Vallis Rheita: [SE/N14] At 276 miles, the Rheita Valley is the longest distinct valley on the Moon. If you look closely at this formation you will see that it is not a valley in the traditional sense but is made up of a series of interlocking craters whose alignment significantly points back to Mare Nectaris, their place of origin. When the Nectaris basin was blasted out 3.9 billion years ago, more than a dozen mountain-sized chunks of debris took flight in a curiously straight line, and when they landed they ploughed out a 240-mi. long trough which we enjoy observing today as the Rheita Valley.
Although the Moon usually appears absolutely flat, this sector of the Moon gives you a noticeable three-dimensional effect as Rheita Valley diminishes into the distance around the curve of the Moon.1
Cauchy domes: [NE/J13] During sunrise over this area you will have an opportunity to view good examples of lunar domes, low rounded features that resulted from magma which rose from underneath and created blister-like hills on the Moon’s surface. Sometimes the lava actually burst out of the tops of these domes and you can still see the resulting vents. Both types of domes can be seen here just south of Rupes Cauchy. Can you see the tiny crater pit on top of Cauchy ω (omega), the dome to the east?
1 During a lunar eclipse you will frequently notice a striking three-dimensional effect as light being refracted through the atmosphere on opposites sides of the Earth strike the lunar surface from different angles.
It is highly recommended that you get a copy of Sky and Telescope’s Field Map of the Moon, the very finest Moon map available for use at the telescope. It is available for $10.95 at www.skyandtelescope.com and on Amazon. All features mentioned in this blog will be keyed to the grid on the Field Map and will look like this: Plato: [NW/D9]
Courtesy of Gray Photography of Corpus Christi, Texas
Lunar photos: NASA / USGS / BMDO / LROC / ASU / DLR / LOLA / Moon Globe. Used by permission
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