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'''Eris''', formal designation '''136199 Eris''', is the most massive known dwarf planet in the [http://aliens.wikia.com/wiki/Sol_System Sol System] and the ninth most massive body known to orbit the [http://aliens.wikia.com/wiki/Sun Sun] directly. It is estimated to be approximately 2300–2400 km in diameter, and 27% more massive than Pluto or about 0.27% of the Earth's mass. [[File:240px-Eris_and_dysnomia2.jpg|thumb|A picture of Eris (Center) and its moon Dysnomia (Left of Center).]]
 
'''Eris''', formal designation '''136199 Eris''', is the most massive known dwarf planet in the [http://aliens.wikia.com/wiki/Sol_System Sol System] and the ninth most massive body known to orbit the [http://aliens.wikia.com/wiki/Sun Sun] directly. It is estimated to be approximately 2300–2400 km in diameter, and 27% more massive than Pluto or about 0.27% of the Earth's mass. [[File:240px-Eris_and_dysnomia2.jpg|thumb|A picture of Eris (Center) and its moon Dysnomia (Left of Center).]]
   
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 and has one known moon, Dysnomia. As of 2011, its distance from the Sun is 96.6 AU, roughly three times that of Pluto. With the exception of some comets, Eris and Dysnomia are currently the most distant known natural objects in the Solar System.
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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 and has one known moon, [[Dysnomia]]. As of 2011, its distance from the Sun is 96.6 AU, roughly three times that of Pluto. With the exception of some comets, Eris and Dysnomia are currently the most distant known natural objects in the Solar System.
   
 
Because Eris appeared possibly to be larger than Pluto, its discoverers and NASA [[File:Outer_Solar_system.png|thumb|304px|This map shows 4 worlds, Neptune (Representing the inner Solar system or helio sphere region) ,Pluto and Eris (Representing the Kuipler belt region) and finally Sedna (Representing the Sednoids sub-region of the Kupler belt). The Map is titled to show the Galactic plane Edge on in the foreground for instance Neptune's orbit in center is relatively where the 8 main planters are including Earth and Neptune. Pluto and Eris are also shown for scale. Sedna is the red colored orbit. ]]initially described it as the Solar System’s tenth planet. This, along with the prospect of other similarly sized objects being discovered in the future, motivated the International Astronomical Union [[File:2007OR10-orbit.png|thumb]](IAU) to define the term planet for the first time. Under the IAU definition approved on August 24, 2006, Eris is a "dwarf planet" along with [[Pluto]], [[Ceres]], [[Haumea]] and [[Makemake]].
 
Because Eris appeared possibly to be larger than Pluto, its discoverers and NASA [[File:Outer_Solar_system.png|thumb|304px|This map shows 4 worlds, Neptune (Representing the inner Solar system or helio sphere region) ,Pluto and Eris (Representing the Kuipler belt region) and finally Sedna (Representing the Sednoids sub-region of the Kupler belt). The Map is titled to show the Galactic plane Edge on in the foreground for instance Neptune's orbit in center is relatively where the 8 main planters are including Earth and Neptune. Pluto and Eris are also shown for scale. Sedna is the red colored orbit. ]]initially described it as the Solar System’s tenth planet. This, along with the prospect of other similarly sized objects being discovered in the future, motivated the International Astronomical Union [[File:2007OR10-orbit.png|thumb]](IAU) to define the term planet for the first time. Under the IAU definition approved on August 24, 2006, Eris is a "dwarf planet" along with [[Pluto]], [[Ceres]], [[Haumea]] and [[Makemake]].

Revision as of 06:16, April 8, 2016

Eris, formal designation 136199 Eris, is the most massive known dwarf planet in the Sol System and the ninth most massive body known to orbit the Sun directly. It is estimated to be approximately 2300–2400 km in diameter, and 27% more massive than Pluto or about 0.27% of the Earth's mass.
240px-Eris and dysnomia2

A picture of Eris (Center) and its moon Dysnomia (Left of Center).

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 and has one known moon, Dysnomia. As of 2011, its distance from the Sun is 96.6 AU, roughly three times that of Pluto. With the exception of some comets, Eris and Dysnomia are currently the most distant known natural objects in the Solar System.

Because Eris appeared possibly to be larger than Pluto, its discoverers and NASA
Outer Solar system

This map shows 4 worlds, Neptune (Representing the inner Solar system or helio sphere region) ,Pluto and Eris (Representing the Kuipler belt region) and finally Sedna (Representing the Sednoids sub-region of the Kupler belt). The Map is titled to show the Galactic plane Edge on in the foreground for instance Neptune's orbit in center is relatively where the 8 main planters are including Earth and Neptune. Pluto and Eris are also shown for scale. Sedna is the red colored orbit.

initially described it as the Solar System’s tenth planet. This, along with the prospect of other similarly sized objects being discovered in the future, motivated the International Astronomical Union
2007OR10-orbit
(IAU) to define the term planet for the first time. Under the IAU definition approved on August 24, 2006, Eris is a "dwarf planet" along with Pluto, Ceres, Haumea and Makemake.

In 2010, preliminary results from observations of a stellar occultation by Eris on November 6 suggested that its diameter may be only 2320 km, which would make it almost the same size as Pluto. Given the error bars in the different size estimates, it is currently uncertain whether Eris or Pluto has the larger diameter. Both Pluto and Eris are estimated to have solid-body diameters of about 2330 km.

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