Mercury = Hermes Mythology. Planet Mercury, Element, Mercredi God of Commerce, Messenger God, guide to Hades Winged sandals and staff

Similar documents
The Moon. Tidal Coupling Surface Features Impact Cratering Moon Rocks History and Origin of the Moon

crater density: number of craters per unit area on a surface

Announcements. NRAO REU program Feb 1, summerstudents

10. Our Barren Moon. Moon Data (Table 10-1) Moon Data: Numbers. Moon Data: Special Features 1. The Moon As Seen From Earth

Mercury and Venus 3/20/07

Lecture Outlines. Chapter 8. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

Terrestrial World Surfaces

Moon and Mercury 3/8/07

The Moon & Mercury: Dead Worlds

Lecture #10: Plan. The Moon Terrestrial Planets

Astronomy Ch. 8 The Moon and Mercury. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Lunar Geology ASTR 2120 Sarazin

Learning Objectives. they differ in density (composition, core), atmosphere, surface age, size, geological activity, magnetic field?

The Moon. Tides. Tides. Mass = 7.4 x 1025 g = MEarth. = 0.27 REarth. (Earth 5.5 g/cm3) Gravity = 1/6 that of Earth

The Moon. Part II: Solar System. The Moon. A. Orbital Motion. The Moon s Orbit. Earth-Moon is a Binary Planet

Vital Statistics. The Moon. The Tides The gravitational pull between the Earth, the Moon and the Sun causes three inter-related effects: Lunar Phases

ASTRONOMY. Chapter 9 CRATERED WORLDS PowerPoint Image Slideshow

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Lecture 11 Earth s Moon January 6d, 2014

Moon Formation. Capture Hypothesis Many Hypothesis Fission Hypothesis Double Impact Hypothesis Giant Impact Hypothesis

9. Moon, Mercury, Venus

The Sun and Planets Lecture Notes 5. The Moon

Exercise 1: Earth s Moon

Chapter 17. Chapter 17

Where we are now. The Moon Chapters 8.2, 9. Topography. Outline

Chapter 21. The Moon and Mercury: Comparing Airless Worlds

Q. Some rays cross maria. What does this imply about the relative age of the rays and the maria?

Planetary Impacts Planetary Impacts

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am

Chapter 9: The Moon, Earth s Satellite

KEY. Planetary Sciences Section 2 Midterm Examination #2 9:30-10:45 a.m., Tuesday, October 8, 2013

Agenda. Chapter 7. The Earth s Moon. The Moon. Surface Features. Magnificent Desolation. The Moon

9/15/16. Guiding Questions. Our Barren Moon. The Moon s Orbit

The MOON!!! Our Closest Celestial Neighbor

Our Barren Moon. Chapter Ten. Guiding Questions

Astro 210 Lecture 19 October 8, 2010

Astronomy 1 Fall 2016

What is the Moon? A natural satellite One of more than 96 moons in our Solar System The only moon of the planet Earth

Solar System. Sun, 8 planets, hundred moons, thousand.dwarf.planets million asteroids, billion comets etc.

Surface Features. Chapter 7. Rays. Craters. Origin of Lunar Surface Features. Rilles 5/10/12. The Moon

The Moon. A look at our nearest neighbor in Space! Free powerpoints at

Giant Impact Theory Fission Theory Capture Theory Condensation Theory Colliding Planetisimals Theory Regolith Mountain and Mounds Craters and Impacts

The Moon s radius is about 1100 miles. The mass of the Moon is 7.3x10 22 kg

Class Announcements. Solar System. Objectives for today. Will you read Chap 32 before Wed. class? Chap 32 Beyond the Earth

Chapter 7. The Moon. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

MARINER VENUS / MERCURY 1973 STATUS BULLETIN

The Sun Earth Moon System

The Terrestrial Planets

I always wanted to be somebody, but I should have been more specific. Lilly Tomlin Reading has been updated. (All of Chaps. 9& 10) Friday, first sit

The Earth's Moon. The Earth's Moon, in many ways, is prototypical of a substantial fraction of the objects in the Solar System.

