 Geocentric vs. Heliocentric Model  Geocentric Model- astronomers assumed that the Sun, planets, and the stars orbited around a stationary Earth 

Slides:



Advertisements
Similar presentations
2 pt 3 pt 4 pt 5 pt 1 pt 2 pt 3 pt 4 pt 5 pt 1 pt 2 pt 3 pt 4 pt 5 pt 1 pt 2 pt 3 pt 4 pt 5 pt 1 pt 2 pt 3 pt 4 pt 5 pt 1 pt StarsGalaxiesThe SunPlanets.
Advertisements

Astronomy Chapter 2 The Solar System
UNIT 2 THE SOLAR SYSTEM Vocabulary Review. THE FORCE OF ATTRACTION BETWEEN OBJECTS THAT IS DUE TO THEIR MASSES gravity.
Structure & Formation of the Solar System
Review Vocabulary magnetic field: the portion of space near a magnetic or current-carrying body where magnetic forces can be detected The Sun contains.
UNIT 2 THE SOLAR SYSTEM Vocabulary Review. IN THE ORBIT OF A PLANET OR ANOTHER BODY IN THE SOLAR SYSTEM, THE POINT THAT IS FARTHEST FROM THE SUN aphelion.
Touring the Night Sky. What is Astronomy? Astronomy is the branch of science that studies objects beyond Earth. These “objects” include the Sun, billions.
Unit 1 Lesson 1 Structure of the Universe
Bell Ringer 9/8 OPINION QUESTION – How do you believe the solar system was formed?
Earth in the Universe Or...where the heck did we come from?
JOURNAL #17 – THE SOLAR SYSTEM 1.What is the order of the planets from the Sun outward? 2.If during a solar eclipse the moon must be between the Sun and.
The Big Bang! (pg 20). Origins How did the: How did the: Universe form? Universe form? Solar system / Earth form? Solar system / Earth form? How Do We.
Unit 2 Lesson 1 Structure of the Universe
 Our Cosmic Neighborhood  the collection of eight planets and their moons in orbit around the sun, together with smaller bodies in the form of asteroids,
Space Science Chapter 16.
Astronomy. List what you know about astronomy so already.
Astronomy and Space Ms. Woodard. DAY 1 Objective Objective – I can explain how the universe formed and the laws governing it.
Objectives  1.1j The shape of Earth, the other planets, and stars is nearly spherical.  1.1a Earth’s Sun is an average-sized star. The Sun is more than.
Big Bang theory Parts of our solar system Planet characteristics Galaxies Constellations Nebulas.
Daily Review: 8/14 Fill in the blank. You only have to write the word 1. The hydrosphere is made up of all ___________ on earth. 2. All energy for life.
Grade 9 Academic Science – Unit 3 Space – What I already know StarsPlanetsDeep SpaceEarth and MoonOther Stuff
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.
Unit 4: Astronomy Chapter 14: The Solar System Big Idea: The solar system includes the sun, the planets & their moons, & smaller objects such as comets,
Solar System.
Gravitation Chapter 7, section 3. Geocentric Models Aristotle (384 – 322 BC) taught that the earth was surrounded by crystalline spheres on which the.
Unit 2 Lesson 1 Structure of the Universe
Jeopardy Planetary Motion Sun Inner Planets Outer Planets Solar System Q $100 Q $200 Q $300 Q $400 Q $500 Q $100 Q $200 Q $300 Q $400 Q $500 Final Jeopardy.
The Big Bang! Unit 1. Origins How and when did the: How and when did the: universe form? universe form? solar system / Earth form? solar system / Earth.
Planets, Solar Systems, and Galaxies…..Oh my!
Astronomy The study of objects and matter outside the earth's atmosphere and of their physical and chemical properties.
ACTIVITY 1. For distances to stars and galaxies, astronomers use a unit called a light- year. A light-year is the distance that light travels in a year.
The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these.
Origins of the Universe and Solar System From Universe to Galaxy to Solar System.
Study Guide Answers. 1. What is the difference between geocentric and heliocentric? Geocentric: Earth is the center of the universe Heliocentric: Sun.
Exploring Space. Solar system Our solar system consists of an average star we call the Sun, the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn,
Earth’s Motion and the Universe. – The Universe is made of galaxies – Galaxies are made of many stars – Some stars have planetary systems (similar to.
Patterns in the Solar System Ch 23. Plane of the ecliptic All planets are within 3 o of a line Drawn outward from the Sun’s equator The path of the Sun.
Know about the Sun’s Energy Know about the Sun’s Core, Atmosphere, and Sunspots Comprehend the Solar System’s Structure The Sun and It’s Domain.
Galaxies and Stars 8.E.4A.1 Obtain and communicate information to model the position of the Sun in the universe, the shapes and composition of galaxies,
The Big Bang!.
Ch 26 The Sun & the Solar System Review. Name & describe the location of the layers of the sun. What happens in each layer? How does the temperature change?
Our Solar System.
1. The Universe and the Solar System 2 © Zanichelli editore 2015.
Astronomy kdY7aA.
NEXT Gravity and the Solar System Properties of Planets Gas Giants Terrestrial Planets Word!
Classroom Room 274. Cross roads County/ City Grosse Pointe Farms.
Image From: Astronomy Notes Part 1 Notes Created by Harris Middle School with graphics cited.
Chapter 27 Formation of the Solar System The sun and all of the planets and other bodies that revolve around the sun.
THE SOLAR SYSTEM. BODIES IN THE SOLAR SYSTEM Our planet, Earth, is part of a system of planets that orbit a star, the sun. The solar system is comprised.
Ch. 20 and 21.  Our solar system has been here for awhile  5 billion years!  It formed from a solar nebula  Clouds of dust in space that combined.
11.2 The Sun and the Planets Our Sun, an average star in the universe, is the center of our solar system. Planets, moons, asteroids and comets revolve.
Astronomy and Space Ms. Woodard. DAY 1 Objective Objective – I can explain how the universe formed and the laws governing it.
Structure of the Universe Unit 1 Lesson 1. Big Bang Theory Scientific origin of the Universe 1.All matter in the universe began moving together to a single.
Warm Up- Do this on the next blank page should be page 10 1)Think about your current location at this exact moment. If someone asked for your current location,
The Big Bang! ESCI 518 Fall Origins How and when did the: How and when did the: universe form? universe form? solar system / Earth form? solar system.
Astronomy and Space Mr. Norris. DAY 1 Objective Objective – I can explain how the universe formed and the laws governing it.
Formation of the Solar System and The Universe. Our Solar System Sun is the center of a huge rotating system of: Sun is the center of a huge rotating.
Topic IV Astronomy Part II “Earth in Space” I. Laws of Planetary Motion: 3 laws proposed by Johannes Kepler to explain the shape, velocity, and distance.
General Concepts The Universe began with an explosion, the big bang, over 13 billion years ago. Our galaxy, the Milky Way, contains billions of stars.
Unit 2 Vocabulary. 1.) Astronomy – the scientific study of the universe; it includes the observation and interpretation of celestial bodies and phenomena.
Astronomy Cosmology.
The Universe.
Gravity and the Solar System
Do Now What is the geocentric model?
The Planets and the Solar System
Solar System #17.
Warm-up Explain the difference between precession and nutation.
Planets Inner vs. outer Composition – inner planets are rocky/outer are gas Size – inner are smaller/outer are much larger Distance from sun – inner are.
Planets Inner vs. outer Composition – inner planets are rocky/outer are gas Size – inner are smaller/outer are much larger Distance from sun – inner are.
“Earth in Space” Astronomy Part II
Presentation transcript:

