Astronomy Universe: all of space and everything in it

Similar documents
Stars and Galaxies 1

CHAPTER 4 STARS, GALAXIES & THE UNIVERSE

What is the sun? The sun is a star at the center of our solar system.

Stars, Galaxies, and the Universe

The Big Bang Theory (page 854)

25.2 Stellar Evolution. By studying stars of different ages, astronomers have been able to piece together the evolution of a star.

Stars & Galaxies. Chapter 27 Modern Earth Science

Beyond Our Solar System Chapter 24

Earth Science, 13e Tarbuck & Lutgens

Directions: For numbers 1-30 please choose the letter that best fits the description.

The Universe. But first, let s talk about light! 2012 Pearson Education, Inc.

Stars & Galaxies. Chapter 27, Section 1. Composition & Temperature. Chapter 27 Modern Earth Science Characteristics of Stars

Chapter 28 Stars and Their Characteristics

The Universe. is space and everything in it.

Directed Reading A. Section: The Life Cycle of Stars TYPES OF STARS THE LIFE CYCLE OF SUNLIKE STARS A TOOL FOR STUDYING STARS.

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars

What is a star? A body of gases that gives off tremendous amounts of energy in the form of light & heat. What star is closest to the earth?

The Universe and Galaxies. Adapted from:

Galaxies Galore. Types of Galaxies: Star Clusters. Spiral spinning wit arms Elliptical roundish Irregular no set pattern

Prentice Hall EARTH SCIENCE

Chapter 21: Stars Notes

Stars. The composition of the star It s temperature It s lifespan

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE

Universe Celestial Object Galaxy Solar System

ANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study

The Universe. What is it? What is in it? How did it form? How will it end? How do we know?

What is the solar system?

chapter 31 Stars and Galaxies

STARS AND GALAXIES STARS

Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc)

Beyond the Solar System 2006 Oct 17 Page 1 of 5

TAKE A LOOK 2. Identify This star is in the last stage of its life cycle. What is that stage?

Study Guide Chapter 2

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following:

LESSON 1. Solar System

Cosmic Microwave Background Radiation

Earth Space Systems. Semester 1 Exam. Astronomy Vocabulary

CHAPTER 28 STARS AND GALAXIES

CHAPTER 9: STARS AND GALAXIES

25/11/ Cosmological Red Shift:

The Universe and Galaxies

LIFE CYCLE OF A STAR

Edwin Hubble Discovered galaxies other than the milky way. Galaxy:

Textbook Chapters 24 - Stars Textbook Chapter 25 - Universe. Regents Earth Science with Ms. Connery

The Night Sky. The Universe. The Celestial Sphere. Stars. Chapter 14

Chapter Introduction Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars Lesson 3 Evolution of Stars Lesson 4 Galaxies and the Universe

Stars and Galaxies. Content Outline for Teaching

Galaxies and Star Systems

Physics HW Set 3 Spring 2015

Modern Astronomy Review #1

1. The symbols below represent the Milky Way galaxy, the solar system, the Sun, and the universe.

Physics Homework Set 2 Sp 2015

Name Date Period. 10. convection zone 11. radiation zone 12. core

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

27.1: Characteristics of Stars

Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti

Test Name: 09.LCW.0352.SCIENCE.GR Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: Date: 09/21/2017

NSCI 314 LIFE IN THE COSMOS

Stellar Evolution Notes

Lecture PowerPoints. Chapter 33 Physics: Principles with Applications, 7 th edition Giancoli

The Universe. 3. Base your answer to the following question on The diagram below represents the bright-line spectrum for an element.

29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A

Astronomy. Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes

ASTRONOMY 1 FINAL EXAM 1 Name

TEACHER BACKGROUND INFORMATION

Our Galaxy. Milky Way Galaxy = Sun + ~100 billion other stars + gas and dust. Held together by gravity! The Milky Way with the Naked Eye

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

Ch. 25 In-Class Notes: Beyond Our Solar System

Science 30 Unit C Electromagnetic Energy

THE ORIGIN OF THE UNIVERSE AND BLACK HOLES

3. c 4. a 5. f 6. b 7. e. 1. Stars are bright and hot. 2. Distances between stars are measured in light-years. 3. The sun is a yellow star.

Distance Measuring Techniques and The Milky Way Galaxy

Figure 19.19: HST photo called Hubble Deep Field.

Clicker Questions (chapters 6-18)

BROCK UNIVERSITY. Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015

Chapter 15 The Milky Way Galaxy. The Milky Way

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe

The Stars. Chapter 14

GraspIT Questions AQA GCSE Physics Space physics

Arvind Borde / AST 10, Week 2: Our Home: The Milky Way

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

Astronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe.

