HD 202908

Last updated
HD 202908
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Equuleus [1]
A
Right ascension 21h 18m 34.85s [2]
Declination +11° 34′ 08.2″ [2]
Apparent magnitude  (V)7.25±0.03 [3]
B
Right ascension 21h 18m 34.80s [2]
Declination +11° 34′ 08.0″ [2]
Apparent magnitude  (V)8.87±0.14 [3]
Characteristics
Spectral type G0 V (combined) [4]
U−B color index +0.07 [5]
B−V color index +0.56 [5]
Aa
Spectral type F9 V [6] or G1 V [7]
Ab
Spectral type G0 V [6] or G2 V [7]
B
Spectral type G1.5 V [6] or G6 V [8]
Astrometry
Radial velocity (Rv)6.24±0.04 [9] km/s
Proper motion (μ)RA: +29.213 mas/yr [10]
Dec.: −49.564 mas/yr [10]
Parallax (π)19.3447±0.0543  mas [10]
Distance 168.6 ± 0.5  ly
(51.7 ± 0.1  pc)
A
Absolute magnitude  (MV)+3.73±0.13 [3]
B
Absolute magnitude  (MV)+5.35±0.19 [3]
Orbit [11]
PrimaryA
CompanionB
Period (P)28,685±173  d
Semi-major axis (a)0.5177±0.0046″
Eccentricity (e)0.8651±0.0008
Inclination (i)100.36±0.16°
Longitude of the node (Ω)255.03±0.17°
Periastron epoch (T)24,468,123±3  JD
Argument of periastron (ω)
(secondary)		171.9±0.3°
Semi-amplitude (K1)
(primary)		6.13±0.07 km/s
Semi-amplitude (K2)
(secondary)		13.95±0.09 km/s
Orbit [11]
PrimaryAa
CompanionAb
Period (P)3.9660465±0.0000015  d
Eccentricity (e)0.0033±0.0008
Argument of periastron (ω)
(secondary)		271±13°
Semi-amplitude (K1)
(primary)		66.03±0.06 km/s
Semi-amplitude (K2)
(secondary)		69.69±0.06 km/s
Details
The System
Metallicity [Fe/H]−0.04 [12]   dex
Age 6.4±0.7 [13]   Gyr
The A Subystem
Temperature 6,100±150 [14]   K
Rotational velocity (v sin i)10 [15]  km/s
Aa
Mass 1.14 [16]   M☉
Radius 1.06±0.08 [14]   R☉
Luminosity 1.41+0.15
−0.14 [14]   L☉
Ab
Mass 1.08 [16]   M☉
Radius 0.97±0.08 [14]   R☉
Luminosity1.16+0.13
−0.11 [14]   L☉
B
Mass 0.97 [16]   M☉
Radius 0.91±0.08 [14]   R☉
Luminosity 0.84+0.09
−0.08 [14]   L☉
Temperature 5,703±1,090 [3]   K
Rotational velocity (v sin i)9 [15]  km/s
Other designations
AG+11°2644, BD+10°4514, GC 29812, HD 202908, HIP 105200, SAO 107015, ADS 14839AB, CCDM J21186+1134AB, WDS J21186+1134AB [17]
Database references
SIMBAD data

HD 202908, also known as HIP 105200, is a triple star located in the equatorial constellation Equuleus. It has an apparent magnitude of 7.01, [18] making it readily visible in binoculars but not to the naked eye. When resolved, the components have apparent magnitudes of 7.25 and 8.87 respectively. [3] The system is located relatively close at a distance of 169 light years based on Gaia DR3 parallax measurements [10] and it is receding with a heliocentric radial velocity of 6.24  km/s . [9]

Contents

Stellar system

Aa
Period = 3.966 d
Ab
Separation = 0.5″
Period = 78 y
B

Hierarchy of orbits in the HD 202908 system [6]

The system was first observed by astronomer S.W. Burnham. [19]

The "A" component is a double-lined spectroscopic binary that contains two solar-type stars with spectral classifications of F9 V and G0 V respectively. [6] The pair take roughly 4 days to orbit each other. [11]

The tertiary companion designated "B" has a class of G1.5 V, indicating that it is an ordinary G-type main-sequence star like the Sun. HD 202908 A and B both complete an eccentric orbit every 78 years. [11]

Physical characteristics

HD 202908 Aa and Ab have masses 1.08 and 1.14 times that of the Sun [16] and radii 97% and 106% of the Sun respectively. [14] The former radiates 1.41 times the luminosity of the Sun from its photosphere and the latter radiates 1.16 times the Sun's luminosity. [14] The A subsystem has an effective temperature of 6,100  K , [14] giving it a whitish-yellow hue.

