Lecture 26 The Dark Side of the Universe Announcements • Homework Read Ch. 24: Life in the Universe Mastering Astronomy: Chapter 24 Due Friday, Dec 6, at.
Download ReportTranscript Lecture 26 The Dark Side of the Universe Announcements • Homework Read Ch. 24: Life in the Universe Mastering Astronomy: Chapter 24 Due Friday, Dec 6, at.
Lecture 26 The Dark Side of the Universe Announcements • Homework Read Ch. 24: Life in the Universe Mastering Astronomy: Chapter 24 Due Friday, Dec 6, at 6pm • Today’s lecture covers Ch. 22: All you need to know is in the lecture. • Winter Break: Read Chapter 22 for fun. Final Exam: Thursday, Dec 19, 11:30-2:30 RSF Field House: Main Floor Gym • Multiple Choice • All Chapters: 1-5, 9-14, 24 & All Lectures. Emphasis on Chapters 12, 13, 14, 24 • Review Sessions: Tue and Thu (Dec 10 & 12) at 5-6:30 in 2040 VLSB Come with questions ! Lecture 26 The Dark Side of the Universe Most of the Universe is Dark You, me, Earth, Planets, stars How do we know the Universe is Mostly Dark ? Example 1: Gravity by Central Mass (Sun) determines orbital speed of planets. Mercury Venus Earth GM(< r) V = G M / Distancer 2 Orbital Speed = Mars Jupiter Solar System: “Keplerian orbits” How do we know the Universe is Mostly Dark ? Gravity by Central Mass (galaxy) determines orbital speed of stars. Orbital Speed = Galaxies: “Flat rotation curve” G M / Distance How do we know the Universe is Mostly Dark ? Gravity by Central Mass (galaxy) determines orbital speed of stars. Orbital Speed = G M / Distance Speed doesn’t fall ! Mass, M, must be increasing outward! Galaxies: “Flat rotation curve” How do we know the Universe is Mostly Dark ? Example 2: Gravitational Bending of Light by Mass Light Source Telescope How do we know the Universe is Mostly Dark ? How do we know the Universe is Mostly Dark ? Four images of the same galaxy Four images of the same galaxy How do we know the Universe is Mostly Dark ? What can dark matter be? Planets? Not enough mass: even Jupiter weighs only 0.1% of the Sun What can dark matter be? Black Holes? Graveyards of massive stars. But massive stars are rare and made of normal atoms. Once formed, black holes suck in normal matter. So you can’t hide much dark matter in it. What can dark matter be? Anti-matter? Antimatter and matter have identical mass but opposite quantum numbers (electric charge, spin…) Antimatter and matter annihilate each other into flashes of easily detectable gamma rays What can dark matter be? Top candidate: Elementary Particles: Yet to be discovered ! 17 Dark Energy 18 Supernova Explosions as Standard Candles Type Ia supernovae, which give off a standard amount of light. The distance to the galaxy that contains the supernova: Compare how bright they know the explosion should be with how bright the explosion appears. Using the inverse square law of light, they can compute the distance to the supernova and thus to the supernova's home galaxy. How do we know the Universe is Dark? Example 4: Distant supernovae After Before 20 How do we know the Universe is Dark? Example 4: Distant supernovae are standard candles 22 23 24 Most of the Universe is Dark You, me, Earth, Planets, stars How do we know the Universe is Dark? Example 3: Cosmic Microwave Background CMB: very cold (-270.275 C, -454.495 F) and nearly uniform relic radiation left over from the hot big bang How do we know the Universe is Dark? Example 3: Cosmic Microwave Background If you had microwave eyes: (1965) (1992) 28 (2010) How do we know the Universe is Dark? White points: WMAP (2010) 7-year data Red curve: Theoretical prediction for a universe made of 73% dark energy, 23% dark matter, 4% atoms Accelerating Expansion of the Universe: Dark Energy 30 How do we know the Universe is Dark? Kowalski et al (2008) Supernovae probe Dark Energy CMB probes Concordance region: 73% dark energy 23% dark matter 4% atoms Dark Matter