Unit 06 “Circular Motion, Gravitation and Black Holes” “Gravitation and Black Holes”

Slides:



Advertisements
Similar presentations
Universal Gravitation
Advertisements

Gravity- I’m Attracted to You
Neutron Stars and Black Holes Please press “1” to test your transmitter.
Gravity. Review Question What are Kepler’s laws of planetary motion?
Universal Gravitation & Universal Circular Motion Review Questions Divided by Category.
Neutron Stars and Black Holes
13.1 – The Falling Apple Newton realized all accelerations are caused by net forces The apple accel to earth in the same way the moon accel to earth The.
Explain why the Earth precesses and the consequences
Mass vs. Weight and Gravity
Black Holes Astronomy 315 Professor Lee Carkner Lecture 16.
Chapter 12 Gravitation. Theories of Gravity Newton’s Einstein’s.
Black Holes By Irina Plaks. What is a black hole? A black hole is a region in spacetime where the gravitational field is so strong that nothing, not even.
13.3 Black Holes: Gravity’s Ultimate Victory Our Goals for Learning What is a black hole? What would it be like to visit a black hole? Do black holes really.
Today’s APODAPOD  Start Reading NASA website (Oncourse)  2 nd Homework due TODAY  IN-CLASS QUIZ NEXT FRIDAY!! The Sun Today A100 Solar System.
Black Holes.
Goal: To understand gravity Objectives: 1)To understand who discovered what about gravity. 2)To learn about the Universal nature of gravity 3)To explore.
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
Unit 06 “Circular Motion, Gravitation and Black Holes” Test Review.
Universal Gravitation
Gravity Chapter 7. Newton  Noticed the moon followed a curved path  Knew a force was required to allow an object to follow a curved path  Therefore,
Chapter 8 Universal Gravitation
Newton’s Law of Gravitation. Newton concluded that gravity was a force that acts through even great distances Newton did calculations on the a r of the.
Bellringer Give the date and the name for the day in which the southern hemisphere will be experiencing the most direct sunlight and have the longest amount.
Kepler’s first law of planetary motion says that the paths of the planets are A. Parabolas B. Hyperbolas C. Ellipses D. Circles Ans: C.
Universal Gravitation Chapter 8. Isaac Newton and Gravity Newton realized an apple falls because of force Moon follows circular path, force needed Newton.
Test Review Chapters Relativity. Question #1 What happens to the gravitational force when 2 objects get farther away from each other?
Black Holes. Gravity is not a force – it is the curvature of space-time - Objects try and move in a straight line. When space is curved, they appear to.
A black hole is a region of space with such a strong gravitational field that not even light can escape.
Remnant of a Type II supernova explosion Iron core collapses until neutrons are squeezed tightly together During the explosion core remains intact, outer.
Gravitational Interactions
Law of Universal Gravitation
Universal Gravitation Physics Mr. Padilla. Falling Apple hits Newton on the head. According to the law of inertia, it would not fall unless acted upon.
Review Question What are Kepler’s laws?. Review Question What are Newton’s laws?
Black Holes. Objectives of this Unit Recognize that a gravitational force exists between any two objects. This force is proportional to the masses and.
Law of Universal Gravitation Chapter 12 November 9/10.
Black Holes This one’s green. I like green.. What happens after a SN? Material remaining after a supernova is 3 times more massive than the sun or more.
Lecture 27: Black Holes. Stellar Corpses: white dwarfs white dwarfs  collapsed cores of low-mass stars  supported by electron degeneracy  white dwarf.
Black Holes
Unit 06 “ Circular Motion, Gravitation and Black Holes” Gravitation Problem Solving.
By Katy O’Donohue. Black Holes Black Holes are a region of space from which nothing can escape, including light. Light is made up of massless particles.
Gravity- I’m Attracted to You S8P5. Students will recognize characteristics of gravity, electricity, and magnetism as major kinds of forces acting in nature.
Unit 1 Lesson 4 Gravity and Motion
Unit 1 Lesson 4 Gravity and Motion. Down to Earth Copyright © Houghton Mifflin Harcourt Publishing Company What is gravity? Gravity is a noncontact force.
Newton’s Law of Universal Gravitation
It was discovered in the early 1990’s that the pulse period of a millisecond pulsar 500 parsecs from earth varies in a regular way.
Today is all about GRAVITY!!!
Gravitation Using the law of universal gravitation to gain perspective on planets, moons, stars and black holes.
Gravity, Energy, and Light Einstein and Newton 1.
Black Holes. Escape Velocity The minimum velocity needed to leave the vicinity of a body without ever being pulled back by the body’s gravity is the escape.
Review Question What is retrograde motion?. Review Question Explain why the phases of Venus proved to Galileo that Venus must orbit the Sun when the Moon.
BLACK HOLE Cindy,Robin, Selina. A black hole is a place in space where gravity pulls so much that even light can not get out. The gravity is so strong.
Black Holes and Gravity 1)Type II Supernova 2)Neutron Stars 3)Black Holes 4)More Gravity April 7, 2003
Gravitational Forces. What is Gravity? Gravity is the tendency of all objects (with mass) to attract one another. We often refer to this as a gravitational.
Universal Gravitation Does the moon stay at a certain distance from the Earth or is it falling toward the Earth? - the moon is actually falling around.
Black Hole. Special Relativity Einstein’s special theory of relativity has two parts. –All objects moving at constant velocity have the same laws of physics.
 Sun-like star  WHITE DWARF  Huge Star  NEUTRON STAR  Massive Star  BLACK HOLE.
Gravity.
Motion of Objects in Space S6E1e Explain that gravity is the force that governs the motion in the solar system.
Gravity & Motion Unit 1 Lesson 4
Lots of fun! Win valuable prizes!
Gravity (Act III, Scene II)
GRAVITY.
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Black Holes and Neutron Stars
Unit 2 Force & Motion Ch 6 Sec 4 Gravity.
Unit 1 Lesson 4 Gravity and Motion
Universal Gravitation
Gravity and Motion.
Newton’s Law of Gravitation
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Presentation transcript:

