Phi1 Pavonis
  | |
| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Pavo[1] |
| Right ascension | 20h 35m 34.85007s[2] |
| Declination | −60° 34′ 54.2968″[2] |
| Apparent magnitude (V) | 4.75[1] |
| Characteristics | |
| Evolutionary stage | main sequence[2] |
| Spectral type | F0V[3] |
| U−B color index | +0.04[4] |
| B−V color index | +0.29[1] |
| Astrometry | |
| Radial velocity (Rv) | −20.0±4.2[5] km/s |
| Proper motion (μ) | RA: +69.912[2] mas/yr Dec.: −185.861[2] mas/yr |
| Parallax (π) | 35.6214±0.0982 mas[2] |
| Distance | 91.6 ± 0.3 ly (28.07 ± 0.08 pc) |
| Absolute magnitude (MV) | 2.53[1] |
| Details | |
| Mass | 1.51[6] M☉ |
| Radius | 1.76[7] R☉ |
| Luminosity | 7.8[7] L☉ |
| Surface gravity (log g) | 4.16[7] cgs |
| Temperature | 7,273[7] K |
| Rotational velocity (v sin i) | 150.0[8] km/s |
| Age | 30+230 −10[9] Myr |
| Other designations | |
| phi1 Pav, CPD−61°6492, GC 28609, HD 195627, HIP 101612, HR 7848, SAO 254823[10] | |
| Database references | |
| SIMBAD | data |
Phi1 Pavonis, latinized from φ1 Pavonis, is a single[11] star in the southern constellation of Pavo. It has a yellow-white hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.75.[1] The star is located at a distance of approximately 92 light years away based on parallax. It is drifting closer to the Sun with a radial velocity of −20 km/s.[5]
This is an ordinary F-type main-sequence star with a stellar classification of F0V.[3] It has 1.5 times the mass of the Sun[6] and 1.8 times the Sun's radius.[7] This is a young star, perhaps 30 million years old,[9] and has a high rate of spin with a projected rotational velocity of 150 km/s.[8] It is radiating 7.8 times the luminosity of the Sun from its photosphere at an effective temperature of 7,273 K.[7]
Phi1 Pavonis is a candidate debris disk star, although Gray et al. (2006) reported a non-detection of an infrared excess.[3] Nilsson et al. (2010) report a marginal detection, orbiting 74 AU from the host star with a temperature of 57 K and an estimated 3.1±1.7 times the mass of the Moon.[9]
References
- 1 2 3 4 5 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. XHIP record for this object at VizieR.
- 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- 1 2 3 Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637, S2CID 119476992
- ↑ Mermilliod, J. C. (2006). "VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991)". VizieR On-line Data Catalog: II/168. Originally Published in: Institut d'Astronomie. 2168. Bibcode:2006yCat.2168....0M.Vizier catalog entry
- 1 2 Gontcharov, G. A. (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.
- 1 2 David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv:1501.03154. Bibcode:2015ApJ...804..146D. doi:10.1088/0004-637X/804/2/146. S2CID 33401607. Vizier catalog entry
- 1 2 3 4 5 6 Stassun, Keivan G.; et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467.
- 1 2 Glebocki, R.; Gnacinski, P. (2005). "VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005)". VizieR On-line Data Catalog: III/244. Originally Published in: 2005csss...13..571G; 2005yCat.3244....0G. 3244. Bibcode:2005yCat.3244....0G. Vizier catalog entry
- 1 2 3 Nilsson, R.; et al. (July 2010). "Kuiper belts around nearby stars". Astronomy and Astrophysics. 518: 15. arXiv:1005.3215. Bibcode:2010A&A...518A..40N. doi:10.1051/0004-6361/201014444. S2CID 9703586. A40.
- ↑ "phi01 Pav". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-05-11.
- ↑ Rodriguez, David R.; Zuckerman, B. (February 2012). "Binaries among Debris Disk Stars". The Astrophysical Journal. 745 (2): 13. arXiv:1111.5618. Bibcode:2012ApJ...745..147R. doi:10.1088/0004-637X/745/2/147. S2CID 73681879. 147.
