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83 Cancri is an astrometric binary star system in the northern constellation of Cancer, positioned near the constellation border with Leo. It is a challenge to view with the naked eye, having an apparent visual magnitude of 6.61. Despite having a Flamsteed designation, the system was too faint to be included in the Bright Star Catalogue. It is located at a distance of 133 light years from the Sun, based on parallax, but is drifting closer with a radial velocity of −15 km/s. 83 Cancri has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.185″ per annum.

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  • 83 Cancri (en)
  • 83 Cancri (sv)
  • 83 Рака (ru)
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  • 83 Ра́ка (лат. 83 Cancri) — звезда главной последовательности, которая находится в созвездии Рака. Звезда удалена от Земли на 40 парсек и имеет видимую звёздную величину +6,64m, то есть не может быть наблюдаема невооружённым глазом, но может быть различима в бинокль. Это жёлто-белая звезда спектрального класса F. (ru)
  • 83 Cancri, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna, belägen i den mellersta delen av stjärnbilden Kräftan. Den har en kombinerad skenbar magnitud av ca 6,61 och kräver åtminstone en handkikare för att kunna observeras. Trots att den har en Flamsteed-beteckning är den för svag för att ingå i Bright Star Catalogue. Baserat på parallax enligt Gaia Data Release 2 på ca 24,6 mas, beräknas den befinna sig på ett avstånd på ca 133 ljusår (ca 41 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -15 km/s. Paret har en relativt stor egenrörelse och rör sig över himlavalvet med en vinkelhastighet av 0,185 bågsekunder per år. (sv)
  • 83 Cancri is an astrometric binary star system in the northern constellation of Cancer, positioned near the constellation border with Leo. It is a challenge to view with the naked eye, having an apparent visual magnitude of 6.61. Despite having a Flamsteed designation, the system was too faint to be included in the Bright Star Catalogue. It is located at a distance of 133 light years from the Sun, based on parallax, but is drifting closer with a radial velocity of −15 km/s. 83 Cancri has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.185″ per annum. (en)
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  • F4V + WD (en)
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