The tiniest of impact craters [Guest post]

When we think about craters on the Moon, we usually think of ones that can be seen with a telescope. But there are also ones we can only see with a microscope, like today’s featured image of a micro-sized crater on a Moon rock!

A truly tiny crater, little more than 10 microns wide, on a Moon rock brought to Earth from Apollo 12. Credit: NASA

Astronauts on the Apollo 12 mission brought 45 rocks from the Moon to Earth. The featured micro crater into an olivine mineral grain is from the rock 12075, seen in a scanning electron microscope (SEM). It spans a little more than 10 microns, compared to the ~60 micron width of a human hair strand. The grain of dust that created this tiny impact crater was probably only about a micron wide. Here’s a quick size comparison with a tardigrade and a human hair strand (thanks Dad for the suggestion!).

Comparison of micro-sized lunar crater with a small tardigrade and a human hair strand. Image sources: 1, 2.

We don’t see such micro craters on Earth, as our atmosphere protects us and small things burn up before they even reach the ground. We see some of those burning things as “shooting stars”, but the grain that made this impact is too small even for that. Because the Moon doesn’t have an atmosphere, every little piece of cosmic dust can make an impact. Such small impact craters are called “micrometeorite impacts” or sometimes “zap pits”.

Some of the rocks that the Apollo program returned were covered with micro craters on the surface, but just on one side, the side that faced upwards on the Moon and was exposed to space. Like this one from Apollo 17, lunar rock 70215.

Apollo 17 rock 70215, subjected to space weathering. Credit: NASA

Image credit: NASA Lunar Reconnaissance Orbiter

Micrometeorite impacts are part of the process of “space weathering”, which slowly changes the properties of lunar rocks and soils, making them appear darker with time. That is why young craters are bright and sometimes have bright rays.

Impacts expose fresh material that is bright, but over time (millions of years), because of all of these tiny impacts, and effects of the solar wind, those rays disappear and the soil gets dark.

Micrometeorites could be a hazard to future lunar visitors and residents. While these tiny grains seem to hit all the time on a geologic time scale, on a human scale, they are actually pretty rare. You’d have to be very unlucky to get hit by one on a short EVA, but if you are designing habitats for long-term use, they are definitely something you need to take into account.

Did you know? You can view Apollo samples with a virtual microscope! Here’s rock 12075


This is a guest post by Dr. Sarah Noble.
Sarah Noble (@intrplnetsarah) is a planetary geologist and a Program Scientist in the Planetary Sciences division at NASA HQ. Her area of expertise is space weathering processes. She was the Program Scientist for NASA’s LADEE spacecraft, and is currently the Program Scientist for the Psyche mission.

Comments are closed.

Create a website or blog at

Up ↑