Space, Time and Einstein Penelope Constanta Fermilab 1.

Slides:



Advertisements
Similar presentations
Space, Time and Einstein
Advertisements

The Big Bang Theory. Time begins The universe begins ~13.7 Billion years ago The universe begins as the size of a single atom The universe began as a.
Mr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path.
The Big Bang Theory Unit: Space Birth of a Theory Hypothesis: Educated Guess. Theory: Hypothesis that’s supported by consistent results & experimentation.
Chapter 18: Relativity and Black Holes
9.2 The Universe Homework: page 376 # 2, 3, 5, 6.
Space, Time and Dr. Einstein 1 Spacetime and Einstein 1905: Clerk in Patent Office Grand Old Man! Schoolboy.
Origin & Evolution of the 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.
Galaxies and the Universe
Galileo, Newton and the Birth of Astrophysics
Earth Science 25.3 The Universe
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.
Einstein, String Theory, and the Future Jonathan Feng University of California, Irvine Einstein: A Century of Relativity Skirball Cultural Center, Los.
GRAVITY.
Hubble Diagram: Distribution of Galaxies. Hubble’s Law: v = H o d Velocity increases with distance.
Origin of the Universe Big Bang Theory.
Astronomers, Theories, and Galaxies!
Please explain on your note card how this picture explains the Doppler Effect and how it relates to “Shifts in light”.
Unit 06 “Circular Motion, Gravitation and Black Holes” “Gravitation and Black Holes”
Hubble’s Law Our goals for learning What is Hubble’s Law?
Special and General Relativity Marcus Han 3O3 (!0)
Astronomy Part 1 General Science I Spring ‘09. History of the Universe Earth = 1 of 9 planets Sun= 1 of 100 billion stars in the Milky Way, 1 of infinite.
OGT: Chapter Eight  Origins Of The Universe. Astronomy  Study of stars and planets Aristotle  Earth is center of the universe (geocentric). Sun, planets.
Ch.18.1 Astronomy: The Original Science! P.554 1) Please take a copy of this unit standards and glue it in your IAN. 2)Next, copy down today’s lesson title.
Special Relativity Chapters 15 and 16.
Chapter 13 Black Holes. What do you think? Are black holes just holes in space? What is at the surface of a black hole? What power or force enables black.
Special Theory of Relativity Space and Time. Inertial reference frames Reference frames in which Newton’s first law is valid. –In other words, a reference.
Gravity, Energy, and Light Einstein and Newton 1.
Galileo, Newton and the Birth of Astrophysics
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.
Black Holes Formation Spacetime Curved spacetime Event horizon Seeing black holes Demo: 1L Gravity Well - Black Hole.
Hubble’s Observations - Edwin Hubble, in the late 1920's, discovered that all galaxies are moving away from each other as he observed the red shift in.
Astro-2: History of the Universe Lecture 3; April
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.
Astronomy 1143 – Spring 2014 Lecture 18: Special Relativity.
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”
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.
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.
Movement. Doppler Effect the apparent change in wavelength of light that occurs when the object is moving toward or away from the Earth. Using the spectroscope,
Gravity – A Familiar Force. Gravitational Force Gravitational force – an attractive force that every object in the universe exerts on every other object.
Monday, November Warm-Up: Grade Content Frame 2. Astronomy Intro.
Gravity, Energy, and Light Einstein and Newton 1.
THE BIG BANG THEORY The Expanding Universe. Review Human demonstration.
Einstein’s relativity Y&feature=relatedhttp:// Y&feature=related Did Newton's.
General Relativity and Grade-9 Astronomy. 0) Gravity causes time to slow down. Everyday Einstein: The GPS and Relativity OAPT Conference May 12 – 14 McMaster.
STATES THAT THE UNIVERSE BEGAN AS A SINGLE COSMIC EXPLOSION ABOUT 15 BILLION YEARS AGO. THE BIG BANG THEORY.
The UniverseSection 3 Section 3: Origin of the Universe Preview Key Ideas Bellringer What Is the Universe? What Happened at the Beginning? Predicting the.
Study Notes for Chapter 30: Stars, Galaxies, and the Universe.
WHEN YOU WISH UPON A STAR. Spectral lines of elements are unique to each element No other element has these exact spectral lines.
The Expanding Universe  When light or sound moves toward or away from an observer, its frequency/wavelength changes (Known as Doppler effect)  Can be.
Catalyst Pick up a note sheet. Pick up 1 piece of colored paper. Put “Unit 1 Astronomy” on the front of the colored paper. SIT SILENTLY IN YOUR SEAT.
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 Scientific explanation for the forming of the universe.
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.
The Big Bang Theory Origin of the Universe.
The Big Bang Theory.
The Motion of the Universe. What Keeps Celestial Bodies in Orbit?  The First Person to attempt to answer this question was Isaac Newton  Formulated.
Galaxies and the Universe
Galaxies and the Universe
The Universe Chapter 25.3.
WHEN YOU WISH UPON A STAR
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 history of Astronomy!.
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.
Science Notes: Stnd 14 Date Standard 14: 8.ESS1.1 The Big Bang
THE UNIVERSE Part 2:Cosmology.
FORMATION OF THE UNIVERSE
Presentation transcript:

Space, Time and Einstein Penelope Constanta Fermilab 1

Chicago (~40 miles) 2 Still Middle School (~7.5 miles)

