known since prehistoric times almost 10 times larger than Jupiter

Similar documents
Earth & Space Science ~ The Solar System

What s in Our Solar System?

The Solar System. Name Test Date Hour

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

The Solar System. Presented By; Rahul Chaturvedi

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

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

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

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.

Our Solar System and Its Place in the Universe

Which of the following planets are all made up of gas? When a planets orbit around the Sun looks like an oval, it s called a(n)

Your task for each planet...

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

Object Type Moons Rings Planet Terrestrial none none. Max Distance from Sun. Min Distance from Sun. Avg. Distance from Sun 57,910,000 km 0.

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

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

1UNIT. The Universe. What do you remember? Key language. Content objectives

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company

Ch : The Solar System

Our Planetary System. Chapter 7

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

Chapter 3 The Solar System

The Moon s relationship with Earth The formation of the Moon The surface of the Moon Phases of the Moon Travelling to the Moon

Unit 12 Lesson 1 What Objects Are Part of the Solar System?

Contents. Section 1: The Sun s Energy. Section 2: The Solar System. Section 3: The Moon

CLASS PERIOD STUDENT NAME SOLAR SYSTEM PROJECT 2.2 P THE INNER & OUTER PLANETS

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

Inner and Outer Planets

Read each slide then use the red or some underlined words to complete the organizer.

Edmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2

Ag Earth Science Chapter 23

Cosmology Vocabulary

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC

Facts about Mercury. Mercury is a small planet which orbits closer to the sun than any other planet in our solar system.

Directed Reading B. Section: The Outer Planets

Astronomy Unit Notes Name:

Inner and Outer Planets

Motion of the planets

23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System

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

ASTRO 120 Sample Exam

Our Solar System. Lesson 5. Distances Between the Sun and the Planets

Activity 12: Solar System

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

ASTRONOMY SNAP GAME. with interesting facts

What is Earth Science?

After you read this section, you should be able to answer these questions:

SOLAR SYSTEM NOTES. Surface of the Sun appears granulated: 10/2/2015 ENERGY TRANSFERS RADIATION FROM THE SUN

Comparative Planetology I: Our Solar System. Chapter Seven

Exploring The Planets: Jupiter

A Survey of the Planets Earth Mercury Moon Venus

When you have completed this workbook, you should know and understand the following:

Prentice Hall EARTH SCIENCE

Celestial Objects. Background Questions. 1. What was invented in the 17 th century? How did this help the study of our universe? 2. What is a probe?

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

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

Mystery Object #1. Mystery Object #2

ALL ABOUT THE PLANETS

TABLE OF CONTENTS. click one to go to that page, or just go on. What is the Solar System? Neptune (Pluto) The Sun. Asteroids. Mercury.

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.

LESSON topic: formation of the solar system Solar system formation Star formation Models of the solar system Planets in our solar system

The Outer Planets (pages )

Introduction to Astronomy

LEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona

Outline. Question of Scale. Planets Dance. Homework #2 was due today at 11:50am! It s too late now.

Solar System Research Teacher Notes The Sun

The Jovian Planets. Why do we expect planets like this in the outer reaches of the solar system?(lc)

Planetarium observing is over. Nighttime observing starts next week.

Chapter 23 Earth Science 11

Science Practice Astronomy (AstronomyJSuber)

Across the Universe. By Gabrielle Sierra

Planets. Chapter 5 5-1

1. thought the earth was at the center of the solar system and the planets move on small circles that move on bigger circles

Similarities & Differences to Inner Planets

The Solar System. Tour of the Solar System

FCAT Review Space Science

The solar system pt 2 MR. BANKS 8 TH GRADE SCIENCE

1. Galaxy (a) the length of a planet s day. 2. Rotational Period (b) dust and gases floating in space

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

What is the Solar System?

Chapter: The Solar System

Unusual Moon Information

Comparative Planetology I: Our Solar System. Chapter Seven

BELL WORK. What do you know about the planets in our solar system? Download today s keynote

SPACE REVIEW. 1. The time it takes for the Earth to around the sun is one year. a. rotate b. revolve

Chapters 7&8. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 21: Solar System [3/12/07] Announcements.

Lesson 1 The Structure of the Solar System

Chapter 23. Our Solar System

9.2 - Our Solar System

Unit 1: The Earth in the Universe

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary

Overview of Solar System

Ch 23 Touring Our Solar System 23.1 The Solar System 23.2 The Terrestrial Planet 23.3 The Outer Planets 23.4 Minor Members of the Solar System

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..

HNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian

outline 1. in the beginning. The Big Bang 2. galaxies -- different types 3. stars -- life cycle 4. the solar system -- sun and planets

solar system outer planets Planets located beyond the asteroid belt; these are known as the gas giants. CELESTIAL BODIES

ASTR-1010: Astronomy I Course Notes Section X

Unit 3 Lesson 5 The Gas Giant Planets. Copyright Houghton Mifflin Harcourt Publishing Company

Transcription:

Mercury

Venus Earth

Mars Jupiter

Saturn Uranus

Neptune 40.329407-74.667345 Sun Mercury Length of rotation Temperature at surface 8 official planets large number of smaller objects including Pluto, asteroids, and comets 865,000 miles almost 10 times larger than Jupiter 25 Earth days 9,900 F temperature of core is almost 281,000,000 F 70% hydrogen. 28% helium, and 2% other metals star with average size, brightness, and intensity classified as a yellow dwarf provides the energy needed for life on Earth sun contains more than 99.8% of the total mass of the solar system more than 100 billion stars in the Milky Way Galaxy 0 3,030 miles Distance from sun 36 million miles 88 Earth days Length of rotation 58.6 Earth days Temperature at surface -292 F to 800 F Surface features rocky and heavily cratered. Closely resembles Earth s moon very thin Mariner l0 in 1974-1975 NASA s Messenger will make several flybys in 2011 closest planet to the sun. Has a highly eccentric orbit named after Roman god of commerce, travel, and thievery often visible with binoculars, but is always very close to the sun, so is only visible at dawn and dusk

