A Sense of Scale. A Visual Comparison of Various Distances. Thanks to Tim Talbert for providing some of the data.

Size: px
Start display at page:

Download "A Sense of Scale. A Visual Comparison of Various Distances. Thanks to Tim Talbert for providing some of the data."

Transcription

1 A Sense of Scale A Visual Comparison of Various Distances Thanks to Tim Talbert for providing some of the data. Also see a similar page on Wikipedia x10-35 m 1.616x10-35 m the Planck length (the smallest measurement of length that has meaning) 1x10-15 m 1x10-15 m one fermi 1 fm 1x10-15 m diameter of proton (in the nucleus) 2.2 fm 2.2x10-15 m classical diameter of neutron 3.8 fm 3.8x10-15 m diameter of the nucleus of a helium atom fm x10-15 m classical diameter of an electron 7.2 fm 7.2x10-15 m diameter of the nucleus of an aluminum atom 14 fm 1.4x10-14 m diameter of the nucleus of a gold atom (The classical electron diameter is bigger than the proton diameter because the proton's size was measured in the nucleus, where it is trapped in a very deep, narrow potential well. The electron is in a comparatively wide, shallow well, so it takes up much more space. Talking about the sizes of subatomic particles is fairly meaningless anyway; in one sense, electrons and protons are point particles, with no size. And in quantum mechanics, we can only talk about the probability of finding a particle at a particular point, and cannot specify (or define) the exact position and size of a particle. The "classical electron radius" tells us little about the actual physical size of the electron. In short, I'm oversimplifying things.) 14 fm 1.4x10-14 m diameter of the nucleus of a gold atom 1,000 fm 1x10-12 m one picometer 1 pm 1x10-12 m wavelength of gamma rays 1 pm 1x10-12 m wavelength of gamma rays 38 pm 3.8x10-11 m diameter of flourine ion 52.9 pm 5.29x10-11 m most likely distance from electron to nucleus in a hydrogen atom (bohr radius) pm 7.413x10-11 m distance between bonded hydrogen atoms 100 pm 1x10-10 m one angstrom 120 pm 1.2x10-10 m Van Der Waals radius of hydrogen atoms (max distance between atoms that are not bonded) 200 pm 2x10-10 m resolution (size of smallest visible object) of a transmission electron microscope

2 248.2 pm 2.482x10-10 m distance between bonded iron atoms 275 pm 2.75x10-10 m Van Der Waals radius of potassium atoms (max distance between atoms that are not bonded) 282 pm 3x10-10 m diameter of water molecule 340 pm 3.4x10-10 m distance between base pairs in a DNA molecule 380 pm 3.8x10-10 m diameter of xenon ion pm 5.309x10-10 m distance between bonded cesium atoms pm 5.309x10-10 m distance between bonded cesium atoms 1,000 pm 1x10-9 m one nanometer 1 nm 1x10-9 m diameter of glucose molecule 2 nm 2x10-9 m diameter of DNA helix 5 nm 5x10-9 m diameter of insulin molecule 6 nm 6x10-9 m diameter of a hemoglobin molecule 10 nm 1x10-8 m thickness of cell wall (gram negative bacteria) 75 nm 7.5x10-8 m size of typical virus 90 nm 9x10-8 m length of transistor gate in a Pentium 4 chip (minimum feature size) 125 nm 1.25x10-7 m thickness of gold leaf 130 nm 1.3x10-7 m length of transistor gate in a Pentium 3 chip (1.4 Ghz) 200 nm 2x10-7 m diameter of smallest bacteria 200 nm 2x10-7 m resolution (size of smallest visible object) of an optical microscope

3 260 nm 2.6x10-7 m length of the smallest transistor in a Pentium 3 chip 410 nm 4.1x10-7 m wavelength of violet light 680 nm 6.8x10-7 m wavelength of red light 1,000 nm 1x10-6 m one micrometer (micron) 1 µm 1x10-6 m size of typical bacterium 1 µm 1x10-6 m diameter of sperm cell 1.5 µm 1.5x10-6 m length of transistor gate in an Intel 286 chip 1.7 µm 1.7x10-6 m diameter of average human cell nucleus 2.4 µm 2.4x10-6 m thickness of red blood cell 3 µm 3x10-6 m length of transistor gate in an Intel 8086 chip 4 µm 4x10-6 m diameter of capillary 7 µm 7x10-6 m diameter of a single yeast organism 8.4 µm 8.4x10-6 m diameter of red blood cell 10 µm 1x10-5 m diameter of average cell in human body 10 µm 1x10-5 m size of a grain of talcum powder 16 µm 1.6x10-5 m length of the smallest transistor in the first 6502 chips 16 µm 1.6x10-5 m length of the smallest transistor in the first 6502 chips 20 µm 2x10-5 m length of the smallest transistor in an Intel 4004 (the first microprocessor) 20 µm 2.0x10-5 m diameter of a small grain of sand 25 µm 2.5x10-5 m length of sperm cell 25 µm 2.5x10-5 m diameter of a human hair µm 8.382x10-5 m typical thickness of a piece of paper 100 µm 1x10-4 m mimimum size of object the human eye can resolve unaided 100 µm 1x10-4 m diameter of human fertilized egg cell 100 µm 1x10-4 m size of a grain of salt 110 µm 1.1x10-4 m thickness of a dollar bill 300 µm 3x10-4 m diameter of a period on a typewriter

