Search results
Results From The WOW.Com Content Network
An image of Titan's surface from the Huygens lander. Titan is the only object in the outer Solar System where a spacecraft has landed and conducted surface operations. The geology of Titan encompasses the geological characteristics of Titan, the largest moon of Saturn. Titan's density of 1.881 g/cm 3 indicates that it is roughly 40–60% rock ...
Huygens in situ image from Titan's surface—the only image from the surface of a body permanently farther away than Mars Same image with contrast enhanced Huygens was an atmospheric probe that touched down on Titan on January 14, 2005, [ 114 ] discovering that many of its surface features seem to have been formed by fluids at some point in the ...
This is a list of named geological features on Saturn's moon Titan. Official names for these features have only been announced since the 2000s, as Titan's surface was virtually unknown before the arrival of the Cassini–Huygens probe. [1] [2] Some features were known by informal nicknames beforehand; these names are noted where appropriate ...
Huygens (/ ˈ h ɔɪ ɡ ən z / HOY-gənz) was an atmospheric entry robotic space probe that landed successfully on Saturn's moon Titan in 2005. Built and operated by the European Space Agency (ESA), launched by NASA, it was part of the Cassini–Huygens mission and became the first spacecraft to land on Titan and the farthest landing from Earth a spacecraft has ever made. [3]
Titan, shrouded in a smog-like orange haze, is the only known world other than Earth exhibiting liquid seas on the surface, though they are not composed of water but rather nitrogen and the ...
Kraken Mare / ˈ k r ɑː k ən ˈ m ɑːr eɪ / is the largest known hydrocarbon sea on the surface of Saturn's moon Titan.It was discovered by the space probe Cassini in 2006, and was named in 2008 after the Kraken, a legendary sea monster. [1]
Ligeia Mare / l aɪ ˈ dʒ iː ə ˈ m ɑːr eɪ / [2] is a lake in the north polar region of Titan, the planet Saturn's largest moon. It is the second largest body of liquid on the surface of Titan, after Kraken Mare. [3]
Radar images of Titan's surface show that Mayda Insula's coasts display evidence of being changed by fluvial and lacustrine processes. [7] Analyses of these fluvial features suggested that approximately 2 km 3 of material has been eroded from Mayda Insula and deposited elsewhere in the Kraken Mare basin.