Unit 16: Astronomy and space science. Learning aim A Understand the fundamental aspects of the solar system

Similar documents
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

Coursework Booklet 1

OPTION E, ASTROPHYSICS TEST REVIEW

OPTION E, ASTROPHYSICS TEST REVIEW

Galaxies & Introduction to Cosmology

Earth Space Systems. Semester 1 Exam. Astronomy Vocabulary

Universe Now. 12. Revision and highlights

Revision: Sun, Stars (and Planets) See web slides of Dr Clements for Planets revision. Juliet Pickering Office: Huxley 706

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

IB Physics - Astronomy

V. Astronomy Section

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

Planets Inner vs. outer Composition inner planets are rocky/outer are gas Size inner are smaller/outer are much larger Distance from sun inner are

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

The Stars. Chapter 14

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. Review. Semester Recap. Nature of Light. Wavelength. Red/Blue Light 4/30/18

Formation of the Universe The organization of Space

Chapter 8: The Family of Stars

Stars and Galaxies. Content Outline for Teaching

Exam Board Edexcel There are 2 exams, each is worth 50% of the GCSE

Earth and Space Science Quarter 4. Sun-Earth-Moon System (Duration 2 Weeks)

Chapter 23. 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.

FCAT Review Space Science

CONTENT EXPECTATIONS

GCSE Astronomy Course Guide. Each Tuesday after school

Mapping Document. GCSE (9-1) Astronomy. Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0)

Astronomy Part 1 Regents Questions

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

2. The distance between the Sun and the next closest star, Proxima Centuari, is MOST accurately measured in

CHAPTER 29: STARS BELL RINGER:

Lesson 3 THE SOLAR SYSTEM

LESSON 1. Solar System

GALAXIES AND STARS. 2. Which star has a higher luminosity and a lower temperature than the Sun? A Rigel B Barnard s Star C Alpha Centauri D Aldebaran

Universe Review. 3. The light emitted from a star is studied by astronomers to determine which of the following properties?

Unit 1: The Earth in the Universe

Space Test Review. Unit Test on Thursday April 17

Topics and questions for astro presentations

What is the solar system?

Learning About Our Solar System

Proton-proton cycle 3 steps PHYS 162 1

Final Exam. Sample Questions. Final Exam. Which of the following statement is true? THE FINAL IS DECEMBER 15 th : 7-10pm!

E1. This question is about stars. (a) Distinguish between apparent magnitude and absolute magnitude. [2]

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

Test 4 Final Review. 5/2/2018 Lecture 25

Astronomy Study Guide Answer Key

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.

The point in an orbit around the Sun at which an object is at its greatest distance from the Sun (Opposite of perihelion).

Galaxies and Cosmology

Stars and Galaxies. The Sun and Other Stars

Based on the reduction of the intensity of the light from a star with distance. It drops off with the inverse square of the distance.

AyC10 Fall 2007: Midterm 2 Review Sheet. CS Why is Pluto no longer a planet, according to the International Astronomical Union s definition?

Astronomy Unit Notes Name:

Cosmology Vocabulary

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

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

ASTRONOMY QUIZ NUMBER 11

CHAPTER 9: STARS AND GALAXIES

Galaxies: enormous collections of gases, dust and stars held together by gravity Our galaxy is called the milky way

ESS Mrs. Burkey FIRST SEMESTER STUDY GUIDE H/K

Astronomy: Exploring the Universe

Types of Stars 1/31/14 O B A F G K M. 8-6 Luminosity. 8-7 Stellar Temperatures

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

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

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

Answer Key for Exam C

Answer Key for Exam B

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.

Explain how the sun converts matter into energy in its core. Describe the three layers of the sun s atmosphere.

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

Name ANSWER KEY Class Table Seat Date

Answers. The Universe. Year 10 Science Chapter 6

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

Effective August 2007 All indicators in Standard / 14

Answer Key for Exam D

Astronomy 1143 Final Exam Review Answers

AN INTRODUCTIONTO MODERN ASTROPHYSICS

British Olympiad in Astronomy and Astrophysics

Astronomy: Exploring the Universe

THE SUN AND THE SOLAR SYSTEM

edition JIM Koupelis and Karl F.

Chapter 9. Stars. The Hertzsprung-Russell Diagram. Topics for Today s Class. Phys1411 Introductory Astronomy Instructor: Dr.

Our sun is the star in our solar system, which lies within a galaxy (Milky Way) within the universe. A star is a large glowing ball of gas that

Sample Assessment Material Time: 2 hours

Which letter on the timeline best represents the time when scientists estimate that the Big Bang occurred? A) A B) B C) C D) D

Investigations in Earth and Space Science Semester Review: Unit 1 and Unit 2

Science Period. Astronomy Unit PracticeTest 2014 Sci 7

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth)

4 A(n) is a small, rocky object that orbits the sun; many of these objects are located in a band between the orbits of Mars and Jupiter.

