Scientific discovery with the James Webb space telescope
J Kalirai - Contemporary Physics, 2018 - Taylor & Francis
For the past 400 years, astronomers have sought to observe and interpret the Universe by
building more powerful telescopes. These incredible instruments extend the capabilities of …
building more powerful telescopes. These incredible instruments extend the capabilities of …
Scientific rationale for Uranus and Neptune in situ explorations
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 …
system but the most frequently observed type of exoplanets. Presumed to have a small rocky …
The case and context for atmospheric methane as an exoplanet biosignature
MA Thompson, J Krissansen-Totton… - Proceedings of the …, 2022 - National Acad Sciences
Methane has been proposed as an exoplanet biosignature. Imminent observations with the
James Webb Space Telescope may enable methane detections on potentially habitable …
James Webb Space Telescope may enable methane detections on potentially habitable …
Planetary Spectrum Generator: An accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets
GL Villanueva, MD Smith, S Protopapa, S Faggi… - Journal of Quantitative …, 2018 - Elsevier
We have developed an online radiative-transfer suite (https://psg. gsfc. nasa. gov) applicable
to a broad range of planetary objects (eg, planets, moons, comets, asteroids, TNOs, KBOs …
to a broad range of planetary objects (eg, planets, moons, comets, asteroids, TNOs, KBOs …
A comparative study of atmospheric chemistry with VULCAN
We present an update of the open-source photochemical kinetics code VULCAN to include
C–H–N–O–S networks and photochemistry. The additional new features are advection …
C–H–N–O–S networks and photochemistry. The additional new features are advection …
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 …
PICASO 3.0: a one-dimensional climate model for giant planets and brown dwarfs
Abstract Upcoming James Webb Space Telescope observations will allow us to study
exoplanet and brown dwarf atmospheres in great detail. The physical interpretation of these …
exoplanet and brown dwarf atmospheres in great detail. The physical interpretation of these …
Disequilibrium carbon, oxygen, and nitrogen chemistry in the atmospheres of HD 189733b and HD 209458b
We have developed a one-dimensional photochemical and thermochemical kinetics and
diffusion model to study the effects of disequilibrium chemistry on the atmospheric …
diffusion model to study the effects of disequilibrium chemistry on the atmospheric …
The process of tholin formation in Titan's upper atmosphere
Titan's lower atmosphere has long been known to harbor organic aerosols (tholins)
presumed to have been formed from simple molecules, such as methane and nitrogen (CH4 …
presumed to have been formed from simple molecules, such as methane and nitrogen (CH4 …
No thermal inversion and a solar water abundance for the hot Jupiter HD 209458b from HST/WFC3 spectroscopy
MR Line, KB Stevenson, J Bean… - The Astronomical …, 2016 - iopscience.iop.org
The nature of the thermal structure of hot Jupiter atmospheres is one of the key questions
raised by the characterization of transiting exoplanets over the past decade. There have …
raised by the characterization of transiting exoplanets over the past decade. There have …