 Geocentric vs. Heliocentric Model  Geocentric Model- astronomers assumed that the Sun, planets, and the stars orbited around a stationary Earth  Heliocentric Model-the Sun is the center of our solar system(Copernicus). Earth and the other planets orbit around the sun

 Our Cosmic Neighborhood  the collection of eight planets and their moons in orbit around the sun, together with smaller bodies in the form of asteroids, meteoroids, and comets.

 Johannes Kepler in the 1600’s proposed 3 laws of planetary motion.  Kepler was able to summarize the carefully collected data of his mentor - Tycho Brahe - with three statements that described the motion of planets in a sun-centered solar system.

 The path of the planets around the sun is elliptical in shape, with the center of the sun being located at one focus. (The Law of Ellipses)

 An imaginary line drawn from the center of the sun to the center of the planet will sweep out equal areas in equal intervals of time. (The Law of Equal Areas)

 The ratio of the squares of the periods of any two planets is equal to the ratio of the cubes of their average distances from the sun. (The Law of Harmonies)

(Orbital period)

 In this equation P represents the period of revolution for a planet and R represents the length of its semimajor axis. The subscripts "1" and "2" distinguish quantities for planet 1 and 2 respectively. The periods for the two planets are assumed to be in the same time units and the lengths of the semimajor axes for the two planets are assumed to be in the same distance units. Kepler's Third Law implies that the period for a planet to orbit the Sun increases rapidly with the radius of its orbit. Thus, we find that Mercury, the innermost planet, takes only 88 days to orbit the Sun but the outermost planet (Pluto) requires 248 years to do the same.

