MARS. The Red Planet

Similar documents
Learning Objectives. they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field?

InSight Spacecraft Launch for Mission to Interior of Mars

Mars. Asha Hunt Jayden Torrey Manzer

Chapter 17: Mercury, Venus and Mars

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

Mars Exploration Script

Red Planet Mars. Chapter Thirteen

What You Already Know

Mars Update. Presented by NASA/JPL Solar System Educator Don W. Brown

The Main Point. Basic Properties of Mars. Observations. Lecture #19: Mars

Opposition and Conjunction

Traveler s Guide to the Planets Mars Video Worksheet

Jovian Planets Jupiter, Saturn, Uranus and Neptune

Solar System revised.notebook October 12, 2016 Solar Nebula Theory

Terrestrial Atmospheres

Hubble Telescope Picture of Mars

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

SOLAR SYSTEM. planet feature cards

What s in Our Solar System?

Module 4: Astronomy The Solar System Topic 3 Content: The Terrestrial Planets Notes Introduction

The Main Points. The View from the Surface. Geology of Mars. Lecture #20: Reading:

Surface Observations Including from the 2012 Mars Curiosity Rover. Martian Atmosphere

11/4/2015. Venus and Mars. Chapter 13. Venus and Mars. The Rotation of Venus. The Atmosphere of Venus. The Surface of Venus

Mercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0.

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth

The Solar System 6/23

Outline 9: Origin of the Earth: solids, liquids, and gases

Planet Power. Of all the objects in our solar system, eight match these requirements: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, & Neptune

10/31/2010. Opposition and Conjunction. Opposition occurs every 2 years. Best opposition at perihelion. Percival Lowell

known since prehistoric times almost 10 times larger than Jupiter

Starting from closest to the Sun, name the orbiting planets in order.

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury.

Mars: The Red Planet. Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos

The Inner Planets. Chapter 3 Lesson 1. Pages Workbook pages 51-52

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

Mars ( ) The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled

Distance of Mercury to the Sun or the Orbital Radius

Missions mars. Beyond the Book. FOCUS Book

Image of the Moon from the Galileo Space Craft

Terrestrial Bodies of the Solar System. Valerie Rapson

MARS 4 TH ROCK FROM THE SUN MARTIN STEVENS HALESWORTH U3A OCTOBER 2106

Unusual Moon Information

Scale: Mars is 6,787 km in diameter. Image 1. What is the feature across the middle? What do you think the circles on the left side are?

UNIT 3: Chapter 8: The Solar System (pages )

Welcome to Class 13: Is (or was) Life on Mars? Remember: sit only in the first 10 rows of the room

Developed in Consultation with Georgia Educators

The Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour

Activity #1 - Getting Started in Mars Exploration

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

Rocket Science, Reentry and the Race to Mars. From Science Fiction to Simulation

Mission To Mars! A dialogue activity for upper KS2

Exam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280

A medium-sized star. The hottest object found in our solar system.

Exercise 1: Earth s Moon

Mars. Professor Withers Boston University Guest lecture in AS105 Alien Worlds. Thursday :00 NASA

The Solar System. Name Test Date Hour

ASTR 380 Possibilities for Life in the Inner Solar System

DeAnza College Fall 2017 Third Midterm Exam. 1. Use only a #2 pencil on your Parscore sheet, and fill in the bubbles darkly and completely.

Unit 1: The Earth in the Universe

Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006

Welcome to Class 12: Mars Geology & History. Remember: sit only in the first 10 rows of the room

Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of the normal stars.

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN

Directed Reading B. Section: The Outer Planets

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time.

Lesson 2 The Inner Planets

Deimos picture taken on the Viking Mission

Mars Opposition Friday 27 th July 2018

Activity 12: Solar System

Earth & Space Science ~ The Solar System

3. Which of the following statements is false? a. Carnivorous plants get their energy from eating bugs.

Moons of Sol Lecture 13 3/5/2018

Exploring The Planets: Jupiter

Venus: Key Ideas: A Warm Up Exercise. Venus at a Glance -- Orbit. Venus at a Glance Planetary Data

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System

Motion of the planets

ASTRO 120 Sample Exam

Inner Planets (Part II)

The Fathers of the Gods: Jupiter and Saturn

Our Sun. & the Planets. Sun and Planets.notebook. October 18, Our Sun (a quick review) Hydrogen is the main fuel source

Quiz 3 is available for pickup in front

Mystery Object #1. Mystery Object #2

The structure of the Earth and how its motion creates the seasons. The landforms of the earth and the forces that shape the land.

Problem Set 3: Crater Counting

The Solar System. Presented By; Rahul Chaturvedi

Physics Homework Set 3 Fall 2015

SOLAR SYSTEM B Division

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

Shape and Size of the Earth

Chapter: The Solar System

The Latest from Mars: Recent Results and the Next Decade of Exploration

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

Intro to Earth Science Chapter 23 Study Guide

The Jovian Planets (Gas Giants)

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

Astronomy Ch. 10 Mars Review. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MARS, THE RED PLANET.

