LECTURE 27, DECEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.

Slides:



Advertisements
Similar presentations
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL Revision Lecture.
Advertisements

Galaxies & the Universe
LECTURE 21, NOVEMBER 16, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
LECTURE 24, NOVEMBER 30, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
LECTURE 18, NOVEMBER 2, 2010 ASTR 101, SECTION 2 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
LECTURE 14, OCTOBER 12, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
LECTURE 16, OCTOBER 26, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Chapter 21: The Milky Way. William Herschel’s map of the Milky Way based on star counts In the early 1800’s William Herschel, the man who discovered the.
Comprehend other Galaxies and their Classifications Comprehend Dark Matter and Energy Comprehend the Electromagnetic Spectrum Comprehend the Big Bang Theory.
THE ORIGIN AND FATE OF THE UNIVERSE. The Scale of the Universe The solar system (see illustration)
LECTURE 25, DECEMBER 2, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Galaxies and the Universe
Matter Unit Learning Goal #1: Recognize the origin and distribution of elements in the universe.
Galaxies Types Dark Matter Active Galaxies Galaxy Clusters & Gravitational Lensing.
ASTR100 (Spring 2008) Introduction to Astronomy Cosmological Inflation Prof. D.C. Richardson Sections
GENS X1Galaxies1 Lecture 5: Galaxies Dr Michael Burton.
GENS S1 and S2Galaxies1 Dr Michael Burton. GENS S1 and S2Galaxies2 The Structure of our Galaxy How did we find out? Herschel’s 18 th Century.
Types of Galaxies Elliptical: Spiral: Irregular:.
Chapters 17,18: Cosmology and Life in the Universe Nearly every speck of light in the image is a galaxy.
LECTURE 22, NOVEMBER 18, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Chapter 31 Galaxies & the Universe Review & Recap It does this by precisely measuring the speed of gas and stars around a black hole. This provides clues.
Review for Exam 3.
Lecture 4. Big bang, nucleosynthesis, the lives and deaths of stars. reading: Chapter 1.
Overview of Astronomy AST 200. Astronomy Nature designs the Experiment Nature designs the Experiment Tools Tools 1) Imaging 2) Spectroscopy 3) Computational.
Galaxies Read Your Textbook: Foundations of Astronomy
Ch. 31 – Galaxies & the Universe   Have you seen the Milky Way at night? The Sun is one of over 100 billion stars that make up the Milky Way. The Sun.
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2.
Chapters 17,18: Cosmology and Life in the Universe.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 25.
Chapter 16 The Milky Way Galaxy 16.1 Overview n How many stars are in the Milky Way? – About 200 billion n How many galaxies are there? – billions.
The Nature of Galaxies Chapter 17. Other Galaxies External to Milky Way –established by Edwin Hubble –used Cepheid variables to measure distance M31 (Andromeda.
Hubble’s galaxy classes Spheroid Dominates Disk Dominates.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Final Review December 4, 2002 Final Exam will be held in Ruby Diamond Auditorium NOTE THIS!!! not UPL Dec. 11, am-noon Bring your ID, calculator.
The Universe and Galaxies The universe is vast in size and very very old.
Test #3 Same types of questions Bring a calculator Study the other exam reviews.
“OUR GALAXY” Definition of a Galaxy: a huge group of individual stars, star clusters, dust, and gas bound together by gravity.
Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
Astronomy 101 Cumulative Presentation Aleks Alunans.
1 Cosmology HNRT 227 Chapter October 2015 Great Idea: The universe began billions of years ago in the big bang and it has been expanding ever since.
Homework for today was WORKBOOK EXERCISE: “Expansion of the Universe” (pg in workbook)
A Long Time Ago in a Galaxy Far, Far Away…. The Milky Way Galaxy: Home Sweet Home!! Our home Galaxy is called the MILKY WAY (like the candy bar ) Our.
Chapter 25 Galaxies and Dark Matter. 25.1Dark Matter in the Universe 25.2Galaxy Collisions 25.3Galaxy Formation and Evolution 25.4Black Holes in Galaxies.
The Mass of the Galaxy Can be determined using Kepler’s 3 rd Law –Solar System: the orbital velocities of planets determined by mass of Sun –Galaxy: orbital.
Unit 2 - Cosmology Part 1: Stars Part 2: Galaxies Part 3: Origin and Evolution of the Universe.
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.
Chapter 20 Cosmology. Hubble Ultra Deep Field Galaxies and Cosmology A galaxy’s age, its distance, and the age of the universe are all closely related.
Formation of the Solar System and The Universe. Our Solar System Sun is the center of a huge rotating system of: Sun is the center of a huge rotating.
COSMOLOGY The study of the origin, structure, and future of the universe.
Formation of the Solar System and The Universe
GCSE Astronomy.
How fast would a galaxy 2,000 megaparsecs away be moving with respect to us, according to Hubble’s Law? Hint: H0 = 70 km/s/Mpc 1,400 km/s 14,000 km/s 140,000.
© 2017 Pearson Education, Inc.
Formation of the Solar System and The Universe
© 2017 Pearson Education, Inc.
© 2017 Pearson Education, Inc.
Great Ideas in Science: Lecture 8 – Stars & Galaxies
Unit 8 Review Worksheet Solutions.
The Milky Way, Deep Space, and Beyond!
Chapter 16 Active Galaxy.
Types of Galaxies Elliptical: Spiral: Irregular:.
Astronomy 100 Tuesday, Thursday 2:30 - 3:45 pm Tom Burbine
Cosmology Chapter 15 Great Idea:
Introduction to Cosmology
Galaxies.
Ch. 31 – Galaxies & the Universe
Galaxies Astrobiology and Cosmology
Cosmology = Big Questions
Presentation transcript:

LECTURE 27, DECEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010

2

3

4

5

6

a) planets in the Milky Way Galaxy. b) planets with life in the universe. c) stars with planets like Earth. d) civilizations in our Galaxy. e) terrestrial planets with water. Question 1 The Drake equation attempts to define the number of

a) planets in the Milky Way Galaxy. b) planets with life in the universe. c) stars with planets like Earth. d) civilizations in our Galaxy. e) terrestrial planets with water. Question 1 The Drake equation attempts to define the number of

ASTR 101-3, FALL 20109

a) temperatures on a planet are reasonable. b) terrestrial planets can form around a star. c) terrestrial planets could have liquid water on their surfaces. d) liquid water can condense into rain in the atmosphere. e) Sun-like stars can exist in the Milky Way Galaxy. Question 4 The habitable zone is the area where

a) temperatures on a planet are reasonable. b) terrestrial planets can form around a star. c) terrestrial planets could have liquid water on their surfaces. d) liquid water can condense into rain in the atmosphere. e) Sun-like stars can exist in the Milky Way Galaxy. Question 4 The habitable zone is the area where Stellar habitable zones

ASTR 101-3, FALL

ASTR 101-3, FALL

ASTR 101-3, FALL

a) in radio light where natural emissions from our Galaxy are minimal. b) on Mars where liquid water has been proven to exist in the past. c) on the Moon where water is believed to exist under ice in a deep crater. d) in the Oort cloud where comets rich in water are formed. Question 6 The water hole is a region

a) in radio light where natural emissions from our Galaxy are minimal. b) on Mars where liquid water has been proven to exist in the past. c) on the Moon where water is believed to exist under ice in a deep crater. d) in the Oort cloud where comets rich in water are formed. Question 6 The water hole is a region The water hole may be the best part of the electromagnetic spectrum for intelligent civilizations to communicate across the vast reaches of space.

TEST NO. 4 TIME: Tuesday, December 14, 2010, 12:30 PM PLACE: Regener 103 MATERIAL: Topics covered since Test No. 3 NO. 2 PENCIL: Bring one! ASTR 101-3, FALL

REVIEW, CHAPTER 14 THE MILKY WAY GALAXY Milky Way Galaxy-Basic structure (disk, halo, bulge), type, motions, Suns location, formation Important variable stars-RR Lyrae stars, Cepheids Spiral arms-Winding problem, density wave theory, 21-cm line Rotation curve and dark matter Central region-Sgr A*, star orbits, black hole ASTR 101-3, FALL

REVIEW, CHAPTER 15 NORMAL AND ACTIVE GALAXIES Types of galaxies(spirals, barred spirals, ellipticals), Hubbles classification Irregular galaxies, Magellanic Clouds Distance ladder, Standard Candles (Tully-Fisher relation, Type I supernovae) Clusters of galaxies Hubbles Law, Hubbles constant, red shifts Active galaxies, time variations, colliding galaxies Quasars-distances, central engines, and massive black holes ASTR 101-3, FALL

REVIEW, CHAPTER 16 GALAXIES AND DARK MATTER Dark matter clues– rotation curves, clusters of galaxies, Head-Tail galaxies, gravitational lensing, Bullet Cluster Look-back time Galaxy formation and evolution, starburst galaxies, central black holes Galaxy surveys, large-scale structure of the universe Matter in the universe is mostly dark ASTR 101-3, FALL

REVIEW, CHAPTER 17-1 COSMOLOGY Cosmological principle, Olbers paradox Big Bang, expansion of the universe, Hubble time, fate of the universe Curvature of space Cosmic acceleration, dark energy, mass- energy composition of the universe ASTR 101-3, FALL

REVIEW, CHAPTER 17-2 COSMOLOGY Cosmic Microwave Background (CMB), origin, Penzias and Wilson Element formation in the Big Bang Inflation, horizon problem, flatness problem Large-scale structure formation ASTR 101-3, FALL

REVIEW, CHAPTER 18 LIFE IN THE UNIVERSE Necessary chemical compounds are wide- spread in the cosmos Miller-Urey experiment, amino acids Drake equation, habitable zones, estimated number of advanced civilizations in our Galaxy Extra-terrestrial communication, Water-Hole ASTR 101-3, FALL