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

Study Guide Chapter 2

Universe Celestial Object Galaxy Solar System

Introduction to Astronomy

Astronomy Final Exam Study Guide

Earth/Space/Physics Kristy Halteman.

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

Student Instruction Sheet: Unit 4 Lesson 3. Sun

TEK 8 Test Review. 15. Galaxies are best described as -

GraspIT Questions AQA GCSE Physics Space physics

Modern Astronomy Review #1

Transcription:

Unit 16: Astronomy and space science Learning aim A Understand the fundamental aspects of the solar system

Contents page Note: anywhere you see a capital D means you MUST draw a diagram.

Radiative zone Corona Core Convective zone Chromosphere Photosphere

You need a copy of this in your notes Page 6.

Hydrostatic equilibrium Hydrostatic equilibrium occurs when the force due to gas pressure exactly balances out the force due to gravity.

Sun s magnetic field

Sunspots

Life cycle of a star (D)

Hertz sprung-russel diagram Stars DO NOT progress along their stage! What do you notice about this axis?

Spectral classes The Sun has a surface temperature of about 5,300 K. Spectral Class Intrinsic Color Temperature (K) O Blue Over 25,000 B Blue 11,000 25,000 A Blue-white 7,500 11,000 F White 6000-7,500 G Yellow-white 5,000-6,000 K Orange 3,500-5,000 M Red Under 3,500 TYPE Ia Ib II III IV V VI Star Very luminous supergiants Less luminous supergiants Luminous giants Giants Subgiants Main sequence stars (dwarf stars) Subdwarf

Anatomy of the Earth Crust Outer core Mantle Inner core

Composition of Earth s Atmosphere What can you remember?

Earth s tilted axis The Earth s axis is tilted by 23.5.

Day and night

Solar and Sidereal days

Orbits

These orbits are NOT circular:

Kepler s Laws 1. All planets move in elliptical orbits with the Sun at the centre. 2. A line that connects a planet to the Sun sweeps out equal areas in equal times. 3. The square of the period of any planet is proportional to the cube of the semi-major axis of its orbit.

Eclipses

Moon phases

What is this? Have you even see this before?

You only ever see one side of the Moon, why?

The Moon is tidally locked. It s orbital rotation is the same as the time it takes to orbit Earth.

Centripetal force The planets are accelerating just fast enough to remain in their orbits.

Centrifugal force

Van Allen Radiation Belts

Formation of the Aurora Borealis

The Aurora Borealis or Northern lights as viewed from space.

The aurora seen on Earth

Forces involved in the Solar System The 3 mains ones: Gravitational forces Centrifugal forces Centripetal forces

The centripetal force arises from the gravitational pull on a planet from the Sun. (E.g. water in a bucket, if you swing a bucket full with water fast enough, the water will remain in the bucket and the string attached to the bucket will remain taut - this is because of the centripetal force.)

The centrifugal force arises from the planet orbiting the Sun at a great speed. (E.g. a mixture put into a centrifuge, the mixture separated out depending on the density of the substances initially mixed together.)

Inner and outer planets Can you remember the planets in order? You will need to find a diagram of each planet for your assignment.

Moons of the Solar System

Planetary ring systems

Features and characteristics of other Solar System objects Asteroids Meteors Comets Kuiper belt Oort cloud

Asteroid belt

Meteor

Comets

Kuiper Belt

Oort Cloud

Measuring astronomical distances There are a few methods you need to write about: Trigonometric Parallax Cepheid variables as standard candles Eclipsing binaries

Trigonometric parallax Limitations? Inaccurate for distances greater than 65 light years.

Units

Cepheid variables Brighter stars have longer periods

We can use an equation and the inverse square law to calculate the distance:

Cepheid variables can be used to measure distances of 20 million light years. http://hyperphysics.phyastr.gsu.edu/hbase/astro/cepheid.html

Eclipsing binaries

Evidence for an expanding Universe?

Redshift and blue shift

Hubble s Law Hubble s Law The further away a galaxy is from another point in space, the faster it appears to recede, and therefore, the Universe is expanding.

Determining the age of the Universe: Age of Universe = 1 H 0

Possible fate of the Universe based on density: https://futurism.com/four-ways-the-universe-could-end/

Cosmological theories of the present day Big Bang theory. Olbers paradox. Steady state.

Big Bang Theory

Olbers Paradox Is the night sky infinitely bright?

Reasons why the night sky is not infinitely bright: 1. There is too much dust to see the distant stars. 2. The Universe only has a finite (opposite of infinite) number of stars. 3. The position of stars in not even stars could hind behind one another. 4. The Universe is expanding. 5. The Universe is young meaning distant light has not reached us yet.

Steady state theory https://universea ndphysics.wordp ress.com/2017/0 5/08/steadystate-theoryrejected/

Note Anything with a name must have a capital letter: Sun Moon (if you are talking about ours) Earth Solar System