Lava Flows Exposed in Bessel Crater

Spectacular example of layering exposed in the wall of Bessel crater (21.8°N, 17.9°E). Image number M135073175R, incidence angle 13°, image is 500 meters across [NASA/GSFC/Arizona State University].

The outcrops exposed on the interior wall of Bessel crater (~16 km in diameter) are remarkable since they are most likely preserved layering of mare basalt. Today's Featured Image shows a portion of the northern wall, which contains multiple layers that probably represent discrete lava flow deposits in Mare Serenitatis. Over time, large, but relatively thin, lava flows spread across the extent of Mare Serenitatis. Lunar pits imaged by LROC also give us a good look at basalt flow layers. Boulders broken off of the mare layers tumble down the wall toward the floor of the crater. Bessel crater is named after Friedrich Bessel, the developer of Bessel functions. By measuring the thickness of layering found in Bessel and other craters, scientists can put constraints on the thickness of individual lava flows. What else can Bessel crater tell us about Mare Serenitatis?

LROC WAC 100 m/px monochrome mosaic. The interior of Bessel, a ~16 km diameter crater, shows slumping of material from the walls onto the floor [NASA/GSFC/Arizona State University].

Explore the entire NAC frame!

Related images:

Linne Crater

Dark streaks in Diophantus crater

Kepler's Rim


Posted by Sarah Braden on April 19, 2011 09:00 UTC.