Autumnal Equinox CELESTIAL MOTIONS. Winter Solstice CELESTIAL MOTIONS.

Slides:



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

Early Astronomy  As far as we know, humans have always been interested in the motions of objects in the sky.  Not only did early humans navigate by.
Our Solar System. Your Parents Solar System 21 st Century Solar System.
Giants of Science Part Two Tycho Brahe & Johannes Kepler
Kepler’s laws.
Early Astronomers & Planetary Motion
Do our planets move?.
T YCHO B RAHE / J OHANNES K EPLER P LANETARY M OTION Astro Chapter 3-3.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 6.
1. 2 Tycho Brahe ( ) (right around Galileo) Born Tyge Ottesen Brahe (I can’t say that correctly) Last of the great astronomers who came before.
Models of the Solar System *Early Models of the Solar System *Kepler’s Laws.
Johannes Kepler’s Planetary Discoveries Jacqueline DePue.
MODELS OF THE SOLAR SYSTEM. ARISTOTLE Greek philosopher ( BC) He promoted an earth centered called geocentric, model of solar system He said the.
CHAPTER 2: Gravitation and the Waltz of the Planets.
Intro to Astronomy Through the early history of civilization, people made observations about the night sky, sun, and moon. They tried to explain what they.
Bell Ringer 9/8 OPINION QUESTION – How do you believe the solar system was formed?
Objectives Explain how the solar system formed.
At this speed, the Earth makes one full rotation. Definition: the circular movement of a body around a central point called an axis –A full rotation takes.
Advanced Physics LC1 Project Done By:- Supervised by:- Abdulrahman Hussain Mrs. Lina Marouf Rashed Hamdan Zayed Aqeel
MARS JOHANNES KEPLER THE SOLAR SYSTEM LAWS OF PLANETARY MOTION.
The Copernican Revolution. Nicolaus Copernicus 1473 – 1543.
Midterm 1 Review Please swipe your student ID for attendance tracking, and pick up your assigned transmitter.
Reminders Answering cell phones during class shaves a little off your grade each time. Answering cell phones during class shaves a little off your grade.
Astronomy The Science that Studies The Universe Ancient Greeks To Isaac Newton.
Universal Gravitation. Brief Astronomical History A.D Ptolemy Greek Astronomer A.D. Believed in Geo- centrism First to latitude and longitude.
Bellwork 1.Who is credited with the revolutionary model of a HELIOCENTRIC solar system? A. Aristotle B. Ptolemy C. Galileo D. Copernicus 2.The planets.
Chapter 3: Motion of Astronomical Bodies. A bit more on the Celestial Sphere and motions This works OK if we only consider the stars. What happens when.
Kepler’s Laws of planetary motion. Ellipse lab. Tycho Brahe Tycho Brahe was a Danish astronomer who is best known for the astronomical observations which.
The Scientific Revolution pg Why look up at the stars? Once seen as omens and used for fortune telling Help us see our place in the universe We.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
Early Astronomy Chapter 22, Section 1.
Earth’s Place in the Universe. Starter- Do on page 181 in the starter section of your notebook.  Our new unit is Earth’s Role in Space, where do you.
Introduction to Astrophysics
Kepler’s Laws of Orbital Motion Concepts of Physics Mr. Kuffer.
Astronomy Chapter Astronomy People in ancient cultures used the seasonal cycles to determine when they should plant and harvest crops. They built.
Copyright © 2010 Pearson Education, Inc. Chapter 12: Gravitation.
“Pick a flower on Earth and you move the farthest star.”
Gravitation Chapter 7. Planetary Motion & Gravitation 7.1.
Title your notes: Models of the Solar System
Historical Astronomy STARRY STARRY NIGHT. 400 B.C.E. noticed that some of the celestial objects moved relative to the rest. They counted moving objects-
Kepler’s Laws & Planetary Motion
Johannes Kepler ( ) discovered a set of laws that accurately described the motions of the planets.
The “Geocentric Model” Aristotle vs. Aristarchus (3 rd century B.C.): Aristotle: Sun, Moon, Planets and Stars rotate around fixed Earth. Ancient Greek.
Geometry of Earth’s Orbit Kepler’s Laws of Planetary Motion.
Kepler, Brahe and Ptolemy By: Grace. Johannes Kepler Born in 1571 in Weil der Stadt, HRE Naturally intelligent, which earned him a scholarship to University.
Introduction to Classical Astronomy Mr. Ross Brown Brooklyn School for Law and Technology.
6/10/20161 Ch. 22: Astronomers Mr. Litaker 6/10/20162 Our Solar System What do we know? Time required for Earth to make one rotation on its axis? 24.
Astronomy in the Middle Ages to the Modern Era From Copernicus to Galileo to man on the moon.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
Test Review Terms Elliptical orbit Rotation Axis Full moon Aphelion Major axis Foci Semimajor axis Perihelion Sun Maunder minimum Solar day Seasons Lunar.
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.
Warmup Why is “space” called “space”? How did our solar system form?
Johannes Kepler ( ) discovered a set of laws that accurately described the motions of the planets.
Orbital Geometry.
Observing the Solar System
Astronomy-Part 7 Notes Gravity and its Role in the Solar System
Men of the Universe.
Astronomy-Part 7 Notes Gravity and its Role in the Solar System
Kepler’s Laws of Planetary Motion Newton’s Laws of Gravity
7.3 Kepler’s Laws.
MARS JOHANNES KEPLER THE SOLAR SYSTEM LAWS OF PLANETARY MOTION.
LESSON 12: KEPLER’S LAWS OF PLANETARY MOTION
Planetary Motion Intro Video.
WARM UP/ DO NOW 1) Where does nuclear fusion occur and where does nuclear fission happen? 2) Explain the Doppler Effect 3) What is Hubble’s Law and what.
Planetary Orbits using Kepler’s Laws
Kepler’s Laws of Planetary Motion
Planetary Motion.
Early Ideas.
MARS JOHANNES KEPLER THE SOLAR SYSTEM LAWS OF PLANETARY MOTION.
Presentation transcript:

Autumnal Equinox CELESTIAL MOTIONS

Winter Solstice CELESTIAL MOTIONS

Perihelion & Aphelion CELESTIAL MOTIONS

PERIHELION the point in the orbit of a planet, asteroid, or comet at which it is closest to the sun.

