Io's thermal emission from the Galileo photopolarimeter-radiometer.

Galileo's photopolarimeter-radiometer instrument mapped Io's thermal emission during the I24, I25, and I27 flybys with a spatial resolution of 2.2 to 300 kilometers. Mapping of Loki in I24 shows uniform temperatures for most of Loki Patera and high temperatures in the southwest corner, probably resulting from an eruption that began 1 month before the observation. Most of Loki Patera was resurfaced before I27. Pele's caldera floor has a low temperature of 160 kelvin, whereas flows at Pillan and Zamama have temperatures of up to 200 kelvin. Global maps of nighttime temperatures provide a means for estimating global heat flow.

[1]  A. McEwen,et al.  Galileo at Io: results from high-resolution imaging. , 2000, Science.

[2]  S. Kieffer,et al.  A close-up look at Io from Galileo's near-infrared mapping spectrometer. , 2000, Science.

[3]  G. Ballester,et al.  Discovery of gaseous S2 in Io's Pele plume. , 2000, Science.

[4]  Alfred S. McEwen,et al.  Active Volcanism on Io: Global Distribution and Variations in Activity , 1999 .

[5]  Spencer,et al.  Temperatures on europa from galileo photopolarimeter-radiometer: nighttime thermal anomalies , 1999, Science.

[6]  Todd J. Jones,et al.  Active Volcanism on Io as Seen by Galileo SSI , 1998 .

[7]  T V Johnson,et al.  High-temperature silicate volcanism on Jupiter's moon Io. , 1998, Science.

[8]  M. Hicks,et al.  A history of high‐temperature Io volcanism: February 1995 to May 1997 , 1997 .

[9]  A. McEwen,et al.  Temperature and area constraints of the South Volund Volcano on Io from the NIMS and SSI instruments during the Galileo G1 orbit , 1997 .

[10]  R. Howell Thermal Emission from Lava Flows on Io , 1997 .

[11]  J. Goguen,et al.  Io's heat flow from infrared radiometry: 1983–1993 , 1994 .

[12]  R. A. Chandos,et al.  Galileo Photopolarimeter/Radiometer experiment , 1992 .

[13]  H. M. Dyck,et al.  Io hot spots: Infrared photometry of satellite occultations , 1988 .

[14]  O. Hansen Ten-micron eclipse observations of Io, Europa, and Ganymede , 1973 .

[15]  B. Clark,et al.  Io Hot Spots in 1991: Results from Europa Occultation Photometry and Infrared Imaging , 1994 .