Solar System Planets The Earth Moon I Moon

Solar System Planets: The Earth + Moon I. Moon - Atmosphere - Surface/Geological Features/Moon Rocks - Interior - Origin II. Mercury - Basic Facts - Exploration - Cratering 13 Oct 2003 Solar System - Dr. C. C. Lang 1

The Moon has no atmosphere • allows us to see the surface with fine detail • escape speed is too low on the Moon - all gas molecules can escape! • no atmospheric pressure means that water can not exist in liquid form - only in solid or vapor • temperature variations – extreme! - day T = 403 K = 266 F - night T = 93 K = -292 F - day/night are each 2 weeks long! • no weathering of the surface by water, storm • no protection from high energy solar particles, cosmic rays 13 Oct 2003 Solar System - Dr. C. C. Lang 2

Lunar Geological Features 1. Craters • ~30, 000 visible with small telescopes from Earth • millions visible from lunar orbiting satellites • origin: interplanetary debris • sizes: largest 100’s km across a result of fast moving impact rocks of only a few km’s across! • large craters often produce “central peak” craters 13 Oct 2003 Solar System - Dr. C. C. Lang Clavius Crater diameter = 232 km depth of 16, 000 feet 3

Lunar Geological Features 2. Lunar “Maria” - dark, smooth regions • first thought to actually be wet areas (before we knew Moon had no atmosphere) • now believed to be smoother, younger (fewer craters) surfaces • idea is that impacts created large basin and then lava flowed over surface • relatively ‘low’ compared to highlands on moon; 2 -5 km below other parts • rough mountain ranges surrounding ‘maria’ suggest large impact originally • evidence for ‘flows’ (lava? ) along the smooth maria 13 Oct 2003 Solar System - Dr. C. C. Lang 4

Lunar Geological Features 3. Lunar Highlands • most of moon (85%) is actually covered with lighter, higher land: Highlands • predominantly on the side of the Moon facing away from Earth • roughly cratered, but no smooth lava flow ‘maria’ regions • crust must be thicker in the highland areas 13 Oct 2003 Solar System - Dr. C. C. Lang 5

Cratering: Age of Moon’s Surface • can use cratering patterns to determine AGE of surface • no atmosphere to protect bombardment; no erosion by wind/water OLD surface (as old as ~3 billion years) The smaller the planet, the less internal heat (geology) it will have; less geological activity on surface • Earth’s surface only a few 100 Myrs old (geological activity has re-surfaced planet) • highlands have many more craters; maria have fewer craters highlands ‘older’ 13 Oct 2003 Solar System - Dr. C. C. Lang 6

A Brief History of Lunar Exploration • 1959: Soviet Lunas 1, 2, 3 orbited around Moon • 1960’s: US Ranger - flyby mission - first space pictures - many TV cameras • 1966 -67: Lunar Orbiter - 5 orbiting spacecraft - full coverage of pictures • 1966 -68: Lunar Surveyor - surveying for landing sites - testing the “soil” (sink? ) 13 Oct 2003 Solar System - Dr. C. C. Lang 7

Highlights from Apollo 11 mission launch: July 16 th 1969 arrival at Moon: July 20 th 1969 first humans to land on the Moon Command Module (CM): “Columbia” 13 Oct 2003 Neil Armstrong “Buzz” Aldrin Solar System - Dr. C. C. Lang Michael Collins 8

On July 20, 1969, after a four day trip, the Apollo astronauts arrived at the Moon. This photo of Earthrise over the lunar horizon is one of the most famous images returned from the space program, although even the astronauts themselves cannot remember who actually took it. 13 Oct 2003 Solar System - Dr. C. C. Lang 9

First steps on the Moon • July 20 th 1969 - Neil Armstrong - “Buzz” Aldrin 13 Oct 2003 Solar System - Dr. C. C. Lang 10

Touchdown of Moon astronauts near the coast of Hawaii on July 26 th 1969 13 Oct 2003 Solar System - Dr. C. C. Lang 11

