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- Eris is a trans-Neptunian object (TNO) in the scattered disk and has a high-eccentricity orbit12. It is the most massive and second-largest known dwarf planet in the Solar System12. Eris was discovered in January 2005 by a Palomar Observatory-based team led by Mike Brown and verified later that year1. It is slightly smaller than Pluto, but it has more mass than Pluto2. Eris is also called a plutoid because the IAU decided to rename all trans-Neptunian dwarf planets as plutoids2.Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.Eris (minor-planet designation 136199 Eris) is the most massive and second-largest known dwarf planet in the Solar System. It is a trans-Neptunian object (TNO) in the scattered disk and has a high- eccentricity orbit. Eris was discovered in January 2005 by a Palomar Observatory –based team led by Mike Brown and verified later that year.en.wikipedia.org/wiki/Eris_(dwarf_planet)It is the second-largest known dwarf planet in the Solar System. Eris is slightly smaller than Pluto, but it has more mass than Pluto. It is a " scattered disc object" in the Kuiper belt, further out than Pluto. It is also called a plutoid because the IAU decided to rename all trans-Neptunian dwarf planets as plutoids.simple.wikipedia.org/wiki/Eris_(dwarf_planet)
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Eris (dwarf planet) - Wikipedia
Eris (minor-planet designation: 136199 Eris) is the most massive and second-largest known dwarf planet in the Solar System. It is a trans-Neptunian object (TNO) in the scattered disk and has a high-eccentricity orbit. Eris was discovered in January 2005 by a Palomar Observatory–based team led by … See more
Eris was discovered by the team of Mike Brown, Chad Trujillo, and David Rabinowitz on January 5, 2005, from images taken on October 21, 2003. The discovery was … See more
Eris is a trans-Neptunian dwarf planet. Its orbital characteristics more specifically categorize it as a scattered-disk object (SDO), or a TNO that … See more
In November 2010, Eris was the subject of one of the most distant stellar occultations yet from Earth. Preliminary data from this event cast doubt on previous size estimates. The teams announced their final results from the occultation in October 2011, with an … See more
Eris displays very little variation in brightness as it rotates due to its uniform surface, making measurement of its rotation period difficult. … See more
Eris has an orbital period of 559 years. Its maximum possible distance from the Sun (aphelion) is 97.5 AU, and its closest (perihelion) is 38 AU. As the time of perihelion is defined at the epoch chosen using an unperturbed two-body solution, the further the … See more
The discovery team followed up their initial identification of Eris with spectroscopic observations made at the 8 m Gemini North Telescope in … See more
Wikipedia text under CC-BY-SA license Eris (dwarf planet) - Simple English Wikipedia, the free encyclopedia
Dwarf planet - Wikipedia
Eris | Dwarf Planet, Kuiper Belt, Plutoid | Britannica
WEBSep 29, 2006 · Clark R. Chapman. 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 …
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Eris (Dwarf Planet) Facts
WEBEris is the most massive dwarf planet in the Solar System, exceeding Pluto’s mass by 28%. As such, it was a serious contender to be a tenth planet but failed to meet the criteria set out by the International …
Eris: The First Dwarf Planet | Space
WEBJul 10, 2019 · Eris was one of the first dwarf planets to be discovered in the solar system. It is almost the same size as Pluto, and its discovery directly led to the former ninth planet's demotion. Eris also...
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