Javascript must be enabled to continue!
4. The moons of giant planets
View through CrossRef
The giant planets Jupiter, Saturn, Uranus, and Neptune each have an extensive entourage of moons: small inner moonlets, closest to the planets, mostly less than a few tens of kilometres in radius and irregular in shape; next are large regular satellites exceeding about 200 km in radius; and then there are the irregular satellites mostly less than a few tens of kilometres in radius. ‘The moons of giant planets’ describes these different types of moons, the space missions to find them, their orbital resonance and tidal heating, as well as the spectacular and complex rings and shepherd moons of Saturn and the other giant planets.
Title: 4. The moons of giant planets
Description:
The giant planets Jupiter, Saturn, Uranus, and Neptune each have an extensive entourage of moons: small inner moonlets, closest to the planets, mostly less than a few tens of kilometres in radius and irregular in shape; next are large regular satellites exceeding about 200 km in radius; and then there are the irregular satellites mostly less than a few tens of kilometres in radius.
‘The moons of giant planets’ describes these different types of moons, the space missions to find them, their orbital resonance and tidal heating, as well as the spectacular and complex rings and shepherd moons of Saturn and the other giant planets.
Related Results
Survey of Irregular Jovian Moons with IVO
Survey of Irregular Jovian Moons with IVO
The Io Volcano Observer (IVO) [1] is a NASA Discovery mission currently under Phase A study [2]. Its primary goal is a thorough investigation of Io (e.g., [3]), the innermost of Ju...
Dynamics of giant planets in protoplanetary discs
Dynamics of giant planets in protoplanetary discs
New instruments such as the ALMA interferometer and SPHERE on VLT allowed to obtain a large number of high-resolution images of protoplanetary discs. In these images, substructures...
Enceladus' Subsurface Secrets: Scientific Rationale for Future Radar Sounder Measurements
Enceladus' Subsurface Secrets: Scientific Rationale for Future Radar Sounder Measurements
An outstanding question in planetary exploration addresses the habitability of icy moons in the outer Solar System. These bodies can harbor liquid water in substantial amounts over...
Interior dynamics of small-core and coreless exoplanets
Interior dynamics of small-core and coreless exoplanets
Since the first exoplanet detection in 1992, the study of exoplanets has received considerable attention. It is becoming apparent that the diversity of the general exoplanet popula...
Offshore Giant Fields, 1950-1990
Offshore Giant Fields, 1950-1990
ABSTRACT
OFFSHORE GIANT FIELDS
1950 - 1990
During the past forty years...
Multi-fluid hydrodynamical simulations of circumbinary planet formation via pebble accretion
Multi-fluid hydrodynamical simulations of circumbinary planet formation via pebble accretion
Context. Since the detection of the first known transiting circumbinary planet (CBP), Kepler-16b,by the Kepler mission, a total pf 14 CBPs have been detected, raising questions abo...
Icy Moons as Probes of Carbon-Rich Conditions During Giant Planet Formation
Icy Moons as Probes of Carbon-Rich Conditions During Giant Planet Formation
The densities and moments of inertia of Jovian and Saturnian icy moons, dwarf planets, and other trans-Neptunian objects (TNOs) suggest the presence of a significant low-density ca...
JWST Reveals Phyllosilicates on the Small Inner Moons of Neptune
JWST Reveals Phyllosilicates on the Small Inner Moons of Neptune
In the 1980’s, Voyager 2 discovered the abundant satellites and complex ring systems around the ice giants, with 13 small moons around Uranus and 7 around Neptune. Limitations pose...

