PDS logoPlanetary Data System
PDS Information
Find a Node - Use these links to navigate to any of the 8 publicly accessible PDS Nodes.

This bar indicates that you are within the PDS enterprise which includes 6 science discipline nodes and 2 support nodes which are overseen by the Project Management Office at NASA's Goddard Space Flight Center (GSFC). Each node is led by an expert in the subject discipline, supported by an advisory group of other practitioners of that discipline, and subject to selection and approval under a regular NASA Research Announcement.
Click here to return to the Photojournal Home Page Click here to view a list of Photojournal Image Galleries Photojournal_inner_header
Latest Images  |  Spacecraft & Technology  |  Animations  |  Space Images App  |  Feedback  |  Photojournal Search  

PIA26484: Juno Captures North Polar Region of Io
 Target Name:  Io
 Is a satellite of:  Jupiter
 Mission:  Juno
 Spacecraft:  Juno
 Instrument:  JunoCam
 Product Size:  3456 x 2234 pixels (w x h)
 Produced By:  SwRI
 Full-Res TIFF:  PIA26484.tif (12.02 MB)
 Full-Res JPEG:  PIA26484.jpg (381.5 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

The north polar region of Jupiter's volcanic moon Io was captured by NASA's Juno during spacecraft's the 57th close pass of the gas giant on Dec. 30, 2023. The region was imaged at a scale of 1.1 miles (1.8 kilometers) per pixel.

The low illumination angle along the terminator (the line dividing day and night) shows several previously unrecognized mountain blocks rising abruptly above the surrounding plains. These are each characterized by a central, sharp peak and adjacent flanks that appear to be collapsing toward the plains. The higher of these peaks range from 2.3 to 6.1 miles (3.7 to 9.8 kilometers) in elevation. The shadows indicate that some of the mountain flanks grade into plateaus under 0.6 miles (1 kilometer). All mountains here are partly or completely covered by bright white diffuse deposits, which may be sulfur dioxide frosts derived from gases escaping the interior and transported up. Extremely large flow fields are evident here. The most active flow regions in Lei-Kung Fluctus (upper left in this image) are evidenced by their darker color and surrounded by white deposits, perhaps liberated from the surface by thermal action.

More information about Juno is at https://www.nasa.gov/juno and https://missionjuno.swri.edu.

Image Credit:
Image data: NASA/JPL-Caltech/SwRI/MSSS
Image processing by Gerald Eichstädt

Image Addition Date:
2024-12-12