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 …

Nitrogen isotope variations in the Solar System

E Füri, B Marty - Nature Geoscience, 2015 - nature.com
The relative proportion of the two isotopes of nitrogen, 14N and 15N, varies dramatically
across the Solar System, despite little variation on Earth. NASA's Genesis mission directly …

On the origin and evolution of the material in 67P/Churyumov-Gerasimenko

M Rubin, C Engrand, C Snodgrass, P Weissman… - Space science …, 2020 - Springer
Primitive objects like comets hold important information on the material that formed our solar
system. Several comets have been visited by spacecraft and many more have been …

Scientific rationale for Uranus and Neptune in situ explorations

O Mousis, DH Atkinson, T Cavalié, LN Fletcher… - Planetary and Space …, 2018 - Elsevier
The ice giants Uranus and Neptune are the least understood class of planets in our solar
system but the most frequently observed type of exoplanets. Presumed to have a small rocky …

Chemical interactions between Saturn's atmosphere and its rings

JH Waite Jr, RS Perryman, ME Perry, KE Miller, J Bell… - Science, 2018 - science.org
INTRODUCTION Past remote observations of Saturn by Pioneer 11, Voyager 1 and 2, Earth-
based observatories, and the Cassini prime and solstice missions suggested an inflow of …

[HTML][HTML] Mid-infrared mapping of Jupiter's temperatures, aerosol opacity and chemical distributions with IRTF/TEXES

LN Fletcher, TK Greathouse, GS Orton, JA Sinclair… - Icarus, 2016 - Elsevier
Global maps of Jupiter's atmospheric temperatures, gaseous composition and aerosol
opacity are derived from a programme of 5–20 µm mid-infrared spectroscopic observations …

15NH3 in the atmosphere of a cool brown dwarf

D Barrado, P Mollière, P Patapis, M Min, P Tremblin… - Nature, 2023 - nature.com
Brown dwarfs serve as ideal laboratories for studying the atmospheres of giant exoplanets
on wide orbits, as the governing physical and chemical processes within them are nearly …

Jupiter formed as a pebble pile around the N2 ice line

AD Bosman, AJ Cridland, Y Miguel - Astronomy & Astrophysics, 2019 - aanda.org
Context. The region around the H 2 O ice line, due to its higher surface density, seems to be
the ideal location to form planets. The core of Jupiter, as well as the cores of close-in gas …

Isotopic ratios of h, c, n, o, and s in comets c/2012 f6 (lemmon) and c/2014 q2 (lovejoy)

N Biver, R Moreno, D Bockelée-Morvan… - Astronomy & …, 2016 - aanda.org
The apparition of bright comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy) in March-
April 2013 and January 2015, combined with the improved observational capabilities of …

Exploring the hypothesis of an inverted Z gradient inside Jupiter

S Howard, T Guillot, S Markham, R Helled… - Astronomy & …, 2023 - aanda.org
Context. Reconciling models of Jupiter's interior with measurements of the atmospheric
composition still poses a significant challenge. Interior models favour a subsolar or solar …