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Io Volcano Observer (IVO) is a proposed low-cost mission to explore Jupiter's moon Io to understand tidal heating as a fundamental planetary process. [1] The main science goals are to understand (A) how and where tidal heat is generated inside Io, (B) how tidal heat is transported to the surface, and (C) how Io is evolving.
A dedicated mission to Io, called the Io Volcano Observer (IVO), has been proposed for the Discovery Program as a Jupiter orbiter that would perform at least ten flybys of Io over 3.5 years. [96] In 2020, as part of the 2019 Discovery mission call, IVO was selected as one of four missions to continue to a Phase A study. [4]
Visible OpticaL Camera And Near-infrared Observer (VOLCANO) is a visible/near-infrared imager. Multi-Axis Geophysical Magnetometer (MAGMA) is a magnetic instrumentation subpackage. Comprehensive AnaLysis of Dust from ERuptions and Atmosphere (CALDERA), is a dust analyzer that would identify the material in the volcanic plumes.
Volcanism on Io, a moon of Jupiter, is represented by the presence of volcanoes, volcanic pits and lava flows on the surface. Io 's volcanic activity was discovered in 1979 by Linda Morabito , an imaging scientist working on Voyager 1 . [ 1 ]
ɒ ˈ s ɔː l iː /), the highest mountain of Jupiter's moon Io, is one of the tallest mountains in the Solar System. It is located just northwest of the volcano Pele, in the Boösaule Montes. The official name of the mountain range was given in honor of the cave in Egypt where Io gave birth to Epaphus, and approved by the IAU in 1985.
Linda A. Morabito (born November 21, 1953), also known as Linda Kelly, Linda Hyder, and Linda Morabito-Meyer, is the astronomer who discovered volcanic activity on Io, a moon of Jupiter. She made this finding on March 9, 1979, at NASA's Jet Propulsion Laboratory .
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The thrust faulting and uplifting of large crust blocks on Io are interpreted by a model proposed by Schenk and Bulmer's 1998 paper. [3] In the model, Io's crust keeps recycling. Violent volcanic activity brings lava to the surface and older, buried layers are forced to subside. The old volcanic crust materials are compressed laterally as they ...