Sergei Kopeikin Department of Physics and Astronomy,

Slides:



Advertisements
Similar presentations
S PEED OF G RAVITY by Robert Nemiroff Michigan Tech.
Advertisements

March , Birmingham GR tests and micro-arcsecond light bending parameters by global and differential Gaia mesurements Maria Teresa Crosta Astronomical.
How to Study the Universe
Early Astronomers & Planetary Motion
Extragalactic Astronomy & Cosmology First-Half Review [4246] Physics 316.
Binary stellar systems are interesting to study for many reasons. For example, most stars are members of binary systems, and so studies of binary systems.
Chapitre 3- Astrometry PHY6795O – Chapitres Choisis en Astrophysique Naines Brunes et Exoplanètes.
1-я школа по астрометрии, Москва, Октябрь 22-26, Практические приложения фундаментальной теории Д.ф.-м.н. Сергей М. Копейкин Университет штата Миссури,
Please turn off cell phones - thanks! panda.unm.edu/courses/sanfratello/sp09/astro101 Remember - Read syllabus and schedule (contains textbook reading.
General Relativity Physics Honours 2006 A/Prof. Geraint F. Lewis Rm 557, A29 Lecture Notes 5.
Finding Useful Information ON THE WEB. Published papers Most published papers in astronomy can be found on the NASA Astrophysics Data System: Most published.
Spacetime astrometry and gravitational experiments in the solar system Sergei Kopeikin University of Missouri October 14, 2014 Colloquium at the University.
General-Relativistic Effects in Astrometry S.A.Klioner, M.H.Soffel Lohrmann Observatory, Dresden Technical University 2005 Michelson Summer Workshop, Pasadena,
JOVIAN and SOLAR RADIO DEFLECTION EXPERIMENTS Ed Fomalont National Radio Astronomy Observatory Charlottesville, VA USA Sergei Kopeikin University of Missouri.
Gravity & orbits. Isaac Newton ( ) developed a mathematical model of Gravity which predicted the elliptical orbits proposed by Kepler Semi-major.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 2.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Chapter 2.
Which scientist was the first to use the telescope in astronomy?
Physics 215 – Fall 2014Lecture Welcome back to Physics 215 Today’s agenda: Newtonian gravity Planetary orbits Gravitational Potential Energy.
Geodetic VLBI Lecture 2 18 October Lecture plan 1. From measurement of space and time to measurement of space-time 2. Elements of the Special and.
Gravity, Energy, and Light Einstein and Newton 1.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Black Holes Escape velocity Event horizon Black hole parameters Falling into a black hole.
THE UNIVERSE IS FULL OF MAGICAL THINGS PATIENTLY WATING FOR OUR WITS TO GROW SHARPER. - Eden Phillpotts-
FAMOUS ASTRONOMERS  The name "planet" comes from the Greek term π λανήτης (plan ē t ē s), meaning "wanderer".  Came up with geocentric (earth center)
investigated the nature of light, discovering that sunlight is made of light of different colors; the spectrum is, in order from long to short wavelength:
Gravitation. Gravitational Force and Field Newton proposed that a force of attraction exists between any two masses. This force law applies to point masses.
Crash Course of Relativistic Astrometry Four Dimensional Spacetime Poincare Transformation Time Dilatation Wavelength Shift Gravitational Deflection of.
Fundamental Principles of General Relativity  general principle: laws of physics must be the same for all observers (accelerated or not)  general covariance:
Copyright © 2012 Pearson Education, Inc. How do we detect planets around other stars?
Chapter 4 Gravitation and the Waltz of the Planets The important concepts of Chapter 4 pertain to orbital motion of two (or more) bodies, central forces,
Chapter 1: The Copernican Revolution. The Motions of the Planets The Birth of Modern Astronomy The Laws of Planetary Motion Newton’s Laws Summary of Chapter.
FAMOUS ASTRONOMERS  Believed in geocentric universe  earth was the center  used circular orbits with epicycles  was supported by the church for.
Astronomy Final Review. Geocentric Model --Earth is in the center of the system and everything revolves around it.
H8: Evidence for general relativity
Binary stellar systems are interesting to study for many reasons. For example, most stars are members of binary systems, and so studies of binary systems.
Binary stellar systems are interesting to study for many reasons
Gravity, Energy, and Light Einstein and Newton 1.
Time Delay and Light Deflection by a Moving Body Surrounded by a Refractive Medium Adrian Corman and Sergei Kopeikin Department of Physics and Astronomy.
The quest for Gravitation Waves By Benjamin Thayer.
Celestial Mechanics I Introduction Kepler’s Laws.
The Motion of the Universe. What Keeps Celestial Bodies in Orbit?  The First Person to attempt to answer this question was Isaac Newton  Formulated.
Special Relativity without time dilation and length contraction 1 Osvaldo Domann
PHYS 155 – Introductory Astronomy observing sessions: - observing sessions: Sunday – Thursday, 9pm, weather permitting
THE UNIVERSE IS FULL OF MAGICAL THINGS PATIENTLY WATING FOR OUR WITS TO GROW SHARPER. - Eden Phillpotts-
CHAPTER 2: Gravitation and the Waltz of the Planets.
© 2017 Pearson Education, Inc.
Chapter 10: Other Planetary Systems: The New Science of Distant Worlds
The Science of Orbits (Power Point 04) Image Credit: NASA.
Einstein’s Universe Dr Martin Hendry Dept of Physics and Astronomy,
Einstein’s Tests of General Relativity through the Eyes of Newton
Lecture 19 Relativity Chapter 26.1  26.5 Outline
Experimental tests of the no-hair theorems of black holes
Parameterized Newtonian Theory
Exoplanets: The New Science of Distant Worlds
Relativity H7: General relativity.
Jupiter Light-Deflection Experiment and Its Results
Dark Matter, Dark Energy And The Fate Of The Universe
Review for exam1.
Special Relativity Jeffrey Eldred
Lecture 22 Special theory of relativity
PHYS 1443 – Section 003 Lecture #11
Normal gravity field in relativistic geodesy
Lesson 2 Models of the Universe
Newton, Einstein, and Gravity
Black Holes Escape velocity Event horizon Black hole parameters
UNIT NINE: Matter and Motion in the Universe
PHYS 1443 – Section 001 Lecture #8
Presentation transcript:

Gravitational deflection of light:  What else can the Eddington experiment tell us about gravity? Sergei Kopeikin Department of Physics and Astronomy, University of Missouri-Columbia 08/21/2017 The Great American Solar Eclipse Physics Conference The Nature of Time

The Great American Solar Eclipse Physics Conference Shakura Grishchuk Kopeikin Zeldovich Petrov Ya. B. Zeldovich and the department of relativistic astrophysics in Moscow State University (May 1986) 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference Abstract. Standard textbook treatment of the Eddington experiment is given in a static reference frame. However, the observations of the solar eclipse are done from the Earth which moves around the Sun. Effectively, it allows to test the Lorentz-invariance of the gravitational interaction during the solar eclipse. We discuss the mathematical framework of the Eddington experiment from the point of view of a moving observer and the results of testing of the Lorentz-invariance of the gravitational interaction in VLBI experiments with the major planets of the solar system. 08/21/2017 The Great American Solar Eclipse Physics Conference The Nature of Time

The Eddington experiment in a static frame 4-Jun-18 Blue - the stellar positions from astrometric catalogue Red - the stellar positions deflected by the solar gravity field Center of mass of the Sun measured from the gravitational deflection of light 08/21/2017 The Great American Solar Eclipse Physics Conference

What has been never discussed earlier? The Eddington experiment is conducted in a moving frame! The observed positions of stars are shifted in the sky by stellar aberration due to the orbital motion of the Earth. The optical position of Sun is shifted in the sky by stellar aberration as well. How much and in what direction in the sky are shifted the positions of stars having been deflected by the solar gravity? 08/21/2017 The Great American Solar Eclipse Physics Conference

The Eddington experiment in a moving frame 4-Jun-18 Blue - the stellar positions from astrometric catalogue Red - the stellar positions deflected by the solar gravity field Yellow – the shift of the stellar position due to the aberration of light Center of mass of the Sun measured from the gravitational deflection of light Where is the center of mass of the Sun measured from the gravitational deflection of light in a moving frame ? The answer depends on the speed of gravity. ? ? ? ? 08/21/2017 The Great American Solar Eclipse Physics Conference

The Laplace retardation of gravity effect Newtonian theory (Laplace 1825; Van Flandern 1998): Planetary orbits are unstable if the gravity force propagates with finite speed. The finite speed of gravity brings about the aberration of gravity that leads to non-conservation of the orbital angular momentum. It is not observed. The speed of gravity is infinite.     In general relativity: 08/21/2017 The Great American Solar Eclipse Physics Conference

Gravitational Position of the Sun in the Eddington experiment 4-Jun-18 Gravitational Position of the Sun in the Eddington experiment   Position of the quasar deflected by the gravity force and shifted by the aberration of light. The speed of gravity is infinite. Gravitational position of the Sun measured in the geocentric frame in case when the speed of gravity is infinite. Position of the quasar shifted by the aberration of light only. Gravitational deflection of light is switched off. Gravitational position of the Sun measured in the geocentric frame in case when the speed of gravity equals the speed of light. The aberration of gravity angle measured from the Earth

The Aberration of Gravity and its Fundamental Speed 4-Jun-18 The Aberration of Gravity and its Fundamental Speed The aberration of gravity effect is derived from solving the triangles shown in the picture   Gravitational deflection of light  =      The angular impact parameter of the light ray  = d/r r – the distance ‘lens-observer’ d – the impact parameter of the light ray  

Abstract of my APJL paper 08/21/2017 The Great American Solar Eclipse Physics Conference

Linearized General Relativity 4-Jun-18 The Harmonic (Lorentz) gauge Linearized Einstein’s Gravity Field Equations The Great American Solar Eclipse Physics Conference 08/21/2017

The Liénard-Wiechert Retarded Gravitational Potentials 4-Jun-18 The Liénard-Wiechert Retarded Gravitational Potentials 08/21/2017 The Great American Solar Eclipse Physics Conference

The Light-ray Trajectory 08/21/2017 The Great American Solar Eclipse Physics Conference

The Retardation of Gravity Experiment 4-Jun-18 The retarded time due to the finite speed of gravity Lorentz invariant equation for the bending of light Lorentz invariant equation for the electromagnetic phase delay 08/21/2017 The Great American Solar Eclipse Physics Conference

The Minkowski diagram of the interaction of gravity and light Observer Star’s world line Future gravity null cone Observer Time Future gravity null cone Future gravity null cone Space Future gravity null cone Light null cone Future gravity null cone Light null cone Observer’s world line Planet’s world line 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference The speed of gravity and retardation of gravity in the light-ray deflection experiment Observer and planet are at rest Planet moves uniformly relative to observer 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference The speed of gravity experiment (Fomalont & Kopeikin, Astrophys. J., 598, 704, 2003) Position of Jupiter taken from the JPL ephemerides (radio/optics) 1 5 Position of Jupiter as determined from the gravitational deflection of light from a quasar 4 2 3 10 microarcseconds = the width of a typical strand of human hair from a distance of 650 miles. 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference With Ed Fomalont in Albuquerque, NM, June 2002 Picture is taken during my visit to VLA, Socorro, NM 08/21/2017 The Great American Solar Eclipse Physics Conference

08/21/2017

Limitations to Positional Accuracy University of Missouri-Columbia 6/4/2018 Limitations to Positional Accuracy Location of Radio Telescope Position on earth (1 cm) Earth Rotation and orientation (5 cm) Time synchronization (50 psec) Array stability (5 cm) Propagation in troposphere and ionosphere Very variable in time and space (5 cm in 10 min) CONVERSION FACTORS for astrometry: 1 cm = 30 psec = 300 microarcsec 0.03cm = 1 psec = 10 microarcsec Phase-referencing VLBI technique can achieve 10 microarcsec! 08/21/2017 The Great American Solar Eclipse Physics Conference Astrocon 2006, Princeton NJ

The Great American Solar Eclipse Physics Conference Gravitational bending of light by planetary multipoles and its measurement with microarcsecond astronomical interferometers (Kopeikin & Makarov, Phys. Rev. D75, Issue 6, id. 062002, March 15, 2007) Modeling Gravitational Field (Einstein’s theory) Modeling Propagation of Light (Maxwell’s theory) Solving Equations and Predicting the Light-Ray Deflection Patterns Discussing Fitting Parameters of the Model Interpreting Gravitational Physics 08/21/2017 The Great American Solar Eclipse Physics Conference

The deflection equations and the central inverse mapping Real ephemeris of the planet JPL ephemeris of the planet 08/21/2017 The Great American Solar Eclipse Physics Conference

Deflection patterns by gravitational multipoles Circle Cardioid the Caley’s sextic March 21, 1988 Treuhaft & Lowe DSN JPL NASA September 8, 2002 Fomalont & Kopeikin VLBA+Effelsberg 2020-2030 SKA, Gaia, Theia 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference Light-Deflection Experiment with Cassini and Saturn 2009 “Recent VLBA/VERA/IVS tests of general relativity” Fomalont, Kopeikin et al., IAU Symp. 261, 291-295, 2010 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference 08/21/2017 The Great American Solar Eclipse Physics Conference

The Great American Solar Eclipse Physics Conference Thank You ! Happy Birthday to Thom! May the sky be clear! 08/21/2017 The Great American Solar Eclipse Physics Conference