C - More Gravitation.

Slides:



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

UNIT 6 (end of mechanics) Universal Gravitation & SHM.
Chapter 13 Gravitation PhysicsI 2048.
The Beginning of Modern Astronomy
Chapter 8 Gravity.
Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
CHAPTER-13 Gravitation.
Physics 151: Lecture 28 Today’s Agenda
Chapter 13: Gravitation. Newton’s Law of Gravitation A uniform spherical shell shell of matter attracts a particles that is outside the shell as if all.
Physics 111: Elementary Mechanics – Lecture 12 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
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.
Gravitation AP Physics C. Newton’s Law of Gravitation What causes YOU to be pulled down? THE EARTH….or more specifically…the EARTH’S MASS. Anything that.
Gravitational Potential Energy When we are close to the surface of the Earth we use the constant value of g. If we are at some altitude above the surface.
Newton’s Theory of Gravity and Planetary Motion
Newton and Kepler. Newton’s Law of Gravitation The Law of Gravity Isaac Newton deduced that two particles of masses m 1 and m 2, separated by a distance.
Physics 111: Mechanics Lecture 13
Universal Gravitation
Newton’s Law of Gravitation and Kepler’s Third Law We showed already this week that Newton was able to prove Kepler’s third Law, the Harmonic Law, from.
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.
 Galileo was the first who recognize the fact that all bodies, irrespective of their masses, fall towards the earth with a constant acceleration.  The.
Gravitation Part II One of the very first telescopic observations ever was Galileo’s discovery of moons orbiting Jupiter. Here two moons are visible,
AP Physics C. What causes YOU to be pulled down? THE EARTH….or more specifically…the EARTH’S MASS. Anything that has MASS has a gravitational pull towards.
Chapter 13 Gravitation. Newton’s law of gravitation Any two (or more) massive bodies attract each other Gravitational force (Newton's law of gravitation)
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
Gravitation AP Physics 1. Newton’s Law of Gravitation What causes YOU to be pulled down? THE EARTH….or more specifically…the EARTH’S MASS. Anything that.
Gravitational Field Historical facts Geocentric Theory Heliocentric Theory – Nicholas Copernicus (1473 – 1543) Nicholas Copernicus – All planets, including.
Newton’s Law of Universal Gravitation
Physics.
Example How far from the earth's surface must an astronaut in space be if she is to feel a gravitational acceleration that is half what she would feel.
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.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 12 Physics, 4 th Edition James S. Walker.
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.
Questions From Reading Activity? Assessment Statements Gravitational Field, Potential and Energy Explain the concept of escape speed from a planet.
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.
Newton’s Law of Universal Gravitation by Daniel Silver AP Physics C
GRAVITATION.
Gravitation © David Hoult 2009.
Syll. State.: —due Friday, October 3
College Physics, 7th Edition
Chapter 13 Gravitation.
Chapter 12 Gravity.
More Gravitation.
Lecture Outline Chapter 12 Physics, 4th Edition James S. Walker
Last Time: Centripetal Acceleration, Newtonian Gravitation
Universal Law of Gravitation and Orbits
4.2 Fields Gravitation Breithaupt pages 54 to 67 September 20th, 2010.
Unit 2 Review Questions.
Universal Gravitation
Newton’s Law of Universal Gravitation
Gravitational Potential energy Mr. Burns
Chapter-5: Circular Motion, the Planets, and Gravity
Gravitation AP Physics C.
Gravitation AP Physics C.
Chapter 13 Gravitation.
Universal Gravitation
Gravitation AP Physics C.
9. Gravitation 9.1. Newton’s law of gravitation
Gravitation AP Physics C.
Physics 320: Orbital Mechanics (Lecture 7)
Gravitational Fields, Circular Orbits and Kepler
Gravitation AP Physics C.
PHYS 1443 – Section 001 Lecture #8
Gravitational Fields, Circular Orbits and Kepler’s Laws
Presentation transcript:

C - More Gravitation

Gravitational potential energy We need a new formula for Ug because Ug = mgh assumes that h is small as compared to the radius of the earth and therefore changes in g were negligible But in orbit, there will be variations in g due to the large distance from the center of the earth

Why is it negative? Convention has chosen Ug=0 at r=∞ And energy must be added in order to bring an object farther from the earth This means it will become less negative

Escape Speed Consider a rocket leaving the earth. It usually goes up, slows down, and then returns to earth. There exists an initial minimum speed that when reached the rocket will continue on forever. Let's use conservation of energy to analyze this situation! At infinity, we know that Ug = 0, also kinetic energy will be 0 because it will not move anymore at infinity so therefore the total mechanical energy will always equal ZERO

Escape Speed

Escape speed vs orbital speed

Example A rocket is launched vertically from the surface of the earth with an initial velocity of 10000 m/s. What maximum height does it reach? (g is not constant)

Gravitational field of hollow shell Inside a hollow sphere, the gravitation field is 0. Outside a hollow sphere, you can treat the sphere as if its entire mass was concentrated at the center.

Gravitational field of solid sphere Outside a solid sphere, treat the sphere as if all the mass is at the center of the sphere (same as hollow). Inside the sphere, treat the sphere as if the mass inside the radius is all at the center. Only the mass inside the “radius of interest” counts

Kepler's Laws There are three laws that Johannes Kepler formulated when he was studying the heavens THE LAW OF ORBITS - "All planets move in elliptical orbits, with the Sun at one focus.” THE LAW OF AREAS - "A line that connects a planet to the sun sweeps out equal areas in the plane of the planet's orbit in equal times, that is, the rate dA/dt at which it sweeps out area A is constant.” THE LAW OF PERIODS - "The square of the period of any planet is proportional to the cube of the semi major axis of its orbit."

Kepler’s 1st law – The Law of Orbits "All planets move in elliptical orbits, with the Sun at one focus.”

Kepler’s 2nd Law – The Law of Areas "A line that connects a planet to the sun sweeps out equal areas in the plane of the planet's orbit in equal times, that is, the rate dA/dt at which it sweeps out area A is constant.”

Kepler’s 3rd Law – The Law of Periods "The square of the period of any planet is proportional to the cube of the semi major axis of its orbit." Gravitational forces are centripetal, thus we can set them equal to each other! Since we are moving in a circle we can substitute the appropriate velocity formula! Using algebra, you can see that everything in the parenthesis is CONSTANT. Thus the proportionality holds true!

Kinetic Energy in Orbit Using our ORBITAL SPEED derived from K.T.L and the formula for kinetic energy we can define the kinetic energy of an object in a bit more detail when it is in orbit around a body. The question is WHY? Why do we need a new equation for kinetic energy? Well, the answer is that greatly simplifies the math. If we use regular kinetic energy along with potential, we will need both the orbital velocity AND the orbital radius. In this case, we need only the orbital radius.

Total Energy of an orbiting body Notice the lack of velocities in this expression as mentioned in the last slide. So by inspection we see that the kinetic energy function is always positive, the potential is negative and the total energy function is negative. In fact the total energy equation is the negative inverse of the kinetic. The negative is symbolic because it means that the mass “m” is BOUND to the mass of “M” and can never escape from it. It is called a BINDING ENERGY.

Energy from a graphical perspective As the radius of motion gets larger. The orbiting body’s kinetic energy must decrease ( slows down) and its potential energy must increase ( become less negative).