Astronomy:Gamma Scuti
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| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Scutum |
| Right ascension | 18h 29m 11.85388s[1] |
| Declination | −14° 33′ 56.9319″[1] |
| Apparent magnitude (V) | 4.67[2] |
| Characteristics | |
| Spectral type | A2:V[3] |
| U−B color index | +0.04[4] |
| B−V color index | +0.07[4] |
| Astrometry | |
| Radial velocity (Rv) | -41.00[5] km/s |
| Proper motion (μ) | RA: +3.22[1] mas/yr Dec.: −4.02[1] mas/yr |
| Parallax (π) | 10.21 ± 0.24[1] mas |
| Distance | 319 ± 8 ly (98 ± 2 pc) |
| Absolute magnitude (MV) | −0.28[2] |
| Details | |
| Mass | 2.91[6] M☉ |
| Radius | 4.1[7] R☉ |
| Luminosity | 150[6] L☉ |
| Surface gravity (log g) | 2.09[8] cgs |
| Temperature | 9,016[6] K |
| Rotational velocity (v sin i) | 222[6] km/s |
| Age | 237[8] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Gamma Scuti, Latinized from γ Scuti, is a single,[9] white-hued star in the southern constellation of Scutum. The apparent visual magnitude of 4.67[2] indicates this is a dim star but visible to the naked eye. Based upon an annual parallax shift of 10.21 mas as seen from Earth,[1] this star is located about 319 light years from the Sun. Currently it is moving towards the Solar System at 41 km/s, which means in 2.35 million years it will pass at just 20 ly (5.519 pc) distance,[10] probably becoming the brightest star in the night sky, at magnitude −2.1, for a period.[11]
This is an A-type main-sequence star[3] with a stellar classification of A2:V.[3] At the age of 237 million years,[8] it is spinning rapidly with a projected rotational velocity of 222 km/s.[6] This is giving the star an oblate shape with a prominent equatorial bulge that is estimated to be 21% larger than the polar radius.[12] The star has an estimated 2.91[6] times the mass of the Sun and 4.1[7] times the Sun's radius. It is radiating 150 times the Sun's luminosity from its photosphere at an effective temperature of 9,016 K.[6]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V. Vizier catalog entry
- ↑ 2.0 2.1 2.2 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A. Vizier catalog entry
- ↑ 3.0 3.1 3.2 Abt, Helmut A.; Morrell, Nidia I. (1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". Astrophysical Journal Supplement 99: 135. doi:10.1086/192182. Bibcode: 1995ApJS...99..135A.
- ↑ 4.0 4.1 Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers 42 (2): 443. Bibcode: 2014JAVSO..42..443M.Vizier catalog entry
- ↑ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G.
- ↑ 6.0 6.1 6.2 6.3 6.4 6.5 6.6 Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars". Astronomy & Astrophysics 537: A120. doi:10.1051/0004-6361/201117691. Bibcode: 2012A&A...537A.120Z. Vizier catalog entry
- ↑ 7.0 7.1 Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics 352: 555–562. Bibcode: 1999A&A...352..555A. Vizier catalog entry
- ↑ 8.0 8.1 8.2 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. doi:10.1088/0004-637X/804/2/146. Bibcode: 2015ApJ...804..146D. Vizier catalog entry
- ↑ 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.
- ↑ Bailer-Jones, C. A. L. (March 2015), "Close encounters of the stellar kind", Astronomy & Astrophysics 575: 13, doi:10.1051/0004-6361/201425221, A35, Bibcode: 2015A&A...575A..35B.
- ↑ Kaler, Jim. "Gamma Scuti". http://stars.astro.illinois.edu/sow/gammasct.html. Retrieved 2017-04-21.
- ↑ van Belle, Gerard T. (March 2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review 20 (1): 51, doi:10.1007/s00159-012-0051-2, Bibcode: 2012A&ARv..20...51V.
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