocity (Rv) | +6[2] km/s |
| Proper motion (μ) | RA: −331.11[1] mas/yr Dec.: −158.98[1] mas/yr |
| Parallax (π) | 131.42 ± 0.62[1] mas |
| Distance | 24.8 ± 0.1 ly (7.61 ± 0.04 pc) |
| Absolute magnitude (MV) | 7.08[6] |
| Details | |
| Fomalhaut | |
| Mass | 1.92±0.02[6] M☉ |
| Radius | 1.842±0.019[6] R☉ |
| Luminosity | 16.63±0.48[6] L☉ |
| Surface gravity (log g) | 4.21[7] cgs |
| Temperatur | 8,590[6] K |
| Metallicity [Fe/H] | −0.03[8] tae −0.34[9] dex |
| Rotational velocity (v sin i) | 93[7] km/s |
| Age | (4.4±0.4)×108[6] years |
| TW Piscis Austrini | |
| Mass | 0.725 ± 0.036[4] M☉ |
| Radius | 0.629 ± 0.051[4] R☉ |
| Luminosity | 0.19[6] L☉ |
| Temperatur | 4,711 ± 134[4] K |
| Rotational velocity (v sin i) | 2.93[4] km/s |
| Age | 4.4 × 108[6] years |
| Ither designations | |
| Fomalhaut: α Piscis Austrini, α PsA, Alpha PsA, 24 Piscis Austrini, CPD −30° 6685, FK5 867, Gl 881, HD 216956, HIP 113368, HR 8728, SAO 191524 | |
| TW Piscis Austrini: Fomalhaut B, TW PsA, Gl 879, HR 8721, CD -32°17321, HD 216803, LTT 9283, GCTP 5562.00, SAO 214197, CP(D)-32 6550, HIP 113283 | |
| LP 876-10: Fomalhaut C, 2MASS J22480446-2422075, NLTT 54872, GSC 06964-01226 | |
| Database references | |
| Fomalhaut | |
| SIMBAD | data |
| Exoplanet Archive | data |
| ARICNS | data |
| Extrasolar Planets Encyclopaedia | data |
| TW Piscis Austrini | |
| SIMBAD | data |
| ARICNS | data |
Fomalhaut (Alpha Piscis Austrini, Alpha PsA, α Piscis Austrini, α PsA) is the brichtest starn in the constellation Piscis Austrinus an ane o the brichtest starns in the sky.
References
[eedit | edit soorce]- 1 2 3 4 5 6 7 8 9 10 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 "V* TW PsA -- Variable of BY Dra type". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 20 Januar 2010.
- 1 2 3 4 5 "LP 876-10 -- Double or multiple star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 30 Julie 2014.
- 1 2 3 4 5 Demory, B.-O.; et al. (October 2009), "Mass-radius relation of low and very low-mass stars revisited with the VLTI", Astronomy and Astrophysics, 505 (1): 205–215, arXiv:0906.0602, Bibcode:2009A&A...505..205D, doi:10.1051/0004-6361/200911976
- 1 2 Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99). Bibcode:1966CoLPL...4...99J.CS1 maint: multiple names: authors leet (link)
- 1 2 3 4 5 6 7 8 9 Mamajek, E.E. (August 2012). "On the Age and Binarity of Fomalhaut". Astrophysical Journal Letters. 754 (2): L20. arXiv:1206.6353. Bibcode:2012ApJL..754...20M. doi:10.1088/2041-8205/754/2/L20.
- 1 2 Di Folco, E.; Thévenin, F.; Kervella, P.; Domiciano de Souza, A.; Coudé du Foresto, V.; Ségransan, D.; Morel, P. (November 2004). "VLTI near-IR interferometric observations of Vega-like stars. Radius and age of α PsA, β Leo, β Pic, ɛ Eri and τ Cet". Astronomy and Astrophysics. 426 (2): 601–617. Bibcode:2004A&A...426..601D. doi:10.1051/0004-6361:20047189.CS1 maint: multiple names: authors leet (link) This paper lists [Fe/H] = −0.10 dex.
- ↑ Dunkin, S. K.; Barlow, M. J.; Ryan, Sean G.; Barlow; Ryan (Apryle 1997). "High-resolution spectroscopy of Vega-like stars - I. Effective temperatures, gravities and photospheric abundances". Monthly Notices of the Royal Astronomical Society. 286 (3): 604–616. Bibcode:1997MNRAS.286..604D. doi:10.1093/mnras/286.3.604.CS1 maint: multiple names: authors leet (link) This paper lists [Fe/H] = −0.03 dex.
- ↑ Saffe, C.; Gómez, M.; Pintado, O.; González, E. (October 2008). "Spectroscopic metallicities of Vega-like stars". Astronomy and Astrophysics. 490 (1): 297–305. arXiv:0805.3936. Bibcode:2008A&A...490..297S. doi:10.1051/0004-6361:200810260.CS1 maint: multiple names: authors leet (link) This paper lists [Fe/H] = −0.34 dex.
Categeries:
- Fomalhaut
- Triple starn seestems
- Bayer objects
- Flamsteed objects
- Piscis Austrinus
- Variable starns
- A-teep main-sequence starns
- Arabic wirds an phrases
- Circumstellar disks
- Starns wi proper names
- Castor Moving Group
- Henry Draper Catalogue objects
- Hipparcos objects
- HR objects
- Planetary seestems
- Multi-starn planetary seestems