Size and Scale of the Universe What is your Cosmic Address? # Street City State Country Continent Hemisphere Planet …

Slides:



Advertisements
Similar presentations
Size and Scale of the Universe
Advertisements

The Size, Scale and Structure of the Universe
Size and Scale of the Universe Image courtesy of The Cosmic Perspective by Bennett, Donahue, Schneider, & Voit; Addison Wesley, 2002.
July 21, 2004 Tea Break It took Voyager 20 years to get to Pluto. At the same speed, how long does it take to get to the nearest star? How long will it.
Galaxies What is a galaxy? How many stars are there in an average galaxy? About how many galaxies are there in the universe? What is the name of our galaxy?
Galaxies What is a galaxy? How many stars are there in an average galaxy? About how many galaxies are there in the universe? What is the name of our galaxy?
© 2010 Pearson Education, Inc. Chapter 20 Galaxies and the Foundation of Modern Cosmology.
Galaxies What is a galaxy? How many stars are there in an average galaxy? About how many galaxies are there in the universe? What is the name of our galaxy?
Galaxies Chapter Twenty-Six. Guiding Questions How did astronomers first discover other galaxies? How did astronomers first determine the distances to.
Astronomy class: Pages 2-9
What is your “cosmic” address? Where do you live? Your home or your school has an address: a street, a city or town, and a country. When someone sends.
Where is the Solar System in the Universe?. What is the solar system? The solar system consists of: – The sun (which is the name of our star) – Planets.
Important Course Information Syllabus and everything else: How to make a moon observation:
Part 5: The Galaxy and the Universe In this final part of the course, we will: 1. Look at the big spatial picture: Are there organizations of stars? What.
From Here to The Dawn of Time A. Herrold. To the edge of the solar system The orbit of Neptune is not at the edge of the solar system Past the planets.
Chapter 1 Our Place in the Universe
Chapter 1 Our Place in the Universe. 1.1 Our Modern View of the Universe What is our place in the universe? How did we come to be? How can we know what.
Unit 1 Lesson 1 Structure of the Universe
The Planets in our Solar System
The Scale of the Cosmos “ The Universe is a big place. ” “ The Universe is a big place. ” Really big. Really big. Really, really big! Really, really big!
Unit 2 Lesson 1 Structure of the Universe
Chapter 1 Introduction to Astronomy. What is Astronomy? Astronomy is the scientific study of celestial bodies. Astrology is a group of beliefs and schools.
Chapter 1 Our Place in the Universe
… but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field.
The Structure of the Universe All held together by gravitational forces.
The Universe and Galaxies
Galaxies Chapter 16. Topics Types of galaxies Dark Matter Distances to galaxies Speed of galaxies Expansion of the universe and Hubble’s law.
Astronomy in the News It turns out there is five times more material in clusters of galaxies than we would expect from the galaxies and hot gas we can.
Unit Stars and the Universe. Stars A star is a giant, hot ball of gas. Stars generate light and heat through nuclear reactions. They are powered by the.
Unit 2 Lesson 1 Structure of the Universe
Scales of the Universe. The Earth is 12,700 km in diameter. The Sun is 1.39 million km in diameter.
Galaxies Stellar Neighborhoods. What are Galaxies? Galaxies are –Huge –Held together by gravity –Comprised of… Stars Objects that orbit those stars The.
Galaxies GALAXY -comes from the ancient Greeks and their word for “milk”- galactos.
Chapter 20 Galaxies And the Foundation of Modern Cosmology.
The Stars Chapter 14 Great Idea: The Sun and other stars use nuclear fusion reactions to convert mass into energy. Eventually, when a star’s nuclear fuel.
What is the structure of the universe? The universe consists of super clusters of galaxies separated by vast, bubble-shaped voids. Each super cluster consists.
Structure of the Universe. Or What’s Out There and Where is it?
Our Place in Space Where we are 1. We live on Earth 2 Welcome to Earf!
THE MILKY WAY Intro Info.
Astronomy The study of objects and matter outside the earth's atmosphere and of their physical and chemical properties.
Galaxy Dynamics Lab 11. The areas of the sky covered by various surveys.
The Planets in our Solar System. Solar System Basics Our solar system is not only made of the Sun, the nine planets and their satellites, but also asteroids.
The Universe planets planets moons moons stars stars solar systems solar systems galaxies galaxies nebulae nebulae empty space empty space more? more?
Welcome To….. The Trick is to Pick!. THE SUN Sun vs. Earth  Answers  A. 109 times smaller  B. The Earth Stress Ball Over 1 million Earths would fit.
Universe Tenth Edition Chapter 23 Galaxies Roger Freedman Robert Geller William Kaufmann III.
7.2 Galaxies pp
Option E.1 Introduction to the Universe. Collection of planets, moons, asteroids, comets, and other rocky objects travelling in elliptical orbits around.
July 21, 2004 Topics of the Day The Electromagnetic Spectrum (1 hour) –Everyday detectors and Shields Powers of Ten Size and Scale of the Universe (.5.
Stars and Galaxies Chapter 12. Stars Definition: a large ball of gas that emits energy produced by nuclear reactions in the star’s interior Planets, comets,
Solar System The solar system is the gravitationally bound system comprising the sun and the objects that orbit it.
Light: An Introduction
Unit 1 Lesson 1 Structure of the Universe
Size and Scale of the Universe
Cosmic Survey History of the Universe
Size and Scale of the Universe
What is your Cosmic Address?
The Universe.
Astronomy-Part 1 Notes The Structure of the Universe
SIZE and Scale Of The Universe
Size and Mass in the Universe
Structure of the Universe
Unit 2 Lesson 1 Structure of the Universe
Integrated Science.
ALL space and everything that is in it.
Perspectives on Our Solar System Introduction: ‘Our’ Place
The Universe and Galaxies
Size and Scale of the Universe
Introduce.
The Solar System, Galaxies, and Universe
Presentation transcript:

Size and Scale of the Universe What is your Cosmic Address? # Street City State Country Continent Hemisphere Planet …

Size and Scale of the Universe Realm Guesses Group 1Group 2Group 3Group 4Group 5Group 6 EarthSalt grain Sun Solar System Solar Neighborhood Galaxy Local Group Local Supercluster Universe

Size and Scale of the Universe Realm Actual Size (km) Actual Size (light-years) Multiple “X” larger than Earth Scale Model Earth12,700 (1.27E+4) 1.4 billionths (1.4E-9) 1salt grain (0.1 mm) Sun1.39 million (1.39E+6) 1.5 ten-millionths (1.5E-7) 109 (1.09E+2) gum ball (1.9 cm) Solar System30 billion (3.0E+10) (3.2E-3) 2.34 million (2.34E+6) football stadium (234 meters) Solar Neighborhood 617 trillion (6.17E+14) 65 (6.5E+1) 48 billion (4.8E+10) Mercury (4,800 km) Galaxy963 quadrillion (9.63E+17) 100,000 (1.0E+5) 75 trillion (7.5E+13) 5.4 x Sun (7.5 million km) Local Group31 quintillion (3.1E+19) 6.5 million (6.5E+6) 2.4 quadrillion (2.4E+15) Orbit of Mars (1.6 AU) Local Supercluster 1.2 sextillion (1.2E+21) 130 million (1.3E+8) 97 quadrillion (9.7E+16) Orbit of Eris (68 AU) Universe860.9 sextillion (8.6E+23) 91 billion (9.1E+10) 68 quintillion (6.8E+19) Oort Cloud (48,000 AU or 0.76 ly)

Size and Scale of the Universe Realms of the Universe Image courtesy of The Cosmic Perspective by Bennett, Donahue, Schneider, & Voit; Addison Wesley, 2002

Size and Scale of the Universe Earth Planet where we all live Comprised primarily of rock Spherical in shape 12,700 km in diameter It would take 17 days to circumnavigate the globe driving a car at 100 km/hr At the speed of light, it would take 0.13 seconds to go all the way around Earth.

Size and Scale of the Universe Sun Star that Earth orbits Composed primarily of hydrogen and helium gas Uses nuclear fusion in its core to generate heat and light to allow itself to resist the crushing weight of its own mass Spherical in shape 1.39 Million km in diameter

Size and Scale of the Universe Earth & Sun The Sun’s diameter is 109 times greater than that of Earth Over 1 million Earths would fit inside the Sun’s volume Earth orbits the Sun at an average distance of 150 million kilometers. This distance is called an Astronomical Unit (AU) It would take 11,780 Earths lined up side to side to bridge the 1 AU between Earth and Sun.

Size and Scale of the Universe The Solar System 8 planets, thousands and thousands of dwarf planets and asteroids, trillions of comets and meteoroids Mostly distributed in a disk about the Sun Sun blows a constant wind of charged gas into interplanetary space, called the Solar Wind Boundary between Solar Wind and interstellar space at 100 AU from the Sun (200 AU diameter)

Size and Scale of the Universe The Solar Neighborhood The region of the Galaxy within about 32.6 light- years of the Sun (65 light- years diameter) is considered its neighborhood. Here stars move generally with the Sun in its orbit around the center of the Galaxy This region is inside a large bubble of hot interstellar gas called the Local Bubble. Here the gas temperature is about 1 million degrees Kelvin and the density is 1000 times less than average interstellar space. Direction of Galactic Rotation To Center of Galaxy The image is 390 light-years across.

Size and Scale of the Universe The Milky Way Galaxy is a giant disk of stars 100,000 light-years across and 1,000 light-years thick. There are over 100 Billion stars in the Milky Way The Spiral arms are only 5% more dense than average, and are the locations of new star formation The Sun is located at the edge of a spiral arm, 30,000 light-years from the center It takes 250 Million years for the Sun to complete one orbit The Milky Way Galaxy

Size and Scale of the Universe The Local Group Contains 3 large spiral galaxies--Milky Way, Andromeda (M31), and Triangulum (M33)—plus a few dozen dwarf galaxies with elliptical or irregular shapes. Gravitationally bound together—orbiting about a common center of mass Ellipsoidal in shape About 6.5 million light-years in diameter

Size and Scale of the Universe The Local Supercluster A cluster of many groups and clusters of galaxies Largest cluster is the Virgo cluster containing over a thousand galaxies. Clusters and groups of galaxies are gravitationally bound together, however the clusters and groups spread away from each other as the Universe expands. The Local Supercluster gets bigger with time It has a flattened shape The Local Group is on the edge of the majority of galaxies The Local Supercluster is about 130 Million light-years across

Size and Scale of the Universe The Universe Surveys of galaxies reveal a web-like or honeycomb structure to the Universe Great walls and filaments of matter surrounding voids containing no galaxies Probably 100 Billion galaxies in the Universe The plane of the Milky Way Galaxy obscures our view of what lies beyond. This creates the wedge-shaped gaps in all-sky galaxy surveys such as those shown here.

Size and Scale of the Universe The Universe Computer Simulation The observable Universe is 91 Billion light-years in diameter.

Size and Scale of the Universe 1) The Standard Ruler Use knowledge of physical and/or geometric properties of an object to relate an angular size with a physical size to determine distance. Ex: Parallax, Moving Clusters, Time Delays, Water MASERs Considered to be a direct or absolute measurement. There are two basic methods for measuring astronomical distances R d  d = R/Tan()  R/

Size and Scale of the Universe Trigonometric Parallax Requires very precise measurements of stellar positions, and long baselines Need telescopes with high resolution, and must observe over several years. Hipparchos satellite measured distances to tens of thousands of stars within 1,500 light-years of the Sun.

Size and Scale of the Universe 2) The Standard Candle Use knowledge of physical and/or empirical properties of an object to determine its Luminosity, which yields distance via the Inverse Square Law of Light. Ex: Cepheid Variables, Supernovae, TRGB, Tully-Fisher Considered to be relative until tied to an absolute calibration. b = L/4d 2

Size and Scale of the Universe Cepheid Variable Stars There is a kind of giant star whose surface pulsates in and out with a regular period. That period of pulsation is related to the Luminosity of the star. LMC contains hundreds of known Cepheids all at the same distance. Which allows for robust determination of the Period Luminosity Relationship.

Size and Scale of the Universe To measure cosmological distances a ladder of methods is used to reach further out into the Universe. Each “rung” in the ladder of distance measuring methods depends on the calibration of the methods “below.”