THE UNIVERSE OR DECREASING ACCELERATION IS THE EXPANSION RATE PRESENTED BY: JAKE DOTTS & JESS MYERS.

Slides:



Advertisements
Similar presentations
P1.5.4 Red-shift AQA GCSE Science A. There are two main pieces of evidence for the Big Bang: 1.The expansion of the universe 2. Cosmic microwave background.
Advertisements

Origin & Evolution of the Universe
When Galaxies Collide. It is not uncommon for galaxies to gravitationally interact with each other, and even collide!
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 Universe This is a spiral galaxy with other galaxies in the background. The universe is “everything that exists.” The universe is a big place, perhaps.
Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance.
Dark Matter, Dark Energy, and the Expansion of the Universe By Michael Howard
Daniel Schmidt, Liberty University
2011 Nobel Prize in Physics Awarded to Saul Permutter Brian Schmidt Adam Riess "for the discovery of the accelerating expansion of the Universe through.
Objectives Distinguish the different models of the universe.
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.
Lecture 23 Models with Cosmological Constant ASTR 340 Fall 2006 Dennis Papadopoulos Chapter 11 Problems Due 12/5/06.
Cosmology Astronomy 315 Professor Lee Carkner Lecture 22 "In the beginning the Universe was created. This has made a lot of people very angry and been.
Modelling and measuring the Universe the UniverseSummary Volker Beckmann Joint Center for Astrophysics, University of Maryland, Baltimore County & NASA.
Do your course evaluations. I will add 5 points on your final exam if you complete the evaluation.
What can electromagnetic waves tell us about the movement of planets, stars, and galaxies?
Contemporary science issues Lesson 16: Has the universe always been there? © 2006 Gatsby Technical Education Projects.
Modern Physics: Part 2. ALL Galaxies have redshifts – farther from us greater redshifts! Many other scientists made observations similar to Slipher’s.
Theory on the Formation of the Universe
Cosmology: The Study of the Universe as a Whole Physics 360 Geol 360 Astronomy John Swez.
Dark energy: the greatest mystery of the universe Syksy Räsänen Department of Physics and Helsinki Institute of Physics Arkadia.
Gravity Isaac Newton was the first to account for gravity. An attracting force. Gravity = mass/distance So, 1. Massive objects have more gravity 2. Gravity.
Midterm exam: date: March 17, 2006, 8:15 a.m. date: March 17, 2006, 8:15 a.m. location: Conrad Naber Hall location: Conrad Naber Hall bring pocket calculator.
Cosmology The Origin and Future of the Universe Part I Olbers’ Paradox.
Expansion of the Universe Natural consequence of the basic field equations of the General Theory of Relativity (GTR) When GTR was first developed in 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,
General Relativity and the Expanding Universe Allan Johnston 4/4/06.
The Fate of the Universe
Dark Energy. Expanding Universe Galaxies in the universe are spreading out over time. –Hubble’s law From Einstein’s general relativity this happens as.
THEORIES OF UNIVERSE FORMATION. Studying Space Cosmology – the study of the origin, structure, and future of the universe Astronomers study planets, stars,
The “Big Bang” Theory Birth of the Universe. The Big Bang Theory First and foremost – THIS IS A THEORY! – It is up to you whether you want to believe.
HUBBLE’S LAW Edwin Hubble Hubble’s Law “the farther away a galaxy is from its observer, the faster it appears to be moving away from the observer”
Hubble’s Law AST 112. Spectra If a light source is moving toward or away from an observer, its spectral lines shift We can use this to measure approaching.
Welcome to Astronomy!. Prove that the following equation is valid by means of resolution:  xp(x)v  xq(x)   x  p(x)vq(x)  Why can ’ t you do this.
Origins of the Universe. How did it all get here? How did it all get here? MANY THEORIES!!!! MANY THEORIES!!!! Big Bang Theory Big Bang Theory Steady.
25-4: Galaxies Use the following PowerPoint to take notes on the final section of the chapter. Upon completion work with your partner to answer the Self.
The Big Bang Theory Earth and Space Ms. Lizette Gutierrez Austin High School.
Cosmology -- the Origin and Structure of the Universe Cosmological Principle – the Universe appears the same from all directions. There is no preferred.
The Expanding Universe
The UniverseSection 3 Section 3: Origin of the Universe Preview Key Ideas Bellringer What Is the Universe? What Happened at the Beginning? Predicting the.
Dark Energy By Chris Malafis & Amit Sheth. Discovery Two competing groups from different observatories were trying to prove the deceleration of the expansion.
Key Areas covered Evidence for the expanding Universe We can estimate the mass of a galaxy by the orbital speed of stars within it Evidence for dark matter.
The Origin of the Universe Chapter 20.3 Notes. What is the Universe? The universe consists of all space, matter, and energy that exists—now, in the past,
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.
Lecture 23: The Acceleration of the Universe Astronomy 1143 – Spring 2014.
Discovering the Universe Eighth Edition Discovering the Universe Eighth Edition Neil F. Comins William J. Kaufmann III CHAPTER 18 Cosmology Cosmology.
Image of the day Turn in cosmology questions!.
The Origin of the Universe
The Universe
The Big Bang Theory: Origin & Evolution of the Universe
Doesn’t that mean we are in the centre of the universe?
Karnataka Arts, Science & Commerce College, Bidar
Conclusion of Last Class: Hubble’s Law (that far away galaxies recede faster) implies that the universe is expanding uniformly in all directions, like.
BIG BANG THEORY.
The Formation of the.
Expansion of the Universe
Galaxies and the Universe
Contemporary science issues
i>clicker Quiz #12 Which of the following statements is FALSE?
The omega problem There has always been a problem with the expanding universe. Will it go on expanding forever? The answer has depended on the balance.
Cosmology.
Cosmological Expansion and Dark Energy
Georges LeMaitre theorized The Big Bang in 1927 two years before
The Universe.
Theories of Universe Formation
The Universe.
THE UNIVERSE Part 2:Cosmology.
BIG BANG THEORY.
FORMATION OF THE UNIVERSE
Galaxies and the Universe
Presentation transcript:

