83 Девы

83 Девы
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 13ч 44м 29,83с[1]
Склонение −16° 10′ 44,66″[1]
Расстояние 264,76 ± 4,5844 пк[1] и 256,5493 пк[2]
Видимая звёздная величина (V) 5,567 ± 0,009[3]
Созвездие Дева
Астрометрия
Лучевая скорость (Rv) 2,13 ± 0,2 км/с[4]
Собственное движение
 • прямое восхождение 12,522 ± 0,069 mas/год[1]
 • склонение −6,052 ± 0,058 mas/год[1]
Параллакс (π) 3,777 ± 0,0654 mas[1]
Абсолютная звёздная величина (V) −1,46
Спектральные характеристики
Спектральный класс G0II[5][6][…]
Показатель цвета
 • B−V 0,783
Физические характеристики
Радиус 21,81 R☉
Температура 5430 К[7][8]
Металличность 4,2[8]
Коды в каталогах

HD 119605, HIP 67057, HR 5165, SAO 158131, IRAS 13418-1555, GSC 06123-00583, 2MASS J13442982-1610445, FK5 1357, GC 18568, GCRV 8112, HIC 67057, JP11 2418, N30 3130, PMC 90-93 948, PPM 227764, TD1 17015, TYC 6123-583-1, UBV 12276, uvby98 100119605, YZ 105 5171, WEB 11810, Gaia DR2 3605275331575431168, 83 Vir, Gaia DR3 3605275331575431168, TIC 290058791, UBV M 19672, BD-15 3731, GEN# +1.00119605, SKY# 25239 и WISEA J134429.83-161044.6

Информация в базах данных
SIMBAD * 83 Vir
Логотип Викиданных Информация в Викиданных ?

83 Девы (лат. 83 Virginis), HD 119605 — двойная звезда в созвездии Девы на расстоянии приблизительно 837 световых лет (около 257 парсек) от Солнца. Визуальная звёздная величина звезды — +5,567m[9]. Возраст звезды определён как около 190 млн лет[10].

Характеристики

Первый компонент — жёлтая звезда спектрального класса G0Ib-IIa[11][12][13], или G0II:[14][15], или G0[16][17]. Масса — около 4,454 солнечной, радиус — около 25,727 солнечного, светимость — около 454,313 солнечной[4]. Эффективная температура — около 5979 K[2].

Второй компонент — коричневый карлик. Масса — около 23,12 юпитерианской[18]. Удалён в среднем на 2,461 а.е.[18].

Примечания

  1. ↑ 1 2 3 4 5 6 Gaia Early Data Release 3 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2020.
  2. ↑ 1 2 Gaia Data Release 3 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2022.
  3. ↑ Høg E., Fabricius C., Makarov V. V., Urban S., Corbin T., Wycoff G., Bastian U., Schwekendiek P., Wicenec A. The Tycho-2 catalogue of the 2.5 million brightest stars (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2000. — Vol. 355. — P. L27—L30. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846
  4. ↑ 1 2 Gaia Data Release 2 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2018.
  5. ↑ Gray R. O., Napier M. G., Winkler L. I. The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2001. — Vol. 121, Iss. 4. — P. 2148–2158. — ISSN 0004-6256; 1538-3881 — doi:10.1086/319956
  6. ↑ Eggen O. J. Space-velocity vectors for 3483 stars with proper motion and radial velocity (англ.) // (unknown type) — 1962. — Vol. 51. — P. 79.
  7. ↑ Lyubimkov L. S., Lambert D. L., Rostopchin S. I., Rachkovskaya T. M., Poklad D. B. Accurate fundamental parameters for A-, F- and G-type Supergiants in the solar neighbourhood (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2010. — Vol. 402, Iss. 2. — P. 1369–1379. — 11 p. — ISSN 0035-8711; 1365-2966 — doi:10.1111/J.1365-2966.2009.15979.X — arXiv:0911.1335
  8. ↑ 1 2 Lyubimkov L. S., Korotin S. A., Lambert D. L. Oxygen abundance and the N/C versus N/O relation for AFG supergiants and bright giants (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2019. — Vol. 489, Iss. 2. — P. 1533—1542. — 10 p. — ISSN 0035-8711; 1365-2966 — doi:10.1093/MNRAS/STZ2285 — arXiv:1907.04634
  9. ↑ Soubiran C., Brouillet N., Casamiquela L. Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2022. — Vol. 663. — P. A4. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/202142409 — arXiv:2112.07545
  10. ↑ Reffert S., Bergmann C., Quirrenbach A., Trifonov T., Künstler A. Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2015. — Vol. 574. — 13 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201322360 — arXiv:1412.4634
  11. ↑ Lyubimkov L. S., Lambert D. L., Korotin S. A., Rachkovskaya T. M., Poklad D. B. Carbon abundance and the N/C ratio in atmospheres of A-, F- and G-type supergiants and bright giants (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2014. — Vol. 446, Iss. 4. — P. 3447–3460. — 14 p. — ISSN 0035-8711; 1365-2966 — doi:10.1093/MNRAS/STU2299 — arXiv:1411.2722
  12. ↑ Lyubimkov L. S., Lambert D. L., Kaminsky B. M., Pavlenko Y. V., Poklad D. B., Rachkovskaya T. M. Lithium abundance in atmospheres of F- and G-type supergiants and bright giants (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2012. — Vol. 427, Iss. 1. — P. 11–26. — 16 p. — ISSN 0035-8711; 1365-2966 — doi:10.1111/J.1365-2966.2012.21617.X — arXiv:1212.6057
  13. ↑ Eggleton P. P., Tokovinin A. A. A Catalog of Multiplicity among Bright Stellar Systems (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2008. — Vol. 389, Iss. 2. — P. 869–879. — 11 p. — ISSN 0035-8711; 1365-2966 — doi:10.1111/J.1365-2966.2008.13596.X — arXiv:0806.2878
  14. ↑ Cruzalèbes P., Petrov R. G., Robbe-Dubois S., Varga J., Burtscher L., Allouche F., Berio P., Hofmann, K. -H., Hron J., Jaffe W. et al. A catalogue of stellar diameters and fluxes for mid-infrared interferometry (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2019. — Vol. 490, Iss. 3. — P. 3158—3176. — ISSN 0035-8711; 1365-2966 — doi:10.1093/MNRAS/STZ2803 — arXiv:1910.00542
  15. ↑ Park S., Lee J., Kang W., Lee S., Chun M., Kim K., Yuk I., Lee J., Mace G. N., Kaplan K. F. et al. IGRINS Spectral Library (англ.) // The Astrophysical Journal: Supplement Series — AAS, 2018. — Vol. 238, Iss. 2. — 30 p. — ISSN 0067-0049; 1538-4365 — doi:10.3847/1538-4365/AADD14 — arXiv:1808.06629
  16. ↑ Cannon A. J., Pickering E. C. VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) (англ.) // Annals of the Astronomical Observatory of Harvard College — 1918. — Vol. 91-100.
  17. ↑ Roeser S., Bastian U. PPM (Positions and Proper Motions) North Star Catalogue (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 1988. — Vol. 74. — P. 449. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846
  18. ↑ 1 2 Kervella P., Arenou F., Mignard F., Thévenin F. Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2019. — Vol. 623. — P. 72–72. — 23 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201834371 — arXiv:1811.08902

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