Titan's atmosphere and climate
SM Hörst - Journal of Geophysical Research: Planets, 2017 - Wiley Online Library
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 …
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …
Critical review of N, N+, N+ 2, N++, and N++ 2 main production processes and reactions of relevance to Titan's atmosphere
This paper is a detailed critical review of the production processes and reactions of N, N+,
N+ 2, N++, and N++ 2 of relevance to Titan's atmosphere. The review includes neutral, ion …
N+ 2, N++, and N++ 2 of relevance to Titan's atmosphere. The review includes neutral, ion …
Simulating the density of organic species in the atmosphere of Titan with a coupled ion-neutral photochemical model
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 …
model to study the atmospheric composition of Titan in light of new theoretical kinetics …
The cosmic shoreline: The evidence that escape determines which planets have atmospheres, and what this may mean for Proxima Centauri B
KJ Zahnle, DC Catling - The Astrophysical Journal, 2017 - iopscience.iop.org
The Cosmic Shoreline: The Evidence that Escape Determines which Planets Have Atmospheres,
and what this May Mean for Proxima Centauri B - IOPscience This site uses cookies. By …
and what this May Mean for Proxima Centauri B - IOPscience This site uses cookies. By …
[HTML][HTML] Toward RNA life on early Earth: From atmospheric HCN to biomolecule production in warm little ponds
The origin of life on Earth involves the early appearance of an information-containing
molecule such as RNA. The basic building blocks of RNA could have been delivered by …
molecule such as RNA. The basic building blocks of RNA could have been delivered by …
The neutral photochemistry of nitriles, amines and imines in the atmosphere of Titan
The photochemistry of N 2 and CH 4 in the atmosphere of Titan leads to a very rich
chemistry which is not well understood. The aim of our study is to improve our understanding …
chemistry which is not well understood. The aim of our study is to improve our understanding …
Aerosol growth in Titan's ionosphere
P Lavvas, RV Yelle, T Koskinen… - Proceedings of the …, 2013 - National Acad Sciences
Photochemically produced aerosols are common among the atmospheres of our solar
system and beyond. Observations and models have shown that photochemical aerosols …
system and beyond. Observations and models have shown that photochemical aerosols …
Structure and composition of Pluto's atmosphere from the New Horizons solar ultraviolet occultation
The Alice instrument on NASA's New Horizons spacecraft observed an ultraviolet solar
occultation by Pluto's atmosphere on 2015 July 14. The transmission vs. altitude was …
occultation by Pluto's atmosphere on 2015 July 14. The transmission vs. altitude was …
The photochemical production of aromatics in the atmosphere of Titan
The photochemical processes at work in the atmosphere of Titan are very complex and lead
to a great variety of compounds with aerosols as an end-product. One of the most complex …
to a great variety of compounds with aerosols as an end-product. One of the most complex …
Chemical composition of Titan's atmosphere and ionosphere: Observations and the photochemical model
VA Krasnopolsky - Icarus, 2014 - Elsevier
Basic observational data on hydrocarbons, nitriles, and ions on Titan are compared with
predictions of the photochemical model. Uncertainties of the observed abundances and …
predictions of the photochemical model. Uncertainties of the observed abundances and …