Eris has a very thin atmosphere
Eris' atmosphere is primarily composed of nitrogen, with trace amounts of methane and possibly other hydrocarbons. It is a thin and cold atmosphere, keeping the dwarf planet's surface largely frozen and inhospitable.
Eris has a very thin atmosphere that is primarily composed of nitrogen and methane gases. Its atmosphere is estimated to be only about 0.12 to 0.2 microbars in pressure, which is significantly less dense than Earth's atmosphere.
Eris is covered in ice because it is located very far from the Sun in the outer solar system. The low temperatures at that distance allow volatile substances like water to freeze and form a thick icy crust on the surface of Eris.
The atmosphere on Eris is composed mainly of nitrogen and methane. The extremely cold temperatures and distance from the sun result in a very thin and tenuous atmosphere.
Eris has a frozen atmosphere.
Eris has a frozen atmosphere.
Eris has a very thin atmosphere
Eris has a frozen atmosphere.
Current scientific thinking suggests that Eris does not have a gaseous atmosphere. Eris is so cold that its atmosphere is frozen!
Eris' atmosphere is primarily composed of nitrogen, with trace amounts of methane and possibly other hydrocarbons. It is a thin and cold atmosphere, keeping the dwarf planet's surface largely frozen and inhospitable.
Eris has a very thin atmosphere that is primarily composed of nitrogen and methane gases. Its atmosphere is estimated to be only about 0.12 to 0.2 microbars in pressure, which is significantly less dense than Earth's atmosphere.
The atmosphere on Eris is composed mainly of nitrogen and methane. The extremely cold temperatures and distance from the sun result in a very thin and tenuous atmosphere.
Eris is covered in ice because it is located very far from the Sun in the outer solar system. The low temperatures at that distance allow volatile substances like water to freeze and form a thick icy crust on the surface of Eris.
we don't know because we want to find out
Eris has a thin atmosphere composed mainly of nitrogen and methane gas. These gases are thought to be released from the surface ice of the dwarf planet due to sunlight reacting with the frozen molecules.
The dwarf planet Eris probably has no atmosphere to speak of. Eris orbits beyond Neptune, in the bitter cold distances from the Sun; most gasses would condense and freeze, and the tenuous vapors that might remain would be too light to be bound by Eris' weak gravity.