4 375 µm 3.7x10-4 m diameter of the most common type of optical fiber 750 µm 7.5x10-4 m size of largest known bacterium 1,000 µm 1x10-3 m one millimeter 1.7 mm 1.7x10-3 m diameter of the head of the average pin 2 mm 2x10-3 m diameter of a large grain of sand 2 mm 2x10-3 m diameter of a large grain of sand 2 mm 2x10-3 m size of a small ant mm 4.234x10-3 m height of a line of text in 12-point type 10 mm 1x10-2 m one centimeter 1.7 cm 1.7x10-2 m wavelength of 20khz note (highest that can be heard) at 27 degrees celsius 2.5 cm 2.5x10-2 m size of a large ant 2.54 cm 2.540x10-2 m one inch 8.5 cm 8.5x10-2 m length of largest human chromosome if it were stretched end-to-end 12.2 cm 1.22x10-1 m wavelength of microwaves in a microwave oven 30 cm 3.0x10-1 m one foot 79 cm 7.9x10-1 m wavelength of 440 hertz note (A above middle C) at 27 degrees celsius 91 cm 9.1x10-1 m one yard 1 m 1 m one meter

5 1 m 1 m one meter 3 m 3 m average wavelength of FM radio waves 17 m 1.7x10 1 m wavelength of 20 hertz note (lowest that can be heard) at 27 degrees celsius m x10 2 m distance light travels in one microsecond, in a vacuum 343 m 3.43x10 2 m distance sound travels in one second (at 20 degress celsius) 415 m 4.1x10 2 m distance a bullet travels per second, when fired from a m 4.1x10 2 m distance a bullet travels per second, when fired from a.22 1,000 m 1x10 3 m one kilometer km x10 3 m one mile 4.3 km 4.3x10 3 m thickness of Greenland ice cap, at thickest point 4.47 km 4.47x10 3 m greatest measured thickness of antarctic ice cap 8.85 km 8.85x10 3 m height of Mount Everest km x10 4 m depth of Marianas Trench 11 km 1.1x10 4 m average height of top of troposphere (layer of atmosphere affected by weather) km 2.978x10 4 m distance the earth travels per second in its orbit 48 km 4.8x10 4 m average height of top of stratosphere (layer of atmosphere containing ozone; free of weather, good for flying) 50 km 5x10 4 m depth of earth's crust 60 km 6x10 4 m thickness of ozone layer 80 km 8x10 4 m height of ionosphere (ionized region which reflects radio waves) 80 km 8x10 4 m average height of top of mesosphere (strong currents, unstable, bad for flying) 160 km 1x10 5 m 100 miles km x10 5 m distance light travels in one millisecond, in a vacuum

6 km x10 5 m distance light travels in one millisecond, in a vacuum 300 km 3x10 5 m height of space shuttle's typical orbit 354 km 3.54x10 5 m average altitude of International Space Station 640 km 6.4x10 5 m height of lowest point of inner Van Allen belt 792 km 7.92x10 5 m altitude of Iridium satellites (LEO) 825 km 8.25x10 5 m altitude of Orbcomm satellites (LEO) 914 km 9.14x10 5 m diameter of the asteroid Ceres 1,000 km 1x10 6 m thickness of earth's atmosphere 1,375 km 1.375x10 6 m height of Teledesic (low-earth orbit) satellites 1,414 km 1.414x10 6 m altitude of Globalstar satellites (LEO) 2,274 km 2.274x10 6 m diameter of Pluto at its equator 2,890 km 2.89x10 6 m depth of earth's outer (liquid) core 3,474.8 km x10 6 m diameter of moon 3,962 km 3.962x10 6 m distance from New York to Los Angeles 4,879.4 km x10 6 m diameter of Mercury at its equator 5,150 km 5.150x10 6 m diameter of Titan

7 5,150 km 5.150x10 6 m diameter of Titan 5,150 km 5.15x10 6 m depth of earth's inner (solid) core 5,200 km 5.2x10 6 m height of highest point of outer Van Allen belt 5,262 km 5.262x10 6 m diameter of Ganymede 5,613 km 5.613x10 6 m distance from New York to London 6, km x10 6 m distance to center of Earth 6,794.4 km x10 6 m diameter of Mars at its equator 9,084 km 9.084x10 6 m distance from London to Los Angeles 9,380 km 9.38x10 6 m mean distance from Phobos to Mars 10,390 km 1.039x10 7 m altitude of ICO satellites (MEO) 12,103 km x10 7 m diameter of Venus at its equator 12,756.2 km x10 7 m diameter of Earth at its equator 20,200 km 2.02x10 7 m altitude of GPS satellites 23,460 km 2.346x10 7 m mean distance from Deimos to Mars 35,800 km 3.58x10 7 m height of satellite in geostationary orbit 47,810 km 4.781x10 7 m min initial altitude of Geotail satellite (VHO)

8 47,810 km 4.781x10 7 m min initial altitude of Geotail satellite (VHO) 49,492 km x10 7 m diameter of Neptune at its equator 51,118 km x10 7 m diameter of Uranus at its equator 120,536 km x10 8 m diameter of Saturn at its equator 142,984 km x10 8 m diameter of Jupiter at its equator 299,792.5 km x10 8 m distance light travels in one second, in a vacuum 384,400 km 3.844x10 8 m mean distance from earth to moon 868,912 km x10 8 m max initial altitude of Geotail satellite (VHO) 1,070,000 km 1.07x10 9 m mean distance from Jupiter to Ganymede 1,221,850 km x10 9 m mean distance from Saturn to Titan 1,390,000 km 1.39x10 9 m diameter of sun at its equator 1,500,000 km 1.5x10 9 m distance to SOHO satellite (L1 Lagrange point) 1,500,000 km 1.5x10 9 m distance to SOHO satellite (L1 Lagrange point) 17,987,550 km x10 10 m distance light travels in one minute, in a vacuum 57,910,000 km 5.791x10 10 m mean distance of Mercury from the sun

