Science 3210 001 : Introduction to Astronomy Lecture 10 : Relativity, Black Holes Robert Fisher Items ❑ Nathan Hearn guest lecture on dark matter on April 20th. Lunch in the loop (on me) with Nathan following the lecture at Frontera Fresco for anyone who wants to join us. ❑ Second midterm next week. Covers the material in between the last midterm and the end of today’s lecture. ❑ Adler Planetarium field trip on May 4th - $16/person. Sign up today!! ❑ Final projects due May 11th, along with a short (5 minute) presentation that day. Final Project ❑ Your final project is to construct a creative interpretation a scientific theme we encountered during the class. You will present your work in a five minute presentation in front of the entire class on May 11. ❑ The project must have both a scientific component and a creative one. ❑ For instance, a Jackson Pollock-lookalike painting would fly, but ONLY if you said that it was your interpretation of the big bang cosmological model AND you could also demonstrate mastery of the basic astrophysics of the big bang while presenting your work. ❑ Be prepared to be grilled! ❑ Ideas : ❑ Mount your camera on a tripod and shoot star trails. ❑ Create a “harmony of the worlds” soundtrack for the Upsilon Andromeda system. ❑ Paint the night sky as viewed from an observer about to fall behind the horizon of a black hole. ❑ Write a short science fiction story about the discovery of intelligent life in the universe. Review of Three Weeks Ago ❑ Extrasolar planets ❑ 51b Peg ❑ HD209458b Review of Two Weeks Ago ❑ Interstellar Medium and Star Formation ❑ Binary Stars ❑ Star Clusters ❑ HR (Hertzsprung-Russell) Diagram of Stars Review of Last Week ❑ Stellar Structure ❑ Stellar Evolution ❑ Evolution of a low-mass star ❑ Evolution of a high-mass star ❑ Supernovae Today -- Relativity and Black Holes ❑ Special Relativity ❑ Michelson-Morley Experiment ❑ Introduction to Spacetime Physics ❑ Relativity of Simultaneity ❑ General Relativity ❑ Black Holes The Aether ❑ Late 19th century scientists attempting to make sense of the wavelike behavior of light argued that light must be a wave like other waves known at that time -- water waves, sound waves, seismic waves, and so on. ❑ The common opinion developed was that waves are the result of a mechanical disturbance in a physical medium -- for instance, water waves oscillate once a rock is dropped in a pond. ❑ By analogy, light must be the result of a disturbance in an undetected medium known as the aether (sometimes ether or luminiferous aether). ❑ If the aether did exist, it must carry physical properties like mass and momentum, just like a pond. If it has physical properties, it must be detectable. ❑ If that is all true, then where was all of the evidence for the existence of the aether ?? Michelson-Morley Experiment ❑ In 1887, physicists Michelson and Morley devised a brilliant method to detect the aether. ❑ To understand how their experiment worked, consider Alexis, who is standing on the shore watching Bettie, moving on a boat moving at a fixed speed through a river. ❑ When Bettie is moving downstream, the boat moves with a speed relative to Alexis which is the sum of the boat speed and the water speed. Bettie Michelson-Morley Experiment ❑ When Bettie is moving upstream, the boat moves with a speed relative to Alexis which is the difference of the boat speed and the water speed. ❑ Even if Alexis observed only the motion of the boat in both directions, she could easily infer both the direction and speed of the water current. ❑ By analogy, Michelson and Morley hoped to measure the difference in the speed of light as it moved relative to the aether, and from that knowledge, both establish the existence of the aether and also its direction of motion and speed. Bettie Michelson-Morley Experiment ❑ Believing that the speed of light relative to the Earth must vary as the Earth moves through the aether, physicists Michelson and Morley planned a highly-sensitive experiment to measure this effect. Light Light Moves Moves Slower Faster Michelson-Morley Video Classical Space and Classical Time ❑ Classical physics prior to Einstein considered motion taking place upon a fixed space and a universal time. ❑ Space is the stage where all action takes place. Everyone always agrees upon distances measured on the stage -- it is absolute and unchanging. ❑ Time is a universal concept as well. Everyone’s clock always precisely agrees with everyone else’s clock. Spacetime ❑ One of the key ideas in relativity theory is that space and time are dramatically different from the classical viewpoint. ❑ The concepts which Einstein hit upon are radically different than both the classical point of view, and our own everyday experience. ❑ Because relativity is so radically different from our everyday experience, Einstein had proceed using razor-sharp logic, starting from basic axioms. ❑ This reasoning was often applied to extraordinary situations known as thought experiments (sometimes gedankenexperiment from the German). A Short Note on Historical Attributions Einstein & Lorentz ❑ The popular conception