Titan’s abundant lakes and seas exchange methane vapor and energy with the atmosphere via a process generally known as air-sea interaction. This turbulent exchange process is investigated with an atmospheric […]
Titan
Photoreactivity Of Condensed Acetylene On Titan Aerosols Analogues
Volatile organic molecules formed by photochemistry in the upper atmosphere of Titan can undergo condensation as pure ices in the stratosphere and the troposphere as well as condense as ice […]
An Intense Thermospheric Jet on Titan
Winds in Titan’s lower and middle atmosphere have been determined by a variety of techniques. These techniques include direct measurements from the Huygens Probe over 0-150 km, Doppler shifts of […]
Nitrogen-containing Anions and Tholin Growth in Titan's Ionosphere: Implications for Cassini CAPS-ELS Observations
The Cassini Plasma Spectrometer (CAPS) Electron Spectrometer (ELS) instrument onboard Cassini revealed an unexpected abundance of negative ions above 950 km in Titan’s ionosphere. In situ measurements indicated the presence […]
Seasonal Evolution of Temperatures In Titan's Lower Stratosphere
The Cassini mission offered us the opportunity to monitor the seasonal evolution of Titan’s atmosphere from 2004 to 2017, i.e. half a Titan year. The lower part of the stratosphere […]
Evidence of Changing Seasons And Rain On Titan's North Pole
An image from the international Cassini spacecraft provides evidence of rainfall on the north pole of Titan, the largest of Saturn’s moons. The rainfall would be the first indication of […]
Quantitative Estimates of Chemical Disequilibrium in Titan's Atmosphere
We apply previously introduced measures of chemical disequilibrium to Cassini mass spectroscopy data on the atmosphere of Titan. In the analysis presented here, we use an improved description, avoiding the […]
Cutting Through The Mystery of Titan's Atmospheric Haze
A team including Berkeley Lab scientists homes in on a ‘missing link’ in Titan’s one-of-a-kind chemistry. Saturn’s largest moon, Titan, is unique among all moons in our solar system for […]
A possible deep CH4 reservoir in Titan, Super-Titan exoplanets and moons
We investigate the thermal equation of state, bulk modulus, thermal expansion coefficient, and heat capacity of MH-III (CH4 filled-ice Ih), needed for the study of CH4 transport and outgassing for […]
Detection Opportunity For Aromatic Signature in Titan's Aerosols In The 4.1 to 5.3 Micron Range
The Cassini/Huygens mission provided new insights on the chemistry of the upper atmosphere of Titan. The presence of large molecules and ions (>100 s of amu) detected by Cassini at […]
