Encyclopedia

secondary craters

secondary craters

Depressions produced by the impacts of low-velocity crater ejecta. Secondary craters are usually elongated radially with respect to the primary crater and form loops, crater chains, and crater clusters. They tend to lie outside the ejecta blanket.
Collins Dictionary of Astronomy © Market House Books Ltd, 2006
Mentioned in
References in periodicals archive
This alignment of craters points back to the western side of the Imbrium Basin--so could these be a string of large secondary craters like the ones radiating from the Orientale Basin on the lunar farside?
Close to the crater rim, this ejecta deposit forms a continuous blanket smothering the underlying terrain; further out, the ejecta lands as a scattered assortment of fine grained dust and larger bombs that may themselves form small secondary craters. In addition to cratering the surface of the Earth, an impact event initiates several other processes that may have severe environmental consequences.
"Clusters of craters may also be created when a large impact ejects rock fragments with such force that they travel from a few kilometres to hundreds of kilometers before returning to the surface, creating new impacts called secondary craters," ESA adds.
Other portraits show details of a surprisingly high number of secondary craters, small pockmarks created during the formation of larger craters.
With your telescope, look closely at Copernicus's ray system in Mare Imbrium, near the crater Pytheas, and you can see where Copernicus's ejected material excavated numerous small secondary craters.
Some of this includes coherent chunks large enough to create secondary craters.
But some lettered craters are true secondary craters, excavated by ejecta thrown out by the formation of their named crater.
Shoemaker noticed that the 59-km-wide crater Eratosthenes, which interrupts the Montes Apenninus, has small secondary craters and faint rays visible at full Moon on the nearby plains of Mare Imbrium.
Studies of high-resolution spacecraft images demonstrate that at the meter scale, there are millions of secondary craters for every large primary.
Farther away the ejecta do not cover every piece of pre-existing terrain and so are called the discontinuous ejecta deposit; these deposits include secondary craters and rays.
The excavated material creates rays and secondary craters. Because of the projectile's momentum, rays formed in the downrange direction are longer than in the uprange direction.
Copyright © 2003-2025 Farlex, Inc Disclaimer
All content on this website, including dictionary, thesaurus, literature, geography, and other reference data is for informational purposes only. This information should not be considered complete, up to date, and is not intended to be used in place of a visit, consultation, or advice of a legal, medical, or any other professional.