To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com.

Slides:



Advertisements
Similar presentations
Stars A.The Brightness of Stars -________: A hot glowing sphere of gas that produces energy by fusion. -________: The joining of separate nuclei. Common.
Advertisements

Stars.
Stars, Galaxies, and Constellations
Suns Disturbances Stars Lives Galaxies and Constellations Terms to Know Grab Bag
The Sun – Describe characteristics of the Sun (S6C3PO2 high school)
Chapter 22 Test Review.
DO NOW QUESTION Yesterday we talked about the future of the universe. What do you think will happen to the universe?
Solar System. What is the Solar System? Consists of a star, (like the sun) and all of the planets, moons and other bodies that travel around it. Planets.
Stars & Universe.
Chapter 29 Review Stars.
To return to the chapter summary click Escape or close this document. gpscience.com Image Bank Foldables Standardized Test Practice 1 1 Chapter Resources.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. glencoe.com.
Constellations are groups of stars, sometimes in patterns of animals, or objects. Constellations are important because they can help define where in the.
Click on one of the following icons to go to that resource.
THE UNIVERSE Trotter IV. The Sun  A. All life on Earth depends on the energy that comes from the star in the center of our solar system.  B. Energy.
To return to the chapter summary click Escape or close this document. gpscience.com Image Bank Foldables Video Clips and Animations Standardized Test Practice.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com.
Stars, Galaxies, and the Universe Chapter 22 Page 752.
Stars and Galaxies.
I. Stars A.The Brightness of Stars -Star: A hot glowing sphere of gas that produces energy by fusion. -Fusion: The joining of separate nuclei. Common.
Earth Science Notes Stars and Galaxies.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. life.msscience.com.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com.
The UniverseSection 1 Section 1: The Life and Death of Stars Preview Key Ideas Bellringer What Are Stars? Studying Stars The Life Cycle of Stars.
Early cultures observed patterns of stars in the night sky called constellations. Modern astronomy divides the sky into 88 constellations. Constellations.
What is a star? A big ball of gas & nuclear fusion.
Stars. Astronomy The study of space How astronomers measure distance 1. Light years– The distance light travels in one year 9.461x km.
Astronomy 1 Review.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com.
Stars and Galaxies  Constellations: patterns of stars  Represents mythological characters, animals or familiar objects. Modern astronomy divides sky.
Stars The Brightness of Stars -Star: A luminous sphere of gas with enormous mass, that produces energy by fusion. -Fusion: The joining of separate nuclei.
The UniverseSection 1 Key Ideas 〉 How are stars formed? 〉 How can we learn about stars if they are so far away? 〉 What natural cycles do stars go through?
Star Life Cycle Review. Transports energy from the radiative zone to the surface of the sun. Sunspot Corona Photosphere Convective zone.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com.
Vocabulary The words are in lesson order with the lesson the word is from written as: – L # 1.
To return to the chapter summary click Escape or close this document. red.msscience.com Image Bank Foldables Video Clips and Animations Standardized Test.
THE UNIVERSE Trotter IV. The Sun  A. All life on Earth depends on the energy that comes from the star in the center of our solar system.  B. Energy.
To return to the chapter summary click Escape or close this document. glencoe.com Image Bank Foldables Video Clips and Animations Standardized Test Practice.
Light-year The distance light travels in one year. A unit of distance used to measure between stars.
To return to the chapter summary click Escape or close this document. glencoe.com Image Bank Foldables Video Clips and Animations Standardized Test Practice.
Instructions for using this template. Remember this is Jeopardy, so where I have written “Answer” this is the prompt the students will see, and where.
To return to the chapter summary click Escape or close this document. glencoe.com Image Bank Foldables Video Clips and Animations Standardized Test Practice.
To return to the chapter summary click Escape or close this document. glencoe.com Image Bank Foldables Video Clips and Animations Standardized Test Practice.
Stars & Galaxies.
Objects in the Solar System. Comets Composed of dust and rock particles mixed with frozen water, methane, and ammonia Halley’s comet appears every 76.
To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. glencoe.com.
STARS AND GALAXIES The Life Cycle of a Star: Stars have a life cycle and evolve over time. The mass of a star controls its Evolution Lifespan Ultimate.
Stars & Galaxies By Gina Wike. Constellations A constellation is a group of stars that when viewed from Earth look close together. In most cases, they.
Stars and Galaxies Traveling Beyond the Earth Chapter 21.
DAY 16 September 17, Agenda 1 st RP ‘Stuff’ back Grade Sheets Complete Star Notes Star Concept Map.
I. Stars A.The Brightness of Stars -Star: A hot glowing sphere of gas that produces energy by fusion. -Fusion: The joining of separate nuclei. Common.
To return to the chapter summary click Escape or close this document. glencoe.com Image Bank Foldables Video Clips and Animations Standardized Test Practice.
Ch. 25 Stars and Galaxies Earth Science.
Stars Section 1: The Sun Section 2: Measuring the Stars
Stars change over their life cycles.
Chapter 29 Stars Objectives: You will learn…
Since fusing hydrogen into helium causes a star to be on the main sequence, why do smaller stars stay on the main sequence longer than massive stars that.
Chapter 24 Stars and Galaxies.
It contains hundreds of billions of galaxies
Click on one of the following icons to go to that resource.
Star Life Cycle Review.
Galaxies and Constellations
Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars
Click on one of the following icons to go to that resource.
I. Stars The Brightness of Stars
Chapter 26: Stars and Galaxies
Space Space is really big.
Science Unit D Review Chapter 2.
Presentation transcript:

To return to the chapter summary click Escape or close this document. Chapter Resources Click on one of the following icons to go to that resource. earth.msscience.com Image Bank Foldables Standardized Test Practice Chapter Review Questions Chapter Summary

To return to the chapter summary click Escape or close this document. earth.msscience.com

To return to the chapter summary click Escape or close this document. Click on individual thumbnail images to view larger versions. Image Bank

To return to the chapter summary click Escape or close this document. Image Bank To transfer images to your own power point follow the following steps: Open the “Resource” file from the CD-ROM disc – view the file in the “normal view” or “slide sorter view” mode - go to slide #2 – from there you can click through the images and follow these instructions. Click once on the image. Copy the image Go to your own power point document Paste the image. Transfer Images

To return to the chapter summary click Escape or close this document. Image Bank Circle Chart

To return to the chapter summary click Escape or close this document. Image Bank Constellations

To return to the chapter summary click Escape or close this document. Image Bank Judging Distance

To return to the chapter summary click Escape or close this document. Image Bank Judging Distance

To return to the chapter summary click Escape or close this document. Image Bank Parallax

To return to the chapter summary click Escape or close this document. Image Bank Dark Absorption Lines

To return to the chapter summary click Escape or close this document. Image Bank Sun From Space

To return to the chapter summary click Escape or close this document. Image Bank Photosphere

To return to the chapter summary click Escape or close this document. Image Bank Chromosphere

To return to the chapter summary click Escape or close this document. Image Bank Corona

To return to the chapter summary click Escape or close this document. Image Bank Sunspots

To return to the chapter summary click Escape or close this document. Image Bank Prominence

To return to the chapter summary click Escape or close this document. Image Bank Aurora Borealis

To return to the chapter summary click Escape or close this document. Image Bank Star Classification

To return to the chapter summary click Escape or close this document. Image Bank Supergiant Star

To return to the chapter summary click Escape or close this document. Image Bank Fusion

To return to the chapter summary click Escape or close this document. Image Bank Nebula

To return to the chapter summary click Escape or close this document. Image Bank Life of a Star

To return to the chapter summary click Escape or close this document. Image Bank Nebula

To return to the chapter summary click Escape or close this document. Image Bank Milky Way

To return to the chapter summary click Escape or close this document. Image Bank Elliptical Galaxy

To return to the chapter summary click Escape or close this document. Image Bank Magellanic Cloud

To return to the chapter summary click Escape or close this document. Image Bank Doppler Shift

To return to the chapter summary click Escape or close this document. Image Bank Spectrum Star Receding

To return to the chapter summary click Escape or close this document. Image Bank Sun’s Atmosphere

To return to the chapter summary click Escape or close this document. Foldables Stars, Galaxies, and the Universe Make the following Foldable to show what you know about stars, galaxies, and the universe.

To return to the chapter summary click Escape or close this document. Foldables Fold a sheet of paper from side to side. Make the front edge about 1.25 cm shorter than the back edge.

To return to the chapter summary click Escape or close this document. Foldables Turn lengthwise and fold into thirds.

To return to the chapter summary click Escape or close this document. Foldables Unfold and cut only the top layer along both folds to make three tabs.

To return to the chapter summary click Escape or close this document. Foldables Label the tabs Stars, Galaxies, and Universe.

To return to the chapter summary click Escape or close this document. Foldables Before you read the chapter, write what you already know about stars, galaxies, and the universe. As you read the chapter, add to or correct what you have written under the tabs. Read and Write

To return to the chapter summary click Escape or close this document. 1 1 Reviewing Main Ideas Stars Constellations are patterns of stars in the night sky. Some constellations can be seen all year. Other constellations are visible only during certain season. Parallax is the apparent shift in the position of an object when viewed from two different positions. Parallax is used to find the distance to nearby stars.