The B component has 97% the mass of the Sun [16] and 91% of its radius. It radiates 84% of the Sun's luminosity [14] from its photosphere at an effective temperature of 5,703 K. [3] The system is estimated to be 6.4 billion years old. [13]

References

  1. ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode:1987PASP...99..695R. doi: 10.1086/132034 . Constellation record for this object at VizieR.
  2. 1 2 3 4 Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi: 10.1086/323920 . ISSN   0004-6256. S2CID   119533755.
  3. 1 2 3 4 5 6 7 ten Brummelaar, Theo; Mason, Brian D.; McAlister, Harold A.; Roberts, Jr., Lewis C.; Turner, Nils H.; Hartkopf, William I.; Bagnuolo, Jr., William G. (May 2000). "Binary Star Differential Photometry Using the Adaptive Optics System at Mount Wilson Observatory". The Astronomical Journal. 119 (5): 2403–2414. Bibcode:2000AJ....119.2403T. doi: 10.1086/301338 . ISSN   0004-6256.
  4. ↑ Abt, H. A. (March 1981). "Visual multiples. VII - MK classifications". The Astrophysical Journal Supplement Series. 45: 437. Bibcode:1981ApJS...45..437A. doi:10.1086/190719. eISSN   1538-4365. ISSN   0067-0049. S2CID   121286745.
  5. 1 2 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data. SIMBAD, Bibcode:1986EgUBV........0M
  6. 1 2 3 4 5 Fekel, F. C. Jr. (September 1981). "HD 202908 - A young, solar-type triple system". The Astrophysical Journal. 248: 670. Bibcode:1981ApJ...248..670F. doi: 10.1086/159191 . eISSN   1538-4357. ISSN   0004-637X.
  7. 1 2 Docobo, Jose A.; Andrade, Manuel (20 November 2006). "A Methodology for the Description of Multiple Stellar Systems with Spectroscopic Subcomponents". The Astrophysical Journal. 652 (1): 681–695. Bibcode:2006ApJ...652..681D. doi: 10.1086/508053 . eISSN   1538-4357. ISSN   0004-637X.
  8. ↑ Christy, James W.; Walker, R. L. Jr. (October 1969). "MK Classification of 142 Visual Binaries". Publications of the Astronomical Society of the Pacific. 81: 643. Bibcode:1969PASP...81..643C. doi: 10.1086/128831 . eISSN   1538-3873. ISSN   0004-6280. S2CID   122411453.
  9. 1 2 Karataş, Y.; Bilir, S.; Eker, Z.; Demircan, O. (April 2004). "Kinematics of chromospherically active binaries and evidence of an orbital period decrease in binary evolution". Monthly Notices of the Royal Astronomical Society. 349 (3): 1069–1092. arXiv: astro-ph/0404219 . Bibcode:2004MNRAS.349.1069K. doi: 10.1111/j.1365-2966.2004.07588.x . eISSN   1365-2966. ISSN   0035-8711.
  10. 1 2 3 4 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.
  11. 1 2 3 4 Fekel, Francis C.; Scarfe, C. D.; Barlow, D. J.; Duquennoy, Antoine; McAlister, Harold A. (March 1997). "New and Improved Parameters of HD 202908=ADS 14839: A Spectroscopic-Visual Triple System". The Astronomical Journal. 113: 1095. Bibcode:1997AJ....113.1095F. doi:10.1086/118327. ISSN   0004-6256.
  12. ↑ Casagrande, L.; Schönrich, R.; Asplund, M.; Cassisi, S.; Ramírez, I.; Meléndez, J.; Bensby, T.; Feltzing, S. (26 May 2011). "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): Improved astrophysical parameters for the Geneva-Copenhagen Survey⋆". Astronomy & Astrophysics. 530: A138. arXiv: 1103.4651 . Bibcode:2011A&A...530A.138C. doi: 10.1051/0004-6361/201016276 . eISSN   1432-0746. ISSN   0004-6361. S2CID   56118016.
  13. 1 2 Holmberg, J.; Nordström, B.; Andersen, J. (July 2009). "The Geneva-Copenhagen survey of the solar neighbourhood: III. Improved distances, ages, and kinematics". Astronomy & Astrophysics. 501 (3): 941–947. arXiv: 0811.3982 . Bibcode:2009A&A...501..941H. doi: 10.1051/0004-6361/200811191 . ISSN   0004-6361.
  14. 1 2 3 4 5 6 7 8 9 10 11 Torres, G.; Andersen, J.; Giménez, A. (7 October 2009). "Accurate masses and radii of normal stars: modern results and applications". The Astronomy and Astrophysics Review. 18 (1–2): 67–126. arXiv: 0908.2624 . Bibcode:2010A&ARv..18...67T. doi:10.1007/s00159-009-0025-1. eISSN   1432-0754. ISSN   0935-4956.
  15. 1 2 Cutispoto, G.; Pastori, L.; Pasquini, L.; de Medeiros, J. R.; Tagliaferri, G.; Andersen, J. (March 2002). "Fast-rotating nearby solar-type stars". Astronomy & Astrophysics. 384 (2): 491–503. Bibcode:2002A&A...384..491C. doi: 10.1051/0004-6361:20020040 . eISSN   1432-0746. ISSN   0004-6361. S2CID   56201169.
  16. 1 2 3 4 5 Tokovinin, Andrei (14 March 2014). "From Binaries to Multiples. I. Data on F and G Dwarfs within 67 pc of the Sun". The Astronomical Journal. 147 (4): 86. arXiv: 1401.6825 . Bibcode:2014AJ....147...86T. doi: 10.1088/0004-6256/147/4/86 . eISSN   1538-3881. ISSN   0004-6256. S2CID   53965918.
  17. ↑ "HD 202908". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved March 21, 2023.
  18. ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27 –L30. Bibcode:2000A&A...355L..27H. ISSN   0004-6361. S2CID   17128864.
  19. ↑ Burnham, S. W. (12 December 1873). "A Third Catalogue of 76 New Double Stars, discovered with a 6-inch Alvan Clark Refractor". Monthly Notices of the Royal Astronomical Society. 34 (2): 59–71. Bibcode:1873MNRAS..34...59B. doi: 10.1093/mnras/34.2.59 . eISSN   1365-2966. ISSN   0035-8711.
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