Astrometric binary star system in the constellation Delphinus
κ Delphini (Latinised as Kappa Delphini , abbreviated to κ Del or kappa Del) is a binary star system in the constellation Delphinus . It is faintly visible to the naked eye, with an apparent magnitude of 5.05.[ 2] It is located about 98.8 light-years away, based on its parallax .[ 1]
Kappa Delphini is an astrometric binary . The primary star is an early G-type subgiant star. It has a mass 1.61 times that of the Sun, and is 6.8 times more luminous. The companion star regularly perturbs the G-type primary star primary, causing it to wobble around the barycenter . From this, an orbital period of 45 years has been calculated.[ 6] The secondary star is a low-mass star, at only 0.4 M ☉ .[ 6]
A third star is 12th magnitude ADS 14101 B, 10″ away in 2001, but it is a background object. HD 196794 is an 8th magnitude K2 subgiant 214″ away is at the same distance as κ Delphini and shares a common proper motion.[ 6]
References
^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction" . Astronomy and Astrophysics . 474 (2): 653– 664. arXiv :0708.1752 . Bibcode :2007A&A...474..653V . doi :10.1051/0004-6361:20078357 . S2CID 18759600 . Vizier catalog entry
^ a b c d "* kap Del" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 26 December 2016 .
^ Eggl, S.; Pilat-Lohinger, E.; Funk, B.; Georgakarakos, N.; Haghighipour, N. (2012). "Circumstellar habitable zones of binary-star systems in the solar neighbourhood" . Monthly Notices of the Royal Astronomical Society . 428 (4): 3104. arXiv :1210.5411 . Bibcode :2013MNRAS.428.3104E . doi :10.1093/mnras/sts257 .
^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data : 0. Bibcode :1986EgUBV........0M .
^ Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d e f Gontcharov, G.A.; Kiyaeva, O.V. (2010). "Photocentric orbits from a direct combination of ground-based astrometry with Hipparcos II. Preliminary orbits for six astrometric binaries". New Astronomy . 15 (3): 324– 331. arXiv :1606.08182 . Bibcode :2010NewA...15..324G . doi :10.1016/j.newast.2009.09.006 . S2CID 119252073 .
^ Niedzielski, A.; Deka-Szymankiewicz, B.; Adamczyk, M.; Adamów, M.; Nowak, G.; Wolszczan, A. (2016). "The Penn State - Toruń Centre for Astronomy Planet Search stars" . Astronomy and Astrophysics . 585 : A73. Bibcode :2016A&A...585A..73N . doi :10.1051/0004-6361/201527362 .