1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation

Overview of Solar System

Phys 214. Planets and Life

Chapter 17: Mercury, Venus and Mars

Physics Homework Set 3 Fall 2015

Mercury Data (Table 11-1) 11a. Sun-Scorched Mercury. Mercury Data: Numbers

Theories of Moon Formation

Today. Events. Terrestrial Planet Geology. Fall break next week - no class Tuesday

Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds

LESSON 2 THE EARTH-SUN-MOON SYSTEM. Chapter 8 Astronomy

Unit 3 Lesson 4 The Terrestrial Planets. Copyright Houghton Mifflin Harcourt Publishing Company

SOLAR SYSTEM EXAMPLE EXAM B DIVISION

Moon 101. By: Seacrest School Moon Crew Blake Werab David Prue

Chapter: The Earth-Moon-Sun System

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves.

1/3/12. Chapter: The Earth-Moon-Sun System. Ancient Measurements. Earth s Size and Shape. Ancient Measurements. Ancient Measurements

The Sun and Planets Lecture Notes 6.

A geologic process An erosional force A chronological tool An influence on biology

Inner Planets (Part II)

This evening s announcements

Constructing the Moon

Dana Felberg Steven Hester David Nielsen Zach Weddle Jack Williams

Earth. Physical Properties of Earth kg. Average Density g/cm 2. Surface Gravity 9.8 m/s o C to 50 o C. Surface Temperature

Image of the Moon from the Galileo Space Craft

What is there in thee, moon, That thou shouldst move My heart so potently? By John Keats

known since prehistoric times almost 10 times larger than Jupiter

The Planets. The Terrestrial Planets. Admin. 9/19/17. Key Concepts: Lecture 13. Formulae (will be displayed for you in Midterm 1):

Rilles Lunar Rilles are long, narrow, depressions formed by lava flows, resembling channels.

Chapter 22 Exam Study Guide

Lecture Outlines. Chapter 10. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

18.1 Earth and Its Moon Earth s shape and orbit Earth s shape Earth s orbit around the Sun

If your plan is for one year, plant rice. If your plan is for 100 years, educate children. Confucius

Jupiter and Saturn s Satellites of Fire and Ice. Chapter Fifteen

Solar System. The Jovian Satellites. Regular vs. Irregular Satellites. Jovian satellites reside beyond the frost line

Moon 101. Bellaire High School Team: Rachel Fisher, Clint Wu, Omkar Joshi

Name Date Class. Earth in Space

Terrestrial Planets: The Earth as a Planet

Earth s Moon. Origin and Properties of the Moon. The Moon s Motions

Chapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up. Jason Reed/Photodisc/Getty Images

Chapter. Origin of Modern Astronomy

The Solar Nebula Theory. This lecture will help you understand: Conceptual Integrated Science. Chapter 28 THE SOLAR SYSTEM

The Solar System. Tour of the Solar System

Star groups 88 recognized Stars names by brightness in them. Bright star to. Orion is Sirius

General Introduction. The Earth as an evolving geologic body

Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts

Exploring the Lunar Surface

Lunar Cratering and Surface Composition

Lecture: Planetology. Part II: Solar System Planetology. Orbits of Planets. Rotational Oddities. A. Structure of Solar System. B.

Complete the crossword puzzle. The Moon. (Key # )

Transcription:

Mercury = Hermes Mythology Planet Mercury, Element, Mercredi God of Commerce, Messenger God, guide to Hades Winged sandals and staff

Mercury s Orbit Mercury never seen more than 28 from the sun Revolves/orbits 0.4 AU from sun in 88 days Rotates in 59 days (radar) 3 Rotations to 2 revolutions Resonance

Mercury Differentiation Small mass high temperature=no air Most dense planet except Earth Iron core 75% of radius Tiny magnetic field slow rotation? Liquid core? Melted - heat of formation & decay of radioactive elements

