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Journal ArticleDOI

Io on the eve of the galileo mission

John R. Spencer, +1 more
- 01 May 1996 - 
- Vol. 24, Iss: 1, pp 125-190
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TLDR
Io, the innermost of Jupiter's large moons, is one of the most unusual objects in the Solar System as discussed by the authors, which produces a global heat flux 40 times the terrestrial value, producing intense volcanic activity and a global resurfacing rate averaging perhaps 1 cm yr−1.
Abstract
▪ Abstract Io, innermost of Jupiter's large moons, is one of the most unusual objects in the Solar System. Tidal heating of the interior produces a global heat flux 40 times the terrestrial value, producing intense volcanic activity and a global resurfacing rate averaging perhaps 1 cm yr−1. The volcanoes may erupt mostly silicate lavas, but the uppermost surface is dominated by sulfur compounds including SO2 frost. The volcanoes and frost support a thin, patchy SO2 atmosphere with peak pressure near 10−8 bars. Self-sustaining bombardment of the surface and atmosphere by Io-derived plasma trapped in Jupiter's magnetosphere causes escape of material from Io (predominantly sulfur, oxygen, and sodium atoms, ions, and molecules) at a rate of about 103 kg s−1. The resulting Jupiter-encircling torus of ionized sulfur and oxygen dominates the Jovian magnetosphere and, together with an extended cloud of neutral sodium, is readily observable from Earth.

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Journal ArticleDOI

Vegetation's red edge: a possible spectroscopic biosignature of extraterrestrial plants.

TL;DR: This work presents Earthshine observations from Apache Point Observatory to emphasize that time variability is key to detecting weak surface biosignatures such as the vegetation red edge, and implies that future terrestrial-planet-characterizing space missions should obtain data that allow time-varying, sharp spectral features at unknown wavelengths to be identified.
Journal ArticleDOI

The sub-Alfvénic interaction of the Galilean satellites with the Jovian magnetosphere

TL;DR: In this article, it was shown that the sub-Alfvenic, low-beta interaction can be described by an anisotropic conducting atmosphere joined to an Alfven wing as one extreme case and the Jovian ionosphere as the other extreme case.
Journal ArticleDOI

Active Volcanism on Io as Seen by Galileo SSI

TL;DR: Io has been monitored during the nominal Galileo satellite tour from mid 1996 through late 1997 by the Solid State Imaging (SSI) experiment, which was able to observe many manifestations of active volcanism, including changes in the color and albedo of the surface, active airborne plumes, and glowing vents seen in eclipse as discussed by the authors.
BookDOI

Comparative Climatology of Terrestrial Planets

TL;DR: The Comparative Climatology of Terrestrial Planets (CCP) as discussed by the authors is a collection of more than sixty leading experts in the field that sets forth the foundations for this emerging new science and brings the reader to the forefront of our current understanding of atmospheric formation and climate evolution.
References
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Journal ArticleDOI

Eruption and emplacement of flood basalt: An example from the large-volume Teepee Butte Member, Columbia River Basalt Group

TL;DR: In this paper, the authors studied the distribution of lava flows of the Teepee Butte Member, Grande Ronde Basalt, in the Columbia River Basalt Group vent system and showed the importance of linear vent systems and the westward Palouse Slope.
Journal ArticleDOI

Planets and their atmospheres

David J. Stevenson
- 01 Dec 1984 - 
TL;DR: In this article, Lewis and Prinn present a very personal (some would say idiosyncratic) view of planetary atmospheres, and have an overwhelmingly chemical perspective, which is not, in my view, a suitable text for a course.
Journal ArticleDOI

Spatial color variations in the volcanic plume at Loki, on Io

TL;DR: In this article, the authors analyzed multicolor Voyager 1 photographs of the Loki volcanic plume, on Io, to determine the nature and quantity of the scattering material within the plume.
Journal ArticleDOI

Hubble Space Telescope UV spectral observations of Io passing into eclipse

TL;DR: In this article, the authors derived a 3 sigma upper limit to the 2560 A SO emission feature, which is close to what is expected from electron impact on SO2 based on the observed brightness of the FUV S and O lines in shadow.
Journal ArticleDOI

Dual periodicity of the Jovian magnetosphere

TL;DR: Using data from the 1979 Voyager flybys of Jupiter and two sets of ground-based observations of the Io torus, this article presented an extensive analysis concerning the nature of the second magnetospheric periodicity of the Jupiter's magnetic field, along with a definition of a new Jovian matching coordinate system (referred to as system IV).
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