Since its discovery in the first half of the 20th century, scientists have puzzled over the
origins of Titan's atmosphere. Current models suggest that atmospheric N 2 on Titan may …

In the present report, by using a series of data gathered by the Cassini-Huygens mission, we
constrain the bulk content of Titan's interior for various gas species (CH 4, CO 2, CO, NH 3 …

Titan's thick N 2–CH 4 atmosphere is unlike any in the Solar System, and its origin has been
shrouded in mystery for over half a century. Here, I perform a detailed analysis of chemical …

The existence of methane in Titan's atmosphere (∼ 6% level at the surface) presents a
unique enigma, as photochemical models predict that the current inventory will be entirely …

Previous investigations have employed more than 100 close observations of Titan by the
Cassini orbiter to elucidate connections between the production and distribution of Titan's …

The solar systems second largest natural satellite is shrouded by a thick nitrogen
atmosphere, rich in methane, within which sunlight-and cosmic-ray-driven organic chemistry …

The present atmosphere of Titan exhibits evidence of extensive evolution, in the form of
rapid photochemical destruction of methane and a large fractionation of the nitrogen and …

Abstract The current Cassini–Huygens Mission to the Saturn system provides compelling
evidence that the present state of Titan's dense atmosphere is unsustainable over the age of …

Titan's moment of inertia (MoI), estimated from the quadrupole gravity field measured by the
Cassini spacecraft, is 0.342, which has been interpreted as evidence of a partially …

Since the discovery of the main composition of Titan's atmosphere, many laboratory
experiments have been carried out to reproduce its chemical evolution, particularly the …