Impact Craters Heavy bombardment cratered surface Strange dark rimmed crater Crater with gullies run to/from

Intercrater Plains More craters than the Lunar Maria 3.5 Billion, but less than Highlands 4.5 Billion years

Caloris Basin Giant impact creates ringed basin Later flooded by lava Jumbled terrain on opposite hemisphere of planet Mariner 10&MESSENGER

Volcanism on Mercury Volcanic vent is kidney shaped depression

Lobate Scarps When Mercury cooled it shrunk & surface wrinkles formed Which pass through a previously (10 9 years) existing crater Smooth plains and intercrater plains (similar to maria) not saturated with craters so must be younger than other areas

Messenger on its way back to Mercury Launched Aug04; loops around sun 15 times, Earth once, Venus twice and Mercury 3 times Will finally orbit in 2011

Rotation of the Moon Revolves & rotates on axis in 27.3 days synodic=29.53d Always keeping one side facing the Earth Resonance due to tidal coupling

Flooding of Basins by Lava Lowlands = mare in blue 3.5 billion years old basalt Heavily cratered highlands in green 4.5 billion years old Farside of Moon has no Maria due to thicker crust

Impact Crater Formation Impactor has velocity 10 times rifle bullet Releases energy 10 times equal mass of dynamite Impactor vaporized when temperature reaches millions K Shock wave forms shocked quartz found only in impacts Rebound can launch rocks without destroying them

Craters Copernicus and Tycho Moon is covered by craters of all sizes Highlands are saturated with craters Mare/lowlands have fewer craters so are younger Notice rays, ejecta blankets, secondary craters

Largest Impacts - Mare Orientale Mare = sea in Latin are sites of major impacts Note: multiringed basin Which flooded with basalt @ 3.5 billion years ago = volcanism

Volcanism - Hadley Rille 150km long, 1.5km across, 300meters deep Formed by flowing lava 3.3 billion years ago

No Atmosphere to Soften Shadows No Atmosphere => no erosion by wind water Escape velocity too low Maximum temperature of 123C&min of -233C

Only Erosion Is Slow Surface Evolution Regolith is crushed rock/dust; covers surface to depth of a few meters Erosion by micrometeorites, solar wind etc. Breccias glued with glass from impacts

Formation of the Moon Fission Protoearth spun so fast that the moon budded off - but wrong angular momentum Coaccretion- formed near Earth from nebula - but no iron core and no volatiles Capture- formed somewhere else- wrong oxygen isotopes + hard to capture + no iron or volatiles Giant Impact- Earth hit by Mars sized asteroid

Formation of Moon by Giant Impactor Elapsed time is about a day; moon forms in a year Earth ends up spinning once in 5 hours, moon in low orbit Earth was differentiated so moon is made from mantle material Correct isotope ratio, no iron core, volatiles evaporate Robin Canup s simulation

Eagle Has Landed Apollo 11 lands in Mare Tranquillitatis Neil Armstrong and Buzz Aldrin 20 July 1969

One Small Step

Hammer and Feather 6 Moon missions &12 astronauts A week to get there Apollo 12 and Surveyor 3

Young Drives Moon Rover

Last Man on the Moon?

Giant Impactor Painting by Kaufmann Problem of the low density of the Moon Solved by Moon being formed from low density mantle material Is it Science? Testable Prediction = Disprovable

Fox TV Moon Hoax No stars: Not enough exposure Illuminated astronaut: bright background Parallel shadows: topography Flag waving: no atmosphere so waved longer & liked it wrinkled

Precession of Mercury s Orbit Most of the precession is due to other planets Part is due to General Relativity

No Atmosphere = No Erosion But Ice at Mercury s & Moon s Poles? VLA radar observations see echo from poles which resembles ice Surface temperature 100K to 700K, but inclination of rotation axes 0º South Pole of Moon with craters permanently in shadow in white Hydrogen detected from neutron spectrometer on Lunar Prospector

Lunar Impact