Moon Metrics Quest

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Explore lunar science gems

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Nayla P

Estados Unidos

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Moon Metrics QuestVersión en línea Explore lunar science gems por Nayla P 1 Slide 1 — The Moon as a Witness Plate The Moon as a fossil world: with no atmosphere or plate tectonics, it preserves a 4‑billion‑year solar system record erased on Earth by erosion and activity. 2 Slide 2 — Evidence From Apollo Apollo core samples show the solar wind’s chemistry shifted about 2 billion years ago, revealing a changing solar environment. 3 Slide 3 — Connection to Earth Studying lunar impacts helps understand Earth’s major events, including mass extinctions like the K-T event that ended the dinosaurs. 4 Slide 4 — Mapping the Moon (LOLA & LRO) Current maps are imperfect: near side errors up to 1 km, far side several km. Precision matters for missions. 5 Slide 5 — The LOLA Instrument The Lunar Orbiter Laser Altimeter (LOLA) on LRO bounces 28 laser pulses per second, achieving high‑precision 3‑D maps. 6 Slide 6 — How It Works LOLA’s 0.6‑ns timing creates accurate surface elevations, enabling vertical accuracy approaching 1 meter for safe navigation. 7 Slide 7 — The Goal Produce maps as accurate as USGS hiking maps to support astronaut safety and mission planning. 8 Slide 8 — Dust Hazards: Moon vs. Mars Moon dust: abrasive, mechanical damage; Mars dust: chemical toxins and toxicity risks. 9 Slide 9 — Dust Characteristics Moon dust: sharp, glassy fragments; lunar hay fever symptoms. Mars dust: asbestos-like particles with harmful chemicals. 10 Slide 10 — Key Terms & Projects Dust initiatives: Project Dust develops coatings to repel dust. Regolith is the dusty surface layer; Clementine provided earlier maps.

Moon Metrics QuestVersión en línea

Explore lunar science gems

por Nayla P

Slide 1 — The Moon as a Witness Plate

The Moon as a fossil world: with no atmosphere or plate tectonics, it preserves a 4‑billion‑year solar system record erased on Earth by erosion and activity.

Slide 2 — Evidence From Apollo

Apollo core samples show the solar wind’s chemistry shifted about 2 billion years ago, revealing a changing solar environment.

Slide 3 — Connection to Earth

Studying lunar impacts helps understand Earth’s major events, including mass extinctions like the K-T event that ended the dinosaurs.

Slide 4 — Mapping the Moon (LOLA & LRO)

Current maps are imperfect: near side errors up to 1 km, far side several km. Precision matters for missions.

Slide 5 — The LOLA Instrument

The Lunar Orbiter Laser Altimeter (LOLA) on LRO bounces 28 laser pulses per second, achieving high‑precision 3‑D maps.

Slide 6 — How It Works

LOLA’s 0.6‑ns timing creates accurate surface elevations, enabling vertical accuracy approaching 1 meter for safe navigation.

Slide 7 — The Goal

Produce maps as accurate as USGS hiking maps to support astronaut safety and mission planning.

Slide 8 — Dust Hazards: Moon vs. Mars

Moon dust: abrasive, mechanical damage; Mars dust: chemical toxins and toxicity risks.

Slide 9 — Dust Characteristics

Moon dust: sharp, glassy fragments; lunar hay fever symptoms. Mars dust: asbestos-like particles with harmful chemicals.

Slide 10 — Key Terms & Projects

Dust initiatives: Project Dust develops coatings to repel dust. Regolith is the dusty surface layer; Clementine provided earlier maps.

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