9 108,200,000 km 1.082x10 11 m mean distance of Venus from the sun 1 AU x10 11 m mean distance of Earth from the sun (one astronomical unit) AU x10 11 m mean distance of Mars from the sun AU 4.139x10 11 m mean distance of the asteroid Ceres from the sun AU x10 11 m mean distance of Jupiter from the sun AU x10 12 m distance light travels in one hour, in a vacuum AU x10 12 m distance light travels in one hour, in a vacuum AU x10 12 m mean distance of Saturn from the sun AU x10 12 m mean distance of Uranus from the sun AU x10 12 m mean distance of Neptune from the sun 34 AU 5.2x10 12 m maximum distance of Halley's Comet from the sun AU x10 12 m mean distance of Pluto from the sun 43.8 AU 6.56x10 12 m distance of QB1 object from Sun AU 9.323x10 12 m current distance of Voyager 2 from sun (as of 10/27/00) AU x10 13 m current distance of Voyager 1 from sun (as of 10/27/00) 80 AU 1x10 13 m termination shock--point at which solar wind becomes subsonic 134 AU 2.0x10 13 m heliopause (outer edge of Sun's magnetic field) 134 AU 2.01x10 13 m distance of 1996 TL66 object from Sun AU x10 13 m distance light travels in one day, in a vacuum 372 AU 5.56x10 13 m maximum distance of comet Hale-Bopp from the sun 1, AU x10 14 m distance light travels in one week, in a vacuum

10 1, AU x10 14 m distance light travels in one week, in a vacuum 25,000 AU 3.7x10 15 m possible distance of Sol B from Sun 63, AU x10 15 m distance light travels in one year (one light-year) 1.5 ly 1.4x10 16 m possible edge of Oort cloud 3.26 ly 3.08x10 16 m one parsec 4.22 ly 3.99x10 16 m distance to the star Proxima Centauri (nearest star other than sun) 4.3 ly 4.1x10 16 m distance to the stars Alpha Centauri A and B 8.6 ly 8.1x10 16 m distance to the star Sirius 8.6 ly 8.1x10 16 m distance to the star Sirius 25.2 ly 2.39x10 17 m distance to the star Vega 33 ly 3.2x10 17 m distance to the star Pollux 36 ly 3.5x10 17 m distance to the star Arcturus 51 ly 4.9x10 17 m distance to the star Castor 77 ly 7.3x10 17 m distance to the star Regulus 300 ly 2x10 18 m thickness of Milky Way Galaxy 430 ly 4.0x10 18 m distance to the star Polaris 1.6 kly 1.5x10 19 m distance to Horsehead Nebula

11 1.6 kly 1.5x10 19 m distance to Horsehead Nebula 20 kly 1x10 20 m diameter of Large Magellanic Cloud galaxy 27 kly 2.6x10 20 m distance to center of Milky Way Galaxy 44 kly 4.2x10 20 m diameter of M33 galaxy 162 kly 1.54x10 21 m diameter of Milky Way Galaxy 200 kly 1x10 21 m distance to Large Magellanic Cloud galaxy 200 kly 1x10 21 m diameter of M31 galaxy 300 kly 2x10 21 m distance to Small Magellanic Cloud galaxy 300 kly 2x10 21 m distance to Small Magellanic Cloud galaxy 2,200 kly 2.0x10 22 m distance to Andromeda galaxy 3,000 kly 2x10 22 m distance to Pisces galaxy 4,000 kly 3x10 22 m distance to IC 10 galaxy 5,000 kly 4x10 22 m distance to Pegasus galaxy 11,000 kly 1.0x10 23 m distance to the M81 galaxy cluster 15,000 kly 1.4x10 23 m distance to the M83 galaxy 27,000 kly 2.5x10 23 m distance to the M101 galaxy 35,000 kly 3.3x10 23 m distance to the M66 galaxy cluster 37,000 kly 3.5x10 23 m distance to the M51 galaxy cluster 38,000 kly 3.5x10 23 m distance to the M95 galaxy 41,000 kly 3.8x10 23 m distance to the M96 galaxy 60,000 kly 5x10 23 m distance to the Virgo galaxy cluster

12 60,000 kly 5x10 23 m distance to the Virgo galaxy cluster 340,000 kly 3.2x10 24 m distance to the Coma galaxy cluster 2,000,000 kly 1x10 25 m distance to brightest quasar (3C 273) 4,000,000 kly 3x10 25 m distance to quasar 3C 48 26,000,000 kly 2.4x10 26 m distance to farthest known object (quasar SDSS_1044_0125) www@falstad.com

Scale the Universe. Exploring your Universe from Inner to Outer Space. Linda L. Smith NASA Astrophysics Educator Ambassador

Scale the Universe. Exploring your Universe from Inner to Outer Space. Linda L. Smith NASA Astrophysics Educator Ambassador Scale the Universe Exploring your Universe from Inner to Outer Space Linda L. Smith NASA Astrophysics Educator Ambassador lsmith@paulsboro.k12.nj.us 1 The Booklet This book is organized into 3-stand-alone

More information

The Earth in the Universe Geology

The Earth in the Universe Geology The Earth in the Univers e The Earth in the Universe Geology The origin of the Universe The position of the Earth in the Universe Distances in the Universe Galaxies The Milky Way Stars: The Sun The Solar

More information

Explain why miles cannot be used to measure distances in space.

Explain why miles cannot be used to measure distances in space. Space SC.8.E.5.1 SC.8.E.5.1: Recognize that there are enormous distances between objects in space and apply our knowledge of light and space travel to understand this difference. Essential Questions: Distances

More information

Motion of the planets

Motion of the planets Our Solar system Motion of the planets Our solar system is made up of the sun and the 9 planets that revolve around the sun Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune & Pluto (maybe?)

