ASTR 1020 – April 27 Last Lecture, next Thursday .

Slides:



Advertisements
Similar presentations
Origin & Evolution of the Universe
Advertisements

When Galaxies Collide. It is not uncommon for galaxies to gravitationally interact with each other, and even collide!
© 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Chapter 26: Cosmology Why is the sky dark? The expanding universe Beginning of the universe: The Big Bang Cosmic microwave background The early universe.
The Fate of the Universe. The cosmological principle The simplest universes is: Homogenous – the same everywhere you go Isotropic – the same in all directions.
A Brief Tour of the Universe Don’t Panic The Sun in UV.
Cosmology Past, present and future of the universe Is space flat or curved? Where is the center? What lies beyond our limit of vision? What is the universe.
19 The Big Bang Evidence The Science of Creation.
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.
No Structure on Largest Scales (Galaxies distributed fairly uniformly)‏ Surprising given structure on smaller scales Cosmological Principle: Universe is.
Cosmology Physics466 Olbers Paradox Cosmological principle Expansion of the Universe Big Bang Theory Steady State Model Dark Matter Dark Energy Structure.
Do your course evaluations. I will add 5 points on your final exam if you complete the evaluation.
The Big Bang Astrophysics Lesson 18. Learning Objectives To know:-  What is the big bang theory  What is the evidence supporting it including:-  Cosmological.
Chapter 26: Cosmology How big is the universe? How long has it been around and how long will it last?
Chapter 26.
Contemporary science issues Lesson 16: Has the universe always been there? © 2006 Gatsby Technical Education Projects.
Please press “1” to test your transmitter.
Cosmology: The Study of the Universe as a Whole Physics 360 Geol 360 Astronomy John Swez.
The Birth of the Universe. Hubble Expansion and the Big Bang The fact that more distant galaxies are moving away from us more rapidly indicates that the.
Introduction to Cosmology. Types of Universes If you were to make a universe, would you give it a finite size, or make it infinite? In a finite universe,
EXPANDING UNIVERSE. OLBERS PARADOX Olbers’ paradox “The night sky is dark.” This statement is called Olbers’ paradox, after astronomer who discussed.
The Tully-Fisher Relation A relation between the rotation speed of a spiral galaxy and its luminosity The more mass a galaxy has  the brighter it is 
The Big Bang: what happened, and when did it happen?
10B The Big Bang Where do we come from, where are we going?
ASTR 1200 Announcements Website Last Lecture on Thursday. Final Exam Wednesday Dec 17 1:30-4:00 In.
Cosmology II - The nature of the universe What kind of universe do we live in (positive, Negative, or zero curvature)
Ch. 22 Cosmology - Part 1 The Beginning. Beginnings ???? - Newton suggested that for the stars not to have coalesced, the universe must be infinite and.
The Universe. Galaxies are believed to have formed from mergers of smaller galaxies and star clusters. Galaxy Formation and Evolution.
Olber’s Paradox Why is the night sky dark?. Night Sky.
Questions From Reading Activity? IB Assessment Statements  Olbers’ Paradox E.4.1.Describe Newton’s model of the universe. E.4.2.Explain Olbers’paradox.
THE BIG BANG THEORY. STATES THAT THE UNIVERSE BEGAN AS A SINGLE COSMIC EXPANSION ABOUT 15 BILLION YEARS AGO. THE BIG BANG THEORY.
The Expanding Universe
Lecture 38 – Cosmology II How do we describe (and understand) the expansion of the universe, what is happening now, what happened in the remote past, and.
STATES THAT THE UNIVERSE BEGAN AS A SINGLE COSMIC EXPLOSION ABOUT 15 BILLION YEARS AGO. THE BIG BANG THEORY.
ASTR 113 – 003 Spring 2006 Lecture 12 April 19, 2006 Review (Ch4-5): the Foundation Galaxy (Ch 25-27) Cosmology (Ch28-29) Introduction To Modern Astronomy.
The Shape and Fate of the Universe Assumptions in cosmology Olber’s paradox Expansion of the Universe Curvature of the Universe Fate of the Universe.
The Fate of the Universe. The fate depends on the rate of expansion and the density Density greater than critical value – gravity will halt expansion.
The Scientific explanation for the forming of the universe.
© 2017 Pearson Education, Inc.
ASTR 1020 – March 9 Homework 5 due today .
Astrophysics and Cosmology
ASTR 1020 – May 2 Last Lecture on Thursday – Largely Review per vote
The Science of Creation
The Universe
The Big Bang Theory: Origin & Evolution of the Universe
ASTR 1200 Announcements Exam 3 Returned Today
17. 3 The Big Bang and Inflation 17
ASTR 1040 – November 30 Planetarium, December 5
Where do we come from, where are we going?
HOT Big Bang Tuesday, January 22.
Exam 3 average: 65%. You will have all of class time on Thursday to do the group review. The response “Exams” will be on Learning Suite by Wed noon. They.
ASTR 1020 – April 13 . Final Problem Set Due Today
Expansion of the Universe
Contemporary science issues
Cosmological Assumptions
Lectures on galaxies and cosmology
i>clicker Quiz #12 Which of the following statements is FALSE?
Cosmology The study of the structure and evolution of the Universe as a whole. Seeks to answer questions such as: How big is the Universe? What shape is.
Cosmology.
The Universe.
The Expanding Universe
General Relativity: Part II
Theories of Universe Formation
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
The Expanding Universe
A galaxy like the Milky Way contains about 10 billion stars.
Cosmology.
The Universe.
How was it formed? How old is it? What does the future hold?
You!!! Questions for the Lab were due at Midnight
Presentation transcript:

