Apollo 15 Mission

Lunar Sample Overview

Apollo 15 basalt 15016 Apollo 15 basalt 15016. This sample has a mass of 923 grams and is up to 13 centimeters across. NASA/Johnson Space Center photograph S71-45477.
Apollo 15 green glass clod 15426 Apollo 15 green glass clod 15426. This sample has a mass of 224 grams. The clods as a whole are several centimeters in size, but the individual glass beads are typically about 0.2 millimeters across. NASA/Johnson Space Center photograph S71-43584.
Apollo 15 sample 15445 Apollo 15 sample 15445 was melted during the Imbrium basin-forming impact 3.84 billion years ago. This sample has a mass of 287 grams and is about 6 centimeters across. NASA/Johnson Space Center photograph S71-44129.

Mare Volcanism

The surface rocks in Mare Imbrium are basalt, as was the case for both the Apollo 11 and Apollo 12 samples. Basalts are dark-colored rocks that solidified from molten lava and consist primarily of the minerals pyroxene and plagioclase. The basalts in Mare Imbrium formed 3.3 billion years ago, 500 million years after the Imbrium impact basin formed. Like the Apollo 12 basalts from Oceanus Procellarum, the Imbrium basalts have low abundances of the element titanium. The basalt photo shown above includes numerous holes, which geologists call vesicles. The vesicles formed as gas bubbles when the lava approached the Moon's surface. The gas later escaped, but it was most likely a combination of carbon dioxide and carbon monoxide. Basalt samples without vesicles were also found on Apollo 15. Vesicles are also found in some basalts on Earth.

Hadley Rille is 135 kilometers long. Near the Apollo 15 landing site, the rille is 1.5 kilometers wide and 300 meters deep. Observations by the crew indicate that the rille formed as a volcanic feature, probably originating as a lava tube whose roof later collapsed. Volcanic channels and lava tubes are also known to occur at many basaltic volcanos on Earth, such as in Hawai'i, but Hadley Rille is much larger than terrestrial volcanic channels.

Mare basalts were emplaced as fluids that flowed easily across the Moon's surface. Another type of volcanic material found at the Apollo 15 landing site is pyroclastic glass. In order for lava to form a glass rather than to crystallize into mineral grains, it must cool very quickly. This sort of rapid cooling can occur if an explosive volcanic eruption hurls material high above the Moon's surface and the material falls back down in the form of small beads. This type of explosive volcanic eruption is also known to occur on Earth and is called a pyroclastic eruption or fire fountain by geologists. Several types of volcanic glass occur in the Apollo 15 samples, the most common and famous of which is the green glass. This glass is very rich in the element magnesium, which causes the green color. Studies of the green glass indicate that it originated at about 400 kilometers below the Moon's surface. Pyroclastic glass was also collected on Apollo 17.

The Apennine Front: Rocks from the Lunar Highlands

The Imbrium basin formed from the impact of a large asteroid or comet with the Moon. The Apennine Mountains were pushed up by the Imbrium basin impact. It was hoped that samples collected from these mountains would include ancient rocks that originated deep in the Moon's crust. The shock of the Imbrium impact melted many rocks. Studies of such rocks indicate that this impact occurred 3.84 to 3.87 billion years ago.

The astronauts were also successful in returning material that was even older than the Imbrium impact. In particular, at Spur Crater on Mount Hadley Delta, they collected an anorthosite, a rock that is composed almost entirely of the mineral plagioclase. This rock is now known as "Genesis Rock." Early in the Moon's history, there was a stage known as the magma ocean in which the Moon's outer layers were molten. As the magma ocean cooled and solidified, the plagioclase-rich anorthosite floated on the surface like icebergs in the Earth's oceans. The existence of the magma ocean phase was first recognized from small fragments in the Apollo 11 samples, but Apollo 15's Genesis Rock is important because it is much larger than any previous sample of lunar anorthosite. Apollo 16 later collected an anorthosite sample that is both larger and older than Genesis Rock. Studies of Genesis Rock indicate an age of about 4 billion years. However, it is believed that this represents a time when the rock experienced a metamorphic alteration and that the rock is actually older than 4 billion years. A norite sample, composed primarily of plagioclase and pyroxene, is about 4.5 billion years old, virtually as old as the Moon itself.

Collecting Moon Rocks
This document describes the tools and procedures used by the Apollo astronauts to collect lunar samples.