When a star is described as a spectral class G2V, we know its approximate mass, temperature, age, and size. At more than 5,700 exoplanets discovered, it is a natural developmental […]
Uranus
Storms and Convection on Uranus and Neptune: Impact of Methane Abundance Revealed by a 3D Cloud-resolving Model
Uranus and Neptune have atmospheres dominated by molecular hydrogen and helium. In the upper troposphere, methane is the third main molecule and condenses, yielding a vertical gradient in CH4. This […]
Ice Giant Systems Seminar Series: Are Uranus’ Large Moons Ocean Worlds? The Developing Spectroscopic Picture
Date/Time: September 10, 11am ETSpeaker: Dr. Richard Cartwright (JHU/APL)Topic: Are Uranus’ Large Moons Ocean Worlds? The Developing Spectroscopic Picture
The Astrobiological Potential of the Uranian Moon System
The 2023-2032 Planetary Science and Astrobiology Decadal Survey prioritized the Uranus Orbiter and Probe (UOP) mission concept as the next priority flagship mission. The UOP concept includes scientific studies of […]
Webb Observes Carbon Oxides On Uranus’ Moon Ariel That Hint At A Hidden Ocean
The surface of Uranus’ moon Ariel is coated with a significant amount of carbon dioxide ice, especially on its “trailing hemisphere” that always faces away from the moon’s direction of […]
Atmospheric Science Questions for a Uranian Probe
The Ice Giants represent a unique and relatively poorly characterized class of planets that have been largely unexplored since the brief Voyager 2 flyby in the late 1980’s.
Insights on the Formation Conditions of Uranus and Neptune from their Deep Elemental Compositions
This study, placed in the context of the preparation for the Uranus Orbiter Probe mission, aims to predict the bulk volatile compositions of Uranus and Neptune. Using a protoplanetary disk […]
Uranus And Neptune As Methane Planets: Producing Icy Giants From Refractory Planetesimals
Uranus and Neptune are commonly considered ice giants, and it is often assumed that, in addition to a solar mix of hydrogen and helium, they contain roughly twice as much […]
JWST Spectrophotometry of the Small Satellites of Uranus and Neptune
We use 1.4-4.6 micron multi-band photometry of the small inner Uranian and Neptunian satellites obtained with the James Webb Space Telescope’s near-infrared imager NIRCam to characterize their surface compositions.
Neptune-like Exoplanets Can Be Cloudy Or Clear — New Findings Suggest The Reason Why
The study of “exoplanets,” the sci-fi-sounding name for all planets in the cosmos beyond our own solar system, is a pretty new field. Mainly, exoplanet researchers like those in the […]
