["}},"i":12}},"\n",{"template":{"target":{"wt":"Starbox reference\n ","href":"./Template:Starbox_reference"},"params":{"Simbad":{"wt":"HD+202908"},"Simbad2":{"wt":"HD+202908A"},"Simbad3":{"wt":"HD+202908B"},"sn":{"wt":"The system"},"sn2":{"wt":"A"},"sn3":{"wt":"B"}},"i":13}},"\n",{"template":{"target":{"wt":"Starbox end","href":"./Template:Starbox_end"},"params":{},"i":14}}]}" id="mwBA">] HD 202908 Observation data Epoch J2000.0 Equinox J2000.0 (ICRS ) Constellation Equuleus A Right ascension 21h 18m 34.85s [ 1] Declination +11° 34′ 08.2″ [ 1] Apparent magnitude (V) 7.25± 0.03 [ 2] B Right ascension 21h 18m 34.80s [ 1] Declination +11° 34′ 08.0″ [ 1] Apparent magnitude (V) 8.87± 0.14 [ 2] Characteristics Spectral type G0 V (combined) [ 3] U−B color index +0.07 [ 4] B−V color index +0.56 [ 4] Aa Spectral type F9 V [ 5] or G1 V [ 6] Ab Spectral type G0 V [ 5] or G2 V [ 6] B Spectral type G1.5 V [ 5] or G6 V [ 7] Astrometry Radial velocity (Rv ) 6.24± 0.04 [ 8] km/s Proper motion (μ) RA: +29.213 mas /yr [ 9] Dec.: −49.564 mas /yr [ 9] Parallax (π) 19.3447± 0.0543 mas [ 9] Distance 168.6 ± 0.5 ly (51.7 ± 0.1 pc ) A Absolute magnitude (MV ) +3.73± 0.13 [ 2] B Absolute magnitude (MV ) +5.35± 0.19 [ 2] Orbit [ 10] Primary A Companion B 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 [ 10] Primary Aa Companion Ab 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 [ 11] dex Age 6.4± 0.7 [ 12] Gyr The A Subystem Temperature 6,100± 150 [ 13] K Rotational velocity (v sin i ) 10 [ 14] km/s Aa Mass 1.14 [ 15] M ☉ Radius 1.06± 0.08 [ 13] R ☉ Luminosity 1.41+0.15 − 0.14 [ 13] L ☉ Ab Mass 1.08 [ 15] M ☉ Radius 0.97± 0.08 [ 13] R ☉ Luminosity 1.16+0.13 − 0.11 [ 13] L ☉ B Mass 0.97 [ 15] M ☉ Radius 0.91± 0.08 [ 13] R ☉ Luminosity 0.84+0.09 − 0.08 [ 13] L ☉ Temperature 5,703± 1,090 [ 2] K Rotational velocity (v sin i ) 9 [ 14] km/s Other designations Database references SIMBAD The system A B 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, [ 17] 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. [ 2] The system is located relatively close at a distance of 169 light years based on Gaia DR3 parallax measurements [ 9] and it is receding with a heliocentric radial velocity of 6.24 km/s . [ 8]
Stellar system Aa Period = 3.966 d Ab Separation = 0.5″ Period = 78 y B
Hierarchy of orbits in the HD 202908 system [ 5]
The system was first observed by astronomer S.W. Burnham. [ 18]
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. [ 5] The pair take roughly 4 days to orbit each other. [ 10]
The tertiary companion designated "B" has a class of G1.5 V, indicating that it is an ordinary G-type main-sequence star like our Sun . HD 202908 A and B both complete an eccentric orbit every 78 years . [ 10]
Physical characteristics HD 202908 Aa and Ab have masses 1.08 and 1.14 times that of the Sun [ 15] and radii 97% and 106% of the Sun respectively. [ 13] 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. [ 13] The A subsystem has an effective temperature of 6,100 K , [ 13] giving it a whitish-yellow hue.
The B component has 97% the mass of the Sun [ 15] and 91% of its radius. It radiates 84% of the Sun's luminosity [ 13] from its photosphere at an effective temperature of 5,703 K. [ 2] The system is estimated to be 6.4 billion years old. [ 12]
References 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 . 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 . ↑ 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 . 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 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 . 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 . ↑ 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 . 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 . 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 . 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 . ↑ 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 . 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 . 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 . 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 . 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 . ↑ "HD 202908" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved March 21, 2023 . ↑ 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 . ↑ 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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