KS

Astro 105

Apollo 14 (February 1971)

Mission Overview

  • 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.

Key Activities

  • 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.

Scientific Impact

  • 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.


Apollo 15 (July 1971)

Mission Overview

  • 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.

Key Activities

  • 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.

Scientific Impact

  • 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.


Apollo 16 (April 1972)

Mission Overview

  • 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.

Key Activities

  • 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.

Scientific Impact

  • 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.


Final Summary and Exam Tips

Major Themes Across Apollo 14–16:

  • 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.