Triton (moon)

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Triton
The orbit of Triton (red) is different from most moons' orbit (green) in the movement's direction, and the orbit is tilted
Retrograde orbit: the satellite (red) orbits in the direction opposite to the rotation of its primary (blue/black)
The Kuiper belt (green), in the Solar System's outskirts, is where Triton is thought to have originated.

Triton, or Neptune I, is the largest moon of the planet Neptune.[1][2] It is the seventh largest moon in the Solar System. Triton is slightly smaller than Earth's Moon. Triton has a complicated geological history and it is thought to have a comparatively young surface compared to the age of the Solar System itself.

It was discovered by the British astronomer William Lassell on 10 October 1846, just 17 days after Neptune itself was discovered by the German astronomer Johann Gottfried Galle and Heinrich Louis d'Arrest.[1]

Triton is believed to be a captured Kuiper Belt object,[1] and is the coldest known body in the Solar System.[1] The surface temperature of Triton was recorded by Voyager 2 as -235°C (-391°F).[1]. Triton has its own magnetic field and has a faint trace of an atmosphere.

Orbit[change | change source]

Drag and tidal interaction cause Triton to fall into a lower orbit. This process is immensely slow. 3.6 billion years from now, Triton will pass within Neptune's Roche limit.[3] It will either collide with Neptune's atmosphere or break up, forming a ring system similar to that found around Saturn.[3]

The reason why Triton is thought to be a captured object is its orbit, which is unique in the Solar System. It is both retrograde (see diagram) and highly tilted. Although there are other satellites with retrograde orbits, they are much smaller than Titan, and much more distant from their host planets (their "primaries"). Triton, like our Moon, shows only one face to the planet: it rotates in synchrony to Neptune.

Surface[change | change source]

All we know about the surface of Titan comes from one fly-by of Voyager 2 in 1989. There are few impact craters. This suggests the surface is quite young: estimates are six to 50 million years.[4]

Despite its very cold temperature, the surface of Triton is geologically active. There are events which look like geysers, volcanos and earthquakes. All the materials involved are quite different from those on Earth. Most of the gases are frozen most of the time. Gases like nitrogen are frozen until something occurs to melt them, then it turns back into a gas. A temperature increase of just 4° K is enough to make this happen.

References[change | change source]

  1. 1.0 1.1 1.2 1.3 1.4 "NASA: Solar System Exploration: Planets: Neptune: Moons: Triton". NASA. http://solarsystem.nasa.gov/planets/profile.cfm?Object=Nep_Triton. Retrieved 2011-03-29.
  2. "BBC Home: Science: Space: Solar System: Moons: Triton". BBC. http://www.bbc.co.uk/science/space/solarsystem/moons/triton_(moon). Retrieved 2011-03-29.
  3. 3.0 3.1 Chyba C.F; Jankowski D.G. & Nicholson P.D. 1989. Tidal evolution in the Neptune-Triton system. Astronomy and Astrophysics 219 (1–2): L23–L26. [1]
  4. Schenk, Paul M. & Zahnle, Kevin 2007. On the negligible surface age of Triton. Icarus 192 (1): 135–49. [2]

Other websites[change | change source]