B
bonzelite
Guest
anvel, good points. <br /><br />what differs, perhaps, in the case of Enceladus from, say, Io at Jupiter (besides it's composition), is it's farther distance from the planet. Io is tidally tortured to death by Jupiter in it's extremely close proximity, embedded in the plasma torus. and activity appears throughout Io's surface. <br /><br />a question arises, then: at what distance is tidal heating no longer a dynamic or relevant force acting upon a body? i would assume tidal forces can act over vast distances. for example, look at how far out the sun's influence extends, gravitationally speaking, reaching far beyond Pluto. <br /><br />it is said that tidal forces acting upon Enceladus are "not enough" to create such a radical event as internal heating with water plumes, notably a hot spot at the south pole. it appears, then, that the heating is localized and not happeing throughout the surface as is seen on Io. <br /><br />why? and why is it dead-on at the south pole? <br /><br />in it's asymmetry of heat signature and erosional distribution, ie, skewed to the southern hemispehre of Enceladus, perhaps, too, there is an asymmetrical distribution of mass and density: maybe the southern hemisphere has a greater porosity than the northern, is thinner and acts a funnel or outlet for the entire moon's inner heat source. <br /><br />i'm only brainstorming of course.