Eris: The Dwarf Planet That Redefined Our Solar System

Eris: The Dwarf Planet

Discover the celestial body that challenged our understanding of the solar system and led to Pluto's reclassification

What is Eris?

Eris is a dwarf planet located in the scattered disc of our solar system, beyond the orbit of Neptune. It was discovered in 2005 by a team of astronomers led by Mike Brown at the Palomar Observatory.

Initially thought to be larger than Pluto, Eris's discovery sparked a debate in the astronomical community about what constitutes a planet, ultimately leading to the reclassification of Pluto as a dwarf planet in 2006.

Eris is named after the Greek goddess of strife and discord, reflecting the controversy its discovery caused in the scientific community regarding the definition of a planet.

Artistic representation of Eris

Artistic representation of Eris and its surface features

Discovery and Naming

Palomar Observatory where Eris was discovered

Palomar Observatory where Eris was discovered

Eris was discovered on January 5, 2005, from data collected on October 21, 2003. The discovery was announced on July 29, 2005, the same day as two other large trans-Neptunian objects: Haumea and Makemake.

The team that discovered Eris consisted of Mike Brown, Chad Trujillo, and David Rabinowitz. They used the Samuel Oschin telescope at Palomar Observatory in California.

Initially designated as 2003 UB313, the object was later named Eris after the Greek goddess of strife and discord. Its moon was named Dysnomia, after the daughter of Eris and the demon goddess of lawlessness.

October 21, 2003

First images of Eris captured by the Samuel Oschin telescope

January 5, 2005

Eris officially discovered during re-analysis of the 2003 data

July 29, 2005

Discovery announced to the public along with Haumea and Makemake

September 13, 2006

Officially named Eris by the International Astronomical Union

Physical Characteristics

Eris is one of the largest known dwarf planets in our solar system. It has a highly eccentric orbit that takes it from 38 AU to 97 AU from the Sun, with an orbital period of about 557 years.

Eris has one known moon, Dysnomia, which was discovered in September 2005. The presence of this moon helped astronomers determine Eris's mass through Kepler's third law.

The surface of Eris is highly reflective, suggesting it's covered with methane ice. Its high albedo (reflectivity) makes it one of the brightest objects in the solar system.

Eris's Orbit Sun Eris Dysnomia Diagram showing Eris's orbit and its moon Dysnomia

Diagram showing Eris's orbit and its moon Dysnomia

Size and Mass

Diameter: Approximately 2,326 km (slightly smaller than Pluto)

Mass: 1.66 × 10²² kg (about 27% more massive than Pluto)

Density: 2.43 g/cm³

Orbital Characteristics

Average distance from Sun: 68 AU

Orbital period: 557 Earth years

Orbital eccentricity: 0.44 (highly elliptical)

Physical Properties

Surface temperature: ≈ -243°C

Albedo: 0.96 (very reflective)

Rotation period: 25.9 hours

Comparing Dwarf Planets

Eris

Diameter: 2,326 km

Mass: 1.66×10²² kg

Orbital Period: 557 years

Moons: 1 (Dysnomia)

Pluto

Diameter: 2,377 km

Mass: 1.30×10²² kg

Orbital Period: 248 years

Moons: 5

Haumea

Diameter: 1,632 km

Mass: 4.01×10²¹ kg

Orbital Period: 283 years

Moons: 2

Impact on Planetary Science

The discovery of Eris had a profound impact on our understanding of the solar system. Initially thought to be larger than Pluto, it raised the question: if Pluto is a planet, shouldn't Eris be one too?

This debate led the International Astronomical Union (IAU) to formally define the term "planet" for the first time in 2006. According to the new definition, a planet must:

  • Orbit the Sun
  • Be massive enough to be rounded by its own gravity
  • Have cleared the neighborhood around its orbit

Since Eris, like Pluto, has not cleared its orbital neighborhood, both were classified as dwarf planets. This reclassification demoted Pluto from its status as the ninth planet.

Solar System The 2006 IAU meeting that redefined what constitutes a planet

The 2006 IAU meeting that redefined what constitutes a planet