  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pavo |
| Right ascension | 20h 35m 34.84931s [1] |
| Declination | −60° 34′ 54.3103″ [1] |
| Apparent magnitude (V) | 4.75 [2] |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | F0V [3] |
| U−B color index | +0.04 [4] |
| B−V color index | +0.29 [2] |
| Astrometry | |
| Radial velocity (Rv) | −20.0±4.2 [5] km/s |
| Proper motion (μ) |
RA: +70.271
[1]
mas/
yr Dec.: −184.963 [1] mas/ yr |
| Parallax (π) | 35.3436 ± 0.2300 mas [1] |
| Distance | 92.3 ± 0.6
ly (28.3 ± 0.2 pc) |
| Absolute magnitude (MV) | 2.53 [2] |
| Details | |
| Mass | 1.51 [6] M☉ |
| Radius | 1.83+0.15 −0.09 [1] R☉ |
| Luminosity | 8.17±0.06 [1] L☉ |
| Temperature | 7,209+190 −281 [1] K |
| Rotational velocity (v sin i) | 150.0 [7] km/s |
| Age | 30+230 −10 [8] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Phi1 Pavonis, latinized from φ1 Pavonis, is a single [10] 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. [2] 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 [6] times the mass of the Sun and 1.8 [1] times the Sun's radius. This is a young star, perhaps 30 [8] million years old, and has a high rate of spin with a projected rotational velocity of 150 km/s. [7] It is radiating 8.2 [1] times the luminosity of the Sun from its photosphere at an effective temperature of 7,209 K. [1]
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. [8]
References
- ^ a b c d e f g h i j k 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 d 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. Vizier catalog entry
- ^ a b c 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
- ^ a b 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.
- ^ a b 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
- ^ a b 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
- ^ a b c 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.
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| Galaxies |
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| |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pavo |
| Right ascension | 20h 35m 34.84931s [1] |
| Declination | −60° 34′ 54.3103″ [1] |
| Apparent magnitude (V) | 4.75 [2] |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | F0V [3] |
| U−B color index | +0.04 [4] |
| B−V color index | +0.29 [2] |
| Astrometry | |
| Radial velocity (Rv) | −20.0±4.2 [5] km/s |
| Proper motion (μ) |
RA: +70.271
[1]
mas/
yr Dec.: −184.963 [1] mas/ yr |
| Parallax (π) | 35.3436 ± 0.2300 mas [1] |
| Distance | 92.3 ± 0.6
ly (28.3 ± 0.2 pc) |
| Absolute magnitude (MV) | 2.53 [2] |
| Details | |
| Mass | 1.51 [6] M☉ |
| Radius | 1.83+0.15 −0.09 [1] R☉ |
| Luminosity | 8.17±0.06 [1] L☉ |
| Temperature | 7,209+190 −281 [1] K |
| Rotational velocity (v sin i) | 150.0 [7] km/s |
| Age | 30+230 −10 [8] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Phi1 Pavonis, latinized from φ1 Pavonis, is a single [10] 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. [2] 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 [6] times the mass of the Sun and 1.8 [1] times the Sun's radius. This is a young star, perhaps 30 [8] million years old, and has a high rate of spin with a projected rotational velocity of 150 km/s. [7] It is radiating 8.2 [1] times the luminosity of the Sun from its photosphere at an effective temperature of 7,209 K. [1]
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. [8]
References
- ^ a b c d e f g h i j k 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 d 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. Vizier catalog entry
- ^ a b c 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
- ^ a b 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.
- ^ a b 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
- ^ a b 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
- ^ a b c 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.
| Stars |
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| Galaxies |
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