More information

ASTRONOMY SNAP GAME. with interesting facts

ASTRONOMY SNAP GAME. with interesting facts ASTRONOMY SNAP GAME with interesting facts Sun Sun The Sun is the largest object in the solar system The Sun's life expectancy is approximately 5 billion more years At its core, the Sun s temperature is

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets SPI 0607.6.2 Explain how the relative distance of objects from the earth affects how they appear. Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial

More information

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

The Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour Name Test Date Hour Astronomy#3 - Notebook The Solar System LEARNING TARGETS I can describe the objects that make up our solar system. I can identify the inner and outer planets. I can explain the difference

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial planets are made mostly of rock and have similar characteristics to Earth. There are four terrestrial

More information

What is the Solar System?

What is the Solar System? What is the Solar System? Our Solar System is one of many planetary systems. It consists of: The Sun Eight planets with their natural satellites Five dwarf planets Billions of asteroids, comets and meteors

More information

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

Edmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2 Edmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2 Instructor: L. M. Khandro 1. Relatively speaking, objects with high temperatures emit their peak radiation in short wavelengths

More information

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

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects. The Solar System Sun Center of the solar system About 150,000,000 km from the Earth An averaged sized, yellow star Spherical in shape due to gravity Made of about ¾ hydrogen and ¼ helium, both of which

More information

The Solar System. Name Test Date Hour

The Solar System. Name Test Date Hour Name Test Date Hour Astronomy#3 - Notebook The Solar System LEARNING TARGETS I can describe the objects that make up our solar system. I can identify the inner and outer planets. I can explain the difference

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 23.1 The Solar System The Planets: An Overview The terrestrial planets are planets that are small and rocky Mercury, Venus, Earth, and Mars. The Jovian planets

More information

Contents of the Solar System

Contents of the Solar System The Solar System Contents of the Solar System Sun Planets 9 known (now: 8) Mercury, Venus, Earth, Mars ( Terrestrials ) Jupiter, Saturn, Uranus, Neptune ( Jovians ) Pluto (a Kuiper Belt object?) Natural

More information

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

UNIT 3: Chapter 8: The Solar System (pages ) CORNELL NOTES Directions: You must create a minimum of 5 questions in this column per page (average). Use these to study your notes and prepare for tests and quizzes. Notes will be turned in to your teacher

More information

Introduction to the Universe. What makes up the Universe?

Introduction to the Universe. What makes up the Universe? Introduction to the Universe What makes up the Universe? Objects in the Universe Astrophysics is the science that tries to make sense of the universe by - describing the Universe (Astronomy) - understanding

More information

Cosmology Vocabulary

Cosmology Vocabulary Cosmology Vocabulary Vocabulary Words Terrestrial Planets The Sun Gravity Galaxy Lightyear Axis Comets Kuiper Belt Oort Cloud Meteors AU Nebula Solar System Cosmology Universe Coalescence Jovian Planets

More information

4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises

4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises 4. THE SOLAR SYSTEM 1.1. THE SUN The sun is the star located in the center of the solar system. The sun is a yellow star, since its superficial temperature is about 5.500 C (although, the temperature can

More information

Solar System Scales. PTYS/ASTR 206 The Golden Age of Planetary Exploration Shane Byrne

Solar System Scales. PTYS/ASTR 206 The Golden Age of Planetary Exploration Shane Byrne Solar System Scales PTYS/ASTR 206 The Golden Age of Planetary Exploration Shane Byrne shane@lpl.arizona.edu PYTS/ASTR 206 Solar System Scales 2 In this lecture Measuring length, mass and time Angular sizes

More information

Unit 1: The Earth in the Universe

Unit 1: The Earth in the Universe Unit 1: The Earth in the Universe 1. The Universe 1.1. First ideas about the Universe 1.2. Components and origin 1.3. Sizes and distances 2. The Solar System 3. The planet Earth 3.1. Movements of the Earth

More information

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017 Lecture 6: The Physics of Light, Part 1 Astronomy 111 Wednesday September 13, 2017 Reminders Star party tonight! Homework #3 due Monday Exam #1 Monday, September 25 The nature of light Look, but don t

More information

Our Planetary System. Chapter 7

Our Planetary System. Chapter 7 Our Planetary System Chapter 7 Key Concepts for Chapter 7 and 8 Inventory of the Solar System Origin of the Solar System What does the Solar System consist of? The Sun: It has 99.85% of the mass of the

More information

Station #1 Galaxy Cards. Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes.

Station #1 Galaxy Cards. Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes. Station #1 Galaxy Cards Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes. Materials: Galaxy cards, your textbook Using your text book answers the following

More information

Introduction to the Universe

Introduction to the Universe What makes up the Universe? Introduction to the Universe Book page 642-644 Objects in the Universe Astrophysics is the science that tries to make sense of the universe by - describing the Universe (Astronomy)

More information

North Carolina Science Olympiad Elementary Division 2010 Sky Quest. Sky Quest. NCSO Sample Event 2010 Elementary Tournament Grade 3 Goal 3

North Carolina Science Olympiad Elementary Division 2010 Sky Quest. Sky Quest. NCSO Sample Event 2010 Elementary Tournament Grade 3 Goal 3 NCSO Sample Event 2010 Elementary Tournament Grade 3 Goal 3 STATION 1 1. Which of the following is NOT one of the inner planets? a. Earth b. Neptune c. Venus d. Mercury 2. Which planet is famous for its

More information

28-Aug-17. A Tour of Our Solar System and Beyond. The Sun

28-Aug-17. A Tour of Our Solar System and Beyond. The Sun A Tour of Our Solar System and Beyond The Sun diameter = 1,390,000 km = 864,000 mi >99.8% of the mass of the entire solar system surface temperature 5800 C 600 x 10 6 tons H -> 596 x 10 6 tons He per second

More information

THE UNIVERSE AND THE EARTH

THE UNIVERSE AND THE EARTH ESO1 THE UNIVERSE AND THE EARTH Unit 1 What is the Universe like? Universe theories Ideas about the Universe: Geocentric theory Aristotle (B.C) and Ptolomy (A.D) Heliocentric theory Copernicus in 1542

More information

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

1UNIT. The Universe. What do you remember? Key language. Content objectives 1UNIT The Universe What do you remember? What are the points of light in this photo? What is the difference between a star and a planet? a moon and a comet? Content objectives In this unit, you will Learn

More information

PH104 Lab 1 Light and Matter Pre-lab

PH104 Lab 1 Light and Matter Pre-lab Name: Lab Time: PH04 Lab Light and Matter Pre-lab. Goals Since this is the first lab, we don t want to try to do things that are too complex. We would like to get used to the lab room and some of the steps

More information

TAKEN FROM HORIZONS 7TH EDITION CHAPTER 1 TUTORIAL QUIZ

TAKEN FROM HORIZONS 7TH EDITION CHAPTER 1 TUTORIAL QUIZ TAKEN FROM HORIZONS 7TH EDITION CHAPTER 1 TUTORIAL QUIZ 1. If the solar system is scaled down so that the Sun is represented by a basketball, a. a ping-pong ball located 500 feet away would properly represent

More information

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

Human Understanding of both Earth and Space has Changed Over Time. Unit E: Topic One Human Understanding of both Earth and Space has Changed Over Time Unit E: Topic One 1.4 Our Solar Neighbourhood Nebular Hypothesis The theory of how solar systems are formed Evolution of solar system

More information

9/5/16. Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM. Astronomy 1001 First Assignments: Chapter 1: A Modern View of the Universe

9/5/16. Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM. Astronomy 1001 First Assignments: Chapter 1: A Modern View of the Universe 9/5/16 Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM Syllabus: http://www.astro.umn.edu/courses/1001/syllabi/ Lecture notes: http://www.astro.umn.edu/courses/1001/ lecnotes/ Exams: http://www.astro.umn.edu/courses/1001/

More information

PHYSICS 160: Cosmos Spring 2015 Homework #1 MODEL SOLAR SYSTEM. To get an intuitive feeling for the size of the solar system.

PHYSICS 160: Cosmos Spring 2015 Homework #1 MODEL SOLAR SYSTEM. To get an intuitive feeling for the size of the solar system. Name Date PHYSICS 160: Cosmos Spring 2015 Homework #1 MODEL SOLAR SYSTEM Purpose: To get an intuitive feeling for the size of the solar system. Perhaps you ve heard the phrase to disappear into empty space.

More information

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

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) Page1 Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) HS-ESSI-1; HS-ESS1-2; HS-ESS1-3; HS-ESSI-4 NGSS Civic Memorial High School - Earth Science A Concept # What we will be learning Mandatory

More information

Chapter 1 Review Clickers. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.

Chapter 1 Review Clickers. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc. Review Clickers The Cosmic Perspective Seventh Edition A Modern View of the Universe Put these objects in the correct order, from nearest to farthest from Earth: a) The Moon, Mars, the Sun, the nearest

More information

Astronomy (Geology 360, Physics 360) take-home test. There is no class on Monday March 16th

Astronomy (Geology 360, Physics 360) take-home test. There is no class on Monday March 16th Astronomy (Geology 360, Physics 360) take-home test. Reminder: Test must be answered on a ScanTron sheet. Be sure to use a No. 2 pencil. Be sure to "bubble in" your name and Student ID on the ScanTron

More information

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

Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006 Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006 Instructor: L. M. Khandro 10/19/06 Please Note: the following test derives from a course and text that covers the entire topic of

More information

The Solar System 6/23

The Solar System 6/23 6/23 The Solar System I. Earth A. Earth is the prototype terrestrial planet 1. Only planet in the solar system (we know of so far) with life 2. Temperature 290 K B. Physical Characteristics 1. Mass: 6

More information

The Universe in my pocket. The Solar System. Gloria Delgado Inglada. 4 No. 4. Instituto de Astronomía, UNAM, Mexico

The Universe in my pocket. The Solar System. Gloria Delgado Inglada. 4 No. 4. Instituto de Astronomía, UNAM, Mexico The Universe in my pocket The Solar System 4 No. 4 Gloria Delgado Inglada Instituto de Astronomía, UNAM, Mexico 2 The Solar System is composed of the Sun and of all the bodies travelling around it: planets,

More information

Solar System Test Review

Solar System Test Review Solar System Test Review There are several planets in the solar system. What do all of these planets have in common? A.They all orbit the Sun. B. They are all close to the Moon. C.They are all called Earth.

More information

Chapter 1 Our Place in the Universe. Copyright 2012 Pearson Education, Inc.