Unit 06 “Circular Motion, Gravitation and Black Holes” “Gravitation and Black Holes”

What would happen to the Earth if the Sun suddenly disappeared? What if the Sun suddenly disappeared? Would the Earth … …keep moving in a circle? …move out in a straight line? …stop moving &stay in one place? …spiral out into space

The Gravitational Force We learned about Gravity previously. – We learned gravity on Earth pulls all objects down to Earth. – The force of gravity accelerates all objects at the rate of a=-9.8m/s 2. But WHY does Earth attract these objects? – Newton realized that the force attracting objects toward Earth is the SAME as the force pulling the Moon around the Earth … or the Earth around the Sun! GRAVITY!

The Gravitational Force Definition: The force of attraction between ANY two masses. Examples: – The Earth is gravitational attracted to the Sun – The moon is gravitational attracted to the Earth – You are gravitational attracted to the Earth! – You are gravitational attracted to the table! – ANY two masses have a gravitational attraction between then!

We are attracted to ANY object? YES! Any two masses have a gravitational attraction to one another! Obviously the attraction between you and the table is much less than you and the Earth… why? The force of gravity depends on…. The masses of the objects (more mass, more gravity) The distance the objects are apart (closer objects, more gravity) – Since the Earth is HUGE the force between You and Earth is much BIGGER than between You and the Table. This is why you don’t “fall into the table” or get “pulled into another person” due to the gravitational force between you. If there were no other forces … like in outer space, YOU WOULD! (slowly, but you would!)

