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Dive into the fascinating Nebular Theory and the formation of our Solar System. Learn about the planetary evolution and characteristics, from the Terrestrial to Gas/Ice Giants, and explore the measurements and components of the inner solar system. Enhance your knowledge with engaging activities and discover the wonders of the universe!
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Warm-up 4/22/15 Take out your Study Guides!! Review for 10 minutes Target TEST TIME!
Diagram 1 Diagram 4 Diagram 7 Diagram 5 Diagram 2 A B C 8 5 D Diagram 8 Diagram 3 Diagram 6
THE SOLAR SYSTEM \ Update your Table of Contents! 3
Origin of the Solar System • Our solar system formed 4.6 billion years ago. • Would you believe me if I told you it formed from a large cloud of dust and gas? • http://www.youtube.com/watch?v=Uhy1fucSRQI
The Nebular Theory • Nebular Theory- solar system formed from a rotating cloud of dust and gas. • Solar nebula- a large, thin cloud of dust and gas. • Formed from material expelled by previous stars.
The Nebular Theory • (A): • Nebula began with slight rotation… • As the cloud contracted, it began to spin faster… • More gravitational attraction between particles (dust)… • Nebula shrinks, accelerating the process.
The Nebular Theory • (B): • Solar nebula rotates faster… • Begins to flatten out… • Over 100,000 yrs a protoplanetarydisk formed (looks like a giant fried egg)… • The disk was densest in the center and thinner toward the edges.
The Nebular Theory • (C): • About 99.9 % of the mass became concentrated at the center (egg yolk)… • This became our sun. • At this time our sun was a few million degrees!
The Nebular Theory • (D): • Dust grains are colliding… • Weak forces hold them together… • Forming loose balls of dust… • As these balls of dust collided they grew larger… • …formed planetesimals.
The Nebular Theory • (D): • Planetesimals(asteroid like bodies that eventually combined to form planets) grew by accretion (process of adding mass by colliding with other planetesimals)…
Protoplanets • Once they grew large enough they had a gravitational force… • Attracted more material… • Became larger… • Now protoplanets… • Protoplanets formed current planets in a series of violent collisions.
E.Terrestrial Planets • Terrestrial planets- Mercury, Venus, Earth and Mars. • Small, and rocky planets. • Why aren’t they as large as the gas giants? • Answer- it was too hot near the sun, and much of the material couldn’t condense… • …not until it got farther from the sun.
E. Gas/Ice Giants • Ice forming materials (water, ammonia, methane, etc.) condensed farther away from the sun (it’s colder) • As these planets grew, gravity increased, and these planets captured Hydrogen (H) and Helium (He) from space…grew even larger!!
Can you come up with saying to help you remember the order?? • How many planets do we have in our Solar System? • List them. 14
Warm-up 4/24/15 1. Describe the Nebular Theory and how our Solar System was formed. 2. List the 8 planets that make up our Solar System.
Bellwork 4/27/15 • On Your Desk: • PRIDE Card • I.N. • Pen/Pencil • Which planet is the largest in size? • Jupiter is the largest planet. • 2. Which planet is the smallest in size? • Mercury is the smallest planet. • 3. List the rocky planets. • Mercury, Venus, Earth and Mars are the 4 rocky planets.
On Your Desk: • PRIDE Card • I.N. • Pen/Pencil Warm-up 4/28/15 • 1. How many planets away from the SUN is your planet (or object in the solar system)? • 2. How many planets away from the EARTH is your planet (or object in the solar system)?
Planet Brochure Day 1: Research *Cite your sources Day 2: Rough Draft Day 3/4: Final Draft **Due Thursday!!!
Warm-up 4/29/15 • On Your Desk: • PRIDE Card • I.N. • Pen/Pencil • Rough Draft • 1. List two amazing things you learned about your planet!!
SONGS!!! Planets Around a Star: http://www.cleanvideosearch.com/media/action/yt/watch?v=nQfJ7j2UGGk Planets Song: http://www.cleanvideosearch.com/media/action/yt/watch?v=GH61v4_eVNA
Asteroids Comets Meteors Meteoroids Meteorites Use Chapter 4: Section 5 to discover the differences! -Create “Flip” Cards for each vocabulary term
Measurements • Light Year: distance that light travels in a year • Used for measurements within our galaxy • 5.88 trillion miles in a year • 1 light year equals 63,000 AU • AU: Astronomical Unit • Used for measurements within our solar system • Distance from Earth to Sun • 1 AU equals 93,000,000 miles
Inner solar system… • Consists of: • Sun • Mercury • Venus • Earth • Moon • Mars • Asteroid belt • Ceres • Other debris • Asteroids
Sun • Contains 99.8% of all the mass of the solar system • Only star in our solar system • 865,000 miles in diameter
Mercury • Closest planet to the sun • The smallest of the 8 planets • 2nd hottest planet • Very rocky… like Earth • No stable atmosphere
Venus • 2nd closest planet to the sun • Hottest planet • Reach 860 degrees Fahrenheit • Dense atmosphere • Mainly Carbon Dioxide • Greenhouse effect • Why its so hot! • Sister planet
Mars • 4th planet from the sun • After Earth • Atmosphere mainly Carbon Dioxide • Polar ice caps • Frozen water • Used to have liquid water in the past
Asteroid belt • Rocks that never clumped together to form a planet • Proto-planet • Ceres • Can sometimes make way into inner solar system
Outer solar system… • Consists of: • Jupiter • Saturn • Uranus • Neptune • Kuiper belt • Pluto • Scattered disc • Eris
Jupiter • Largest planet in solar system • Mainly Hydrogen and Helium • Enough gravity to hold onto these light elements • Not rocky… Gas giant • Has 63 moons… 47 of which are named
Saturn • 2nd largest planet • Known for its ringsdebris orbiting the planet • Very similar to Jupiter • One of its moons, Titan, is larger than Mercury… and is the only moon to possess an atmosphere
Uranus • 7th planet from the sun • Completely tilted on its axis • 97.77 degrees • Winds can reach up to 560 mph • Many poisonous gases in the atmosphere
Neptune • Farthest planet from the sun • Fastest winds in the solar system • 1300 mph • Methane atmosphere • Dark spots are huge hurricanes
Kuiper belt • This is where Pluto is found • Similar to the asteroid belt • Contains debris that didn’t become part of a planet
Put it all together… Mercury-Venus-Earth-Mars-Asteroid belt-Jupiter-Saturn-Uranus-Neptune-Kuiper belt (Pluto)-Scattered disc (Eris)