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

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

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

Chapter 23. Our Solar System

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.

FCAT Review Space Science

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

Chapter 3 The Solar System

Inner and Outer Planets

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

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.

Inner and Outer Planets

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

CHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration

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

What s in Our Solar System?

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

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

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

The Big Bang Theory (page 854)

Announcement Test 2. is coming up on Mar 19. Start preparing! This test will cover the classes from Feb 27 - Mar points, scantron, 1 hr.

IX. Dwarf Planets A. A planet is defined to be an object that is large enough to coalesce into a sphere and to have cleared its orbit of other

Our Planetary System. Chapter 7

Chapter 23: Touring Our Solar System

Earth Science 11 Learning Guide Unit Complete the following table with information about the sun:

Chapter 17 Solar System

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

1. Cosmology is the study of. a. The sun is the center of the Universe. b. The Earth is the center of the Universe

known since prehistoric times almost 10 times larger than Jupiter

Space Notes 2. Covers Objectives 3, 4, and 8

Your task for each planet...

Universe Celestial Object Galaxy Solar System

The Outer Planets (pages )

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

Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM)

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects.

Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017

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

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

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

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)

The Universe and Galaxies

Cosmology Vocabulary

Directed Reading B. Section: The Outer Planets

Coriolis Effect - the apparent curved paths of projectiles, winds, and ocean currents

The History of the Earth

Comparative Planetology I: Our Solar System. Chapter Seven

Unit 1: The Earth in the Universe

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

Chapter 11 Review Clickers. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.

Lesson 3 THE 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

SPACE NOTES 2. Covers Objectives 3, 4, and 8

9/22/ A Brief Tour of the Solar System. Chapter 6: Formation of the Solar System. What does the solar system look like?

Our Solar System and Its Place in the Universe

The Solar System. Name Test Date Hour

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..

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

1. The Sun is a huge ball of very hot gas in space, which radiates heat and light in one direction.

The Solar System 6/23

ESS Mrs. Burkey FIRST SEMESTER STUDY GUIDE H/K

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

A star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars.

Comparative Planetology I: Our Solar System

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

The Fathers of the Gods: Jupiter and Saturn

Comparative Planetology I: Our Solar System. Chapter Seven

3. Titan is a moon that orbits A) Jupiter B) Mars C) Saturn D) Neptune E) Uranus

The Sun. - this is the visible surface of the Sun. The gases here are very still hot, but much cooler than inside about 6,000 C.

Which of the following statements best describes the general pattern of composition among the four jovian

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)

3. The moon with the most substantial atmosphere in the Solar System is A) Iapetus B) Io C) Titan D) Triton E) Europa

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

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

The Solar System consists of

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

The Solar System. Presented By; Rahul Chaturvedi

Name Date Class. Earth in Space

Human Understanding of both Earth and Space has Changed Over Time. Unit E: Topic One

-Melissa Greenberg, Arielle Hoffman, Zachary Feldmann, Ryan Pozin, Elizabeth Weeks, Christopher Pesota, & Sara Pilcher

CST Prep- 8 th Grade Astronomy

Astronomy Unit Notes Name:

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

Joy of Science Experience the evolution of the Universe, Earth and Life

The Solar System. Chapter Test A. Multiple Choice. Write the letter of the correct answer on the line at the left.

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

Science Practice Astronomy (AstronomyJSuber)

Motion of the planets

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

4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises

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

- newmanlib.ibri.org - The Solar System. Robert C. Newman. Abstracts of Powerpoint Talks

12. Jovian Planet Systems Pearson Education Inc., publishing as Addison Wesley

ASTRONOMY SNAP GAME. with interesting facts

Prentice Hall EARTH SCIENCE

Mass: 1.99 x 1030 kg. Diameter: about km = 100 x the Earth diameter. Density: about kg/m3

A Look at Our Solar System: The Sun, the planets and more. by Firdevs Duru

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999

Similarities & Differences to Inner Planets

Comparative Planetology II: The Origin of Our Solar System. Chapter Eight

Overview of Solar System

Transcription:

SOLAR SYSTEM NOTES

ENERGY TRANSFERS Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium Convection - The transfer of heat through the movement of particles

SUN 99.86% of the mass of the solar system Primary source of energy, light, and heat. The planets are lit because of the light we see reflected from the Sun.

SUN IS A 2 ND OR 3 RD GENERATION STAR HOW DO WE KNOW THAT? Shortly after the big bang, most of the atoms in the universe were hydrogen. (Trace amounts of helium and lithium, but for all intensive purposes, hydrogen was pretty much 'it.') Those first stars, through fusion, began creating heavier elements, as heavy as iron. Some of those stars were massive enough to "go" supernova, and create even heavier elements. Our sun, and the planets that orbit it, all formed from a nebulous cloud of a star that had previously gone supernova. Based on the amount of heavy elements in our solar system, there must have been at least two predecessor stars to have been "precursors" to our sun and it's planets. The sun, being about 4.5 billion years old, vs. a galaxy that is estimated to be about 13.7 billion years old, seems to have formed in the timespan when 2nd and 3rd generation high-mass stars would have been going supernova. So we have methods that support this statement.

