- Eris (dwarf planet) - Wikipedia
Eris is the ninth-most massive known object orbiting the Sun and the sixteenth-most massive in the Solar System (counting moons) It is also the largest known object in the Solar System that has not been visited by a spacecraft
- Eris - Science@NASA
Eris is one of largest the dwarf planets in our solar system It's about the same size as Pluto, but it's three times farther from the Sun Eyes of the Solar System uses data and images from NASA missions to give you a simulated view of Eris
- The discovery of - New Planet
In Greek mythology, Eris is the goddess of warfare and strife She stirs up jealousy and envy to cause fighting and anger among men
- Eris Dwarf Planet: Discovery, Classification, Mass And Other Facts
Eris is a dwarf planet situated beyond Neptune in the edges of the Kuiper Belt It is an icy rocky planet, bigger than Pluto and twice as far from the Sun
- Eris | Dwarf Planet, Kuiper Belt, Plutoid | Britannica
Eris, large, distant body of the solar system, revolving around the Sun well beyond the orbits of Neptune and Pluto in the Kuiper belt It was discovered in 2005 in images taken two years earlier at Palomar Observatory in California, U S
- Eris, a Dwarf Planet - Windows to the Universe
Eris is a large sphere of ice and rock similar to Pluto It orbits the Sun on the edge of the Solar System The diameter of Eris is about 2,500 km (1,553 miles) We aren't sure of its exact size because it is so far away and very hard to see, even with the world's biggest telescopes
- Eris (dwarf planet) - scientificlib. com
Eris was first identified in January 2005 by a Palomar Observatory-based team led by Mike Brown, and its identity verified later that year It is a trans-Neptunian object (TNO) native to a region of space beyond the Kuiper belt known as the scattered disc
- Eris: The Dwarf Planet Guarding the Kuiper Belt | Astronoo
Discovered in 2005 by the team of Mike Brown (Caltech), Eris is the most massive known dwarf planet, with a mass 27% greater than Pluto's Located in the scattered disk, a region beyond the Kuiper Belt, its eccentric orbit (perihelion at 37 9 AU, aphelion at 97 6 AU) makes it an extreme trans-Neptunian object
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