To return to the chapter summary click Escape or close this document. 2 2 Reviewing Main Ideas The Sun The Sun is the closest star to Earth. Sunspots are areas on the Sun's surface that are cooler and less bright than surrounding areas.

To return to the chapter summary click Escape or close this document. 3 3 Reviewing Main Ideas Evolution of Stars Stars are classified according to their position on the H-R diagram. Low-mass stars end their lives as white dwarfs. High-mass stars become neutron stars or black holes.

To return to the chapter summary click Escape or close this document. 4 4 Reviewing Main Ideas Galaxies and the Universe A galaxy consists of stars, gas, and dust held together by gravity. Earth's solar system is in the Milky Way, a spiral galaxy. The universe is expanding. Scientists don't know whether the universe will expand forever or contract to a single point.

To return to the chapter summary click Escape or close this document. Chapter Review Question 1 Answer Why do constellations appear to move? Constellations appear to move because Earth is moving. As Earth rotates on its axis, stars appear to complete a circle in the sky.

To return to the chapter summary click Escape or close this document. Chapter Review Question 2 Distances between stars and galaxies are measured in __________. A. astronomical units B. light-years C. red shifts D. spectral lines

To return to the chapter summary click Escape or close this document. Chapter Review Answer The answer is B. A light-year is the distance that light travels in one year, about 9.5 trillion km.

To return to the chapter summary click Escape or close this document. Chapter Review Question 3 Sudden violent eruptions from the Sun’s surface are called __________. A. prominences B. solar flares C. solar winds D. sunspots

To return to the chapter summary click Escape or close this document. Chapter Review Answer The answer is B. Solar flares occur when gases near a sunspot brighten suddenly and shoot outward at high speed.

To return to the chapter summary click Escape or close this document. Chapter Review Question 4 The closer the star, the greater the __________. A. absolute magnitude B. blue shift C. parallax D. red shift

To return to the chapter summary click Escape or close this document. Chapter Review Answer The answer is C. The nearer an object is to the observer, the greater its parallax is.

To return to the chapter summary click Escape or close this document. Chapter Review Question 5 Fusion of hydrogen in a star’s core forms _________. A. carbon B. helium C. oxygen D. water

To return to the chapter summary click Escape or close this document. Chapter Review Answer The answer is B. Temperatures must be high to cause the hydrogen atoms to fuse.

To return to the chapter summary click Escape or close this document. Standardized Test Practice Question 1 What is the name of the star located at X? A. Betelgeuse B. Meissa C. Orion D. Polaris

To return to the chapter summary click Escape or close this document. Standardized Test Practice Answer The answer is D. Polaris is also known as the North Star and is positioned almost directly over Earth’s north pole.

To return to the chapter summary click Escape or close this document. Standardized Test Practice Question 2 Use the diagram to determine which of the following statements is true.

To return to the chapter summary click Escape or close this document. Standardized Test Practice A. Star A must be closest because it has a larger parallax than Star B. B. Star A must be farther because it has a larger parallax than Star B.

To return to the chapter summary click Escape or close this document. Standardized Test Practice C. Star B must be closest because it has a larger parallax than Star A. D. Star B must be farther because it has a larger parallax than Star A.

To return to the chapter summary click Escape or close this document. Standardized Test Practice Answer The answer is C. The nearer an object is to the observer, the greater its parallax. Star B has a large parallax.

To return to the chapter summary click Escape or close this document. Standardized Test Practice Question 3 Which of these would be the most likely meter reading if the light were at a distance of 100 cm A. 120 luxes B. 325 luxes C. 750 luxes D luxes

To return to the chapter summary click Escape or close this document. Standardized Test Practice Answer The answer is A. As distance increases, light intensity decreases.

To return to the chapter summary click Escape or close this document. Standardized Test Practice Question 4 Which structure on the diagram generates CMEs? A. A B. B C. C D. D

To return to the chapter summary click Escape or close this document. Standardized Test Practice Answer The answer is D. This is the corona, which generates coronal mass ejections (CMEs).

To return to the chapter summary click Escape or close this document. Standardized Test Practice Question 5 Which structure in the diagram has the strongest gravity? A. A B. B C. C D. D

To return to the chapter summary click Escape or close this document. Standardized Test Practice Answer The answer is C. This is a black hole, where gravity is so strong that nothing can escape from it.

To return to the chapter summary click Escape or close this document. To advance to the next item or next page click on any of the following keys: mouse, space bar, enter, down or forward arrow. Click on this icon to return to the table of contents Click on this icon to return to the previous slide Click on this icon to move to the next slide Click on this icon to open the resources file. Help Click on this icon to go to the end of the presentation.

To return to the chapter summary click Escape or close this document. End of Chapter Resources File