- 17 km/s
orbital velocity at
Io), and are thus
ejected in jets
leading away from
Io.
Io orbits within a belt of
intense radiation known as the
Io plasma...
-
Laplace created a
mathematical theory to
explain the
resonant orbits of
three of Jupiter's moons,
Io, Europa, and Ganymede. This
resonance was
later found to...
-
Tidal heating of
Io (also
known as
tidal working)
occurs through the
tidal friction processes between Jupiter and its moon.
Orbital and
rotational energy...
- mechanics,
orbital resonance occurs when
orbiting bodies exert regular,
periodic gravitational influence on each other,
usually because their orbital periods...
- its
orbit,
causing a
varying tidal bulge. This
variation in the
shape of
Io causes frictional heating in its interior.
Without this
tidal heating,
Io might...
-
plate tectonics is dominant.
Io is
exceptional for the
strong tidal heating it undergoes,
caused by the
eccentricity of its
orbit (which
results from its resonance...
-
smaller ones,
Io and Europa, are
about the size of the Moon. The
three inner moons —
Io, Europa, and
Ganymede — are in a 4:2:1
orbital resonance with...
- Jupiter's formation. At
least 95
moons orbit the planet; the four
largest moons—
Io, Europa, Ganymede, and Callisto—
orbit within the magnetosphere, and were...
-
PowerDC XtractIM PowerSI Broadband ****E SPEED2000
Channel Designer XcitePI OrbitIO Planner Unified Package Designer (UPD)
acquired from
Synopsys Forte Design...
- (2003) 85
Io at AstDyS-2, Asteroids—Dynamic Site Ephemeris ·
Observation prediction ·
Orbital info ·
Proper elements ·
Observational info 85
Io at the JPL...
