Mound on the floor of Antoniadi crater floor. Image width is 1.03 km. Sunlight is from the top of this image. M154024477R, image center latitude 69.380°S, longitude 184.678°E [NASA/GSFC/Arizona State University].
Today's Featured Image highlights a circular mound with about 1.1 km in diameter, located on the floor of Antoniadi crater. Central portion, about 650 m across, consists of steeper hemispherical dome, and shallower outer skirt. This unusual feature looks like a flattened "Kagami-mochi" (A Japanese new year decoration composed of two flat circled rice cakes, the smaller placed atop the larger). How did this mound form?
Antoniadi crater is about 143 km in diameter, and is located in the south portion of South Pole-Aitken basin. The central circular portion of the crater floor, about 55 km across, is relatively flat and smooth, formed as a very fluid mare basalt flooded the floor and then hardened. The mound in today's Featured Image is found on this flat surface. Perhaps the mound started out as a small pyroclactic cone, and was covered by late stage lavas? How did the skirt form? There are still many mysteries on the Moon. As LRO collects more measurements the seemingly odd features, like this "Kagami-mochi" mound, will become more familiar.
LRO WAC monochrome mosaic around Antoniadi cater. Image center is lat:69.38°S, lon:186.47°E. Note that north is to the bottom. Footprint of NAC frame and the location of today's Featured Image are indicated by blue box and white arrow [NASA/GSFC/Arizona State University].
Many similar shaped mounds are found on Antoniadi's smooth and flat floor, but are relatively rare on other mare surfaces. Why only in this particular crater? The reason might be due to the relatively young age, this mare basalt is younger than 2.6 billion years. Over time such small features will erode into the background due to the relentless effects of micro-meteorite impacts which work to equalize topographic features.
Find other "Kagami-mochi" shaped mounds in full NAC frame yourself!