WebNov 7, 2009 · In comparison, Amalthea is a relatively easy object. The main obstacle to imaging these moons is Jupiter's glow, so a position near elongation is a must. Thebe's orbital period is 16h 11m. For example, if Thebe is in eastern elongation, it will be a western elongation one day later. The hours of these moments are moving only slowly from day to … WebAmalthea is a small, very red, irregular-shaped moon of the planet Jupiter. Dust ejected from it's surface formed the Amalthea Gossamer Ring around Jupiter. ... 1.8 ; Distance from …
Amalthea satellite of Jupiter Britannica
WebJul 3, 2024 · Amalthea (Stooke) (PLY 94 KB) (OBJ 167 KB) Please note that the models are in planetocentric coordinate system, with Z axis passing through north pole. Actual rotational axis may differ from planetocentric poles, especially for small irregular bodies. Surface Textures WebApr 10, 2024 · The orbital inclination, the angle at which Amalthea orbits to the orbital plane, is 5.04287 degrees.. The orbital eccentricity is 0.0860935, the degree at which Amalthea orbits close to a circular (0) orbit as opposed to an elliptical (1).. Amalthea has not been classed as a Near Earth Object (NEO) asteroid as its path doesn't come close (proximity) … impark seton calgary
Amalthea Fact Sheet - Jet Propulsion Laboratory
WebMay 21, 2011 · It seems that Amalthea and Thebe stay pretty close to the plane of the Jovian 4, but Himalia and Elara appear to be above the "ring" plane either above or below the planet. How come? ... According to Wikipedia, Elara is inclined 31 degrees from Jupiter's equator with an orbital period of 260 days. Its mean radius is 43km (a pretty small moon). WebAmalthea circles Jupiter once every 11 hours 57 minutes (0.498 Earth day) at a distance of 181,000 km (112,500 miles) in a nearly circular orbit that lies within half a degree of Jupiter’s equatorial plane. WebAmalthea the only other Jovian satellite over 200 ... It must be distinguished from the tidal deformations due to periodic forces varying on timescales of the orbital period due to the orbital eccentricity or inclination, non-negligible obliquity, or because of a nonsynchronous rotational state.) Deviations from hydrostatic equilibrium may ... listwanite rough