Chapter 1 Our Place in the Universe. Copyright 2012 Pearson Education, Inc. Chapter 1 Our Place in the Universe 1 1.1 Our Modern View of the Universe Our goals for learning: What is our place in the universe? How did we come to be? How can we know what the universe was like in

More information

The Size of the Solar System

The Size of the Solar System The Size of the Solar System Overview Questions: My answers: Become familiar with the scale of the planets vs. their distances. Get an overview of the solar system. Introduction It is easy to flip to the

More information

Astronomy Test Review. 3 rd Grade

Astronomy Test Review. 3 rd Grade Astronomy Test Review 3 rd Grade Match the vocabulary word to its definition. Outer Planets The path a planet takes around the sun. Inner Planets Orbit Sun The center of our solar system. Small, rocky

More information

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

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999 Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999 Reminder: When I write these questions, I believe that there is one one correct answer. The questions consist of all parts a e. Read the entire

More information

Observational Astronomy Astro-25. Professor Meyer-Canales Saddleback College

Observational Astronomy Astro-25. Professor Meyer-Canales Saddleback College Observational Astronomy Astro-25 Professor Meyer-Canales Saddleback College Astronomy Courses Offered at Saddleback College Astronomy 20 - General Astronomy Survey/Lecture course Astronomy 21 - Solar System

More information

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

1. The Sun is a huge ball of very hot gas in space, which radiates heat and light in one direction. PLEASE ANSWER YOUR QUESTIONS ON THIS PROVIDED QUESTION PAPER. EACH QUESTION IS FOLLOWED BY ANSWERS MARKED A AND B, OR A, B, C AND D. ONLY ONE ANSWER IS CORRECT. CHOOSE THE MOST CORRECT ANSWER AND CIRCLE

More information

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

Earth Science 11 Learning Guide Unit Complete the following table with information about the sun: Earth Science 11 Learning Guide Unit 2 Name: 2-1 The sun 1. Complete the following table with information about the sun: a. Mass compare to the Earth: b. Temperature of the gases: c. The light and heat

More information

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

CHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration CHAPTER 11 We continue to Learn a lot about the Solar System by using Space Exploration Section 11.1 The Sun page 390 -Average sized star -Millions of km away -300,000 more massive then Earth, 99% of all

More information

Sun Mercury Venus. Earth Mars Jupiter

Sun Mercury Venus. Earth Mars Jupiter Sun Mercury Venus Earth Mars Jupiter Venus is the hottest planet in our solar system. The thick clouds on Venus hold the heat in. The sun s lights reflect off Venus s clouds making it look like the brightest

More information

The Outer Planets (pages )

The Outer Planets (pages ) The Outer Planets (pages 720 727) Gas Giants and Pluto (page 721) Key Concept: The first four outer planets Jupiter, Saturn, Uranus, and Neptune are much larger and more massive than Earth, and they do

More information

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Chapter 1 Lecture The Cosmic Perspective Seventh Edition A Modern View of the Universe 1.1 The Scale of the Universe Our goals for learning: What is our place in the universe? How big is the universe?

More information

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

23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System 23.1 The Solar System Orbits of the Planets The Planets: An Overview The terrestrial planets are planets that are small and rocky Mercury, Venus, Earth, and Mars. The Jovian planets are the huge gas giants

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 23 Touring Our Solar System 23.1 The Solar System The Planets: An Overview The terrestrial planets are planets that are small and rocky Mercury, Venus,

More information

Science Practice Astronomy (AstronomyJSuber)

Science Practice Astronomy (AstronomyJSuber) Name: Date: 1. The pull of gravity on Earth is a direct result of the A. mass of Earth. B. magnetic field of Earth. C. rotation of Earth on its axis. D. weight of Earth's atmosphere. This online assessment

More information

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.

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. Mercury Mercury is the closest planet to the sun. It is extremely hot on the side of the planet facing the sun and very cold on the other. There is no water on the surface. There is practically no atmosphere.

More information

Sky Quest This event has 12 stations. Print in color, use as many sets as you need for the number of teams you have.

Sky Quest This event has 12 stations. Print in color, use as many sets as you need for the number of teams you have. Sky Quest 2012 This event has 12 stations. Print in color, use as many sets as you need for the number of teams you have. Student response sheet and answer key are at the end. Station 1- Planet Questions

More information

Chapter 17 Solar System

Chapter 17 Solar System Chapter 17 Solar System Rotation Earth spinning on its axis (like a top) "TOP" imaginary rod running through the center of the Earth from North pole to South pole The Earth is tilted on its axis at an

More information

Star. Chapter 1: Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning:

Star. Chapter 1: Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning: Chapter 1: Our Place in the Universe 1.1 A Modern View of the Universe Our goals for learning: What is our physical place in the Universe? How did we come to be? How can we know what the Universe was like

More information

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes

More information

The Universe and Galaxies

The Universe and Galaxies The Universe and Galaxies 16.1 http://dingo.care-mail.com/cards/flash/5409/galaxy.swf Universe The sum of all matter and energy that exists, that has ever existed, and that will ever exist. We will focus

More information

At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion?

At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion? At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion? These small, rocky worlds orbit the sun generally between the orbits of

More information

Lesson 1 The Structure of the Solar System

Lesson 1 The Structure of the Solar System Lesson 1 Student Labs and Activities Page Launch Lab 8 Content Vocabulary 9 Lesson Outline 10 MiniLab 12 Content Practice A 13 Content Practice B 14 School to Home 15 Key Concept Builders 16 Enrichment

More information

STARS AND THE SOLAR SYSTEM

STARS AND THE SOLAR SYSTEM 17 STARS AND THE SOLAR SYSTEM TEXTBOOK QUESTIONS AND THEIR ANSWERS 1. Which of the following is NOT a member of the solar system? (a) An asteroid (c) A constellation (b) A satellite (d) A comet Ans. (c)

More information

Lunar Eclipse. Solar Eclipse

Lunar Eclipse. Solar Eclipse Lunar Eclipse SUN Moon Solar Eclipse SUN SUN Moon Total solar eclipse Partial solar eclipse Moon Phases What does the moon look like from at each position? G H F A E B D C SUNLIGHT Refracting Telescopes

More information

UNIT 1: EARTH AND THE SOLAR SYSTEM.