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

Level One, Lesson 1: The Red Planet

Transcription:

MARS The Red Planet

About the Planet Common Name: Mars Mythological Name(s): - Greek: Ares - Roman: Mars Mars is named after the Roman God of War

A few Pictures...

Distance, Size, and Gravity Compared to Earth Mars average distance from the sun is 228M km, or 1.524 AU Mars diameter is 4220 miles The surface gravity on Mars is roughly 37% of Earth s surface gravity Earth s average distance from the sun is 93M km, or 1 AU Earth s diameter is 7926 miles Mars diameter is 2110/3963 the diameter of Earth

Size Comparison Mars appearance and size compared to Earth

Travel Distance and Time, and Natural Satellites The journey time from Earth to Mars takes approximately 150 to 300 Earth days, depending on the speed of launch, the planets positions in their orbits, and length of the journey. Unlike mars, Earth has a magnetic field which prevents the Sun's dangerous radiation from reaching the planet. Due to the fact that mars does not have a magnetic field the Sun's solar blasts striped away at Mars atmosphere.

Examples include: Viking I in 1976 Viking II in 1976 Mars Recon Orbiter in 2006 Phoenix Lander in 2008 Curiosity Lander in 2012 Viking I took 335 days Viking II took 360 days MRO took 210 days Phoenix Lander took 295 days Curiosity Lander took 253 days

Pictures of Travel Time and Orbit

Mars Natural Satellites Phobos: 6000 km from Mars takes 7 hours and 39 minutes to orbit Mars Deimos: 23460 km from Mars takes 30.3 hours to orbit Mars

Composition of the Planet The Martian Crust is mostly composed of volcanic basalt rock The soil of Mars holds sodium, potassium, chloride, and magnesium The crust is about 30 miles thick Mars does not have tectonic plates Mars has huge volcanoes.

Missions to Mars The Viking missions to Mars are composed of spacecrafts Viking I and Viking II Both consist of an orbiter and a lander Objectives included obtaining high resolution images of the surface, characterizing the structure and composition, and search for possible life on Mars

Missions to Mars (con t) The Mars Observer was launched on September 15, 1992 It was based on a commercial Earth-orbiting communications satellite which was converted into an orbiter for Mars The mission ended prematurely on August 22, 1993 when contact with the spacecraft was lost before entering orbit around Mars

Missions to Mars (con t) The Mars Climate Observer s objective was to function as an interplanetary weather satellite, and was also a communications relay for the Mars Polar Lander It carried a copy of the atmospheric sounder on the Mars Observer spacecraft and lightweight color images combining wide and medium angle cameras

Missions to Mars (con t) The Phoenix mission was the first to return information from one of the polar regions Provides an important contribution to the overall strategy of Mars Objectives included studying the arctic water in the poles, locating a habitable zone, and assess the biological potential for the ice-soil boundary

Missions to Mars (con t) The well known Pathfinder contains a lander and the Sojourner Rover Unprecedented amounts of information have returned from the rover as it explored the Ancient Flood Plains, known as Ares Vallis The Pathfinder Mission was the second launch in the Discovery Program, and cost $150 million for development The Pathfinder was mostly an engineering demonstration for key technologies and concepts that will be used in future missions to Mars

Missions to Mars (con t) Mars Observer (bottom left), landing zones (center), Viking lander (bottom right)

Revolution and Rotation Mars has a rotational period of 1.03 Earth days Mars has a revolution period of 1.88 Earth years The Martian atmosphere is 100 times thinner than Earth s, and is composed of about 95% carbon dioxide, 2.7% nitrogen,.13% oxygen

Comparisons Between Earth and Mars Atmosphere Composition (left), Axial Tilt and Rotation (right)

Did you know? If you weighed 100 lbs. On, Earth you would weigh only 37 lbs on Mars! (Janelle Bundy-Lesley) Mars has seasons like Earth, but they last twice as long. This is because Mars is tilted on its axis by about 25.19 degrees, while the axial tilt of Earth is about 22.5 degrees. (Avery Crawford) Dust storms on Mars are some of the largest storms in the universe; they can last for months and can cover the entire planet (Michael Flicker) Olympus Mons is a 21 km high shield volcano with a diameter of 600 km. It is the second largest mountain in the solar system (Aaron Berry) Phobos is gradually spiraling toward Mars, drawing about 6 feet (1.8 meters) closer to the red planet each century. Within 50 million years, Phobos will either smash into Mars or break up and form a ring of debris around the planet (Erica Barnes)

References http://www.space.com/16903-mars-atmosphere-climate-weather.html http://www.space.com/16895-what-is-mars-made-of.html marsprogram.jpl.nasa.gov/mpf/mpf/science_obj.html space-facts.com/mars/ www.behindthename.com/name/mars coolcosmos.ipac.caltech.edu/ask/86-how-did-mars-and-its-moons-get-theirnames- www.universetoday.com/14822/how-far-is-mars-from-the-sun/