Johannes Kepler was always sick as a child and lived in poverty. His hands were crippled and his eyesight permanently impaired by smallpox. His father, a mercenary, was killed in a battle and he was raised by his mother and grandfather. Despite these difficulties, guests at his grandfathers’ inn were astonished at his ability to solve any problem they could bring to him involving numbers. YOUNG KEPLER

His mother Katharina, who was an herbalist, conveyed her love of the natural world to her son. She made a point of taking him out at night to show him interesting things in the night sky, including a comet and a lunar eclipse. In doing so, she set Johannes on a course which would eventually transform our understanding of our solar system and the universe.

After being inspired by the sight of the moon turning red during a lunar eclipse at age nine; Kepler, with an incredible amount of hard work worked, attended and lectured at the University of Tübingen; where he began to develop his ideas on astronomy. YOUNG KEPLER

Tyco Brahe was a Danish nobleman known for his accurate and comprehensive astronomical and planetary observations. He was born in Scania, then part of Denmark, now part of modern-day Sweden. TYCO BRAHE

Brahe was ridiculously rich and good friends with royalty. He lived on an island on which he built his own observatory. He also drank in excess and lost his nose in an intoxicated fight with his cousin over a math equation. Instead of replacing his nose with wax like everyone else during the time; he had two prosthetics made. One gold, one silver. TYCO BRAHE’S PRIVATE LIFE

THE SLICE

Tyco also had a pet moose at his castle, that he trained to follow him around like a puppy. One night at a party, the moose drank too much beer, fell down a castle staircase and died. THE MOOSE

Eventually, Johannes Kepler becomes Tyco Brahe’s assistant. Brahe was insecure and distrustful; so he gave Kepler what he thought was an unsolvable problem to discourage him and force him to quit.

In 1601 Brahe died and for centuries people thought that Brahe had been murdered by mercury poisoning. But when researchers exhumed his remains in 2012, they found the real cause… A MYSTERIOUS DEATH

Brahe is now thought to have died from a bladder infection after politeness kept him from excusing himself to use the bathroom during a royal banquet in October 1601, causing his bladder to rupture. HE WAS KILLED BY PEE

They also found that instead of gold or silver; the nose he was wearing when he died was brass. THE NOSE

Once Brahe died, Kepler returned to the lab to pick up his notes on the almost impossible problem he was working on. However, Brahe’s family had locked the doors and was about to sell everything. So Kepler did what any good mathematician would do in that scenario. He broke in and stole his work. THE BREAK-IN

Kepler eventually solved the problem that Brahe had given him. People thought that the planets had traveled In circles and the motion of planets was unpredictable. However, by observing mars, Kepler discovered that all heavenly bodies travel in elliptical or oval paths. THE KEY - MARS

ELLIPTICAL ORBITS

PERIHELION AND APHELION

KEPLER’S LAWS As a result Kepler created three laws that mathematically confirmed Nicolaus Copernicus’ idea that the Sun was at the center of the Solar System. These laws eventually helped Galileo develop his ideas as well.

KEPLER’S FIRST LAW Planetary orbits are ellipses, with the Sun at one focus The distance of a planet from the Sun therefore varies. When the planet is furthest away it is at aphelion (apogee, in general), and when it is closest it is at perihelion (perigee, in general). The terms described as 'in general' are those terms that can be used whatever the central attracting body is. The terms perihelion and aphelion apply only when the central attracting body is the Sun.

KEPLER’S SECOND LAW An imaginary line between a planet and the Sun will sweep out the same area in equal periods of time. This law is equivalent to the present-day Law of Conservation of Angular Momentum. The classic example of this latter law is an ice-skater who rotates faster when (s)he draws in initially-outstretched arms.

KEPLER’S THIRD LAW

“Where there is matter, there is geometry.” JOHANNES KEPLER

If we ever want to go to Mars; we have to wait for Mars to be close and time our launch perfectly. TRANSLATION

NOTEBOOK TEST 1.When a planet, asteroid, or comet is at its closest point to the sun; we call this moment its _______. 2.In three sentences describe young Johannes Kepler’s life. 3.What did Kepler’s mom do that inspired Kepler to become an astronomer? 4. What event motivated Kepler the most to study the stars and planets? 5.What was the name of the university at which Kepler attended and taught? 6.In three sentences describe what Tyco Brahe was like. 7.How did Brahe loose his nose and what was it replaced with? 8.Where did Tyco Brahe live? 9.What did Brahe have as a pet, and what happened to it? 10.Describe Brahe’s relationship with Kepler. 11.How did Brahe die? 12.After Brahe’s death, what happened to Kepler’s work. 13.What was the key that helped Kepler solve the “impossible problem.” 14.On January 2 the earth is ________ to the sun; and on July 4 the earth is ________ from the sun. 15.How many laws did Kepler create? 16.What does the first law state? 17.What does the second law say? 18.What does the third law state? 19.When is the best time to take a trip to Mars?

Spring Equinox CELESTIAL MOTIONS

Summer Solstice CELESTIAL MOTIONS