|
Collection:
|
|
NASA Planetary Photo Journal Collection
Collection
NASA Planetary Photo Journal Collection
Collection
|
|
Title:
|
|
NIMS: hotspots on Io during G2
Title
NIMS: hotspots on Io during G2
Title
|
|
Original Caption Released with Image:
|
|
The Near Infrared Mapping Spectrometer (NIMS) on the Galileo spacecraft imaged Io at high spectral resolution at a range of 439,000 km (275,000 miles) during the G2 encounter on 7 September 1996. This image shows (on the right) Io as seen in the infrared by NIMS. The image on the left shows the same view from Voyager in 1979. This NIMS image can be compared to the NIMS images from the G1 orbit (June 1996) to monitor changes on Io. The NIMS image is at 4.9 microns, showing thermal emissions from the hotspots. The brightness of the pixels is a function of size and temperature. At least 10 hotspots have been identified and can be matched with surface features. An accurate determination of the position of the hotspot in the vicinity of Shamash Patera is pending. Hotspots are seen in the vicinity of Prometheus, Volund and Marduk, all sites of volcanic plume activity during the Galileo encounters, and also of active plumes in 1979. Temperatures and areas have been calculated for the hotspots shown. Temperatures range from 828 K (1031 F) to 210 K (- 81.4 F). The lowest temperature is significantly higher than the Io background (non-hotspot) surface temperature of about 100 K (-279 F). Hotspot areas range from 6.5 square km (2.5 sq miles) to 40,000 sq km (15,400 sq miles). The hottest hotspots have smallest areas, and the cooler hotspots have the largest areas. NIMS is continuing to observe Io to monitor volcanic activity throughout the Galileo mission. The Galileo mission is managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, D.C. This image and other images and data received from Galileo are posted on the Galileo mission home page on the World Wide Web at http://galileo.jpl.n asa.gov.
Original_Caption_Rel eased_with_Image
The Near Infrared Mapping Spectrometer (NIMS) on the Galileo spacecraft imaged Io at high spectral resolution at a range of 439,000 km (275,000 miles) during the G2 encounter on 7 September 1996. This image shows (on the right) Io as seen in the infrared by NIMS. The image on the left shows the same view from Voyager in 1979. This NIMS image can be compared to the NIMS images from the G1 orbit (June 1996) to monitor changes on Io. The NIMS image is at 4.9 microns, showing thermal emissions from the hotspots. The brightness of the pixels is a function of size and temperature. At least 10 hotspots have been identified and can be matched with surface features. An accurate determination of the position of the hotspot in the vicinity of Shamash Patera is pending. Hotspots are seen in the vicinity of Prometheus, Volund and Marduk, all sites of volcanic plume activity during the Galileo encounters, and also of active plumes in 1979. Temperatures and areas have been calculated for the hotspots shown. Temperatures range from 828 K (1031 F) to 210 K (- 81.4 F). The lowest temperature is significantly higher than the Io background (non-hotspot) surface temperature of about 100 K (-279 F). Hotspot areas range from 6.5 square km (2.5 sq miles) to 40,000 sq km (15,400 sq miles). The hottest hotspots have smallest areas, and the cooler hotspots have the largest areas. NIMS is continuing to observe Io to monitor volcanic activity throughout the Galileo mission. The Galileo mission is managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, D.C. This image and other images and data received from Galileo are posted on the Galileo mission home page on the World Wide Web at http://galileo.jpl.n asa.gov.
Original Caption Released with Image
|
|
Addition Date:
|
|
1998-03-26
Addition_Date
1998-03-26
Addition Date
|
|
Produced By:
|
|
JPL
Produced_By
JPL
Produced By
|
|
Mission:
|
|
Galileo
|
|
Spacecraft:
|
|
Galileo Orbiter
Spacecraft
Galileo Orbiter
Spacecraft
|
|
Target Name:
|
|
Io
Target_Name
Io
Target Name
|
|
Is a satellite of:
|
|
Jupiter
Is_a_satellite_of
Jupiter
Is a satellite of
|
|
Instrument:
|
|
Near Infrared Mapping Spectrometer
Instrument
Near Infrared Mapping Spectrometer
Instrument
|
|
Product Size:
|
|
1900 samples x 1300 lines
Product_Size
1900 samples x 1300 lines
Product Size
|
|
Primary Data Set:
|
|
Galileo EDRs
Primary_Data_Set
Galileo EDRs
Primary Data Set
|
|
Producer ID:
|
|
P48141 MRPS77796
Producer_ID
P48141 MRPS77796
Producer ID
|
|
facet_what:
|
|
Jupiter
facet_what
Jupiter
facet_what
|
|
facet_what:
|
|
Voyager
facet_what
Voyager
facet_what
|
|
facet_what:
|
|
Galileo
facet_what
Galileo
facet_what
|
|
facet_what:
|
|
Galileo Orbiter
facet_what
Galileo Orbiter
facet_what
|
|
facet_what:
|
|
Spectrometer
facet_what
Spectrometer
facet_what
|
|
facet_what:
|
|
Io
|
|
facet_what:
|
|
Near Infrared Mapping Spectrometer (NIMS)
facet_what
Near Infrared Mapping Spectrometer (NIMS)
facet_what
|
|
facet_where:
|
|
Jet Propulsion Laboratory
facet_where
Jet Propulsion Laboratory
facet_where
|
|
facet_where:
|
|
Jupiter
facet_where
Jupiter
facet_where
|
|
facet_where:
|
|
Washington
facet_where
Washington
facet_where
|
|
facet_where:
|
|
Jet Propulsion Laboratory (JPL)
facet_where
Jet Propulsion Laboratory (JPL)
facet_where
|
|
facet_where:
|
|
Washington, D.C.
facet_where
Washington, D.C.
facet_where
|
|
facet_when:
|
|
1979
facet_when
1979
facet_when
|
|
facet_when:
|
|
June 1996
facet_when
June 1996
facet_when
|
|
facet_when:
|
|
September 1996
facet_when
September 1996
facet_when
|
|
facet_when_year:
|
|
1979
facet_when_year
1979
facet_when_year
|
|
facet_when_year:
|
|
1996
facet_when_year
1996
facet_when_year
|
|
Image #:
|
|
PIA00520
|
|
UID:
|
|
SPD-PHOTJ-PIA00520
UID
SPD-PHOTJ-PIA00520
UID
|
|
orignial url:
|
orignial_url
orignial url
|