Understanding Titan’s planetary boundary layer (PBL) — the lowest region of the atmosphere influenced by surface conditions — remains challenging due to Titan’s thick atmosphere and limited observations.
Huygens
Posted inAstrogeology, Atmospheres, Climate, Weather, Biochemistry & Organic Chemistry, Biosignatures & Paleobiology, Cryobiology, Icy Worlds, Mapping, Geodesy, Cartography, Bathymetry, Missions & Hardware, Press Release, Robotics/Rovers/UAVs, Saturn, Titan, Water/Hycean Worlds & Oceanography
The Top 10 Huygens Discoveries At Titan
On 14 January 2005, at 13:34 CET (12:34 UTC), ESA’s Huygens probe entered the history books by descending to the surface of Titan, Saturn’s largest moon.
Posted inAstrochemistry, Astrogeology, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Cryobiology, Icy Worlds, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Missions & Hardware, Saturn, Status Report, Titan
Titan’s Fluvial and Lacustrine Landscapes
In this chapter we begin with a review of Titan’s fluvial and lacustrine landscapes as observed with Cassini remote sensing data, and what the many discoveries have revealed about Titan’s […]
Posted inAstrochemistry, Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Cryobiology, Exploration Gear & Tech, Icy Worlds, Imaging & Spectroscopy, Saturn, Status Report, Titan
Titan’s Rocks Of Ice – An Interview with Christopher McKay
Huygens sent back only one picture from the surface of Titan. Some people ask, “Are there any more pictures?” They’re used to the Mars rovers, where every day you get […]
