Results 131 to 140 of about 34,434 (269)

Astronomical studies of the major planets, natural satellites and asteroids using the 2.24 m telescope [PDF]

Directional features in the Jovian sodium torus, high quality CCD images of the major planets, methane bands in the spectrum of Triton, the central wavelength of the SO2 absorption band on Io, a component on the icy surfaces of the satellites of Uranus ...
Jefferies, J. T.
core   +1 more source

Understanding the Transport Properties of Methane–Hydrogen Mixtures under the Interior Conditions of Ice Giants

The Astrophysical Journal
Inaccuracy in our knowledge of the transport properties of relevant mixtures under planetary interior conditions is a roadblock in predicting the observable properties of planets in our solar system and beyond.
Argha Jyoti Roy, Mandy Bethkenhagen, Armin Bergermann, Ronald Redmer   +3 more
doaj   +1 more source

The Rotation of Uranus [PDF]

, 1982
R. M. Goody
openalex   +1 more source

Uranus’ Stratospheric HCl Upper Limit from Herschel/SPIRE* [PDF]

, 2020
N. A. Teanby, P. G. J. Irwin
openalex   +1 more source

Radio Science Experiments during a Cruise Phase to Uranus

Aerospace
The exploration of Uranus, a key archetype for ice giant planets and a gateway to understanding distant exoplanets, is acquiring increasing interest in recent years, especially after the Uranus Orbiter and Probe (UOP) mission has been prioritized in the ...
Ivan di Stefano, Daniele Durante, Paolo Cappuccio, Paolo Racioppa   +3 more
doaj   +1 more source

Plasma Environment, Radiation, Structure, and Evolution of the Uranian System (PERSEUS): A Dedicated Orbiter Mission Concept to Study Space Physics at Uranus. [PDF]

Space Sci Rev, 2023
Cohen IJ, Smith EJ, Clark GB, Turner DL, Ellison DH, Clare B, Regoli LH, Kollmann P, Gallagher DT, Holtzman GA, Likar JJ, Morizono T, Shannon M, Vodusek KS.   +13 more
europepmc   +1 more source

The 10 February 1977 lunar occultation of Uranus. Radius, limb darkening, and polar brightening at 6900 A [PDF]

Contact timings, corrected for lunar limb effects, indicate an equatorial radius of 25700 + or - 500 km for the visible disk for Uranus. A modified Minnaert function is used to model limb darkening and polar brightening.
Radick, R. R., Tetley, W. C.
core   +1 more source

Insights on the Formation Conditions of Uranus and Neptune from Their Deep Elemental Compositions

The Planetary Science Journal
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.
Olivier Mousis, Antoine Schneeberger, Thibault Cavalié, Kathleen E. Mandt, Artyom Aguichine, Jonathan I. Lunine, Tom Benest Couzinou, Vincent Hue, Raphaël Moreno   +8 more
doaj   +1 more source

Double superionicity in icy compounds at planetary interior conditions. [PDF]

Nat Commun, 2023
de Villa K, González-Cataldo F, Militzer B.   +2 more
europepmc   +1 more source

Magnesium oxide-water compounds at megabar pressure and implications on planetary interiors. [PDF]

Nat Commun, 2023
Pan S, Huang T, Vazan A, Liang Z, Liu C, Wang J, Pickard CJ, Wang HT, Xing D, Sun J.   +9 more
europepmc   +1 more source