Apollo 15

Parent collection: 

The Apollo 15 landing site was in the Apennine Highlands, and close to Hadley Rille - a long, narrow winding valley. Approximately 76 kg of lunar material including soil, rock, core-tube and deep-core samples were returned to Earth.

This mission was the first flight of the Lunar Roving Vehicle which allowed the astronauts to venture further from the Lunar Module than in previous missions. During three periods of extravehicular activity, or EVA, on July 31st, and August 1st and 2nd, Scott and Irwin completed a record 18 hours, 37 minutes of exploration, travelled 17.5 miles in the first car that humans had ever driven on the Moon.

Apollo 15 was launched on July 26th 1971.

Main image: 
status: 
active

When you look at the Moon on a clear night with the naked eye, you can see colour variations. The overall pattern that they make is sometimes called ‘the man in the Moon’ because some people think they see a face. The lighter areas are the highlands and the darker areas are maria (mare is the singular form).

The lunar highlands represent the original lunar crust, as seen in the previous step. The oldest highland rocks are more than 4.15 billion years old and sometimes as old as 4.4 billion years, which is older than any rock found on Earth. They are mainly anorthosite, but also include dunite and gabbro with increasing depth. These are the oldest rocks on the Moon and are evidence for a magma ocean, as discussed earlier.

In contrast, the maria are basins filled in with basalt and were formed mostly between roughly 3.0 and 3.5 billion years ago. However, there are some small patches that are thought to be as young as around 1.0 billion years. The mare basalts are secondary to the Moon’s formation, in the sense that they did not form from the magma ocean stage like anorthosite, but by later heating and melting of the mantle in the same way that volcanoes are formed on Earth.

Two other types of deposit are found on the surface of the Moon:

regolith: the crushed remains of other rock types that coat much of the surface
breccia: a rock formed of regolith that has been welded together at high temperature and pressure.
Regolith is the mixture of dust, mineral fragments and rock fragments that lies on the surface. Breccia is formed in the explosions when large asteroids hit the Moon.

The Moon has no atmosphere, so even the smallest meteorites just millimetres across reach the surface and form craters. (Such meteorites are called micrometeorites.) Some of the Moon rocks returned to Earth by the Apollo astronauts have small pock marks formed when tiny particles hit them. Each is filled by a thin layer of rock that melted in the impact and then re-solidified.

additional_image: 
Apollo 15 crew: David Scott, Al Worden & James Irwin (courtesy of NASA)
Apollo 15 lunar module and rover (courtesy of NASA)
Apollo 15 rover (courtesy of NASA)
Apollo 15 rover (courtesy of NASA)
Sampling regolith (courtesy of NASA)
Hadley Rille (courtesy of NASA)
Apollo 15 sample locations

Nid: 897
Microscope asset URL
 >View Microscope
Asset URL
Nid: 1356
Microscope asset URL
 >View Microscope
Asset URL
Nid: 898
Microscope asset URL
 >View Microscope
Asset URL
Nid: 899
Microscope asset URL
 >View Microscope
Asset URL
Nid: 900
Microscope asset URL
 >View Microscope
Asset URL
Nid: 901
Microscope asset URL
 >View Microscope
Asset URL
Nid: 902
Microscope asset URL
 >View Microscope
Asset URL
Nid: 903
Microscope asset URL
 >View Microscope
Asset URL
Nid: 904
Microscope asset URL
 >View Microscope
Asset URL
Nid: 905
Microscope asset URL
 >View Microscope
Asset URL
Nid: 906
Microscope asset URL
 >View Microscope
Asset URL
Nid: 907
Microscope asset URL
 >View Microscope
Asset URL
Nid: 908
Microscope asset URL
 >View Microscope
Asset URL
Nid: 1357
Microscope asset URL
 >View Microscope
Asset URL

Pages

Collection description

When you look at the Moon on a clear night with the naked eye, you can see colour variations. The overall pattern that they make is sometimes called ‘the man in the Moon’ because some people think they see a face. The lighter areas are the highlands and the darker areas are maria (mare is the singular form).

The lunar highlands represent the original lunar crust, as seen in the previous step. The oldest highland rocks are more than 4.15 billion years old and sometimes as old as 4.4 billion years, which is older than any rock found on Earth. They are mainly anorthosite, but also include dunite and gabbro with increasing depth. These are the oldest rocks on the Moon and are evidence for a magma ocean, as discussed earlier.

In contrast, the maria are basins filled in with basalt and were formed mostly between roughly 3.0 and 3.5 billion years ago. However, there are some small patches that are thought to be as young as around 1.0 billion years. The mare basalts are secondary to the Moon’s formation, in the sense that they did not form from the magma ocean stage like anorthosite, but by later heating and melting of the mantle in the same way that volcanoes are formed on Earth.

Two other types of deposit are found on the surface of the Moon:

regolith: the crushed remains of other rock types that coat much of the surface
breccia: a rock formed of regolith that has been welded together at high temperature and pressure.
Regolith is the mixture of dust, mineral fragments and rock fragments that lies on the surface. Breccia is formed in the explosions when large asteroids hit the Moon.

The Moon has no atmosphere, so even the smallest meteorites just millimetres across reach the surface and form craters. (Such meteorites are called micrometeorites.) Some of the Moon rocks returned to Earth by the Apollo astronauts have small pock marks formed when tiny particles hit them. Each is filled by a thin layer of rock that melted in the impact and then re-solidified.