Results 191 to 200 of about 33,171 (317)
Pluto near the edge of chaos. [PDF]
Proc Natl Acad Sci U S A, 2022 Malhotra R, Ito T.
europepmc +1 more source
Compositions and Interior Structures of the Large Moons of Uranus and Implications for Future Spacecraft Observations. [PDF]
J Geophys Res Planets, 2023 Castillo-Rogez J +7 more
europepmc +1 more source
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
Observations of Uranus and Saturn taken with the 6-inch Telescope of the Transit Circle of the Sydney Observatory [PDF]
, 1905 C. J. Merfield
openalex +1 more source
III. Value of the Mass of Uranus, deduced from Observations of its Satellites, made at the Royal Observatory of Munich during the year 1837 [PDF]
F. Lamont
openalex +1 more source
Are the aerosols on Uranus and Neptune composed of methane photopolymers? [PDF]
The measured optical properties of photochemically produced aerosols in an adding-doubling radiative transfer code were used to match various points in the spectra of Uranus and Neptune.
Giver, L., Goorvitch, D., Podolak, M.
core +1 more source
The bolometric Bond albedo and energy balance of Uranus [PDF]
arXivUsing a newly developed `holistic' atmospheric model of the aerosol structure in Uranus's atmosphere, based upon observations made by HST/STIS, Gemini/NIFS and IRTF/SpeX from 2000 -- 2009, we make a new estimate the bolometric Bond albedo of Uranus during this time of $A^* = 0.338 \pm 0.011$, with a phase integral of $q^* = 1.36 \pm 0.03$.
arxiv