Aim: How do we calculate the eccentricity of an ellipse?

Slides:



Advertisements
Similar presentations
UCM & Gravity – Kepler’s Laws
Advertisements

Gravity. We know that planets travel around the Sun. Earth travels around the sun every 365 ¼ days. But what keeps the planets in this constant motion.
Planets of the Solar System Section 2 Section 2: Models of the Solar System Preview Key Ideas Early Models Kepler’s Laws Newton’s Explanation of Kepler’s.
The Solar System Planetary Orbits
What do you notice about the Orbit of the Planet’s compared to the Comet’s?
Solar System Overview. Early Ideas  It was assumed that the Sun, planets, and stars orbited a stationary universe  This is known as a “geocentric” model,
What is rotation? Spinning on an imaginary axis Period of rotation is the time it takes for a planet to make 1 spin on its axis =length of a planet day.
Daily Science Pg.30 Write a formula for finding eccentricity. Assign each measurement a variable letter. If two focus points are 450 km away from one another.
Nicolaus Copernicus Tycho Brahe Johannes Kepler
The planets 12/1/14.
(1) 150 million kilometers (2) 228 million kilometers
Kepler’s Three Laws of Planetary Motion. YMXtohttp:// YMXto.
Geometry of Earth’s Orbit Kepler’s Laws of Planetary Motion.
Laws of Planetary Motion KEPLER & NEWTON. Kepler’s 3 Laws  1 st Law- Law of Ellipses  2 nd Law- Law of Equal Areas  3 rd Law- Law of Periods.
KEPLER’S LAWS OF PLANETARY MOTION Objective: I will summarize Kepler’s three laws of planetary motion. 11/10/15.
 Danish astronomer ( )  Built an astronomical observatory on an island  Measured positions of stars and planets over a period of 20 years.
Eccentricity. Definition Degree of ovalness of an orbit around the sun.
Our Solar System. Views of our solar system Early explanations of our solar system was thought to be a Geocentric Model -also called Ptolemy model Earth.
1.1.1c.  Through observations, Newton realized that any two bodies attract each other with a force that depends on their masses and the distance between.
Gravitation Chapter 7. Kepler’s Laws  In the 1600s Johannes Kepler proposed three laws of planetary motion based on observational data. The laws are:
Aristotle suggested an Earth-centered, or geocentric, model of the solar system. In this model, the sun, the stars, an the planets revolved around Earth.
Orbits, Asteroids, and Comets. The Geometry of Orbits Planets revolve in an ellipse around the sun –An ellipse has two fixed points called foci that are.
Kepler’s Three Laws of Planetary Motion
Our Solar System.
Question of the Day What is the Shape of Earth’s Orbit?
Write a polar equation in r and {image} of a parabola with the focus at the origin and directrix x = {image}
Warmup Why is “space” called “space”? How did our solar system form?
Orbital Geometry.
Kepler’s laws of planetary motion
Orbits and Eccentricity
Kepler’s Laws of Planetary Motion
The Solar System.
Do now: If a planet has a mostly oval orbit,
Our Solar System PAGE 16.
Earth Among the Stars Earth Rotates… Earth rotation causes…
Part 1: Planets and SS models Part 2: Kepler’s Laws of Motion
Warm up: With your group determine your advice to the general on the aerial attack and beach landing dates and time. Be ready to justify your choice!!
Part 1: Planets and SS models Part 2: Kepler’s Laws of Motion
) Use any graphics program, Photoshop for instance, to create a puzzle. Hint: Google images is.
Science Starter Kepler’s 1st law states that planetary orbits are _________________ shapes? Kepler’s 2nd law states that 2 equal intervals of time an imaginary.
Science Starter Answer the following in your notebook: 1. When is the Earth closest to the Sun? 2. Does the speed of the Earth’s revolution change? 3.
History of our Knowledge of the Solar System
L. O: swbat calculate the elliptical orbits of planets
Section 2: Models of the Solar System
Solar System Overview.
Kepler’s Laws: Physics not optional!
The Movements of the Earth and its Effects
Write a polar equation of the ellipse that has eccentricity {image} and whose directrix is the line x = 35. Choose the answer from the following : 1. 2.
Our Solar System ©Mark Place,
Section 2: Models of the Solar System
The sun makes up about 99% of our solar systems mass.
Which planet has the most eccentric orbit?
Earth’s Role as a Body in Space
The sun makes up about 99% of our solar systems mass.
Orbits Round and round we go!.
Nicolaus Copernicus Johannes Kepler Tycho Brahe
Aim: How can we explain the laws that control the planets orbits?
Aim: How do we compute Eccentricity?
Our Solar System ©Mark Place,
Kepler’s Laws of Planetary Motion
Aim: How do planets move?
After Tycho Brahe’s death, Johannes Kepler (pictured here with Tycho in the background) used Tycho’s observations to deduce the three laws of planetary.
Kepler’s Laws Ms. Jeffrey- Physics.
3.3 Kepler’s Three Laws of Planetary Motion
Early Ideas.
Kepler’s Three Laws of Planetary Motion
8.8 Kepler’s Laws Unit 8: Astronomy May 16, 2012 Sanders.
Eccentricity.
Kepler’s Laws of Planetary Motion
Motion of Objects in Space
Presentation transcript:

Aim: How do we calculate the eccentricity of an ellipse? Do Now: Are there perfect circles in nature?

Where do theses planets belong? Why? I am Planet Y Made of gas Feel really cold 1,430 million km from the sun I am Planet X Made of Rock Feel Super Hot 100 million km from the sun I am: Planet Z Made of Rock Feel Warm 230 million km from the sun 1 2 3

How do we define eccentricity? Eccentricity Many early astronomers believed that planets revolved around the sun in orbits that were thought to be shaped as circles. However, observations of the planets shows that their motions could be explained best if their orbits were not circles, but ellipses. The shape of an orbit is best described by its eccentricity or how elongated the ellipse is. The eccentricity of an orbit is a calculated value that describes the out-of-roundness of an ellipse or how elliptical (oval) it is from being a circle. Eccentricity – out-of-roundness of an ellipse Major axis – longest distance from one end of the ellipse to the other end. Goes through the foci ( 2 focus points) Sun Focus 2 Focus 1 Ellipse – orbit Distance between foci Major axis

How does the shape of each elliptical orbit differ? (a line) Least Eccentric As foci distance increases, the orbit becomes more elliptical Most Eccentric Eccentricity will always be a number between 0 and 1 (decimal) Can NEVER be greater than 1 When Eccentricity equals Zero = shape will be circular The closer the eccentricity is to 0, the least eccentric orbit  When Eccentricity equals One = shape will be a line The closer the eccentricity is to 1, the more eccentric orbit

Identify the planet that has the highest eccentricity Identify the planet that has the highest eccentricity? Lowest eccentricity? Mercury has the highest eccentricity = most elliptical orbit Venus has the lowest eccentricity = most circular orbit

How do we calculate the eccentricity of Planet X’s ellipse? Sun Foci distance = 7.7 cm Eccentricity = 7.7 X 11.2 Major axis = 11.2 cm Eccentricity = 0.6875… Round to the nearest thousandth Eccentricity = 0.688 How is the eccentricity of our planet’s ellipse compared to Neptune's (0.009)? Our planets ellipse is more eccentric than Neptune's orbit. Place an X where our planet will move the fastest on our ellipse. Why will our planet move the fastest when it is next to the sun? Greater gravitational attraction when the planet is closest to the sun

Eccentricity = 1.8 Eccentricity = 0.375 = 4.8 Calculate the Eccentricity of Planet Heckman Round to the nearest thousandth Foci distance = 1.8 cm Major axis = 4.8 cm Eccentricity = 1.8 Eccentricity = 0.375 = 4.8 How is the eccentricity of Planet Heckman compared to Mercury? Mercury is less eccentric than Planet Heckman

How does the shape of each elliptical orbit differ? (a line)

How do we calculate the eccentricity of Planet X’s ellipse? Sun Foci distance = Major axis = Round to the nearest thousandth How is the eccentricity of our planet’s ellipse compared to Neptune's (0.009)? Place an X where our planet will move the fastest on our ellipse. Why will our planet move the fastest when it is next to the sun?

Calculate the Eccentricity of Planet Heckman Round to the nearest thousandth Foci distance = Major axis = How is the eccentricity of Planet Heckman compared to Mercury?

Summary Activity- Exit Card

Extra Questions Earth’s eccentricity of orbit is 0.017 Base your answers to questions 1 through3 on the diagram below, which represents a model of Earth’s orbit. Earth is closest to the Sun at one point in its orbit (perhelion) and farthest from the Sun at another point in its orbit (aphelion). The Sun and point B represent the foci of this orbit. 1) Explain why Earth’s orbit is considered to be elliptical. Earth’s eccentricity of orbit is 0.017 2) Describe the change that takes place in the gravitational attraction between Earth and the Sun as Earth moves from perihelion to aphelion and back to perihelion during one year. The force of gravity decreases, then increases 3) Describe how the shape of Earth’s orbit would differ if the Sun and focus B were farther apart. The orbit would become more eccentric