Habitability of planets on eccentric orbits: Limits of the mean flux approximation

E Bolmont, AS Libert, J Leconte, F Selsis - Astronomy & Astrophysics, 2016 - aanda.org
Unlike the Earth, which has a small orbital eccentricity, some exoplanets discovered in the
insolation habitable zone (HZ) have high orbital eccentricities (eg, up to an eccentricity of …

Gas-grain model of carbon fractionation in dense molecular clouds

JC Loison, V Wakelam, P Gratier… - Monthly Notices of the …, 2020 - academic.oup.com
Carbon containing molecules in cold molecular clouds show various levels of isotopic
fractionation through multiple observations. To understand such effects, we have developed …

Cassini-Huygens' exploration of the Saturn system: 13 years of discovery

L Spilker - Science, 2019 - science.org
The Cassini-Huygens mission to Saturn provided a close-up study of the gas giant planet, as
well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in …

Detection of propene in Titan's stratosphere

CA Nixon, DE Jennings, B Bezard… - The Astrophysical …, 2013 - iopscience.iop.org
ABSTRACT The Voyager 1 flyby of Titan in 1980 gave a first glimpse of the chemical
complexity of Titan's atmosphere, detecting many new molecules with the infrared …

Is Titan's shape caused by its meteorology and carbon cycle?

M Choukroun, C Sotin - Geophysical Research Letters, 2012 - Wiley Online Library
Titan's shape is characterized by a difference between the long equatorial radius and the
polar radius that is several hundred meters larger than that predicted by the flattening due to …

Decomposition of Benzene during Impacts in N2-dominated Atmospheres

L Petera, A Knížek, V Laitl, M Ferus - The Astrophysical Journal, 2023 - iopscience.iop.org
Benzene is a simple neutral aromatic compound found in molecular clouds, comets, and
planetary atmospheres. It has been confirmed on Jupiter, Saturn, Titan, and is expected on …

Titan's interior structure and dynamics after the Cassini-Huygens mission

C Sotin, K Kalousová, G Tobie - Annual Review of Earth and …, 2021 - annualreviews.org
The Cassini-Huygens mission that explored the Saturn system during the period 2004–2017
revolutionized our understanding of Titan, the only known moon with a dense atmosphere …

Doubly-charged ions in the planetary ionospheres: a review

R Thissen, O Witasse, O Dutuit, CS Wedlund… - Physical Chemistry …, 2011 - pubs.rsc.org
This paper presents a review of the current knowledge on the doubly-charged atomic and
molecular positive ions in the planetary atmospheres of the Solar System. It is focused on …

Contributions from accreted organics to Titan's atmosphere: new insights from cometary and chondritic data

KE Miller, CR Glein, JH Waite - The Astrophysical Journal, 2019 - iopscience.iop.org
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 …

Identifiable acetylene features predicted for young earth-like exoplanets with reducing atmospheres undergoing heavy bombardment

PB Rimmer, M Ferus, IP Waldmann… - The Astrophysical …, 2019 - iopscience.iop.org
The chemical environments of young planets are assumed to be largely influenced by the
impacts of bodies lingering on unstable trajectories after the dissolution of the protoplanetary …