UNIT 1: EARTH AND THE SOLAR SYSTEM. UNIT 1: EARTH AND THE SOLAR SYSTEM. 1) A BRIEF HISTORY Theories of the Universe In the second century BC, the astronomer Ptolemy proposed that the Earth was the centre of the Universe, and that the Sun,

More information

Space Science Jeopardy!

Space Science Jeopardy! Space Science Jeopardy! Structure of the Universe Stars & HR Diagram Seasons, Tides, Phases, Eclipses Astronomical Bodies The Sun & Gravity 10 10 10 10 10 20 20 20 20 20 30 30 30 30 30 40 40 40 40 40 50

More information

ASTR 380 Possibilities for Life in the Outer Solar System

ASTR 380 Possibilities for Life in the Outer Solar System ASTR 380 Possibilities for Life in the Outer Solar System Possibility of Life in the Inner Solar System The Moon, Mercury, and the Moons of Mars Deimos NO LIFE NOW or EVER This is a 98% conclusion! Phobos

More information

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

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System The Solar System Chapter 29 The Solar System Section 29.1 Models of the Solar System 29.1 notes Models of the Solar System Geocentric: : Earth-centered model of the solar system. (Everything revolves around

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Chapter 4 - Group Homework Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Density is defined as A) mass times weight. B) mass per unit volume.

More information

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

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company 11 Video Script: 1. For thousands of years people have looked up at the night sky pondering the limits of our solar system. 2. Perhaps you too, have looked up at the evening stars and planets, and wondered

More information

Homework 3, Tuesday Jan 31 DUE Tuesday Feb 14 (beginning of class! -- You have TWO weeks) ET Life, ASTRO/GEOL 3300, Tues/Thurs 2:00

Homework 3, Tuesday Jan 31 DUE Tuesday Feb 14 (beginning of class! -- You have TWO weeks) ET Life, ASTRO/GEOL 3300, Tues/Thurs 2:00 Homework 3, Tuesday Jan 31 DUE Tuesday Feb 14 (beginning of class! -- You have TWO weeks) ET Life, ASTRO/GEOL 3300, Tues/Thurs 2:00 The idea behind this homework assignment is that a walk through a model

More information

Inner Planets (Part II)

Inner Planets (Part II) Inner Planets (Part II) Sept. 18, 2002 1) Atmospheres 2) Greenhouse Effect 3) Mercury 4) Venus 5) Mars 6) Moon Announcements Due to technical difficulties, Monday s quiz doesn t count An extra credit problem

More information

Ag Earth Science Chapter 23

Ag Earth Science Chapter 23 Ag Earth Science Chapter 23 Chapter 23.1 Vocabulary Any of the Earth- like planets, including Mercury, Venus, and Earth terrestrial planet Jovian planet The Jupiter- like planets: Jupiter, Saturn, Uranus,

More information

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

2. The distance between the Sun and the next closest star, Proxima Centuari, is MOST accurately measured in Name: Date: 1. Some scientists study the revolution of the Moon very closely and have recently suggested that the Moon is gradually moving away from Earth. Which statement below would be a prediction of

More information

The Solar Nebula Theory. This lecture will help you understand: Conceptual Integrated Science. Chapter 28 THE SOLAR SYSTEM

The Solar Nebula Theory. This lecture will help you understand: Conceptual Integrated Science. Chapter 28 THE SOLAR SYSTEM This lecture will help you understand: Hewitt/Lyons/Suchocki/Yeh Conceptual Integrated Science Chapter 28 THE SOLAR SYSTEM Overview of the Solar System The Nebular Theory The Sun Asteroids, Comets, and

More information

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc. Chapter 1 Lecture The Cosmic Perspective Seventh Edition A Modern View of the Universe Chapter Opener 1.1 The Scale of the Universe Our goals for learning: What is our place in the universe? How big is

More information

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

Starting from closest to the Sun, name the orbiting planets in order. Chapter 9 Section 1: Our Solar System Solar System: The solar system includes the sun, planets and many smaller structures. A planet and its moon(s) make up smaller systems in the solar system. Scientist

More information

Mini 4-H. Developed by Area VII Extension Youth Educators Draft Purdue University Cooperative Extension Service

Mini 4-H. Developed by Area VII Extension Youth Educators Draft Purdue University Cooperative Extension Service & Mini 4-H Developed by Area VII Extension Youth Educators Draft Purdue University Cooperative Extension Service Mini 4-Her's Page a special to Mini 4-H! are now a of the 4-H family. You Mini have lots

More information

Unit 3 Lesson 6 Small Bodies in the Solar System. Copyright Houghton Mifflin Harcourt Publishing Company

Unit 3 Lesson 6 Small Bodies in the Solar System. Copyright Houghton Mifflin Harcourt Publishing Company Florida Benchmarks SC.8.N.1.1 Define a problem from the eighth grade curriculum using appropriate reference materials to support scientific understanding, plan and carry out scientific investigations of

More information

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary Vocabulary STUDENT RESOURCE 1.1 INFORMATION SHEET asteroids thousands of rocky objects that orbit the Sun Most asteroids orbit in a belt between the orbits of Mars and Jupiter. More than 9, asteroids have

More information

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.

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. 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 0.387 astronomical units Diameter: 4,879.4 km (3,031.92 miles)

More information

Observing Habitable Environments Light & Radiation

Observing Habitable Environments Light & Radiation Homework 1 Due Thurs 1/14 Observing Habitable Environments Light & Radiation Given what we know about the origin of life on Earth, how would you recognize life on another world? Would this require a physical

More information

Your task for each planet...

