Law of gravitation Kepler’s laws Energy in planetary motion Atomic spectra and the Bohr model Orbital motion (chapter eleven)

Slides:



Advertisements
Similar presentations
UNIT 6 (end of mechanics) Universal Gravitation & SHM
Advertisements

Review Chap. 12 Gravitation
The Beginning of Modern Astronomy
Chapter 9 & 10 Gravity Pythagoras (550 BC) n Claimed that natural phenomena could be described by mathematics.
Chapter 8 Gravity.
Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
18-1 Physics I Class 18 Newton’s Theory of Gravitation.
D. Roberts PHYS 121 University of Maryland Physic² 121: Phundament°ls of Phy²ics I November 6, 2006.
Physics 151: Lecture 28 Today’s Agenda
Gravitation Newton’s Law of Gravitation; Kepler’s Laws of Planetary Motion. Lecture 14 Monday: 1 March 2004.
Quantum Physics. Black Body Radiation Intensity of blackbody radiation Classical Rayleigh-Jeans law for radiation emission Planck’s expression h =
Physics 111: Mechanics Lecture 13 Dale Gary NJIT Physics Department.
Chapter 13 Gravitation.
2006: Assoc. Prof. R. J. Reeves Gravitation 3.1 P113 Gravitation: Lecture 3 Escape speed from orbit Planets and satellites: Keplers Laws Orbital energy.
Chapter 12 Gravitation. Theories of Gravity Newton’s Einstein’s.
CH 12: Gravitation. We have used the gravitational acceleration of an object to determine the weight of that object relative to the Earth. Where does.
Newton’s Theory of Gravity and Planetary Motion
Sect. 13.3: Kepler’s Laws & Planetary Motion. German astronomer (1571 – 1630) Spent most of his career tediously analyzing huge amounts of observational.
Physics 111: Mechanics Lecture 13
Universal Gravitation
Monday, Nov. 25, 2002PHYS , Fall 2002 Dr. Jaehoon Yu 1 PHYS 1443 – Section 003 Lecture #20 Monday, Nov. 25, 2002 Dr. Jaehoon Yu 1.Simple Harmonic.
-Energy Considerations in Satellite and Planetary Motion -Escape Velocity -Black Holes AP Physics C Mrs. Coyle.
Planetary Dynamics § 13.4–13.8. Closed Orbits U g + K tr = constant < 0 The closer the satellite is to the main body, the faster it moves Objects do not.
Physics 201: Lecture 24, Pg 1 Chapter 13 The beautiful rings of Saturn consist of countless centimeter-sized ice crystals, all orbiting the planet under.
Gravitation Part II One of the very first telescopic observations ever was Galileo’s discovery of moons orbiting Jupiter. Here two moons are visible,
Physics 215 – Fall 2014Lecture Welcome back to Physics 215 Today’s agenda: Newtonian gravity Planetary orbits Gravitational Potential Energy.
Chapter 13 Universal Gravitation. Newton’s Law of Universal Gravitation Every particle in the Universe attracts every other particle with a force that.
Physics 221 Chapter 13 Is there gravity on Mars? Newton's Law of Universal Gravitation F = GmM/r 2 Compare with F = mg so g = GM/r 2 g depends inversely.
Chapter 13 Gravitation. Newton’s law of gravitation Any two (or more) massive bodies attract each other Gravitational force (Newton's law of gravitation)
Monday, Oct. 4, 2004PHYS , Fall 2004 Dr. Jaehoon Yu 1 1.Newton’s Law of Universal Gravitation 2.Kepler’s Laws 3.Motion in Accelerated Frames PHYS.
Gravitation. Gravitational Force and Field Newton proposed that a force of attraction exists between any two masses. This force law applies to point masses.
Chapter 12 Universal Law of Gravity
Chapter 13 Universal Gravitation. Newton’s Law of Universal Gravitation Every particle in the Universe attracts every other particle with a force that.
Chapter 11 Gravity, Planetary Orbits, and the Hydrogen Atom.
Gravity, Planetary Orbits, and the Hydrogen Atom
