
Working with image data from NASA's Cassini mission, researchers have found evidence that Saturn's moon Enceladus may have tipped over, reorienting itself so that terrain closer to its original equator was relocated to the poles. This phenomenon is known as true polar wander. Researchers discovered a chain of basins across the surface of Enceladus along with a pair of depressions that line up with an equator and poles, respectively, if the moon's axis of rotation was reoriented by about 55 degrees of latitude. These maps look toward the icy moon's southern hemisphere, with colors representing highs and lows. Purple represents the lowest elevations, while red represents the highest. The map at left shows the surface of Enceladus in its possible ancient orientation, millions of years ago. The chain of basins representing topographic lows can be seen in blue and purple, running along the equator, with an additional low region around the original south pole. The region that encloses the moon's currently active south polar terrain, with its long, linear "tiger stripe" fractures, would have been at middle latitudes just south of the equator. The map at right shows the current orientation of Enceladus. https://photojournal.jpl.nasa.gov/catalog/PIA21612
Most NASA images are in the public domain and free to use. Credit NASA as the source. Check NASA's media usage guidelines for details. Images featuring identifiable individuals may require additional permissions.
NASA ID
PIA21612
Date Created
May 30, 2017
Center
JPL
Media Type
image
Download this image in multiple resolutions. All NASA media are free for public use.
480px