Mercury: detail of the Caloris basin 3.4
Detail of the lower left of the main Caloris basin image, showing a 350km-wide area within the basin. Ridges and fractures can be seen on the basin floor as well as a number of younger impact craters.
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Image Credit: NASA.  

The large expanses of the floor of the Caloris basin that have not been overprinted with more recent cratering show extensive fracturing and ridging of the surface. This material is best interpreted as flows of lava, that welled up and filled the basin some time after its formation. Lava-filled depressions on Earth have mixtures of fractures and ridges as those seen (albiet on a much larger scale) on Mercury. Many of the ridges are compressional features where flows converged, or indicate inflation by injection of lava below a solidified carapace, whereas the straight-edged fractures indicate settling of the surface as the lava cooled and contracted.  
David A Rothery Return to top of page