Astronomy:Phi Boötis
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| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Boötes |
| Right ascension | 15h 37m 49.598s[1] |
| Declination | +40° 21′ 12.36″[1] |
| Apparent magnitude (V) | +5.24[2] |
| Characteristics | |
| Evolutionary stage | red clump[3] |
| Spectral type | G7 III-IV Fe-2[4] |
| U−B color index | +0.53[2] |
| B−V color index | +0.88[2] |
| Astrometry | |
| Radial velocity (Rv) | −10.62±0.30[5] km/s |
| Proper motion (μ) | RA: +61.380[1] mas/yr Dec.: +59.791[1] mas/yr |
| Parallax (π) | 18.5752 ± 0.0555[1] mas |
| Distance | 175.6 ± 0.5 ly (53.8 ± 0.2 pc) |
| Absolute magnitude (MV) | +1.67[6] |
| Details | |
| Mass | 1.43[6] M☉ |
| Radius | 5[5] R☉ |
| Luminosity | 17[5] L☉ |
| Surface gravity (log g) | 2.82±0.14[7] cgs |
| Temperature | 4,945±57[7] K |
| Metallicity [Fe/H] | −0.51±0.06[7] dex |
| Rotational velocity (v sin i) | 0.0[5] km/s |
| Age | 3.16[6] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Phi Boötis is a single,[9] yellow-hued star in the northern constellation of Boötes. Its name is a Bayer designation that is Latinized from φ Boötis, and abbreviated Phi Boo or φ Boo. This star is dimly visible to the naked eye with an apparent visual magnitude of +5.24.[2] Based upon an annual parallax shift of 18.58 mas as seen from the Earth,[1] it is located 176 light-years (54 pc) from the Sun. At that distance, the visual magnitude is diminished by an extinction of 0.09 due to interstellar dust.[6] It is moving closer to the Sun with a radial velocity of −10.6 km/s.[5]
The stellar classification of Phi Boötis is G7 III-IV Fe-2,[4] which would suggest it is an evolving G-type star that shows spectral traits of both a subgiant and a giant star. However, Alves (2000) has it listed as a member of the so-called "red clump", indicating that it is an aging giant star that is generating energy through helium fusion at its core.[3] The 'Fe-2' suffix notation in its class means that it displays a significant underabundance of iron in its spectrum. Around three billion years old,[6] Phi Boötis has an estimated 1.43[6] times the mass of the Sun and 5[5] times the Sun's radius. It is radiating 17[5] times the Sun's luminosity from its enlarged photosphere at an effective temperature of about 4,945 K.[7]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940. Gaia DR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode: 1966CoLPL...4...99J.
- ↑ 3.0 3.1 Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal 539 (2): 732–741, doi:10.1086/309278, Bibcode: 2000ApJ...539..732A.
- ↑ 4.0 4.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", The Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode: 1989ApJS...71..245K.
- ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 Massarotti, Alessandro et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal 135 (1): 209–231, doi:10.1088/0004-6256/135/1/209, Bibcode: 2008AJ....135..209M.
- ↑ 6.0 6.1 6.2 6.3 6.4 6.5 Takeda, Yoichi et al. (August 2008), "Stellar Parameters and Elemental Abundances of Late-G Giants", Publications of the Astronomical Society of Japan 60 (4): 781–802, doi:10.1093/pasj/60.4.781, Bibcode: 2008PASJ...60..781T.
- ↑ 7.0 7.1 7.2 7.3 Prugniel, Ph. et al. (2011), "The atmospheric parameters and spectral interpolator for the MILES stars", Astronomy & Astrophysics 531: A165, doi:10.1051/0004-6361/201116769, Bibcode: 2011A&A...531A.165P.
- ↑ "phi Boo". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=phi+Boo.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
References
- Hoffleit (1991), "HR 5823", Bright Star Catalogue, http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%205823, retrieved 2017-09-11.
- "phi Boo", Aladin previewer (Centre de Données astronomiques de Strasbourg), http://aladin.u-strasbg.fr/AladinPreview?-c=15+37+49.5973%2B40+21+12.358&ident=*+phi+Boo&submit=Aladin+previewer, retrieved 2017-09-11.
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