Uh–Was it Saturn’s Titan, or Neptune’s Triton that Voyager 2 explored in 1989? (Answer below)

Watch this VIDEO: 1 min. 56 sec., and you will see how spectography clarifies topography of a planet, and simplifies identification of geological processes at work. This video identifies how Titan’s cryovolcano, Sotra Facula, was identified, and is known by spectographic analysis to erupt a frozen mixture of water, ammonia, methane and ethane. In 2005, another cryovolcano, Sotra Patera, was felt to be another clear example of a cryovolcano.

However, Titan’s hypothesized cryovolcanism has subsequently been questioned. See this article.

(ANSWER: It was Tritan (Neptune’s moon) that Voyager 2 explored in 1989. The video below is about Saturn’s moon, Titan.)

Notes from this video on Youtube state:

Uploaded on Dec 14, 2010

NASA’s Cassini spacecraft has found possible ice volcanoes on Saturn’s moon Titan that are similar in shape to those on Earth that spew molten rock.

Topography and surface composition data have enabled scientists to make the best case yet in the outer solar system for an Earth-like volcano landform that erupts in ice. The results were presented today at the American Geophysical Union meeting in San Francisco.

“When we look at our new 3-D map of Sotra Facula on Titan, we are struck by its resemblance to volcanoes like Mt. Etna in Italy, Laki in Iceland and even some small volcanic cones and flows near my hometown of Flagstaff,” said Randolph Kirk, who led the 3-D mapping work, and is a Cassini radar team member and geophysicist at the U.S. Geological Survey (USGS) Astrogeology Science Center in Flagstaff, Ariz.

Scientists have been debating for years whether ice volcanoes, also called cryovolcanoes, exist on ice-rich moons, and if they do, what their characteristics are. The working definition assumes some kind of subterranean geological activity warms the cold environment enough to melt part of the satellite’s interior and sends slushy ice or other materials through an opening in the surface. Volcanoes on Jupiter’s moon, Io, and Earth spew silicate lava.

Some cryovolcanoes bear little resemblance to terrestrial volcanoes, such as the tiger stripes at Saturn’s moon, Enceladus, where long fissures spray jets of water and icy particles that leave little trace on the surface. At other sites, eruption of denser materials might build up volcanic peaks or finger-like flows. But when such flows were spotted on Titan in the past, theories explained them as non-volcanic processes, such as rivers depositing sediment. At Sotra, however, cryovolcanism is the best explanation for two peaks more than 1,000 meters (3,000 feet) high with deep volcanic craters and finger-like flows.

“This is the very best evidence, by far, for volcanic topography anywhere documented on an icy satellite,” said Jeffrey Kargel, a planetary scientist at the University of Arizona, Tucson. “It’s possible the mountains are tectonic in origin, but the interpretation of cryovolcano is a much simpler, more consistent explanation.”

Kirk and colleagues analyzed new Cassini radar images. His USGS group created the topographic map and 3-D flyover images of Sotra Facula. Data from Cassini’s visual and infrared mapping spectrometer revealed the lobed flows had a composition different from the surrounding surface. Scientists have no evidence of current activity at Sotra, but they plan to monitor the area.

“Cryovolcanoes help explain the geological forces sculpting some of these exotic places in our solar system,” said Linda Spilker, Cassini project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “At Titan, for instance, they explain how methane can be continually replenished in the atmosphere when the sun is constantly breaking that molecule down.”

To see two theories of how cryovolcanism works, visit the next page.