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 […]
Titan
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 […]
Implications for growth of organic aerosols by CH3 addition in the atmospheres of Titan and early Earth
Formation of organic aerosols driven by photochemical reactions has been observed and suggested in CH4-containing atmospheres, including Titan and early Earth. However the detailed production and growth mechanisms of organic […]
Possible Organic Precursors in Titan's Hydrocarbon
NASA researchers have confirmed the existence in Titan’s atmosphere of vinyl cyanide, which is an organic compound that could potentially provide the cellular membranes for microbial life to form in […]
Building An Alien Ocean To Test Space Submarines
Building a submarine gets tricky when the temperature drops to -300 Fahrenheit and the ocean is made of methane and ethane.
Cassini Finds Titan Has A Sea Level Like Earth Does
Saturn’s moon Titan may be nearly a billion miles away from Earth, but a recently published paper based on data from NASA’s Cassini spacecraft reveals a new way this distant […]
New Titan Topographic Map
Using the now-complete Cassini data set, Cornell University astronomers have created a new global topographic map of Saturn’s moon Titan that has opened new windows into understanding its liquid flows […]
Atmospheric Circulation, Chemistry, and Infrared Spectra of Titan-like Exoplanets Around Different Stellar Types
With the discovery of ever smaller and colder exoplanets, terrestrial worlds with hazy atmospheres must be increasingly considered. Our Solar System’s Titan is a prototypical hazy planet, whose atmosphere may […]
Role Of The Global Water Ocean On The Evolution of Titan's Primitive Atmosphere
During the accretion of Titan, impact heating may have been sufficient to allow the global melting of water ice and the release of volatile compounds, mainly constituted of CO2, CH4 […]
Cloud Of Hydrogen Cyanide and Benzene Found On Titan
Researchers with NASA’s Cassini mission found evidence of a toxic hybrid ice in a wispy cloud high above the south pole of Saturn’s largest moon, Titan. The finding is a […]
