Doom Mons, one of the most reliably identified cryovolcanoes on Saturn's moon Titan
Pictured in 2012 in natural color. The thick atmosphere is orange due to a dense haze.
Plumes of Enceladus, feeding Saturn's E Ring, seem to arise from the "Tiger Stripes" near the south pole.
Christiaan Huygens discovered Titan in 1655.
William Lassell, the discoverer of Triton
Titan's orbit (highlighted in red) among the other large inner moons of Saturn. The moons outside its orbit are (from the outside to the inside) Iapetus and Hyperion; those inside are Rhea, Dione, Tethys, Enceladus, and Mimas.
The orbit of Triton (red) is opposite in direction and tilted −23° compared to a typical moon's orbit (green) in the plane of Neptune's equator.
True-color image of layers of haze in Titan's atmosphere
Animation of Triton
Trace organic gases in Titan's atmosphere—HNC (left) and HC3N (right).
The Kuiper belt (green), in the Solar System's outskirts, is where Triton is thought to have originated.
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Artist's impression of Triton, showing its tenuous atmosphere just over the limb.
Methane clouds (animated; July 2014).
Clouds observed above Triton's limb by Voyager 2.
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Interpretative geomorphological map of Triton
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Triton's bright south polar cap above a region of cantaloupe terrain
False-color Cassini radar mosaic of Titan's north polar region. Blue coloring indicates low radar reflectivity, caused by hydrocarbon seas, lakes and tributary networks filled with liquid ethane, methane and dissolved . About half of the large body at lower left, Kraken Mare, is shown. Ligeia Mare is at lower right.
Cantaloupe terrain viewed from 130,000 km by Voyager 2, with crosscutting Europa-like double ridges. Slidr Sulci (vertical) and Tano Sulci form the prominent "X".
Mosaic of three Huygens images of channel system on Titan
Tuonela Planitia (left) and Ruach Planitia (center) are two of Triton's cryovolcanic "walled plains". The paucity of craters is evidence of extensive, relatively recent, geologic activity.
Rimmed lakes of Titan (artist concept)
NASA illustration detailing the studies of the proposed Trident mission
Near-infrared radiation from the Sun reflecting off Titan's hydrocarbon seas
Neptune (top) and Triton (bottom) three days after flyby of Voyager 2
Radar image of a 139 km-diameter impact crater on Titan's surface, showing a smooth floor, rugged rim, and possibly a central peak.
thumb|Close up of the volcanic province of Leviathan Patera, the caldera in the center of the image. Several pit chains extend radially from the caldera to the right of the image, while the smaller of the two cryolava lakes is seen to the upper left. Just off-screen to the lower left is a fault zone aligned radially with the caldera, indicating a close connection between the tectonics and volcanology of this geologic unit.
Ligeia Mare – SAR and clearer despeckled views.
thumb|Dark streaks across Triton's south polar cap surface, thought to be dust deposits left by eruptions of nitrogen geysers
Near-infrared image of Tortola Facula, thought to be a possible cryovolcano
thumb|Two large cryolava lakes on Triton, seen west of Leviathan Patera. Combined, they are nearly the size of Kraken Mare on Titan. These features are unusually crater free, indicating they are young and were recently molten.
False-color VIMS image of the possible cryovolcano Sotra Patera, combined with a 3D map based on radar data, showing 1000-meter-high peaks and a 1500-meter-deep crater.
Sand dunes in the Namib Desert on Earth (top), compared with dunes in Belet on Titan
Titan - three dust storms detected in 2009–2010.
Voyager 1 view of haze on Titan's limb (1980)
Cassini's Titan flyby radio signal studies (artist's concept)
The balloon proposed for the Titan Saturn System Mission (artistic rendition)
Global map of Titan – with IAU labels (August 2016).
Titan – infrared views (2004–2017)
Titan's North Pole (2014)
Titan's South Pole (2014)

Triton is one of the few moons in the Solar System known to be geologically active (the others being Jupiter's Io and Europa, and Saturn's Enceladus and Titan).

- Triton (moon)

A number of features have been identified as possible cryovolcanoes on Pluto, Titan and Ceres, and a subset of domes on Europa may have cryovolcanic origins.

- Cryovolcano

In addition, although they are not known to form volcanoes, ice geysers have been observed on Enceladus and potentially Triton.

- Cryovolcano

Intricate cryovolcanic and tectonic terrains suggest a complex geological history.

- Triton (moon)

The geologically young surface is generally smooth, with few impact craters, although mountains and several possible cryovolcanoes have been found.

- Titan (moon)

It is second in terms of relative diameter of moons to a gas giant; Titan being 1/22.609 of Saturn's diameter, Triton is larger in diameter relative to Neptune at 1/18.092.

- Titan (moon)
Doom Mons, one of the most reliably identified cryovolcanoes on Saturn's moon Titan

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