Enceladus, the sixth moon of Saturn is a very interesting faraway, celestial object.
Not long ago, researchers who studied Enceladus showed that plumes of vapor continuously escaping from cracks in the moon’s icy shell are rich in molecular hydrogen.
It indicates that there are very promising conditions for life in Enceladus’s subsurface sea.
Now, according to most recent research from NASA’s Cassini mission, there is evidence that the moon’s spin axis – the line through the north and south poles – has reoriented.
It probably happened in the distant past due to a collision with a smaller body, such as an asteroid.
Examining the moon’s features, astronomers from from Cornell University, the University of Texas and NASA showed that Enceladus appears to have tipped away from its original axis by about 55 degrees — more than halfway toward rolling completely onto its side.
The area around the icy moon’s current south pole is a geologically active region where long – about 80 miles long and a little over a mile wide – linear fractures referred to as tiger stripes slice across the surface. Tajeddine and colleagues speculate that an asteroid may have struck the region in the past when it was closer to the equator.
After this asteroid blow, it took long time for Enceladus to recover; it remained for a long time unsteady and wobbly until it finally re-established its stability. The process, however, likely took over a million years. To do that, the north-south axis needed to change — a mechanism called “true polar wander.”
Enceladus’ topographic and geological features can be explained through geophysical processes, but the moon’s north and south poles are quite different. The south is active and geologically young, while the north is covered in craters and appears much older.
Research is published in Icarus.