Crew: Alan Shepard (Commander), Stuart Roosa (Command Module Pilot), Edgar Mitchell (Lunar Module Pilot)
Landing Site: Fra Mauro formation, chosen as an alternative after Apollo 13 failed to land.
Objective: Study the Fra Mauro highlands to gather samples ejected by the Imbrium impact, one of the Moon’s most significant ancient impacts.
Cone Crater Traverse:
The astronauts aimed to collect deep-seated lunar materials by climbing the steep slope of Cone Crater.
Due to navigation difficulties, they stopped just 15 meters from the rim, unknowingly missing the ideal sampling location.
Nevertheless, they retrieved rocks likely ejected from deeper lunar layers.
“Big Bertha” (Sample 14321):
A 9 kg breccia found at the landing site.
Later studies suggested it may contain a piece of Earth’s crust, potentially making it the first known terrestrial rock found on the Moon.
Lunar Equipment Used:
Modular Equipment Transporter (MET): A hand-pulled cart to carry tools and samples.
ALSEP (Apollo Lunar Surface Experiments Package): Left behind to measure moonquakes, solar wind, and heat flow.
Dating the Imbrium Basin:
Samples from Fra Mauro were found to be 3.85 to 3.9 billion years old, confirming the impact age.
This was a key step in establishing a lunar impact chronology.
Moon’s Surface Evolution:
Showed that highland regions were heavily reworked by impacts rather than volcanism.
Provided key insight into how early planetary crusts evolved.
Crew: David Scott (Commander), Alfred Worden (Command Module Pilot), James Irwin (Lunar Module Pilot)
Landing Site: Hadley-Apennine region, near Hadley Rille and the Apennine mountains, at the edge of the Imbrium Basin.
Firsts in Apollo 15:
First extended lunar stay (67 hours on the surface).
First mission with the Lunar Rover, enabling greater mobility (traveled over 27 km).
First deep-space EVA: Worden conducted an EVA outside the Command Module to retrieve film from scientific cameras.
Hadley Rille Exploration:
A deep channel believed to be a collapsed lava tube.
Provided insight into lunar volcanic processes and how lava once flowed on the Moon.
Spur Crater and the “Genesis Rock” (Sample 15415):
A 4.5 billion-year-old anorthosite, believed to be a piece of the Moon’s original crust.
Confirmed that the Moon’s early crust was rich in feldspar, supporting the magma ocean hypothesis.
Green Glass Spherules (Sample 15426):
Volcanic glass indicating fire-fountain eruptions occurred in the Moon’s past.
Helped scientists understand the presence of lunar volatiles, possibly including traces of water.
ALSEP Deployment:
Measured moonquakes and heat flow, providing new data on the Moon’s interior.
Lunar Crust Formation:
The Genesis Rock provided direct evidence of the Moon’s differentiation, meaning it had once been covered in a molten ocean.
Ancient Lunar Volcanism:
Samples showed that lava flows were more extensive than previously thought.
The discovery of Hadley Rille’s structure hinted at underground lava tubes, which could be useful for future lunar bases.
Increased Exploration Capabilities:
The Lunar Rover significantly improved scientific returns, setting the stage for Apollo 16 and 17.
Crew: John Young (Commander), Thomas Mattingly (Command Module Pilot), Charles Duke (Lunar Module Pilot)
Landing Site: Descartes Highlands, chosen to investigate whether the Moon’s highlands were formed by volcanic activity.
Objective:
Test the “Hot Moon” hypothesis (theory that highland regions formed through volcanic processes).
Study materials from outside the mare regions to understand early lunar crust evolution.
Traverse to North Ray Crater:
The largest crater visited by Apollo astronauts.
Collected large breccias, some over 11 kg, showing that the highlands were formed by impact, not volcanism.
House Rock (Sample 67015):
A massive breccia boulder, estimated to be 4.2 billion years old.
Provided a look into the Moon’s earliest impact history.
Lunar Rover Performance:
Allowed them to explore 26.7 km across rough terrain.
Equipment overheating became an issue but was managed successfully.
ALSEP Deployment:
Included a magnetometer, revealing that some lunar rocks had weak magnetic fields.
Gave new clues about the Moon’s early magnetic history.
Disproving the “Hot Moon” Hypothesis:
No volcanic rocks were found—highlands were shaped by impacts.
This helped confirm that the Moon’s surface evolved primarily through impacts, not internal volcanism.
Early Lunar History:
The breccias collected at North Ray Crater showed that major impact events occurred over 4 billion years ago.
Reinforced the idea of the Late Heavy Bombardment, a period of intense asteroid impacts between 4.1 and 3.8 billion years ago.
Lunar Magnetic Field Evidence:
Some highland rocks had traces of magnetization.
Suggested that the early Moon may have had a weak magnetic field at some point.
Lunar Impact History:
Apollo 14: Helped date the Imbrium Basin impact (~3.85 billion years old).
Apollo 16: Showed that the highlands were shaped by even earlier impacts (~4.2 billion years ago).
Apollo 15: The Genesis Rock provided evidence of the Moon’s primordial crust.
Volcanism vs. Impact Processes:
Apollo 14 & 15: Found evidence of ancient lunar volcanism (green glass, Hadley Rille lava tubes).
Apollo 16: Disproved the idea that the highlands were volcanic—they were shaped by asteroid impacts.
Evolution of the Moon’s Surface:
Apollo 14: Fra Mauro samples confirmed the age and scale of Imbrium ejecta.
Apollo 15: Showed the magma ocean hypothesis was correct.
Apollo 16: Indicated the Moon’s crust formed over 4 billion years ago.