Clouds and hazes are abundant in the thin and cold atmospheres of Triton and Pluto, where they are thought to be produced by interactions between atmospheric gases and ultraviolet photons […]
icy world
Enhanced Voyager 2 Approach Image Sequence Of Icy Ocean World Triton
Original Caption Released with Image: Triton Voyager 2 approach sequence with latitude-longitude grid superposed. The color image was reconstructed by making a computer composite of three black and white images […]
Distinguishing Potential Organic Biosignatures on Ocean Worlds from Abiotic Geochemical Products using Thermodynamic Calculations
The search for life in our solar system often involves efforts to detect organic molecules, which have been found on many extraterrestrial bodies, including planets, moons, meteorites, comets, and asteroids. […]
Europa Clipper Planetary Protection Probabilistic Risk Assessment Summary
Protecting Jupiter’s Icy Moons from the Earth’s biological contamination is a key consideration for the Europa Clipper mission. The mission’s goal is to explore Jupiter’s moon, Europa, and investigate its […]
Prominent Mid-infrared Excess Of The Dwarf Planet (136472) Makemake Discovered by JWST/MIRI Indicates Ongoing Activity
We report on the discovery of a very prominent mid-infrared (18-25 um) excess associated with the trans-Neptunian dwarf planet (136472) Makemake.
Uranus’ Moon Miranda May Have An Ocean Beneath Its Surface
A new study suggests Uranus’ moon Miranda may harbor a water ocean beneath its surface, a finding that would challenge many assumptions about the moon’s history and composition and could […]
Modifications Of SPH Towards Three-dimensional Simulations Of An Icy Moon With Internal Ocean
There are some traces of the existence of internal ocean in some icy moons, such as the vapor plumes of Europa and Enceladus. This implies a region of liquid water […]
H2-H2O Demixing In Uranus And Neptune: Adiabatic Structure Models
Demixing properties of planetary major constituents influence the interior structure and evolution of planets. Comparing experimental and computational data on the miscibility of hydrogen and water to adiabatic profiles suggests […]
Sealing Europa’s Vents By Vapor Deposition: An Order Of Magnitude Study
Fractures and vents in the ice crust of Europa, exposing the sub-surface ocean to the vacuum, might be responsible for the generation of planetary-scale water-vapor plumes.
LunaIcy: Exploring Europa’s Icy Surface Microstructure through Multiphysics Simulations
A multiphysics simulation model incorporating a sintering model coupled with the MultIHeaTS thermal solver was developed to study the evolution of icy moons’ microstructure.