THE UNIVERSE OR DECREASING ACCELERATION IS THE EXPANSION RATE PRESENTED BY: JAKE DOTTS & JESS MYERS

NEWTON’S CONTRIBUTIONS For a long time, it has been widely accepted that the universe is expanding. Isaac Newton claimed that every object was attracted to each other because of the law of gravity — yet if this were the case, everything in the universe would collide with one another. ISAAC NEWTON

EINSTEIN’S CONTRIBUTIONS ALBERT EINSTEIN Einstein figured out that gravity is due to the curvature of space time, and he applied this theory to cosmology (the study of the origin and development of the universe). This created a dynamic equation correlating the reaction of gravity with that of the curvature of the universe. However, he made a great error in thinking that the universe was static — that is, that it was unchanging in its entirety.

SLIPHER’S CONTRIBUTIONS VESTO SLIPHER However, between 1912 and 1922, Vesto Slipher made an important discovery: the wavelengths of light spectra are systematically redshifting. This means that the light from objects shifts to longer wavelengths, allowing for the measurement of distance between the observer and the object due to Einstein’s equations involving gravity.

HUBBLE’S CONTRIBUTIONS EDWIN HUBBLE Lastly, in 1929 Hubble figured out that the redshift of an object correlates directly with an increasing linear function — that is, distance between objects seemed to be increasing. The universe was currently expanding. However, the notion was that this expansion was not increasing, but rather decreasing — indeed the universe was still getting bigger, but less and less with time.

PRESENT PIONEERS In 2011, the Nobel Prize in Physics was divided amongst three scientists: Saul Perlmutter receiving half of the awards credit, while Brian P. Schmidt, and Adam G. Riess split the remained. The award was received for their discovery of proof that the universe is not only expanding, but is indeed accelerating positively in size. SAUL PERLMUTTER BRIAN P. SCHMIDTADAM G. REISS

In Einstein’s equation relating gravity to the curvature of spacetime, two more crucial components were added: one of pressure, and one of density. This negative gravitational pressure causes things to repel from one another, while the density (if high enough) would cause things to attract one another. EINSTEIN’S MISSING LINK ALBERT EINSTEIN

The Nobel-winning scientists were on a mission to figure out whether or not the energy density of the universe was increasing, and thus continuing to expand space, or whether it was decreasing, and would lead to an eventual collapse in the future. They measured this by studying the redshift of distant stars, which can chart out a map of the history of the universe’s expansion. Upon doing this, they discovered that the universe was not expanding at a decelerating rate, but rather that it was accelerating exponentially with the passing of time. MAP OF OUR UNIVERSE’S REDSHIFT PATTERNS REDSHIFT MAPPING

In addition, they discovered that the density factor was reliant on something known as dark energy — this is the stuff in space that is dark in color, and has an energy because it has a pressure; this is the “nothingness” that one often thinks of, the total blackness surrounding galaxies and points of light. Because this energy fills in the gaps left by the expanding universe, it continues to be a constant fixture in space — and thus allows the universe to expand outward at an ever- increasing rate. DARK ENERGY OUR DARK UNIVERSE

The discovery that the universe is constantly accelerating does not have any immediate impacts. However, it brings up one very crucial and important realization: there is no time in the relatively near future, or perhaps ever, when the universe will buckle in on itself. If this were to happen the universe would become a dimensionless singularity. This process if referred to as the Big Crunch. IMPACT OF DISCOVERY THE BIG CRUNCH

INCREASING ACCELERATION Before, when the universe was thought to be slowly decelerating, the idea of a collapsing universe was very real and had to be dealt with. Now, there is no such fear — the dark energy continues to be a constant within the realms of space, and as a result, the curvature of space time is constant. The universe will continue to get larger and more expansive, doubling every 10 billion years. OUR UNIVERSE