Lunar Exploration: Apollo Missions • Apollo 1 -10: pre-landing missions (Apollo 1 module fire killed 3 astronauts while being tested) • Apollo 11 -17 landed (except Apollo 13, which had an explosion and returned to Earth) 12 different astronauts walked on the Moon during 1969 -1972 • Principal Scientific results of the Apollo missions: 1. The Moon is ancient and still preserves an early history (the first billion years) that must be common to all terrestrial planets. 2. The youngest Moon rocks are virtually as old as the oldest Earth rocks. The earliest processes and events that probably affected both planetary bodies can now only be found on the Moon. 3. Early in its history, the Moon was melted to great depths to form a "magma ocean. " The lunar highlands contain the remnants of early, low density rocks that floated to the surface of the magma ocean. 4. The Moon is not a primordial object; it is an evolved terrestrial planet with internal zoning similar to that of Earth. 5. The Moon is lifeless; it contains no living organisms, fossils, or native organic compounds 13 Oct 2003 Solar System - Dr. C. C. Lang 12

Recent Lunar Exploration • 1994: Clementine - UV, IR, visible cameras - possible water ice at poles - radio waves reflected off ice • 1998: Lunar Prospector - also found evidence for ice - crashed near pole in 1999 • Currently: Smart 1 Probe - European satellite - ion propulsion (several months!) - will search for water at poles 13 Oct 2003 Solar System - Dr. C. C. Lang 13

Moon Rocks: Sampling the Surface of the Moon • surface material: “regolith” – pulverized by constant impacts • ~2500 samples brought back by astronauts; ~850 lbs total!! • all rocks are IGNEOUS (i. e. , from molten processes) • totally dry rocks (no water) • all rocks older than 3 Byr 13 Oct 2003 Solar System - Dr. C. C. Lang 14

Moonquakes: Studying the Moon’s Interior • ~ 3000 quakes/year • much lower intensity than Earth: 0. 5 -1. 5 Richter • indicate that Moon’s interior is more rigid than Earth’s (some ‘plasticity’) Seismometer placed on Moon by lunar astronauts Solar System - Dr. C. C. Lang 13 Oct 2003 15

Moon’s interior structure crust is thicker on non-Earth facing side • iron-rich core like Earth • asthenosphere layer: somewhat pliable “plastic” layer • solid layer just below surface – no plate tectonics • smaller planet than Earth – less internal energy, less geological activity! • moon probably had a weak magnetic field early in history 13 Oct 2003 Solar so System - Dr. C. C. is Lang 16 - core is now solid, no current generated

Color-coded images illustrate surface geography Clementine data Galileo data – flyby in 1989 • blue – lowland marias 13 Oct 2003 • red - highlands Solar System - Dr. C. C. Lang • red - highlands 17

Theories for Origin of Moon • Fission: originally part of Earth but torn free – Problem: would have fallen back or been flung into space, not into orbit. – Fails to explain why lunar chemistry differs from Earth's • Co-Creation: formed in its present orbit – can not explain why lunar chemistry differs from Earth's • Capture: formed as a separate planet but captured by Earth – Conditions for successful capture very stringent • Impact: formed from Mega-Impact of Mars-sized planet – Computer modeling suggests SS forms 100 or so small planets, then collide to make larger objects – can explain differences in chemistry: – impact occurred after chemical differentiation in Earth; therefore, not as much iron was part of the Moon – high temperatures during impact would have vaporized the volatile and water vapor in rocks – Currently favored model 13 Oct 2003 Solar System - Dr. C. C. Lang 18

Computer Simulation of Formation of Moon • Moon may have formed by a Mars-sized object impact on Earth • Some of the material does not fall back onto the Earth, but forms a satellite of Earth 13 Oct 2003 Solar System - Dr. C. C. Lang 19

This powerpoint was kindly donated to www. worldofteaching. com http: //www. worldofteaching. com is home to over a thousand powerpoints submitted by teachers. This is a completely free site and requires no registration. Please visit and I hope it will help in your teaching. 13 Oct 2003 Solar System - Dr. C. C. Lang 20