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UV Pisces is a binary star system in the constellation of Pisces. With a peak apparent visual magnitude of 8.98, it is too faint to be visible to the naked eye. This is an eclipsing binary system that decreases to magnitude 10.05 during the primary eclipse, then to magnitude 9.54 with the secondary eclipse. It is located at a distance of 232 light years from the Sun based on parallax measurements, and is receding with a radial velocity of 6.5 km/s. The position of this star near the ecliptic means it is subject to lunar occultation.

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  • UV Piscium (ca)
  • UV Piscium (es)
  • UV Piscium (en)
  • UV Piscium (sv)
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  • UV Piscium (UV Psc / HD 7700 / HIP 5980) és un sistema estel·lar de magnitud aparent +8,91 situat a la constel·lació dels Peixos, un grau al sud de ζ Piscium. S'hi troba a 275 anys llum del sistema solar. (ca)
  • UV Piscium (UV Psc / HD 7700 / HIP 5980) es un sistema estelar de magnitud aparente +8,91​situado en la constelación de Piscis, 1º al sur de .Se encuentra a 275 años luz del Sistema Solar.​ UV Piscium es un binaria espectroscópica en donde la componente más brillante es una enana amarilla de tipo espectral G5V​muy parecida a Sol.Tiene una temperatura efectiva de 5780 ± 100 K y su luminosidad es un 23% mayor que la luminosidad solar.Con una masa de 0,98 masas solares, su radio es un 11% más grande que el del Sol y gira sobre sí misma con una velocidad de rotación proyectada de 68 km/s.​La estrella secundaria es una enana naranja de tipo K3V cuya temperatura es de 4750 ± 80 K.Su luminosidad equivale al 30% de la que tiene el Sol y su masa es igual a 3/4 partes de la masa solar.Su radio es un (es)
  • UV Pisces is a binary star system in the constellation of Pisces. With a peak apparent visual magnitude of 8.98, it is too faint to be visible to the naked eye. This is an eclipsing binary system that decreases to magnitude 10.05 during the primary eclipse, then to magnitude 9.54 with the secondary eclipse. It is located at a distance of 232 light years from the Sun based on parallax measurements, and is receding with a radial velocity of 6.5 km/s. The position of this star near the ecliptic means it is subject to lunar occultation. (en)
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