Venus Earth Moon 0 7,520 miles Distance from sun 67 million miles 224.7 Earth days Length of rotation 243.2 Earth days Temperature at surface 870 F Surface features flat, volcanic plains and shallow craters very thick cloud layer of sulfuric acid in a carbon dioxide atmosphere Mariner 2 in 1962 has most nearly circular orbit of any planet roughly the same size as Earth, at 95% of Earth s diameter and 80% of Earth s mass named for Roman goddess of lose and beauty one Venus day lasts longer than Venus year dense clouds prevent even the most powerful telescopes from seeing surface understood during 16 century that Earth is another planet orbiting the sun 1 7,930 miles Distance from sun 93 million miles 365.25 days Length of rotation 23 hours, 56 minutes Temperature at surface -95 F to 130 F Surface features 71% covered with mater many different landforms and ecosystems have developed 77% nitrogen, 21% oxygen, and traces of argon, carbon dioxide, and water only known planet to support life oldest known fossils of living organisms are 3.9 billion years old only planet with liquid water on surface only planet with an English name not derived from Greek or Roman mythology Earth s core can reach temperatures higher than surface of sun light from sun takes about eight minutes to reach Earth 2,160 miles 239,000 miles Distance from sun 29.5 Earth days Length of rotation 27.3 Earth days Temperature at surface -245 F to 220 F Surface features rocky and heavily cratered none Luna2 in 1959 Neil Armstrong was the first human to walk on the moon (July 20, 1969) gravitational forces between Earth and moon create high and low ocean tides revolution of the moon around Earth, and its location with respect to the sun, create phases of the moon seen in Earth s sky only extraterrestrial body to have been visited by humans only 12 people have walked on moon

Mars 2 4,220 miles Distance from sun 141 million miles 687 Earth days Length of rotation 24 hours, 37 minutes (Earth time) Temperature at surface -184 F to 77 F Surface features red dust covering a rocky desert environment craters, canyons, volcanoes, polar ice caps very thin composed mostly of carbon dioxide Mariner 4 in 1965 has some of the most varied terrain of any terrestrial planet easily visible from Earth with the unaided eye named for Roman god of war nicknamed the Red Planet several and rovers have landed on and explored surface surface area equivalent to Earth s land surface area Asteroid Belt first asteroid discovered by Giuseppe Piazzi in 1801 Distance from sun many wore discovered by mid1800s range from a few feet to hundreds of miles wide elliptical orbit of asteroid belt around sun takes three to six Earth years rocky material remaining from the formation of the solar system located between the orbits of Mars and Jupiter total mass of all asteroids equals less than that of Earth s moon largest discovered asteroid is as big as Texas Jupiter Distance from sun Length of rotation Temperature at cloud tops 63 known 89,350 miles 484 million miles 11.86 Earth years 9 hours, 55 minutes (Earth time) -238 F no solid surface 90% hydrogen and 10% helium increasing density condenses gas to liquid and metal in the core alternating bands of light and dark clouds circle planet Pioneer l0 in 1973 largest planet. Great Red Spot has been observed since 1 7th century and is big enough to hold two Earths named for the Roman king of the gods more than twice as massive as all other planets combined Galileo Galilei s discovery of four moons in 1610 was first observation of celestial movement not centered around Earth

Saturn Distance from sun Length of rotation Temperature at cloud tops first observed with telescope by Galileo Galilei in 1610 60 known 74,900 miles 886 million miles 29.4 Earth years 10 hours, 40 minutes (Earth time) 292 F No solid surface. 75% hydrogen, 25% helium. Rings composed of innumerable small particles, primarily water ice, in orbit around the planet Pioneer 11in 1979 least dense of all planets has most prominent and easily visible rings of any giant planet rings are less than 1 km thick named for Roman god of agriculture (father of Jupiter) has the strongest winds in the solar system, measured at over 1,100 mph at the equator Uranus Neptune Sir William Herschel, 1781 27 known 31,765 miles Distance from sun 1.785 billion miles 83.8 Earth years Length of rotation 17 hours, 14 minutes (Earth time) Temperature at cloud -345 F tops no solid surface. Consists of hydrogen, helium, and methane Voyager 2 in 1986 (only visit) not visible to the unaided eye named for the Greek sky god and father of the Titans (including Cronus/Saturn) Johann Gottfried Gate, 1846 13 known 30,775 miles Distance from sun 2.795 billion miles 163.7 Earth years Length of rotation 16 hours, 7 minutes (Earth time) Temperature at cloud tops -346 F no solid surface consists of hydrogen, helium, and methane Voyager 2 in 1986 (only visit) not visible to the unaided eye atmosphere makes the planet appear blue named for Roman god of the sea has very faint and thin rings

Pluto Clyde Tombaugh, 1930 3 1,485 miles Distance from sun 3.65 billion miles 248 Earth years Length of rotation 6 days. 9 hours (Earth time) Temperature at surface -391 F to -346 F little is known never visited by New Horizons launched in 2006 and scheduled to reach Pluto in 2015 classified as a dwarf planet not visible to the unaided eye orbit is highly eccentric sometimes closer to sun than Neptune smaller than seven of the solar system s moons light from sun takes about five and a half hours to reach Pluto