Add to ORKGWe have completed a new 1:15,000,000 global geologic map of Jupiter's volcanic moon, Io, based on a set of 1 km/pixel combined Galileo- Voyager mosaics produced by the U.S. Geological Survey. The map was produced over the last three years using ArcGIS(TM) software, and has undergone peer-review. Here we report some of the key results from our global mapping efforts, and how these results relate to questions regarding the volcano-tectonic evolution of Io
We present measurements of the near-infrared brightness of Io's hot spots derived from 2 to 5 μm ima...
The extreme and time-variable volcanic activity on Jupiter’s moon Io is the result of periodic tidal...
The distribution of Io's volcanic activity likely reflects the position and magnitude of internal ti...
We are preparing a new global geo-logic map of Jupiter s volcanic moon, Io. Here we report the type ...
A new global geologic map of Jupiter's volcanic moon, Io is being prepared, with the focus being on ...
Geologic mapping of the Jovian satellite Io has been completed at 1:15,000,000 scale for an area lyi...
Since the end of the Galileo epoch, ground-based observations have been crucial for the continued mo...
Io, the innermost of Jupiter's Galilean satellites, is the most volcanically active body in the Sola...
Io's surface is younger and has more active volcanism than any other terrestrial body in the solar s...
Jupiter’s moon Io is the most volcanically active body in the solar system. This paper seeks to qu...
During late 1999/early 2000, the solid state imaging experiment on the Galileo spacecraft returned m...
Io is the most volcanically-active object in the solar system. The moon ejects a tonne per second of...
We present in this Keck AO paper the first global high angular resolution observations of Io in thre...
Global volcanism has implications for planetary evolution far beyond the surface features that we ob...
Tidal dissipation makes Jupiter's moon Io the most volcanically active body in the solar system. Mos...
We present measurements of the near-infrared brightness of Io's hot spots derived from 2 to 5 μm ima...
The extreme and time-variable volcanic activity on Jupiter’s moon Io is the result of periodic tidal...
The distribution of Io's volcanic activity likely reflects the position and magnitude of internal ti...
We are preparing a new global geo-logic map of Jupiter s volcanic moon, Io. Here we report the type ...
A new global geologic map of Jupiter's volcanic moon, Io is being prepared, with the focus being on ...
Geologic mapping of the Jovian satellite Io has been completed at 1:15,000,000 scale for an area lyi...
Since the end of the Galileo epoch, ground-based observations have been crucial for the continued mo...
Io, the innermost of Jupiter's Galilean satellites, is the most volcanically active body in the Sola...
Io's surface is younger and has more active volcanism than any other terrestrial body in the solar s...
Jupiter’s moon Io is the most volcanically active body in the solar system. This paper seeks to qu...
During late 1999/early 2000, the solid state imaging experiment on the Galileo spacecraft returned m...
Io is the most volcanically-active object in the solar system. The moon ejects a tonne per second of...
We present in this Keck AO paper the first global high angular resolution observations of Io in thre...
Global volcanism has implications for planetary evolution far beyond the surface features that we ob...
Tidal dissipation makes Jupiter's moon Io the most volcanically active body in the solar system. Mos...
We present measurements of the near-infrared brightness of Io's hot spots derived from 2 to 5 μm ima...
The extreme and time-variable volcanic activity on Jupiter’s moon Io is the result of periodic tidal...
The distribution of Io's volcanic activity likely reflects the position and magnitude of internal ti...