Why space and time?  Related to our work at Fermilab  Hopefully related to things you’re learning in school Physics and astronomy, but also chemistry  Some really interesting questions about the world Where do things happen? In space … When do things happen? In time … 3

Why Einstein?  Because … he was Einstein!  Widely regarded as one of the most influential and best known scientists and intellectuals in modern history. Often regarded as the father of modern physics 1905: Clerk in Patent Office At older age! School boy 4

What did Einstein do?  Many, many discoveries. Easily could have won 3-4 Nobel prizes. Won only one for the discovery of the law of the photoelectric effect. He was a really smart man!  I will talk today about his two theories of relativity (Special Relativity and General Relativity) E=mc 2 (special relativity) Black holes (general relativity) 5

Space and Time  Space This piece of paper is 8 inches long It is 1.5 miles from the school to the store  Time I have to get up at 7 am The bus is 20 minutes late  But … What do we mean by distance (such as 1.5 miles)? What do we mean by a time (such as 7 am)? 6

Space and Time for Aristotle  The “prime mover” A privileged being in THE state of perpetual, absolute rest  Space Defined by (x, y, z) coordinate system with respect to the prime mover Unique and clearly defined  Time Time is measured by the prime mover’s clocks Aristotle ( BC) 7

Space for Galileo  No such things as “absolute rest”  The laws of nature and physics are identical for anybody moving with a constant speed along a straight line Galileo Galilei ( ) 8

Space for Sir Isaac Newton  “Absolute Space, in its own nature, without regard to any thing external, remains always similar and immovable. Relative Space is some moveable dimension or measure of the absolute spaces; which our senses determine, by its position to bodies; and which is vulgarly taken for immovable space... And so instead of absolute places and motions, we use relative ones” There exists absolute space, but we measure space only relative to other objects in space Isaac Newton ( ) 9

Time for Sir Isaac Newton  “ Absolute, True, and Mathematical Time … flows equably without regard to any thing external … Relative, Apparent, and Common Time is some sensible and external (whether accurate or unequal) measure of Duration by the means of motion, which is commonly used instead of True time; such as an Hour, a Day, a Month, a Year. ” There exists an absolute time, but we measure relative time only Isaac Newton ( ) 10

Einstein’s genius Change the definition of time: “It might appear possible to overcome all the difficulties attending the definition of ‘time’ by substituting ‘the position of the small hand of my watch’ for ‘time’ ”. Example: By “ ‘That train arrives here at 7 o’clock,’ I mean something like this: ‘The pointing of the small hand of my watch to 7 and the arrival of the train are simultaneous events’ ” - famous 1905 Einstein paper 11

So what? 12 Jack sees the flashes at clocks A and B to be simultaneous events Jack John What does John see?

Jack John But … Simultaneity is relative - things occurring at the same time at one place may occur at different times in another place! 13 John sees the two light signals arrive at the moving midpoint at the same moment. But he sees the flash at the A clock happened earlier, (giving the signal from the A clock more time to cover the greater distance) and the flash at the B clock happened later (as it needed less time to cover the distance to moving midpoint).

How do we see moving things? Relativity of distance! Moving sign appears to be shorter! 14 Moving at 10% of speed of light Moving at 99% of speed of light

How do we measure time? Imagine a clock that measures time by how long it takes light to bounce back and forth … Relativity of distance -> relativity of time! c=speed of light 15

Putting it all together  The only way we can measure time and distance is by sending signals Time and distance are relative  The fastest signal travels at the speed of light Nothing can travel faster than light  Moving objects appear smaller and slower in space But the effect is really small for everyday movement  A result of the theory of special relativity: E=mc 2 16

Fermilab Protons traveling % speed of light Anti-protons traveling % speed of light 4 miles The protons: Seem 1000 times thinner Have clocks that run 1000 times slower 17

What about the other definition of space (all the stuff up in the sky and in the universe?) 18

Einstein’s General Relativity  We already know that space and time are intertwined  Gravity is a distortion of space and time itself Moon orbiting the earthAsteroid pulled into earth 19

Even light is bent by gravity! The position of a star observed during an eclipse confirmed Einstein’s theory 20

Black holes Dying stars can become black holes - gravity to an extreme! At some point, even light cannot escape! So named as “black holes” because you cannot see them … but you can see stuff around them 21

Black hole evidence Hubble telescope observing a disk of dust orbiting around a black hole! 22

(Object moving away) Relative motion in the Universe Red shift (Object moving away) Blue shift 23

24 Doppler Effect

25 Red and Blue Shift

The Universe is expanding! A small view from the Hubble Space Telescope. Each blob is a galaxy with 100,000,000,000 stars! The stars are all moving away from us, and away from one another The Big Bang: The Universe was really tiny at its birth 13.5 billion years ago 26

Summary  Space and time are relative  Moving things look shorter and move slower  Space-time is bent by matter  Light is bent by matter  Red shift and Blue shift of light is used to detect relative motion in the universe  The present universe is expanding  If you want to learn more about the universe, Einstein or smashing protons and anti-protons together … 27

Fermilab  Come visit Fermilab!  Lots of fun science demos at the lab’s Lederman Science Center  Walk the prairies  See the lab’s bison  Come for ask-a- scientist  28