Your task for each planet... Solar System Your task for each planet... Slide 1: What type of planet is it? (either rocky terrestrial world, gas giant or ice giant) What is it made of? Does it have any moons? What is its mass relative

More information

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

Space Notes 2. Covers Objectives 3, 4, and 8 Space Notes 2 Covers Objectives 3, 4, and 8 Sun Average Size Star Sun 101 Sun s Mass almost 100 times the mass of all the planets combined. Most of the mass is hydrogen gas Thermonuclear Reaction Thermonuclear

More information

BOOK 3 OUR PLANET SECTION 1 OUR PLANET IN THE UNIVERSE

BOOK 3 OUR PLANET SECTION 1 OUR PLANET IN THE UNIVERSE BOOK 3 OUR PLANET SECTION 1 OUR PLANET IN THE UNIVERSE THE ELECTROMAGNETIC SPECTRUM (EMS) The Electromagnetic spectrum (EMS) is a range of wavelengths and frequencies which extend from gamma rays to radio

More information

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

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 What Objects Are Part of the Solar System? Florida Benchmarks SC.5.E.5.2 Recognize the major common characteristics of all planets and compare/contrast the properties of inner and outer

More information

EARTH AND UNIVERSE. Earth

EARTH AND UNIVERSE. Earth EARTH AND UNIVERSE Earth Earth is the third planet from the Sun and the only object in the Universe known to harbor life. According to radiometric dating and other sources of evidence, Earth formed over

More information

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

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth) The Sun - It is located at the centre of our solar system with all planets and objects (comets and asteroids) revolving around it Page 1 of 6 - It s gravitational pull keeps the planets and other objects

More information

Bell Ringer. want to do someday? 1. Briefly describe the Doppler effect in one sentence. 2. What do you want to do someday, like, in life?

Bell Ringer. want to do someday? 1. Briefly describe the Doppler effect in one sentence. 2. What do you want to do someday, like, in life? Bell Ringer 1. Briefly describe the Doppler effect in one sentence. 2. What do you want to do someday, like, in life? 3. How do you think science might apply to what you want to do someday? SCIENCE MATTERS

More information

ASTRONOMY 1 FINAL EXAM 1 Name

ASTRONOMY 1 FINAL EXAM 1 Name ASTRONOMY 1 FINAL EXAM 1 Name Multiple Choice (2 pts each) 1. Sullivan Star is an F spectral class star that is part of a binary star system. It has a MS lifetime of 5 billion years. Its life will eventually

More information

Light and Telescopes

Light and Telescopes Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we

More information

Cosmic Landscape Introduction Study Notes

Cosmic Landscape Introduction Study Notes Cosmic Landscape Introduction Study Notes About how much bigger in radius is the Sun than the Earth? The ratio of the Sun's radius to the Earth's radius is 1,392,000/12756 = 109.1 How big is an astronomical

More information

Name Date Class. Earth in Space

Name Date Class. Earth in Space Chapter Review Earth in Space Part A. Vocabulary Review Directions: Select the term from the following list that matches each description. axis orbit rotation revolution equinox solstice lunar eclipse

More information

Planets. Chapter 5 5-1

Planets. Chapter 5 5-1 Planets Chapter 5 5-1 The Solar System Terrestrial Planets: Earth-Like Jovian Planets: Gaseous Sun Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto Inferior Planets Superior Planets Inferior

More information

1. The Sun is the largest and brightest object in the universe. 2. The period that the Earth takes to revolve once around the Sun is approximately a

1. The Sun is the largest and brightest object in the universe. 2. The period that the Earth takes to revolve once around the Sun is approximately a PLEASE ANSWER YOUR QUESTIONS ON THIS PROVIDED QUESTION PAPER. EACH QUESTION IS FOLLOWED BY ANSWERS MARKED A AND B, OR A, B, C AND D. ONLY ONE ANSWER IS CORRECT. CHOOSE THE MOST CORRECT ANSWER AND CIRCLE

More information

THE SIZE AND SCALE OF THE UNIVERSE

THE SIZE AND SCALE OF THE UNIVERSE 1 THE SIZE AND SCALE OF THE UNIVERSE 1. Scientific notation review Write the following in proper scientific notation, giving the proper number of significant figures. 1.a Thirty-one million, seven hundred

More information

1 of 5 5/2/2015 5:50 PM

1 of 5 5/2/2015 5:50 PM 1 of 5 5/2/2015 5:50 PM 1. A comet that has a semi-major axis of 100 AU must have a period of about 10 years. 20 years. 100 years. 1000 years. 2. Astronomers believe chondrite meteorites are about 4.6

More information

Unit 2. Galaxies, Stars and the Solar System

Unit 2. Galaxies, Stars and the Solar System Strand K Astrophysics Unit 2 Galaxies, Stars and the Solar System Contents Page The Early Universe 2 The Life Cycle of Stars 4 Features of the Solar System 7 K21 The Early Universe Running the current

More information

CST Prep- 8 th Grade Astronomy

CST Prep- 8 th Grade Astronomy CST Prep- 8 th Grade Astronomy Chapter 15 (Part 1) 1. The theory of how the universe was created is called the 2. Which equation states that matter and energy are interchangeable? 3. All matter in the

More information

Comets, Asteroids, and Meteors. By: Annette Miles

Comets, Asteroids, and Meteors. By: Annette Miles Comets, Asteroids, and Meteors By: Annette Miles What is a comet? A comet is a small body which scientists sometimes call a planetesimal. They are made out of dust, ice rock, gas, and. They are kind of

More information