Neptune's Moon Triton
Triton From The Hubble Space Telescope
This image of Triton was taken by the Hubble Space Telescope's Faint Object Camera in September of 1995.  It was created from a blue and ultraviolet image.  The color is false but closely matches the color observed from voyager images. Triton appears to be roughly 10% darker than in images taken by the Voyager 2 spacecraft. Also note that the equatorial region is bright, but there is a darker region around the pole.  With Triton's long seasons, the southern summer has been progressing, and the south pole has received increasing sunlight; thus, it is probable that much of the frost covering the region in 1989 has evaporated, some of which may have condensed at the equator (hence the bright region there).  This image truly pushes the limit of HST's resolving power.  The image is centered at roughly 215 degrees latitude. (Courtesy of Ted Stryk)
South Pole of Triton
This high resolution image of Triton was obtained by Voyager 2 on August 25, 1989.  It shows the moon's south polar cap.  One of the unusual aspect of this image is the dark streaks in the images.  Perhaps they were made by geyser-like eruptions of nitrogen. The geyser eruptions could have carried darker materials from the crust. The light regions probably consist of layers of nitrogen. (Credit: Calvin J. Hamilton)
Triton in 3D
This is a computer-generated perspective rendering of one of the caldera -like depressions on Triton, as it would appear if viewed from the northeast. The image was obtained Aug. 24, 1989, when the Voyager spacecraft was about 181,800 kilometers  (112,900 miles) from Triton. The caldera floor shown in this image is approximately  200 kilometers (120 miles) in diameter. It is extremely flat and probably was formed by the volcanic eruption of ice lavas of very low viscosity. The bench visible in the foreground may be a remnant of earlier flooding to a level about 200 meters (600 feet) higher than the present caldera floor. (Courtesy NASA/JPL)
Surface of Triton
This is one of the most detailed views of the surface  of Triton taken by Voyager 2 on its flyby of the large satellite of        Neptune early in the morning of August 25, 1989. The picture was taken from a distance of 40,000 kilometers (25,000 miles), the frame is about 220 kilometers (140      miles) across and shows details as small as 750 meters (0.5 miles). Most   of the area is covered by a peculiar landscape of roughly circular         depressions separated by rugged ridges. This type of terrain, which covers large tracts of Triton's northern hemisphere, is unlike anything seen      elsewhere in the solar system. The depressions are probably not impact     craters: They are too similar in size and too regularly spaced. Their      origin is still unknown, but may involve local melting and collapse of the icy surface. A conspicuous set of grooves and ridges cuts across the       landscape, indicating fracturing and deformation of Triton's surface. The  rarity of impact craters suggests a young surface by solarsystem           standards, probably less than a few billion years old. (Courtesy NASA/JPL)
Dark Areas on Triton
Voyager 2 acquired this black and white image of       Triton during the night of August 24-25, 1989. Triton's limb cuts obliquely across the middle of the image. The field of  view is about 1,000 km (600 miles) across. Three irregular dark areas,     surrounded by brighter material, dominate the image. Low-lying material    with intermediate albedo occupies the central area, and fresh craters      occur along the right margin. Sub-parallel alignment of linear patches of  dark material shown in the lower and left part of the image suggests that  the patches are structurally controlled. (Courtesy NASA/JPL)
Post Encounter Images of Triton
This set of images shows the best views of Neptune's moon Triton taken by Voyager 2 as the spacecraft withdrew from the Neptune system on August 25, 1989. The top four images were constructed from various color image bands as Voyager receded from Triton. (Courtesy Ted Stryk)
Montage of Neptune and Triton
This computer generated montage shows Neptune as it    would appear from a spacecraft approaching Triton. The wind- and sublimation-eroded south polar cap of Triton is shown at the bottom of the Triton image, a cryovolcanic terrain at the upper right, and the enigmatic cantaloupe terrain at the upper left. Triton's surface is mostly covered by nitrogen frost mixed with traces of condensed methane, carbon dioxide, and carbon monoxide. The tenuous atmosphere of Triton, though only about one-hundredth of one percent of Earth's atmospheric density at the surface, is thick enough to produce wind-deposited streaks of dark and bright materials of unknown composition in the south polar cap region. The southern polar cap was sublimating at the time of the Voyager 2 flyby, as indicated by the irregular and eroded appearance of the edge of the cap. The polar frosts were sublimating because Triton's orbital and rotational motion causes the sun to shine directly on the polar cap for a period of several decades during Neptune's and Triton's long austral summer. Though the polar cap was undergoing heat death, surface temperatures still were only about 38 K (-391 degrees Farenheit). (Courtesy NASA/JPL)
Neptune on Triton's Horizon
Composite view showing Neptune on Triton's horizon. Neptune's south pole is to the left; clearly visible in the planets' southern hemisphere is a Great Dark Spot, a large anticyclonic storm system located about 20 degrees South. The foreground is a computer generated view of Triton's maria as they would appear from a point approximately 45 km above the surface. The terraces visible in this image indicate multiple episodes of 'cryovolcanic' flooding. This three-dimensional view was created from a Voyager image by using a two-dimensional photoclinometric model. Relief has been exaggerated roughly 30-fold, the actual range of the relief is about 1 km. Would Neptune appear to be rising or setting? Neither, due to the motion of Triton relative to Neptune, it would appear to move laterally along the horizon, eventually rising and setting at high latitudes. (Courtesy NASA/JPL)