Results 61 to 70 of about 11,862 (238)
Following recommendations from the 2023–2032 Planetary Science and Astrobiology Decadal Survey, we propose a novel Uranus exploration mission that is centered on using constellations of small spacecraft to observe the Uranus system.
Dylan Barnes, Paula do Vale Pereira
doaj +1 more source
The Deep Composition of Uranus and Neptune from In Situ Exploration and Thermochemical Modeling [PDF]
The distant ice giants of the Solar System, Uranus and Neptune, have only been visited by one space mission, Voyager 2. The current knowledge on their composition remains very limited despite some recent advances.
T. Cavalié +9 more
semanticscholar +1 more source
Detecting an Ocean Inside Callisto With Geodetic Measurements From Europa Clipper and Juice
Abstract Determining whether Callisto hosts a subsurface ocean, and the implications for material and energy transport through its hydrosphere, is of high interest to NASA's Europa Clipper and ESA's Juice missions. A recent reanalysis of Galileo magnetometer data strengthens the ocean hypothesis, but definitive confirmation awaits new measurements.
Flavio Petricca +2 more
wiley +1 more source
Abstract The Uranian moons, last visited in 1986 by Voyager 2, remain an intriguing yet under‐explored set of targets. Understanding the thermal structure and evolution of these moons is key to addressing one of the highest priority goals in planetary science: identifying if any are ocean worlds today or have been in the past. On Oberon, one feature in
M. Blanco‐Rojas +2 more
wiley +1 more source
Aim: The Impact of surface conditioning protocol i.e., Sandblasting (SB), Bioactive glasses particles (BAGPs), and Phthalocyanine (Pc) activated via low-level laser therapy (LLLT) on the surface roughness (Ra) and shear bond strength (SBS) of hybrid ...
Rana Sulaiman Al-Hamdan +2 more
doaj +1 more source
Massive Rocky Planets May Suppress Deep Melting
Abstract Melting properties of silicates are critical to understanding the thermal evolution of rocky planetary interiors. In the deep mantles of massive rocky planets, post‐post‐spinel Mg2SiO4 ${\text{Mg}}_{2}{\text{SiO}}_{4}$ is potentially one of the most abundant mineral phases, yet its melting behavior remains unconstrained. Here, we determine the
Donghao Zheng, Yihang Peng, Jie Deng
wiley +1 more source
To use accumulated resources of UkrVO digital archive, analysis of the available photographic plates containing images of Uranus and Neptune was conducted.
Yu. Protsyuk +6 more
doaj +1 more source
In situ exploration of Uranus has been limited to a single flyby encounter by the Voyager 2 spacecraft in January 1986. Nonetheless, new investigation has led to significant questions about the origin of energetic ions observed in the region between its ...
Ian J. Cohen +6 more
doaj +1 more source
Uranus's complex internal structure
Uranus's bulk composition remains unknown. Although there are clear indications that Uranus's interior is not fully convective, and therefore has a non-adiabatic temperature profile, many interior models continue to assume an adiabatic interior.
A. Neuenschwander +2 more
semanticscholar +1 more source

