50 Весов

50 Весов
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 16ч 00м 47,63с[1]
Склонение −8° 24′ 40,89″[1]
Расстояние 142,225 ± 1,4868 пк[1]
Видимая звёздная величина (V) 5,526 ± 0,009[2]
Созвездие Весы
Астрометрия
Лучевая скорость (Rv) −20,1 ± 1,4 км/с[3]
Собственное движение
 • прямое восхождение −15,544 ± 0,095 mas/год[1]
 • склонение −13,847 ± 0,071 mas/год[1]
Параллакс (π) 7,0311 ± 0,0735 mas[1]
Абсолютная звёздная величина (V) −0,35
Спектральные характеристики
Спектральный класс A0V[4]
Показатель цвета
 • B−V 0,031
Физические характеристики
Радиус 4,49 R☉
Температура 10 689 К[5]
Металличность −0,19[5]
Вращение 36 км/с[6][7]
Коды в каталогах

FK5 1420, GC 21502, GCRV 9207, GSC 05611-01206, HD 143459, HIC 78436, HIP 78436, HR 5959, N30 3592, PPM 199195, SACS 350, SAO 140897, TD1 18754, TYC 5611-1206-1, UBV 13572, YZ 98 5571, uvby98 100143459, 2MASS J16004763-0824408, Gaia DR1 4347852018589647872, WEB 13259, Gaia DR2 4347852022889882624, 50 Lib, Gaia DR3 4347852022889882624, TIC 49549335 и UBV M 21090

Информация в базах данных
SIMBAD * 50 Lib
Логотип Викиданных Информация в Викиданных ?

50 Весов (лат. 50 Librae, HD 143459) — одиночная звезда в созвездии Весов на расстоянии приблизительно 450 световых лет (около 138 парсеков) от Солнца. Видимая звёздная величина звезды — +5,526m[8].

Характеристики

50 Весов — белая звезда спектрального класса A0V[4]. Радиус — около 4,49 солнечных, светимость — около 125,2 солнечных. Эффективная температура — около 10298 К[9].

Примечания

  1. ↑ 1 2 3 4 5 6 Gaia Early Data Release 3 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2020.
  2. ↑ 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
  3. ↑ Gontcharov G. A. Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system (англ.) // Astronomy Letters / R. Sunyaev — Nauka, Springer Science+Business Media, 2006. — Vol. 32, Iss. 11. — P. 759–771. — ISSN 1063-7737; 1562-6873; 0320-0108; 0360-0327 — doi:10.1134/S1063773706110065 — arXiv:1606.08053
  4. ↑ 1 2 Houk N., Swift C. Michigan catalogue of two-dimensional spectral types for the HD Stars (англ.) — 1999. — Vol. 5.
  5. ↑ 1 2 Arentsen A., Prugniel P., Gonneau A., Lançon A., Trager S., Peletier R., Lyubenova M., Chen Y., Falcón Barroso J., Sánchez Blázquez P. et al. Stellar atmospheric parameters for 754 spectra from the X-shooter Spectral Library (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2019. — Vol. 627. — 14 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201834273 — arXiv:1907.06391
  6. ↑ Royer F., Zorec J., Gómez A. E. Rotational velocities of A-type stars. III. Velocity distributions (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2007. — Vol. 463, Iss. 2. — P. 671–682. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361:20065224 — arXiv:astro-ph/0610785
  7. ↑ Royer F., Grenier S., Baylac, M. -O., Gómez A. E., Zorec J. Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2002. — Vol. 393, Iss. 3. — P. 897—911. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361:20020943 — arXiv:astro-ph/0205255
  8. ↑ Hog 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, 2009. — Vol. 500. — P. 583–586. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846
  9. ↑ Koleva M., Vazdekis A. Stellar population models in the UV. I. Characterisation of the New Generation Stellar Library (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2012. — Vol. 538. — P. A143. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201118065 — arXiv:1111.5449

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