54 Рака

54 Рака
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 8ч 51м 1,46с[1]
Склонение +15° 21′ 2,36″[1]
Расстояние 40,237 ± 0,0364 пк[1]
Видимая звёздная величина (V) 6,361 ± 0,01[2]
Созвездие Рак
Астрометрия
Лучевая скорость (Rv) 45,656 ± 0,0018 км/с[3]
Собственное движение
 • прямое восхождение −112,498 ± 0,024 mas/год[1]
 • склонение 75,075 ± 0,018 mas/год[1]
Параллакс (π) 24,8527 ± 0,0225 mas[1]
Абсолютная звёздная величина (V) 3,37
Спектральные характеристики
Спектральный класс G1V[4]
Показатель цвета
 • B−V 0,656
Физические характеристики
Масса 1,26 M☉
Радиус 1,78 R☉
Температура 5862 К[5][6]
Светимость 3,8 L☉
Металличность 0,19[5][6]
Вращение 6 км/с[7]
Коды в каталогах

HD 75528, HIP 43454, SAO 98168, HR 3510, IRAS 08482+1532, 2MASS J08510149+1521022, GSC 01393-01968, BD+15 1917, FK5 2699, GC 12211, GCRV 5821, HIC 43454, N30 2075, PPM 125817, ROT 1392, TD1 13160, TYC 1393-1968-1, UBV 8572, YZ 15 3549, Gaia DR1 609834194381571712, WEB 8375, Gaia DR2 609834198678048512, 54 Cnc, Gaia DR3 609834198678048512, TIC 46297363, AG+15 986, UBV M 14775 и uvby98 100075528

Информация в базах данных
SIMBAD * 54 Cnc
Логотип Викиданных Информация в Викиданных ?

54 Рака (лат. 54 Cancri) — звезда, которая находится в созвездии Рака. Это жёлтый карлик спектрального класса G главной последовательности, похожий на наше Солнце, но немного массивнее, больше, горячее и ярче его. Находится от Земли на расстоянии 130 световых лет и имеет видимую звёздную величину +6.36, то есть звезда невидима невооружённым глазом, но её можно разглядеть в бинокль.

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. ↑ Soubiran C., Jasniewicz G., Chemin L., Zurbach C., Brouillet N., Panuzzo P., Sartoretti P., Katz D., Le Campion, J. -F., Marchal O. et al. Gaia Data Release 2. The catalogue of radial velocity standard stars (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2018. — Vol. 616. — 8 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201832795 — arXiv:1804.09370
  4. ↑ SIMBAD Astronomical Database
  5. ↑ 1 2 Deka-Szymankiewicz B., Niedzielski A., Adamczyk M., Adamów M., Nowak G., Wolszczan A. The Penn State - Torun Centre for Astronomy Planet Search stars. IV. Dwarfs and the complete sample (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2018. — Vol. 615. — 11 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201731696 — arXiv:1801.02899
  6. ↑ 1 2 Niedzielski A., Deka-Szymankiewicz B., Adamczyk M., Adamów M., Nowak G., Wolszczan A. The Penn State - Torun Centre for Astronomy Planet Search stars. III. The sample of evolved stars (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2015. — Vol. 585. — P. 73–73. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201527362
  7. ↑ Luck R. E. Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2016. — Vol. 153, Iss. 1. — 19 p. — ISSN 0004-6256; 1538-3881 — doi:10.3847/1538-3881/153/1/21 — arXiv:1611.02897

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