Astronomy:59 Andromedae
Observation data {{#ifeq:J2000|J2000.0 (ICRS)|Epoch J2000.0 Equinox J2000.0 (ICRS)| Epoch J2000 [[Astronomy:Equinox (celestial coordinates)|Equinox J2000}} | |
---|---|
Constellation | Andromeda |
59 And A | |
Right ascension | 02h 10m 52.82451s[1] |
Declination | +39° 02′ 22.3597″[1] |
Apparent magnitude (V) | 6.09[2] |
59 And B | |
Right ascension | 02h 10m 53.65687s[1] |
Declination | +39° 02′ 35.9164″[1] |
Apparent magnitude (V) | 6.82[2] |
Characteristics | |
59 And A | |
Spectral type | B9 V[3] |
B−V color index | −0.054±0.006[2] |
59 And B | |
Spectral type | A1 Vn[3] |
B−V color index | +0.081±0.005[2] |
Astrometry | |
59 And A | |
Radial velocity (Rv) | −1.00±3.4[4] km/s |
Proper motion (μ) | RA: −13.506[1] mas/yr Dec.: −14.981[1] mas/yr |
Parallax (π) | 7.1469 ± 0.1007[1] mas |
Distance | 456 ± 6 ly (140 ± 2 pc) |
59 And B | |
Radial velocity (Rv) | 6.0±4.6[4] km/s |
Proper motion (μ) | RA: −9.166[1] mas/yr Dec.: −17.208[1] mas/yr |
Parallax (π) | 7.4166 ± 0.0619[1] mas |
Distance | 440 ± 4 ly (135 ± 1 pc) |
Details | |
59 And A | |
Radius | 2.73[5] R☉ |
Luminosity | 83.97[6] L☉ |
Temperature | 10,870[6] K |
Rotational velocity (v sin i) | 176[3] km/s |
59 And B | |
Mass | 2.23±0.09[7] M☉ |
Radius | 2.59[5] R☉ |
Luminosity | 30.4+7.6 −6.1[7] L☉ |
Temperature | 9,498[6] K |
Rotational velocity (v sin i) | 233[3] km/s |
Other designations | |
59 And A: GC 2600, HD 13294, HIP 10176, HR 628, SAO 55330, PPM 67045[9] | |
59 And B: GC 2602, HD 13295, HIP 10180, HR 629, SAO 55331, PPM 67046[10] | |
Database references | |
SIMBAD | data |
SIMBAD | data |
59 Andromedae, abbreviated 59 And, is a sixth-magnitude binary star system in the northern constellation of Andromeda. 59 Andromedae is the Flamsteed designation. As of 2017, the pair had an angular separation of 16.60″ along a position angle (PA) of 36°. Compare this to a separation of 15.3″ along a PA of 35°, as measured in 1783.[11] The two stars have an estimated physical separation of 1,370 astronomical unit|AU.[5]
The magnitude 6.09[2] primary component is a B-type main-sequence star with a stellar classification of B9 V.[3] It has 2.73[5] times the Sun's radius and is radiating 84 times the Sun's luminosity from its photosphere at an effective temperature of 10,870 K.[6] It is spinning with a projected rotational velocity of 176 km/s.[3]
The secondary is a magnitude 6.82[2] A-type main-sequence star with a class of A1 Vn,[3] where the 'n' suffix indicates "nebulous" lines due to rapid rotation. It is spinning with a high projected rotational velocity of 233 km/s.[3] The star has 2.23[7] times the Sun's mass and 2.59[5] times the Sun's radius. It is radiating 30[7] times the luminosity of the Sun and has an effective temperature of 9,498 K.[6]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 Royer, F. et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, doi:10.1051/0004-6361:20065224, Bibcode: 2007A&A...463..671R
- ↑ 4.0 4.1 de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics 546: 14, doi:10.1051/0004-6361/201219219, A61, Bibcode: 2012A&A...546A..61D.
- ↑ 5.0 5.1 5.2 5.3 5.4 Howe, K. S.; Clarke, C. J. (January 2009), "An analysis of v sin (i) correlations in early-type binaries", Monthly Notices of the Royal Astronomical Society 392 (1): 448–454, doi:10.1111/j.1365-2966.2008.14073.x, Bibcode: 2009MNRAS.392..448H.
- ↑ 6.0 6.1 6.2 6.3 6.4 McDonald, I.; Zijlstra, A. A. et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–357, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode: 2012MNRAS.427..343M.
- ↑ 7.0 7.1 7.2 7.3 Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, A120, Bibcode: 2012A&A...537A.120Z.
- ↑ "59 And". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=59+And.
- ↑ "59 And A". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=59+And+A.
- ↑ "59 And B". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=59+And+B.
- ↑ Mason, B. D. et al. (December 2001), "The Washington Visual Double Star Catalog", The Astronomical Journal 122 (6): 3466–3471, doi:10.1086/323920, Bibcode: 2001AJ....122.3466M
External links
Original source: https://en.wikipedia.org/wiki/59 Andromedae.
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