Drippy tumulus

Image: Drippy tumulus

Detailed Description

A “drippy” tumulus near Kamokuna, which is a lava delta where Puʻu ʻŌʻō flows enter the Pacific Ocean. These tumuli form when the upwelling lava has a steady pressure and rate of movement, so the upper crust does not break apart. Instead, the lava slowly squeezes out.

Tumuli are structures usually associated with slow-moving flows. When the top of the flow crusts over, the lava beneath can well upward and create an elliptical, domed structure. Oftentimes, the pressure creates an axial fracture along the length of the structure. The lava might burst through the crust, squeeze out slowly, or only push the crust so far before it freezes.  Tumuli typically range from 2 to 10 meters high. While tumuli are most often associated with pahoehoe lavas, they have been documented in ‘a’a lava as well. Tumuli are one of several related features formed by inflation of lava flows.

Due to their relatively small size, tumuli are difficult to spot aerially. There is often debate over images of suggested Martian tumuli.



Image Dimensions: 3477 x 5204

Date Taken:

Location Taken: Kamokuna Beach, HI, US