SUN S STRUCTURES Photosphere Sunspots Corona Solar flares Convection zone Radiation zone Core

Surface of the Sun appears granulated: Hot material (light) rises to top while cold material (dark) drops down Proof of convection underneath surface!!!

PHOTOSPHERE Photo in Latin means light Outer layer of the Sun Where the light we see comes from.

SUN SPOTS dark spots compared to surrounding regions Early astronomers like Galileo observed these to prove the Sun rotates on an axis.

HELIOSCOPE Helio Greek for Sun scope optical device an instrument used in observing the sun and sun spots

CORONA Latin for crown most easily seen during a total solar eclipse

SOLAR FLARES a sudden brightening observed over the Sun's surface a large energy release Has knocked out power in parts of the World.

SPICULES Short-lived, narrow Jets of gas spewed from surface

SPICULES Short-lived, narrow Jets of gas spewed from surface *Punch out from surface and fold back in. Follows magnetic field lines.

AURORA by the collision of energetic charged particles with atoms in the high altitude atmosphere Aurora Borealis Northern lights Aurora Australis Southern Hemisphere

So we re all gonna die??? Well yeah *since the solar system formed 4.6 billion years ago, the Sun has lost less than 0.1 % of its total mass.

TERRESTRIAL PLANETS MERCURY VENUS EARTH MARS JOVIAN PLANETS JUPITER SATURN URANUS NEPTUNE

ORBITAL ROTATION All planets orbit the same direction around the sun, Counterclockwise.

Axis Tilt

Planets orbit Sun in an elliptical path (oval shape)

Making the Inner Planets - Accretion in the inner solar system: Initially, many moon-sized planetesimals orbited the Sun. Over the course of a hundred million years or so, they gradually collided and coalesced, forming a few large planets in roughly circular orbits.

Inner planets small, solid, dense minerals Iron cores Outer planets large, mostly gas, rings, with solid core

REASONS THE PLANETS ARE SO DIFFERENT The material closest to the Sun was the hottest, and therefore any lighter materials such as gases would have vaporized by the Sun's heat. The materials with a higher melting point (metals) could condense at these higher temperatures and could stay closer to the sun and it s heat. The materials with lower melting points (gases) were able to condense out further from the Sun where it was cooler

Planet Density Saturn is the only planet that is less dense than Water!

MERCURY Rotation Time: 58.6 Earth days Orbit Time: 88 Earth days Does not rotate on same orbital plane as the rest. iron rich planet Mercury has virtually no atmosphere Craters like the Moon

VENUS Rotation Time: 243 days Orbit Time: 224 days Earths' twin sister because same size = same mass = similar density similar gravity similar composition (are made of the same material). atmosphere is made up mostly of carbon dioxide Clouds are filled with sulfuric acid

EARTH Rotation Time: 24 hours Orbit Time: 365.24 days the only planet known to have stable bodies of liquid water on its surface The world is not completely round. It is an oblate spheroid, flattened at the poles and bulging at the equator

MARS Rotation Time: 24.6 hours Orbit Time: 687 Earth days The planet's surface undergoes a chemical process which results in the formation of iron oxide (rust). thin atmosphere of Mars is made of mostly carbon dioxide Valleys and Canyons on Mars suggest that the planet once had large amounts of surface water

JUPITER Rotation Time: 10 hours Orbit Time: 12 Earth years largest planet, has the most moons great red spot on Jupiter is a storm that has been going on for over 300 years Has rings Hydrogen and Helium Would have to be 60x as much mass to be a star

SATURN Rotation Time: 11 hours Orbit Time: 29.46 Earth years Most know for the beautiful rings! Rings are floating chunks of ice, rocks and dust Saturn has the lowest density Atmosphere comprises mostly of Hydrogen and Helium (lightest elements)

URANUS Rotation time: 17.6 hours Orbit Time: 30,685 Earth days Has rings Axis - almost parallel to the plane The nearly horizontal tilt of the axis produces the most extreme seasons in the solar system Uranus is the coldest planet

NEPTUNE Rotation Time: 16.11 hours Orbit Time: 165 Earth Years Has rings Stormiest planet winds up to 1,240 mph methane gas makes it Blue 12 years for Voyager 2 to reach it

PLUTO Considered a planet since 1930 was demoted to a dwarf planet in 2006 Does not rotate on the same orbital plane Smaller and less dense than all planets and Our Moon atmosphere contains traces of methane, nitrogen and carbon dioxide (not a gas giant like other Jovian planets) Sometimes orbits inside Neptune There are similar objects inside the Kuiper Belt

MOONS WORTH LOOKING AT Scientists believe that water could exist below the surface of Europa. (Jupiter moon) Io (another Jupiter Moon) features over 400 active volcanoes Saturn s largest moon is named Titan, it is the only moon known to have a dense atmosphere.