Rho Coronae Borealis

Rho Coronae Borealis (ρ CrB, ρ Coronae Borealis) is a Solar twin, yellow dwarf star approximately 57 light-years away in the constellation of Corona Borealis. The star is thought to be similar to the Sun with nearly the same mass, radius, and luminosity. As of 1997, an extrasolar planet has been confirmed to be orbiting the star. It is thought that the star may have a stellar companion, but it may be just an optical companion.

Read more about Rho Coronae Borealis:  Stellar Components, Planetary System

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... Rho Coronae Borealis b (ρ CrB b / ρ Coronae Borealis b) is an extrasolar planet approximately 57 light-years away in the constellation of Corona Borealis ... The planet was discovered orbiting the Solar twin, yellow dwarf star Rho Coronae Borealis in April 1997 (one of the first discovered) ...
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... disk may extend out to 85 astronomical units out from Rho Coronae Borealis (which is beyond the orbital distances of Neptune and Pluto from the Sun) ...
Corona (planetary Geology) - Coronae On Venus
... See also List of coronae on Venus On Venus, coronae are large (typically several hundred kilometres across), crown-like, volcanic features ... Coronae were first identified in 1983, when the radar imaging equipment aboard the Venera 15 and Venera 16 spacecraft produced higher-resolution images of some ... It is believed that coronae are formed when plumes of rising hot material in the mantle push the crust upwards into a dome shape, which then collapses in the ...