Results 81 to 90 of about 5,831 (201)
Inclination of Miranda as a Constraint on the Tidal Dissipation of Uranus
The five major moons of Uranus record a complicated geological history characterized by both tectonic resurfacing and heavy impact cratering, connecting their evolution to dynamical processes in the solar system.
Maryame El Moutamid, Matija Ćuk
doaj +1 more source
How many jokes can the three astroquarks make about the pronunciation of the seventh planet? You\u27ll have to tune in to this episode of WtG to find out.
Colwell, Joshua +2 more
core
Enhanced Precipitation of Energetic Protons Due to Uranus' Asymmetric Magnetic Field
Uranus remains one of the most unexplored planets in our solar system, featuring a distinctive magnetic field structure first observed by NASA's Voyager 2 mission almost 40 years ago.
M. Acevski, A. Masters
doaj +1 more source
Ice Giants Revisited: Uranus and Neptune as Magma Ocean Worlds
Uranus and Neptune are commonly interpreted as volatile-rich “ice giants,” an assumption that underpins most interior models. Here we show that their observed radii, bulk densities, gravitational harmonics, normalized moments of inertia, intrinsic ...
Edward D. Young +3 more
doaj +1 more source
Internal Heat Flux and Energy Imbalance of Uranus
With its extreme axial tilt, Uranus' radiant energy budget (REB) and internal heat flux remain among the most intriguing mysteries in our solar system.
Xinyue Wang +15 more
doaj +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source
New Moons of Uranus and Neptune from Ultradeep Pencil-beam Surveys
We have conducted extremely ultradeep pencil-beam observations for new satellites around both Uranus and Neptune. Tens of images on several different nights in 2021, 2022, and 2023 were obtained, shifted, and added together to reach as faint as 26.9 and ...
Scott S. Sheppard +6 more
doaj +1 more source
Towards an agnostic algorithm for sampling empirical structure models
We present an algorithm to efficiently sample the full space of planetary interior density profiles. Our approach uses as few assumptions as possible to pursue an agnostic algorithm.
Wirth Stefano, Morf Luca, Helled Ravit
doaj +1 more source
Is the Uranus Heat Flow Puzzling?
The low internal heat flow of Uranus has been confirmed and determined for the first time. It may be representative of the average rather than a fluctuation due to the unusual seasonal or condensation cycles. The very different value for Neptune suggests
David J. Stevenson
doaj +1 more source
Data for: Seasonal Stratospheric Photochemistry on Uranus and Neptune
Ascii files containing seasonal photochemical model results for Uranus and ...
Moses, J (via Mendeley Data) +1 more
core +1 more source