is that the theory of relativity was nearly single- handedly created by Einstein. While largely true, it is far from the entire story. ❑ Early ideas remarkably similar to Einstein’s were espoused by Karl Friedrich Gauss and Behrnard Riemann. ❑ Key contributions to the theory were made by several other scientists, including George Francis Fitzgerald, Hendrik Lorentz, and Henre Poincare. A Short Note on Historical Attributions ❑ “Whoever speaks of absolute space uses a word devoid of meaning. This is a truth Henri Poincare that has been long proclaimed by all who have reflected on the question, but one which we are too often inclined to forget… have shown elsewhere what are the consequences of these facts from the point of view of the idea that we should construct non-Euclidean and other analogous geometries.” -- Henri Poincare, Science and Method, 1897 ❑ Recently more controversial suggestions have been made that Einstein’s first wife Mileva Maric contributed substantially to the relativity, and even that other scientists came upon E = m c2 independently. ❑ What remains true is that the whole of relativity theory owes more to one single individual more than any other major theory in modern physics. Einstein ❑ A large part of the Einstein myth are the circumstances in which his first papers were published. ❑ In 1905, while publishing his “miracle year” papers on relativity and other subjects, Einstein was employed as a clerk (third class) at the Swiss patent office in Zurich. ❑ He remained a clerk in the office well afterwards -- until he was appointed “Extraordinary Professor of Physics” at the University of Zurich -- in 1909. Spacetime Preliminaries ❑ In building a conception of how space and time work, it is first crucial to define what we mean by such basic concepts as ‘space’, ‘time’, ‘event’, and ‘simultaneity’. ❑ The elementary building block in this framework is the event. ❑ An event defines a single point in space and time. ❑ For our thought experiments, we can imagine that events are defined by flashes of light which move spherically outwards from their sources -- for instance, as set off by an electronic light source. The Building Block of Spacetime -- The Event ❑ An event has no duration or spatial extent -- it is a single point in space and in time. ❑ A distant observer will note the event when the light from the event first reaches him or her. ❑ It is important to note that the light flash itself at the source and the event of detection are two distinct events. Spacetime Preliminaries -- Measuring Time ❑ Fundamental to this picture is that spacetime is filled with hypothetical observers who can conduct observations and measurements on their own. ❑ Each observer carries with him or her a clock (which we will describe in detail later) to measure elapsed time. ❑ Using the pulses of light from events, and his or her clock, each observer can measure time intervals between events. Spacetime Preliminaries -- Measuring Distance ❑ Using events, light pulses, and clocks, observers can also measure distances between spacetime events. ❑ Consider, for instance, measuring the distance between yourself and the wall of a room. You send a light pulse out, which defines event A. A mirror hanging on the wall reflects the light pulse, which returns to you at event B. ❑ The distance between you and the wall is easily determined from d = c t -- the speed of light times the elapsed time, divided by two (to account for there and back again). Mirror B A An Important Word of Caution About Spacetime Misconceptions ❑ Most students have common hangups when first learning relativity. ❑ In one hangup, some students do not see any immediate flaw in the logic, and so accept the basic logic and conclusions of the theory. ❑ However, the conclusions are simply too “weird” to fully accept, so they come to believe that because the conclusions are based on measurements made by observers, relativity is actually an illusionary trick played on their instruments. The “real world” behaves differently. ❑ This misses one of the key logical premises of the theory -- that we know of space and time only through our measurements. Any presumed “real world” outside of our measurements cannot be verified by any experiment and so does not exist. ❑ This viewpoint is further refuted by the fact that relativity has real, observable consequences -- sometimes startling. We will discuss some of these later. Spacetime Diagram ❑ A key tool used to understand how spacetime works is the spacetime diagram. ❑ In this diagram, only one spatial dimension is plotted along one axis. The other two spatial dimensions are suppressed. ❑ Along the second axis, time is plotted. time space Question ❑ Which of the following figures represents the spacetime motion of a body (shown in red) at rest? time time space space Question ❑ Which of the following figures represents the spacetime motion of a body (shown in red) moving at constant speed? time time space space Spacetime Diagram of a Pulse of Light ❑ Imagine that an observer sets off a pulse of light at the origin of our spacetime diagram, O.