Origins Lecture 10; May 1 2014. Previously… on Origins: Is Earth a special/unique place? What does the question mean? How do we find planets? What are.

Slides:



Advertisements
Similar presentations
DCMST May 27 th, 2009 Supernovae and cosmology Gavin Lawes Wayne State University David Cinabro Wayne State University Johanna-Laina Fischer DCMST.
Advertisements

Observational Astronomy. Astronomy from space Hubble Space Telescope.
1 Introduction Lecture 1. 2 What is Science? l Science is a way of viewing the world based on the guiding principles: l Nature is lawful l Some of this.
Our Place in the Universe Drew Smith. Important Principles The Cosmological Principle ▫The universe is isotropic and homogenous (it “looks” the same in.
A Universe of Galaxies Ian Dell’Antonio Brown University.
The Universe Around Us Geocentric = Earth-centered
Announcements Homework 14 due Wednesday (5 questions) Monty Python Challenge offer good through this Wednesday! Final exam in SL 228 next Monday or Tuesday.
Cosmic History Big Bang Cosmology is a well accepted theory (12-16 billion years ago) Gravity drives the formation of our Milky Way galaxy (11-14 billion.
Astronomy class: Pages 2-9
Our Universe Lessons 3-4.
Scales in Space and Time in the Cosmos By Dr. Harold Williams of Montgomery College Planetarium
Review for Exam 3.
Hypothesis vs. Theory Unit 1 – Spaceship Earth.
INTRODUCTION TO ASTRONOMY Overview FRONTIERS IN ASTRONOMY PHYS 271.
The Origin of the Universe Massimiliano Galeazzi Miami, 20 November 2002MALS 601.
Cosmic Survey: What are Your Ideas about the Universe?
New Core Curriculum week 3, class-2 Foundations of Scientific Process Visible Objects in the Universe.
Chapter 1 Our Place in the Universe
Origin of the Universe Have you ever heard of a little thing called the “Big Bang?”
Our Galaxy and Beyond. Our Place in Our Galaxy 3 What’s the Difference? Universe Galaxy Image credits: NASA, STScI Solar System.
OGT: Chapter Eight  Origins Of The Universe. Astronomy  Study of stars and planets Aristotle  Earth is center of the universe (geocentric). Sun, planets.
A FEW THINGS ABOUT THE UNIVERSE STUCKENS Daniel ALLOUCHE Ashley
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL 3. Cosmological concepts and Olbers’ paradox.
Origins Lecture 15; May Previously on Origins Time of history/humans vs. time of “god” –What was there before time? –Does this make sense? The.
THE FORMATION OF THE SOLAR SYSTEM. Its all about gravity Gravity can set the particles and dust in a nebula into motion The core of a young star (protostar)
Introduction to Galaxies 5/23/2013. BR: Milky Way Scale The Milky Way has a diameter of approximately 8.25 x 10 9 AU (8.25 billion AU). 206,265 AU = 3.26.
The Milky Way Galaxy. HW #9 – MasteringAstro “Stars and Galaxies” Available now Tuesday April 17 th Due BEFORE CLASS Tuesday April 24 th Observing logs.
1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped.
The theory of the universe. Expanding of our universe In the 1920s, astronomers had the technology to see more Celestial bodies with advance telescope.
The TWO-INCH Universe A powerful set of analogies to examine size and distance in astronomy Source: smithsonianeducation.org.
Astronomy. What is Astronomy? 1. Astronomy is the study of the universe. This includes planets, stars, galaxies, black holes, moons, meteors, comets,
The Universe planets planets moons moons stars stars solar systems solar systems galaxies galaxies nebulae nebulae empty space empty space more? more?
Jeopardy Vocabulary Edwin Hubble Big Bang Theory Red Shift Analysis Q $100 Q $200 Q $300 Q $400 Q $500 Q $100 Q $200 Q $300 Q $400 Q $500 Final Jeopardy.
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.
Astronomy Review. What 3 pieces of evidence supports the Big Bang Theory? 1) Doppler Effect 2) Microwave Radiation 3) Quasars.
Galaxies and Stars 8.E.4A.1 Obtain and communicate information to model the position of the Sun in the universe, the shapes and composition of galaxies,
DCMST May 22 nd, 2007 Dark matter and dark energy Gavin Lawes Wayne State University.
Review of the Scale Problems Scale problems are problems of the style that ask how big or small would something be if all objects were scaled up or down.
Monday, November Warm-Up: Grade Content Frame 2. Astronomy Intro.
The Expanding Universe
1._____began from a nebula that was disturbed (big bang) 2._____observed the phases of Venus (astronomers) 3._____theory of the sun centered view of the.
Angular Separation is not enough! We want to know the answer to the ‘age old question’: How far away are the stars? Ans: A lot farther than anyone imagined!
Nov 19, 2003Astronomy 100 Fall 2003 Next week is Thanksgiving Break. No homework until you get back. On Friday… Exam 2 Grades are posted. Nighttime observing.
The Order of the Universe. Lets start with our Earth. We are one planet in a solar system with one star- our sun. We have seven other planets in our solar.
1 Our place in the Universe. 2 This is what we think our galaxy, the Milky Way, looks like. The Sun is about ½ way from the center on a galactic arm The.
Milky Way Galaxy. Galaxy A group of stars, dust and gases held together by gravity. 170 billion galaxies in the universe 200 billion stars in a galaxy.
The Universe. A Celestial Object is any object in our universe above our atmosphere. A Celestial Object is any object in our universe above our atmosphere.
CHAPTER 31 THE GALAXIES & THE UNIVERSE. GALAXIES Scattered throughout the universe Made up of stars, dust and gas held together by gravity There are three.
Dark Matter, Dark Energy
The Continuing Copernican Revolution... from Heliocentricity to the Cosmological Principle Slides online at:
Open up your laptops, go to MrHyatt.rocks, and do today’s bellwork
Galaxies.
Earth in Our Universe.
Some space objects are visible to the human eye
Our place in the Universe
A Modern View of the Universe
Galaxies and Formation
BIG BANG THEORY.
Ch6: Gravitational Fields
Structure of the Universe
Astronomy Astronomy.
How Did the Universe Begin?
ALL space and everything that is in it.
Astronomy Astronomy.
How big? How old? How far? Intro to space.
Astronomy Terms-Copy & define these terms to be placed in flipbook
BIG BANG THEORY.
The “Big Bang” was an enormous release of energy!
Structure, Types, Known Galaxies
Presentation transcript:

Origins Lecture 10; May

Previously… on Origins: Is Earth a special/unique place? What does the question mean? How do we find planets? What are habitable planets? –Selection effects

Outline: Is Earth a special/unique place? Drake’s equation Is Earth special? –Heliocentrism vs. Geocentrism –How about in our Galaxy? Is our Galaxy special? Is there any special place? –Observations The cosmological principle and its consequences: –Cosmic Time

A physicist’s answer We phrase the question in statistical terms: –Is the location of the Earth in the Universe special in anyway? –Is it at the “center” of something? Let’s take a look! Let’s measure!

Modern “Copernicanism”: Current solar system description Newton: –The Sun and the other bodies orbit around a common center of mass –The Sun is so massive that it is very close to the center of mass and moves very little –Orbits are elliptical, but very slightly so

Modern “Copernicanism”: Current solar system description Einstein: –Mass perturbs local geometry –Space time is curved –Objects move freely in curved space time 43s per century! Another test of general relativity!

Modern “Copernicanism”: Parallax and distances Measurements of stellar parallax indicate that the closest stars are a few light years away! How far is the sun? They also indicate that the Earth “moves” (eppur si muove). With respect to what? How fast?

Modern “Copernicanism”: planets, Sun and other stars

Modern “Copernicanism”: Where are we in our Galaxy?

Modern “Copernicanism”: Current view

Modern “Copernicanism”: Where are we in our Galaxy? Somewhat in the outskirts… 25,000 ly away from the center Moving at about 200 km/s around the center of the Milky Way TRUMPLER’s (1930) discovery of dust

Modern “Copernicanism”: Evidence The Galaxy is more than a 100,000 lyrs in diameter There are 10,000,000,000 solar masses inside the Sun’s orbit!

Modern “Copernicanism”: Galaxies What are they? How far are they? How big are they?

Modern “Copernicanism”: Galaxies Until 1923 there was a debate on the distance of “nebulae” (galaxies) Are they small objects inside our galaxy or are they “external”? Hubble settled this by measuring the distance to Andromeda –A whopping 2.5 million light years!

Modern “Copernicanism”: The Universe is full of galaxies! 10,000 galaxies in a tiny piece of sky! 1/150,000 of the sky

Modern “Copernicanism”: How many galaxies? Based on the deep fields we estimate of order a billion visible galaxies

Modern “Copernicanism”: Large scale structures SDSS and 2dF mapped the positions of about 1,000,000 galaxies Billions of light years

COSMIC MICROWAVE BACKGROUND

Modern “Copernicanism”: Summary Our planet orbits around an average star in the outskirts of an average galaxy All directions in the universe look the same All places in the universe look the same if you average over large enough volumes (100,000,000 light years or so) THE UNIVERSE IS HOMOGENEOUS AND ISOTROPIC (Cosmological Principle) This scientific hypothesis build on observational evidence allows us to construct a simple theory of the universe, including define a cosmic time

Concluding remarks

The End See you on Tuesday