Dorsa Whiston

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Dorsa Whiston is a wrinkle ridge system at 29°24′N56°24′W / 29.4°N 56.4°W / 29.4; -56.4 in Oceanus Procellarum on the Moon. It is 85 km long and was named after William Whiston in 1976.

Wrinkle ridge ridge, feature commonly found on lunar maria

A wrinkle ridge is a type of feature commonly found on lunar maria. These features are low, sinuous ridges formed on the mare surface that can extend for up to several hundred kilometers. Wrinkle ridges are tectonic features created when the basaltic lava cooled and contracted. They frequently outline ring structures buried within the mare, follow circular patterns outlining the mare, or intersect protruding peaks. They are sometimes called veins due to their resemblance to the veins that protrude from beneath the skin. These are found near craters.

Oceanus Procellarum vast lunar mare on the western edge of the near side of Earths Moon

Oceanus Procellarum is a vast lunar mare on the western edge of the near side of the Moon. It is the only one of the lunar maria to be called an "Oceanus" (ocean), due to its size: Oceanus Procellarum is the largest of the maria, stretching more than 2,500 km (1,600 mi) across its north-south axis and covering roughly 4,000,000 km2 (1,500,000 sq mi), accounting for roughly 10.5% of the total lunar surface area.

Moon Earths natural satellite

The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite. It is the fifth-largest natural satellite in the Solar System, and the largest among planetary satellites relative to the size of the planet that it orbits. The Moon is after Jupiter's satellite Io the second-densest satellite in the Solar System among those whose densities are known.

Mosaic of Apollo 15 images, showing part of Dorsa Whiston Dorsa Whiston AS15-97-13264-5.jpg
Mosaic of Apollo 15 images, showing part of Dorsa Whiston

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