AST 102 chapter 5. Radiation and Spectra. Radiation and Spectra. Radiation and Spectra. What is light? What is radiation?

Astronomy Part 1 Regents Questions

Practice Test: ES-5 Galaxies

Introduction to the Universe. What makes up the Universe?

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe

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

1 The Life Cycle of a Star

Galaxies and the Universe

Introduction to the Universe

Life Cycle of a Star - Activities

Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003

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.

The Formation of Stars

Astronomy 104: Second Exam

Galaxies and Stars. 3. Base your answer to the following question on The reaction below represents an energy-producing process.

Cosmic Landscape Introduction Study Notes

Chapter 1 Our Place in the Universe

The Milky Way Galaxy

Transcription:

Astronomy Universe: all of space and everything in it Most (90%) of the universe is made up of: dark matter: stuff we think is there due to amount of mass we think is there but is not detected by the instruments we have available at this time http://media.skysurvey.org/interactive360/index.html

Nebula: large amount of gases spread out in an immense volume All stars start as part of a nebula

Star: large amount of glowing gas in a small volume mostly hydrogen It creates energy through nuclear fusion of hydrogen to helium in its core. We see and feel this release of energy as sunshine

Globular cluster: a group of 10,000 to 1 million stars (that s a LOT)

Galaxy: a giant structure that contains hundreds of BILLIONS of stars 3 main types: 1. spiral 2. elliptical 3. irregular

1. spiral: have arms that spiral outward like a pinwheel Milky Way: our galaxy We are on an outer arm.

2. elliptical: looks like a flattened ball; 3. irregular: No regular shape

Galactic cluster: groups of galaxies held together by gravity The Milky Way is part of a galactic cluster with 30 other galaxies traveling together called, The Local Group.

Life Cycles of Stars

Supernova: explosions of dying large stars. Can be seen without a telescope. Neutron star: extremely small, dense leftovers from a supernova supernovae shrink into neutron stars

Black hole: what remains after the most massive stars die gravity is so strong that nothing can escape (not even light) many scientists think the center of Milky Way contains a black hole Artist s rendition. Not a real photograph!!

How we get information about space: (no man has ever been farther than the moon) One way: space telescopes! the Hubble Space Telescope (looks at distant galaxies & at planets in our solar system) Kepler Space Telescope (looks for planets around other stars (exoplanets))

How do we measure movement and distances in space Within our solar system we use radar and the formula for speed: Speed = distance/time Speed of light = 186,000 mi./sec or 300,000km/sec. That s around Earth 7 ½ times in one second! ALL EM waves travel at the speed of light.

Measuring Distance within our Solar System. Astronomical Unit (AU): distance between the Earth and Sun Approximately 93,000,000 miles Used only within our solar system to measure distances between planets and the sun

Takes about 8 minutes for sunlight to reach Earth Takes about 4 years for starlight from next nearest star to reach Earth.That star is 4 light-years away! Alpha Centauri Measuring Distance outside our Solar System. Light-year: distance light travels in one year at the speed of light. If Speed of light = 186,000 mi./sec, then a Light-year = 5.9 trillion miles (5,900,000,000,000 miles)

Parallax: the apparent change in position of an object when you look at it from different places used to measure distance to nearby stars smaller shift = greater distance.

Doppler effect Red shift - longer wavelenghts : moving away from you. Blue shift- shorter wavelengths: moving toward you. Red -away ; blue toward you.

Doppler effect Red shift Blue shift

Telescopes collect and focus different types of electromagnetic radiation, including visible light. OOptical telescopes are used to see distant or faint objects by magnifying the amount of light they emit. Isaac Newton's telescope Hubble Telescope

Radio Telescopes collect radio waves from space to convert to images so we can see the source. easily detects waves through our atmosphere. Robert C. Byrd Green Bank Telescope (GBT)

Infrared Telescopes Can be on the ground or above atmosphere. Used to measure temperature of celestial objects, their composition and to locate planets around other stars. Exoplanets IInfrared telescopes on Mauna Lea in Hawaii Robert C. Byrd Green Bank Telescope (GBT)

Ultraviolet Telescopes Placed outside Earth s atmosphere. Detect hot, young stars in other galaxies Galex UV Telescope Robert C. Byrd Green Bank Telescope (GBT)

X-Ray Telescopes Are placed outside Earth s atmosphere. Observe supernova remnants, X-ray pulsars, black holes, neutron stars, and hot galactic clusters. Chandra X-ray Telescope Robert C. Byrd Green Bank Telescope (GBT)

Gamma Ray Telescopes Are placed outside Earth s atmosphere. Gamma rays often come from objects like black holes and exploding stars Fermi Gamma Ray Telescope Robert C. Byrd Green Bank Telescope (GBT)