Results 91 to 100 of about 1,113 (144)

The Astrobiology Primer v2.0. [PDF]

open access: yesAstrobiology, 2016
Domagal-Goldman SD   +48 more
europepmc   +1 more source

Astronomical Observations in Support of Planetary Entry-Probes to the Outer Planets. [PDF]

open access: yesSpace Sci Rev
Buratti BJ   +4 more
europepmc   +1 more source

Detection of carbon dioxide and hydrogen peroxide on the stratified surface of Charon with JWST. [PDF]

open access: yesNat Commun
Protopapa S   +16 more
europepmc   +1 more source

Geologic Constraints on the Formation and Evolution of Saturn's Mid-Sized Moons. [PDF]

open access: yesSpace Sci Rev
Rhoden AR   +9 more
europepmc   +1 more source

Multiple Probe Measurements at Uranus Motivated by Spatial Variability. [PDF]

open access: yesSpace Sci Rev
Wong MH   +3 more
europepmc   +1 more source

Dynamical evolution of the Uranian satellite system I.

open access: yesIcarus
Sérgio R.A. Gomes   +1 more
openaire   +1 more source

Orbital Stability of the Uranian Satellite System☆

Icarus, 1997
Abstract We have numerically integrated approximately 500 systems of mutually gravitating bodies which were based on subsets of the uranian satellite system. In each run within a set, the satellite masses were initially multiplied by a common mass enhancement factormf.
M DUNCAN, J LISSAUER
openaire   +1 more source

Surface properties and photometry of the Uranian satellites

Icarus, 1990
Voyager photographic images and photopolarimetric experiment observations have been used to obtain the spectral geometric and Bond albedos, phase integrals, color-dependent phase coefficients, and integrated solar phase-curve parameters of the five Uranian satellites Miranda, Ariel, Umbriel, Titania, and Oberon. While the results obtained confirm those
Bonnie Buratti   +2 more
openaire   +1 more source

Voyager 2 Photopolarimeter observations of the Uranian satellites

Journal of Geophysical Research: Space Physics, 1987
We report the ultraviolet (0.25 µm) and infrared (0.75 µm) geometric albedos, phase curves, and phase coefficients for the large Uranian satellites using full disk photometric observations obtained by the photopolarimeter subsystem during the Voyager 2 encounter with the Uranian system.
Robert M. Nelson   +7 more
openaire   +1 more source

Astrometry in the Uranian system of satellites

AIP Conference Proceedings, 2008
The predicted occultation between the satellites Miranda(UV) and Oberon(UIV) was observed on July 30, 2007 using SpeX/IRTF system and CODAM‐Paris Observatory facility. Data analysis reveals that the predicted magnitude drop for this phenomenon was overestimated and we establish an upper limit of 0m.05 for the phenomenon, perhaps due to a non‐lambertian
Mirel Birlan   +4 more
openaire   +2 more sources

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