Lunar Crater Types
Explanation:
There are 11,462 craters larger than 2 km on the lunar nearside.
But the amazing thing is most of them look pretty similar. In 1978, Leif Andersson
and I compiled data on the 2,598 freshest (unmodified by later impacts or lavas)
craters, and identified five different crater types that accounted for 99% of the
craters. Because we worked at the Lunar & Planetary Lab we called these the LPL
Crater Types. Virtually all craters with diameters smaller than 10 km are our Albategnius
C (ALC) or Biot (BIO) crater types. These are classic bowl-shaped craters, looking
like they were turned out on a lathe. BIO differ from ALC in having small flat floors.
Sosigenes (SOS) craters have broad flat floors, lack central peaks and terraces.
At diameters of 15 to 50 km Triesnecker (TRI) type craters are common. Parts of their
inner walls have slumped onto their floors, sometimes covering their small central
peaks, Virtually all fresh craters larger than 50 km look like Tycho (TYC). They
are deep, have terraced walls, flat floors and often massive peaks. At diameters
larger than a few hundred kilometers, central peaks disappear and craters become
basins. ALC and BIO are called simple craters and TRI and TYC are complex craters
- increasing energy from larger impacting bodies causes the differences in morphology.
SOS are peculiar. It is not clear if they are modified primary impact craters or
basin secondaries. All of these crater types, along with diameters and depths appear
in the LPL crater catalog of 30 years ago that was
never published. The graph shows the percentage of craters of each LPL Type at different
crater diameters
