Lunar Reconnaissance Orbiter Camera

Melt Fractures in Jackson Crater

Fractures can be seen in profuse abundance on the Jackson crater melt pond surface. Illumination from west, north is up, image is  ~700 m across, LROC NAC M118560367L [NASA/GSFC/Arizona State University].

As molten rock cools, it shrinks and often cracks. In this case of impact melt ponded within the Jackson crater floor (22.18°N, 197.24°E), the cracking rate was so high that unfractured melt is almost more of an exception than a rule! Radial and divergent patterns can be seen among the fracture sets that tell a story of the cooling history. The context image below shows a portion of their wider distribution.

Context for Featured Image; ~ 2.5 km m across [NASA/GSFC/Arizona State University].

Solid objects in the melt, together with the 'shore' of the pond, appear to have influenced the way the cracks organized themselves as the melt cooled. Note how the fractures bend around or radiate from some of the positive relief features in the images above. These could be ejecta blocks or portions of the slumped crater walls in the melt that served to locally accelerate cooling. Their influence might thus be to 'seed' the stress field within the shrinking melt volume, helping some of the cracking to grow from these points, and ultimately resulting in the patterns we see today. Sagging along the shore can cause the cracking to parallel the shoreline. Any motion within the volume of melt, possibly influenced by late-stage additions of molten material, may also have contributed to the patterns observed here.

This WAC mosaic context image shows the size of Jackson crater and is ~113 km across, north is up [NASA/GSFC/Arizona State University].

The extent and complexity of the melt pond features can be explored in the full NAC frame below. Additional examples of impact melt cracking include Polygonal fractures on Tycho ejecta deposits, fractured impact melt in Thales crater, and Moore F.

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