 The law states that every pair of bodies in the universe attract each other with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between them.  Newton also determined that each planet orbits a point between it and the sun called the center of mass.

 The center of mass between 2 celestial bodies that orbit each other.

 We are located in the Milky Way Galaxy  The Milky Way is a great disk made of stars orbiting a central point in the disk  The Sun is just one of the BILLION stars that make up the Milky Way

What is it? How did it form?

 The formation of the planets is viewed as a by-product of the formation of the Sun.  The Solar nebula collapsed until the sun was several times larger than it is now surrounded by a disk of dust and gas.  A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way  Solar magnetic fields may have transferred the angular momentum of the sun into the disk.  The disk itself then fragmented into the planets 

 The Big Bang Theory  The Steady-State Theory  The Inflationary Theory

 The theory that the universe began as a point and has been expanding ever since is call The Big Bang Theory.

 The night sky presents the viewer with a picture of a calm and unchanging Universe. So the 1929 discovery by Edwin Hubble that the Universe is in fact expanding at enormous speed was revolutionary. Hubble noted that galaxies outside our own Milky Way were all moving away from us, each at a speed proportional to its distance from us. He quickly realized what this meant that there must have been an instant in time (now known to be about 14 billion years ago) when the entire Universe was contained in a single point in space. The Universe must have been born in this single violent event which came to be known as the "Big Bang."

 The Steady-State Theory proposes that the universe looks the same on large scales to all observers, and that it has always looked that way.  The steady-state universe does NOT change with time.

 The Inflationary Theory (Inflationary Model) states that the universe began as a fluctuation in a vacuum and expanded very rapidly for a fraction of a second, before settling into a more orderly expansion.

 Convection  Conduction  *Radiation

 Energy is transferred by electromagnetic radiation (energy travels in waves).  Electromagnetic radiation (light)- electric and magnetic disturbances, traveling through space as waves.

 Visible Light- the limited range of all the various wavelengths of electromagnetic radiation that is seen by the human eye.  Electromagnetic Spectrum- all types of electromagnetic radiation arranged according to wavelength and frequency.

 Wavelength- is the distance between peaks on a wave.  Frequency- what is the number of waves occurring per second. C=λf C=Speed of light (3.0 x 10^8 m/s) f=frequencyλ= Wavelength

 The sun is the LARGEST object in the solar system in both size and mass.  The Sun’s mass controls the motions of the planets and other objects  The sun is made up of about 70.4% hydrogen and 28% helium (gaseous interior).

Did you know the sun is not technically “stationary?” The gravitational pull of the other celestial bodies that orbit it cause the Sun to orbit its barycenter. So the Sun actually moves!

 The Sun’s magnetic field disturbs the solar atmosphere and creates new features to appear on the sun, like sunspots.  Sunspots- dark spots on the surface of the photosphere of the Sun.  The number of sunspots changes regularly and reaches a maximum number every 11.2 years. (The Solar Activity Cycle)

 Highly Active solar flares are associated with sunspots.  Solar Flares (“storms”) are violent eruptions of particles of radiation from the surface of the Sun.

 Solar Wind- Wind of charged particles that flows throughout the solar system and begins as gas flowing outward from the Sun’s corona at high speeds.  The charged particles emitted by the sun shower the planets in our solar system.  The Earth’s Magnetosphere deflects them.

 The Van Allen Belts-two large rings in Earth’s magnetic field, where the charged particles emitted from the Sun are trapped.  The highly energized particles within the Van Allen Belts combine with the gases in Earth’s atmosphere and emit light known as the Auroras. (Seen at the Poles)

 shows/videos/perfect-disaster-solar- storm.htm shows/videos/perfect-disaster-solar- storm.htm

 rs-solar-storms-which-gives-power-can-also- take-it-away rs-solar-storms-which-gives-power-can-also- take-it-away

=HEheh1BH34Q

 Mercury, Venus, Earth, and Mars are called the terrestrial planets.  These planets lost most of their gases during development, therefore they have a more rocky composition.

 The planets that formed further from the Sun, were cool and massive enough to keep most of their hydrogen.  Jupiter, Saturn, Uranus, and Neptune are known as the Jovian Planets or the gas Giants

Revised by Claire Anne Baird Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, My Very Energetic Mother Just Served Us Nectarines

 In the Universe we are relatively small.  Specifically, Earth is located in the Solar System which is located within the Orion Spiral Arm of the Milky Way Galaxy. The Milky Way Galaxy is a part of the Local Galactic Group. The Local Galactic Group is within the Virgo Supercluster of galaxies within the Universe.