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Epsilon Eridani - Wikipedia Epsilon Eridani (Latinized from ε Eridani), proper name Ran, [17] is a star in the southern constellation of Eridanus At a declination of −9 46°, it is visible from most of Earth's surface
Epsilon Eridani b - NASA Science Epsilon Eridani b is a gas giant exoplanet that orbits a K-type star Its mass is 0 66 Jupiters, it takes 7 3 years to complete one orbit of its star, and is 3 53 AU from its star Its discovery was announced in 2000
Epsilon Eridani (Ran): Star Type, Facts, Planet, Location - Star Facts Epsilon Eridani (ε Eri) is an orange dwarf located 10 475 light-years away in the constellation Eridanus It has the proper name Ran With an apparent magnitude of 3 736, it is the 10th brightest star in Eridanus Epsilon Eridani is the third nearest visible star to the Sun, after Alpha Centauri and Sirius It hosts a confirmed Jupiter-like
Epsilon Eridani - Astronomy Magazine Humanity’s story of Epsilon (ε) Eridani (Ran) is a case of life imitating art Shining at 4th magnitude, Epsilon Eridani lies only 10 5 light-years distant, making it the third closest naked
SOFIA Confirms Nearby Planetary System is Similar to Our Own Located 10 5 light-years away in the southern hemisphere of the constellation Eridanus, the star Epsilon Eridani, eps Eri for short, is the closest planetary system around a star similar to the early sun
Epsilon Eridani - University of Illinois Urbana-Champaign Epsilon Eridani is a fourth magnitude (on the bright side, 3 73) class K (K2) ordinary, though relatively young, hydrogen-fusing dwarf A mere 10 5 light years away, it is the 10th closest star system to the Earth
Epsilon Eridani Information - ThoughtCo Epsilon Eridani is an interesting star in its own right, even without its planets At less than a billion years old, it's very youthful It's also a variable star, which means that its light varies on a regular cycle
Epsilon Eridani - Nova. Org Epsilon Eridani is a relatively young main-sequence star, that is smaller, redder, and dimmer than Sol The star appears to be less enriched in elements heavier than hydrogen ("metals") because it has only 49 to 74 percent of Sol's abundance of iron (Santos et al, 2004; Laws et al, 2003; and Cayrel de Strobel et al, 1991, page 281
Epsilon Eridani - Wikiwand ε Eridani, Latinised to Epsilon Eridani, is the star's Bayer designation Despite being a relatively bright star, it was not given a proper name by early astronomers It has several other catalogue designations Upon its discovery, the planet was designated Epsilon Eridani b, following the usual designation system for extrasolar planets