Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …

We present a one-dimensional coupled ion-neutral photochemical kinetics and diffusion
model to study the atmospheric composition of Titan in light of new theoretical kinetics …

The Cassini‐Huygens probe gas chromatograph mass spectrometer (GCMS) determined
the composition of the Titan atmosphere from∼ 140 km altitude to the surface. After landing …

Much of our knowledge of planetary surface composition is derived from remote sensing
over the ultraviolet through infrared wavelength ranges. Telescopic observations and, in the …

We report the identification of compounds on Titan's surface by spatially resolved imaging
spectroscopy methods through Titan's atmosphere, and set upper limits to other organic …

We present a one dimension simulation of Titan's aerosol distribution and compare our
results with the haze optical properties retrieved by the DISR observations (Tomasko, MG …

We have conducted high-pressure experiments in the H2O–CH4 and H2O–CH4–NH3
systems in order to investigate the stability of methane clathrate hydrates, with an optical …

Abstract We present∼ 1.5 Mars Years (MY) of ozone vertical profiles, covering LS= 163° in
MY34 to LS= 320° in MY35, a period which includes the 2018 global dust storm. Since April …

Context. Terrestrial extrasolar planets around low-mass stars are prime targets when
searching for atmospheric biosignatures with current and near-future telescopes. The …

Titan's middle atmosphere is currently experiencing a rapid change of season after northern
spring arrived in 2009 (refs,). A large cloud was observed for the first time above Titan's …