ASTR 1020 – April 27 Last Lecture, next Thursday . Final Exam: Monday May 8 4:30-7:00pm . Website http://casa.colorado.edu/~wcash/APS1020/APS1020.html

Galaxies are Flying Apart Galaxies remain same size. They just get farther apart. Effect is the same no matter which position you occupy

Expanding Universe Current Universe The volume of the universe is increasing. Early Universe

The Age of the Universe Notice: At time zero, d = 0 All galaxies are at zero distance! The universe has zero volume! when t=1/H

Jets

Radio Galaxies Very Large Array Very Large Baseline Array

Cygnus A

Radio Lobes Lobes contain 1053 Joules of energy in relativistic electrons. Mass energy equivalent of a million stars!

Wind Blows Jets

Full Model

Superluminal Expansion Radio interferometers see blobs emitted by AGN’s from base of jet. Watch them expand. Know distance, so can measure speed. v = 900,000km/s v = 3c Superluminal ! ? Is Einstein’s ghost worried?

Phase Velocity Point of impact can move v > c Nothing traveling that fast.

Better Explanation Blob moves close to speed of light toward us. Its closer later. Makes sideways motion appear speeded up.

Quasar Absorption Lines

The Intergalactic Medium

Intergalactic Medium 70% of the regular matter in the universe is between the galaxies Was probably neutral, then re-ionized Somehow got oxygen and other heavy elements. We didn’t know it was there 20 years ago. Still don’t have any clue how it works. Cutting edge of research.

The Cosmic Web

Structure of the Universe Where is the center of the Universe? Where are the edges? What happens if you fly to the edge and stick your finger through? Newtonian Universe must be infinite. Cosmological Principle: The Universe is Everywhere the Same (when averaged over grand scale)

Classical Universe Euclidean Geometry Infinite in Extent Matter may or may not be everywhere Universe infinitely old always been here, always will be Expansion still possible 2 x ∞ = ∞

Cosmological Principle Cosmological Principle applied to expanding Euclidean Universe New matter must be formed of nothing to keep density everywhere the same.

Olber’s Paradox If universe is infinite with stars everywhere, then there an infinite number of stars. Any line of sight will eventually intersect the surface of star. Sky would be as bright as the surface of the Sun. Well it isn’t. So why not?

Universe Must Change Answer to Olber’s Paradox: Universe must change: Space: ie the stars stop This was the answer until mid 20th Century Time: Universe hasn’t always been here, so can’t see forever. Discovery of Big Bang leads us to this answer.

General Relativity GR provided an answer The presence of matter warps space in on itself. Space is actually DEFINED by the presence of the matter in it!!! Solves the edge problem But geometry is no longer Euclidean

Geometry of Universe Space Curves in on itself There’s no path out!

Curved Space Surface of Earth has no end, but it is finite. There is no “edge” but the volume is finite.