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Synthetic aperture radar image mosaic of Titan's north polar region. Vid Flumina is a river system (termed Flumen) of liquid methane and ethane on Saturn's moon Titan.It is more than 400 km (249 mi) long and flows into Titan's second largest hydrocarbon sea, Ligeia Mare. [1]
The atmosphere of Titan is the dense layer of gases surrounding Titan, the largest moon of Saturn.Titan is the only natural satellite of a planet in the Solar System with an atmosphere that is denser than the atmosphere of Earth and is one of two moons with an atmosphere significant enough to drive weather (the other being the atmosphere of Triton). [4]
In September 2006, Cassini imaged a large cloud at a height of 40 km over Titan's north pole. Although methane is known to condense in Titan's atmosphere, the cloud was more likely to be ethane, as the detected size of the particles was only 1–3 micrometers and ethane can also freeze at these altitudes
Because the tidal period - Titan's day - is long, 16 Earth days, the tidal cycle is slow, so the tidal currents are generally weak," said planetary scientist and study co-author Ralph Lorenz of ...
Titan's dense atmosphere and low gravity mean that the flight power for a given mass is a factor of about 40 times lower than on Earth. [3] The atmosphere has 1.45 times the pressure and about four times the density of Earth's, and local gravity (13.8% of Earth's) make flight easier than on Earth, although cold temperatures, lower light levels ...
This acts to reduce solar energy reaching the surface and lets infrared energy escape, cooling Titan's surface. Titan has both a greenhouse and an anti-greenhouse effect which compete with one another. The greenhouse effect warms Titan by 21 K while the anti-greenhouse effect cools Titan by 9 K, so the net warming is 12 K (= 21 K - 9 K). [3] [4]
Investigate the habitability and potential for life in ocean worlds on both Enceladus and Titan; Investigate Titan as an Earth-like world with an evolving climate and landscape. These goals would be accomplished by measuring the nature, abundance and isotopic properties of solid- and vapor-phase species in Enceladus' plume and Titan's upper ...
Albano Lacus is one of a number of hydrocarbon lakes found on Saturn's largest moon, Titan. [1] The lake is composed of liquid methane and ethane, [2] and was detected by the Cassini space probe. The lake is 6.2 kilometres (3.9 mi) long. The lake is named after Lake Albano in Italy, and the word "lacus" means lake.