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Pi Capricorni

Pi Capricorni is a triple star system in the southern constellation of Capricornus. It has the traditional star name Oculus (meaning eye in Latin); Pi Capricorni is its Bayer designation, which is Latinized from π Capricorni and abbreviated Pi Cap or π Cap. This system appears blue-white in hue and is visible to the naked eye as a 5th magnitude star. It is located approximately 660 light years distant from the Sun based on parallax, but is drifting closer with a radial velocity of −13 km/s. The proximity of this star to the ecliptic means it is subject to lunar occultation.

In Chinese, (), meaning Ox (asterism), refers to an asterism consisting of π Capricorni, β Capricorni, α<sup>2</sup> Capricorni, ξ<sup>2</sup> Capricorni, ο Capricorni and ρ Capricorni. Consequently, the Chinese name for π Capricorni itself is (, .)

The primary member, component A, is a spectroscopic binary whose two components are separated by 0.1 arcseconds. The brighter of the two, component Aa, is a blue-white B-type bright giant or main sequence star with an apparent magnitude of +5.08. It is around 43&nbsp;million years old with six times the mass of the Sun. The star is radiating 238 times the Sun's luminosity from its photosphere at an effective temperature of 9,623&nbsp;K. The third member, component B, is an eighth magnitude star at an angular separation of from the primary.

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