Monday, Oct. 6, 2003PHYS , Fall 2003 Dr. Jaehoon Yu 1 PHYS 1443 – Section 003 Lecture #11 Newton’s Law of Gravitation Kepler’s Laws Work Done by.
Newton’s Law of Universal Gravitation
Monday, June 11, 2007PHYS , Summer 2007 Dr. Jaehoon Yu 1 PHYS 1443 – Section 001 Lecture #8 Monday, June 11, 2007 Dr. Jaehoon Yu Forces in Non-uniform.
17-1 Physics I Class 17 Newton’s Theory of Gravitation.
28.3 THE BOHR THEORY OF HYDROGEN At the beginning of the 20th century, scientists were puzzled by the failure of classical physics to explain the characteristics.
Chapter 28:Atomic Physics
Chapter 6 - Gravitation Newton’s Law of Gravitation (1687)
Chapter 13 Gravitation Newton’s Law of Gravitation Here m 1 and m 2 are the masses of the particles, r is the distance between them, and G is the.
Chapter 13 Gravitation.
Wednesday, Mar. 3, PHYS , Spring 2004 Dr. Andrew Brandt PHYS 1443 – Section 501 Lecture #12 Newton’s Law of Gravitation and Kepler’s Laws.
Spring 2002 Lecture #21 Dr. Jaehoon Yu 1.Kepler’s Laws 2.The Law of Gravity & The Motion of Planets 3.The Gravitational Field 4.Gravitational.
Gravitation. Flat Earth This is true for a flat earth assumption. Is the earth flat? What evidence is there that it is not? Up to now we have parameterized.
1 2. Atoms and Electrons How to describe a new physical phenomenon? New natural phenomenon Previously existing theory Not explained Explained New theoryPredicts.
Kepler’s Laws & Planetary Motion
Wednesday, Oct. 10, 2007 PHYS , Fall 2007 Dr. Jaehoon Yu 1 PHYS 1443 – Section 002 Lecture #11 Wednesday, Oct. 10, 2007 Dr. Jaehoon Yu Free Fall.
Ch2 Bohr’s atomic model Four puzzles –Blackbody radiation –The photoelectric effect –Compton effect –Atomic spectra Balmer formula Bohr’s model Frank-Hertz.
Chapter 13 Gravitation & 13.3 Newton and the Law of Universal Gravitation Newton was an English Scientist He wanted to explain why Kepler’s Laws.
1 The law of gravitation can be written in a vector notation (9.1) Although this law applies strictly to particles, it can be also used to real bodies.
Satellite Motion Satellite – a projectile moving fast enough to fall continually around the Earth rather than into it - the Earth surface drops a vertical.
1 Chapter 11 Gravity, Planetary Orbits, and the Hydrogen Atom.
The Atomic Models of Thomson and Rutherford Rutherford Scattering The Classic Atomic Model The Bohr Model of the Hydrogen Atom Successes & Failures of.
Basic Mechanics. Units Velocity and Acceleration Speed: Time rate of change of position. Velocity: Speed in a specific direction. Velocity is specified.
Physics 141Mechanics Lecture 18 Kepler's Laws of Planetary Motion Yongli Gao The motion of stars and planets has drawn people's imagination since the.
Newton’s Law of Universal Gravitation by Daniel Silver AP Physics C
College Physics, 7th Edition
College Physics, 6th Edition
Chapter 13 Gravitation.
Chapter 12 Gravity.
Chapter 9: Gravity Gravity is the force most familiar to us, and yet, is the least understood of all the fundamental forces of nature.
General Physics (PHY 2140) Lecture 33 Modern Physics Atomic Physics
Chapter 13 Universal Gravitation
Chapter 13 Gravitation.
Universal Gravitation
9. Gravitation 9.1. Newton’s law of gravitation
Gravitational Fields, Circular Orbits and Kepler
Presentation transcript:

Law of gravitation Kepler’s laws Energy in planetary motion Atomic spectra and the Bohr model Orbital motion (chapter eleven)

Newton’s law of universal gravitation, revisited Newton postulated an inverse square law for the gravitational force between any two masses He also showed that the gravitational force exerted by a sphere is equal to that of a point mass at the center, equal to the enclosed mass only.

