  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Vulpecula |
| Right ascension | 20h 37m 04.6724s [1] |
| Declination | +26° 27′ 43.006″ [1] |
| Apparent magnitude (V) | 5.590 [2] |
| Characteristics | |
| Spectral type | B9 V [3] [4] |
| B−V color index | −0.050±0.004 [5] |
| Astrometry | |
| Radial velocity (Rv) | −21.8±4.3 [6] km/s |
| Proper motion (μ) |
RA: 15.349±0.042
[1]
mas/
yr Dec.: −11.775±0.040 [1] mas/ yr |
| Parallax (π) | 10.6692 ± 0.0483 mas [1] |
| Distance | 306 ± 1
ly (93.7 ± 0.4 pc) |
| Absolute magnitude (MV) | 0.65 [5] |
| Details | |
| Mass | 2.77±0.03 [4] M☉ |
| Radius | 3.1 [7] R☉ |
| Luminosity | 75.0+4.8 −4.5 [4] L☉ |
| Surface gravity (log g) | 3.781 [8] cgs |
| Temperature | 10,789+50 −49 [4] K |
| Metallicity [Fe/H] | −0.27±0.04 [5] dex |
| Rotational velocity (v sin i) | 335 [4] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
27 Vulpeculae is a single, [10] blue-white star in the northern constellation of Vulpecula. It is a dim star, visible to the naked eye, with an apparent visual magnitude of 5.59. [2] An annual parallax shift of 10.6692±0.0483 mas [1] provides a distance estimate of about 306 light-years. It is moving closer with a heliocentric radial velocity of −22 km/s, [6] and will make perihelion passage at a distance of around 119 ly (36.56 pc) in 3.75 million years. [5]
This is a B-type main-sequence star with a stellar classification of B9 V. [3] It is spinning rapidly, showing a projected rotational velocity of 335. [4] The star has an estimated 2.77 [4] times the mass of the Sun and about 3.1 [7] times the Sun's radius. It is radiating 75 [4] times the Sun's luminosity from its photosphere at an effective temperature of 10,789 K. [4]
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b Paunzen, E. (2015), "A new catalogue of Strömgren-Crawford uvbyβ photometry", Astronomy & Astrophysics, 580: A23, arXiv: 1506.04568, Bibcode: 2015A&A...580A..23P, doi: 10.1051/0004-6361/201526413, S2CID 73623700.
- ^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode: 1969AJ.....74..375C, doi: 10.1086/110819
- ^ a b c d e f g h i Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv: 1201.2052, Bibcode: 2012A&A...537A.120Z, doi: 10.1051/0004-6361/201117691, S2CID 55586789.
- ^ 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.
- ^ 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 Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy & Astrophysics, 367 (Third ed.): 521–24, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ Huang, W.; Gies, D. R. (August 2008), "Stellar Rotation in Field and Cluster B Stars", The Astrophysical Journal, 683 (2): 1045–1051, arXiv: 0805.2133, Bibcode: 2008ApJ...683.1045H, doi: 10.1086/590106, S2CID 18926523, 1045–1051.
- ^ "27 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-21.
- ^ 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.
- 27 Vulpeculae on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
| |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Vulpecula |
| Right ascension | 20h 37m 04.6724s [1] |
| Declination | +26° 27′ 43.006″ [1] |
| Apparent magnitude (V) | 5.590 [2] |
| Characteristics | |
| Spectral type | B9 V [3] [4] |
| B−V color index | −0.050±0.004 [5] |
| Astrometry | |
| Radial velocity (Rv) | −21.8±4.3 [6] km/s |
| Proper motion (μ) |
RA: 15.349±0.042
[1]
mas/
yr Dec.: −11.775±0.040 [1] mas/ yr |
| Parallax (π) | 10.6692 ± 0.0483 mas [1] |
| Distance | 306 ± 1
ly (93.7 ± 0.4 pc) |
| Absolute magnitude (MV) | 0.65 [5] |
| Details | |
| Mass | 2.77±0.03 [4] M☉ |
| Radius | 3.1 [7] R☉ |
| Luminosity | 75.0+4.8 −4.5 [4] L☉ |
| Surface gravity (log g) | 3.781 [8] cgs |
| Temperature | 10,789+50 −49 [4] K |
| Metallicity [Fe/H] | −0.27±0.04 [5] dex |
| Rotational velocity (v sin i) | 335 [4] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
27 Vulpeculae is a single, [10] blue-white star in the northern constellation of Vulpecula. It is a dim star, visible to the naked eye, with an apparent visual magnitude of 5.59. [2] An annual parallax shift of 10.6692±0.0483 mas [1] provides a distance estimate of about 306 light-years. It is moving closer with a heliocentric radial velocity of −22 km/s, [6] and will make perihelion passage at a distance of around 119 ly (36.56 pc) in 3.75 million years. [5]
This is a B-type main-sequence star with a stellar classification of B9 V. [3] It is spinning rapidly, showing a projected rotational velocity of 335. [4] The star has an estimated 2.77 [4] times the mass of the Sun and about 3.1 [7] times the Sun's radius. It is radiating 75 [4] times the Sun's luminosity from its photosphere at an effective temperature of 10,789 K. [4]
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b Paunzen, E. (2015), "A new catalogue of Strömgren-Crawford uvbyβ photometry", Astronomy & Astrophysics, 580: A23, arXiv: 1506.04568, Bibcode: 2015A&A...580A..23P, doi: 10.1051/0004-6361/201526413, S2CID 73623700.
- ^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode: 1969AJ.....74..375C, doi: 10.1086/110819
- ^ a b c d e f g h i Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv: 1201.2052, Bibcode: 2012A&A...537A.120Z, doi: 10.1051/0004-6361/201117691, S2CID 55586789.
- ^ 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.
- ^ 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 Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy & Astrophysics, 367 (Third ed.): 521–24, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ Huang, W.; Gies, D. R. (August 2008), "Stellar Rotation in Field and Cluster B Stars", The Astrophysical Journal, 683 (2): 1045–1051, arXiv: 0805.2133, Bibcode: 2008ApJ...683.1045H, doi: 10.1086/590106, S2CID 18926523, 1045–1051.
- ^ "27 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-21.
- ^ 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.
- 27 Vulpeculae on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images