Gravitational Force Equation F G = G m 1 m 2 r 2 F G = Gravitation Force m 1 = mass of object 1 m 2 = mass of object 2 r = distance between the objects (“r” is measured center to center) G = constant of universal gravitation Mass and F g are “directly proportional” m F g Example: m increases by factor of 2 … F g increases by factor of 2 m decreases by factor of 4 … F g decreases by a factor of 4 distance and F g are “inverse square proportional” r F g Example: r increases by factor of 2 … F g decreases by factor of 4 (2 2 ) r decreases by factor of 4 … F g increases by a factor of 16 (4 2 )

How do you Escape Gravity!?!? In the picture, 4 cannon balls are shot with different velocities… Ball B has a small velocity and drops back to earth. Ball C has a bigger velocity and falls farther but still back to earth. Ball A has such a big velocity is actually escapes Earth’s gravitational field! This is called “escape velocity” Ball D has a big velocity so that when it falls “down” it actually curves around the Earth! This is an ORBIT, this is a SATELLITE!(imagine if the Earth was flat, this wouldn’t happen, since the Earth is round the Earth curves under the ball as it falls – CIRCULAR MOTION!!!!)

What would happen to the Earth if the Sun suddenly disappeared? …keep moving in a circle? …move out in a straight line? …stop moving &stay in one place? …spiral out into space

Escape Velocity Cannon ball A “escaped” how? If your velocity is greater than the “Escape Velocity” you can escape the gravitational field of an object! Vesc = 2GM planet R planet √ The Escape Velocity of a Black Hole is GREATER THAN the Speed of Light! Not even LIGHT can escape a Black Hole!

Gravity is what is responsible for the formation of our Universe Universe  Galaxies  Solar System  Earth Our Galaxy  The Milky Way

Our Solar System

Relative Sizes of the Planets to the Sun

Black Holes Some definitions (see Black Holes Lab Worksheet) 1.Singularity: A Singularity is a point of infinite density … meaning a HUGE mass but VERY SMALL (too small and massive to even imagine!) The center of a black hole is a “singularity in space-time” 2.Speed of Light: The Speed of Light is 300,000,000m/s (3.00x10 8 m/s) It’s called the “cosmic speed limit” because nothing is known to travel faster than light! 3.Light year (ly): A light year is a DISTANCE, it’s the distance light can travel in one year. The sun is 8 light minutes away from us … it takes 8 minutes for the sun’s light to get to us. If something is 8 light YEARS away, it would take 8 years for that light to get to us. Starts and galaxies are millions and billions of light years away from us! 4. Escape Velocity (V esc ): Velocity needed to escape the gravitation pull of a planet.

Black Holes “Internet Based Lab” Download and complete the Black Holes Lab – Using the videos on the websites as the worksheet explains, you will learn about Black Holes, how they form and why! Some artist images of “black holes” and the space around them…

Completed Lab? Black Hole Basics Black Holes form when a star runs out of fuel and dies. Not all stars turn into Black Holes, only stars about times more massive than our sun. They first expand as they run out of fuel into a Supernovae. Then they collapse in on themselves, creating a point of huge density – a black hole.

Black Holes Continued… Black Holes are not dangerous unless you reach the “Event Horizon” (aka Schwarzchild radius) – This is the distance from the center of a black hole from which you can’t escape (the gravitational force is too strong, not even light can escape) This is why they are called “Black Holes” – Because not even light can escape them – so there is nothing to “see”. This is why if the Sun was replaced with a Black Hole of the same mass it wouldn’t affect the Earth! – We still wouldn’t be CLOSE enough to get pulled in!!!

How Do We Know They Exist? There are many pieces of evidence – so even though we can’t “see” a Black Hole – we know they are there! Two pieces are… – As stars near a Black Hole they experience a strong gravitational pull which accelerates them, we can see the star moving faster around the this area. – As matter in the Universe is pulled into the Black Hole the matter accelerates, speeds up and thus gets HOT – we can see this heat in the form of radiation, X-rays are detected.

What’s the Dilly? Gravity warps time and space…. Black holes warp is SO much, nothing can escape – and scientists wonder if there is more to the story…. Watch part of “The Elegant Universe” for more explanation….. And Homer in 3D