Gravitational force Example: satellites Speed is independent of mass – depends only on radius (height) of orbit.

Structural models Models that describe a system which generally cannot be altered by humans. Often contains the following features: Physical components Location of components Time evolution Agreement between predictions and observations, and even predictions of not-yet- observed phenomena

Kepler’s laws First law: Each planet moves in an elliptical orbit a b F 1, F 2 : foci a: semimajor axis b: semiminor axis e=c/a: eccentricity r2r2 r1r1 F1F1 F2F2 c eccentricity of Earth’s orbit = 0.017, Pluto’s orbit = 0.25 Ellipses: only types of bound orbits for inverse square force

Kepler’s laws Second law: The radius vector from the sun to any planet sweeps out equal area in equal time intervals. Since the force is directed along the line between the two masses, the cross product is identically zero Therefore, the angular momentum of the planet is constant

Kepler’s laws Second law dA Using this result to find the area swept out as a function of time drdr Integrating this gives the same result for identical time intervals

Kepler’s laws Third law The square of the orbital period is proportional to the cube of the semimajor axis of the orbit Easiest to demonstrate with circular orbits: For an elliptical orbit with semimajor axis a

Energy in planetary motion The sum of the kinetic and potential energies of a mass in the gravitational field of a much larger mass is The potential is defined for the case of U g  0 as r . In principle, we can add any constant to it and it will still be valid, since only the change in energy is important. We can use Newton’s 2 nd law to find one other relation

Energy in planetary motion So the total energy is just For elliptical orbits, r  a

Escape speed An object with some speed at the surface of the earth may have enough energy to escape the earth’s gravitational potential. First, suing conservation of energy, consider the maximum height a mass with speed v could reach This gives a general relation for the speed needed to reach a height r max :

Escape speed Setting r max to infinity defines the escape speed of an object Independent of both the direction of v and the mass of the object. Earth: v esc = 11.2 km/s Moon: v esc = 2.3 km/s

Black holes If the escape speed of a mass equals the speed of light – even electromagnetic radiation can’t escape – this is a “black hole”

Atomic spectra and the Bohr theory of hydrogen Emission spectra of gases led Bohr to the conclusion that electrons exist in discrete orbits around nuclei Demo Hydrogen Helium Xenon

Atomic spectra and the Bohr theory of hydrogen The spectra exhibit narrow wavelengths of emission, which follow an empirical rule (for hydrogen) where R H is a constant (Rydberg constant) This dependence, and the discrete nature of the lines, cannot be explained with classical physics

Atomic spectra and the Bohr theory of hydrogen Bohr postulated a model that accounts for the observed phenomena. It’s assumptions are: 1.Electrons in circular orbits 2.Only certain orbits are stable 3.Electrons “jumping” between states conserves energy by absorbing or emitting radiation, with frequency proportional to the energy difference of the levels 4.The angular momentum of the orbits is quantized h=Planck’s constant =6.63  Js

Atomic spectra and the Bohr theory of hydrogen Electric potential energy due to positive charge of the nucleus In the same way as we calculated the total energy for planetary motion, we find

Atomic spectra and the Bohr theory of hydrogen Now solving the the expression for the quantization of the angular momentum for v, and setting these two equations equal yields From Newton’s 2 nd law n=1 defines the “Bohr radius”

Atomic spectra and the Bohr theory of hydrogen Using this to calculate energy differences between levels and the frequency of light corresponding to that energy, we find a general formula Quantized radii imply quantized energies: