Thermal and magmatic evolution of the Moon

CK Shearer, PC Hess… - … in Mineralogy and …, 2006 - pubs.geoscienceworld.org
As with all science, our continually develo** concepts of lunar evolution are firmly tied to
both new types of observations and the integration of these observations to the known pool …

Exploring the Saturn system in the thermal infrared: The composite infrared spectrometer

FM Flasar, VG Kunde, MM Abbas… - The Cassini-Huygens …, 2004 - Springer
Abstract The Composite Infrared Spectrometer (CIRS) is a remote-sensing Fourier
Transform Spectrometer (FTS) on the Cassini orbiter that measures thermal radiation over …

Dynamics of lunar formation

RM Canup - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract The giant impact theory is the leading hypothesis for the origin of the Moon. This
review focuses on dynamical aspects of an impact-induced lunar formation, in particular …

[PDF][PDF] Origin and evolution of the natural satellites

SJ Peale - Annual Review of Astronomy and Astrophysics, 1999 - researchgate.net
The natural satellites of planets in the solar system display a rich variety of orbital
configurations and surface characteristics that have intrigued astronomers, physicists, and …

The Cassini ultraviolet imaging spectrograph investigation

LW Esposito, CA Barth, JE Colwell, GM Lawrence… - Space science …, 2004 - Springer
Abstract The Cassini Ultraviolet Imaging Spectrograph (UVIS) is part of the remote sensing
payload of the Cassini orbiter spacecraft. UVIS has two spectrographic channels that …

Lunar accretion from an impact-generated disk

S Ida, RM Canup, GR Stewart - Nature, 1997 - nature.com
Although the mechanism by which the Moon was formed is currently unknown, several lines
of evidence point to its accretion from a circumterrestrial disk of debris generated by a giant …

Size distribution of particles in Saturn's rings from aggregation and fragmentation

N Brilliantov, PL Krapivsky, A Bodrova… - Proceedings of the …, 2015 - National Acad Sciences
Saturn's rings consist of a huge number of water ice particles, with a tiny addition of rocky
material. They form a flat disk, as the result of an interplay of angular momentum …

Accretion of Saturn's mid-sized moons during the viscous spreading of young massive rings: Solving the paradox of silicate-poor rings versus silicate-rich moons

S Charnoz, A Crida, JC Castillo-Rogez, V Lainey… - Icarus, 2011 - Elsevier
The origin of Saturn's inner mid-sized moons (Mimas, Enceladus, Tethys, Dione and Rhea)
and Saturn's rings is debated. Charnoz et al.[Charnoz, S., Salmon J., Crida A., 2010. Nature …

The recent formation of Saturn's moonlets from viscous spreading of the main rings

S Charnoz, J Salmon, A Crida - Nature, 2010 - nature.com
The regular satellites of the giant planets are believed to have finished their accretion
concurrent with the planets, about 4.5 Gyr ago,,,. A population of Saturn's small moons …

The formation of Jupiter's faint rings

JA Burns, MR Showalter, DP Hamilton, PD Nicholson… - Science, 1999 - science.org
Observations by the Galileo spacecraft and the Keck telescope showed that Jupiter's
outermost (gossamer) ring is actually two rings circumscribed by the orbits of the small …