22 Scorpii
  | |
| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Scorpius[1] |
| Right ascension | 16h 30m 12.47527s[2] |
| Declination | −25° 06′ 54.7966″[2] |
| Apparent magnitude (V) | 4.78[3] |
| Characteristics | |
| Evolutionary stage | main sequence[2] |
| Spectral type | B3 V[4] |
| Astrometry | |
| Proper motion (μ) | RA: −4.192[2] mas/yr Dec.: −26.975[2] mas/yr |
| Parallax (π) | 7.9402±0.1848 mas[2] |
| Distance | 411 ± 10 ly (126 ± 3 pc) |
| Absolute magnitude (MV) | −0.72[1] |
| Details | |
| Mass | 4.4[5] M☉ |
| Radius | 3.4[2] R☉ |
| Luminosity | 601[5] L☉ |
| Surface gravity (log g) | 4.5[6] cgs |
| Temperature | 16,683[5] K |
| Metallicity [Fe/H] | 0.66[2] dex |
| Rotational velocity (v sin i) | 169±4[3] km/s |
| Age | 8[6] Myr |
| Other designations | |
| i Sco, 22 Sco, CD−24°12695, HD 148605, HIP 80815, HR 6141, SAO 184429[7] | |
| Database references | |
| SIMBAD | data |
22 Scorpii (i Scorpii) is a single[8] star in the southern zodiac constellation of Scorpius, about one degree from Antares. It is faintly visible to the naked eye with an apparent visual magnitude of 4.78.[3] The distance to this star is estimated to be around 411 light years, as derived from its annual parallax shift of 7.9±0.2 mas. The star is embedded in, or adjacent to, the diffuse nebulous cloud IC 4605 located in the western regions of the Rho Ophiuchi cloud complex.[9]
22 Scorpii is a B-type main-sequence star with a stellar classification of B3 V.[4] It is ten million years old[10] and has a high rate of spin with a projected rotational velocity of 169 km/s.[3] The star has about 4.4 times the mass of the Sun and is radiating 601 times the Sun's luminosity from its photosphere at an effective temperature of 16,683 K.[3]
References
[edit]- 1 2 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.
- 1 2 3 4 5 6 7 8 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 4 5 Bragança, G. A.; et al. (November 2012), "Projected Rotational Velocities and Stellar Characterization of 350 B Stars in the Nearby Galactic Disk", The Astronomical Journal, 144 (5): 10, arXiv:1208.1674, Bibcode:2012AJ....144..130B, doi:10.1088/0004-6256/144/5/130, S2CID 118868235, 130.
- 1 2 Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1988mcts.book.....H.
- 1 2 3 Fouesneau, M.; Andrae, R.; Dharmawardena, T.; Rybizki, J.; Bailer-Jones, C. A. L.; Demleitner, M. (2022), "Astrophysical parameters from Gaia DR2, 2MASS, and AllWISE", Astronomy and Astrophysics, 662: A125, arXiv:2201.03252, Bibcode:2022A&A...662A.125F, doi:10.1051/0004-6361/202141828
- 1 2 Gullikson, Kevin; Kraus, Adam; Dodson-Robinson, Sarah (2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars", The Astronomical Journal, 152 (2): 40, arXiv:1604.06456, Bibcode:2016AJ....152...40G, doi:10.3847/0004-6256/152/2/40
- ↑ "22 Sco". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-03-16.
- ↑ 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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ↑ Padgett, Deborah L.; et al. (January 2008), "The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. VII. Ophiuchus Observed with MIPS", The Astrophysical Journal, 672 (2): 1013–1037, arXiv:0709.3492, Bibcode:2008ApJ...672.1013P, doi:10.1086/523883, S2CID 12396730, 1013–1037.
- ↑ Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
External links
[edit]- "22 Scorpii - Wolfram Alpha". Wolfram Alpha.
- "22 Scorpii (HIP 80815)". Ashland Astronomy Studio. Retrieved 2012-08-19.
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