Exploring the Solar System: A Fascinating Journey

 
The Solar System
 
Chapter 21
 
21.1 Structure of the Solar System
 
The sun is the center of our solar system
The sun and 9 planets make up our solar system
Planets “wander” or orbit around the sun at different distances
Sometimes when we view stars, we actually see planets that appear to be stars
Venus is the closest planet to Earth and is easily seen most nights
Stars are much farther away than planets so appear as tiny specks of light
 
Objects in the Solar System
 
Sun: largest star in the solar system-makes up 99%, 10x larger than Jupiter, made of gases (hydrogen)
The sun produces energy through nuclear fusion and applies gravity to all planets
Planets: reflect sunlight, spherical shaped object that orbits sun, classified/grouped as inner, outer, dwarf
Asteroids: small rocky objects orbiting sun between Mars & Jupiter (belt), range in size
Comets: Gas, dust, and ice orbiting sun and producing a glowing tail (melting), trillions in space
 
Planets
 
Inner: terrestrial/rocky: Mercury, Venus, Earth, Mars; smaller than outer planets
Outer: gas giants: Jupiter, Saturn, Uranus, Neptune; larger than inner planets
Dwarf: tiny mass, made of rock and ice: Pluto, Ceres, Eris, Makemake
 
Measuring Space
 
AU-astronomical unit is used to measure distance in space
It is the average distance from Earth to the sun
About 150 million kilometers
Each planet’s AU increases as it gets farther from the sun
See Chart p. 764
 
Motion of Planets
 
Sun’s gravitational pull on each planet prevents planets from drifting apart and keeps each planet on a
curved path around the sun
Revolution/revolve-is the time it takes a planet to travel once around the sun (year)
Rotation/spinning on axis-is the time it takes planet to spin once on the axis (day)
Copernicus proposed the idea that Earth and other planets orbit the sun (heliocentric model) instead of
Earth being in the center (geocentric model) in 1500’s
Kepler discovered in 1600’s that planet’s orbit is an ellipse and not a perfect circle and speed increases near
the sun
 
21.2 Inner Planets
 
Terrestrial planets are closest to the sun and made of rock/metal; have solid outer layers
Different sizes, atmospheres, and surfaces
See p. 769
 
Mercury
 
Smallest and closest to the sun
No atmosphere/wind, extreme changes in temps, many craters due to no erosion, solidified lava, cliffs
Very little change over time
Core, mantle, and crust
Largest impact crater in solar system: Caloris Basin 1550 km across formed billions of years ago
P. 770 See Red Table
 
Venus
 
Second closest to sun, hottest, about same size as Earth, many probes and landers visited
Dense atmosphere of CO2 & thick acidic clouds cover the planet
Greenhouse effect traps energy
80% is covered with solidified lava
A day is longer than a year due to slow rotation; rotates east to west
Core, mantle, and crust                                                  p. 771 See Red Table
 
Earth “third rock from the sun”
 
Third planet from the sun; has a moon
Protective atmosphere provides water and temps to support life
Greenhouse effect traps energy
Only planet with liquid water on the surface
Core, mantle, crust
Crust is broken into pieces/ plates that constantly move to create and destroy more crust
P. 772 See Red Table
 
Mars
 
Fourth from the sun; reddish color due to iron oxide (rust) in the soil; many probes have visited
No water or life; polar ice caps hint to water once being available
Thin atmosphere of CO2, extreme temps, Covered with craters and solidified lava; large & long lasting dust
storms
Valles Marineris- largecanyon; larger that the U.S.
Martian Olympus volacano- largest mountain in solar system; wide as Arizona and higher than Everest
P. 773 See Red Table
 
21.3 Outer Planets
 
Gas giants with liquid interiors-hydrogen and helium
Small solid cores
Strong gravitational pull due to large mass/size
All have a rings
 
Jupiter
 
5th planet, largest-twice the mass of all other planets combined, thick atmosphere of clouds
Rotates faster than any other planet causing dense, colorful clouds to stretch out and appear as rings
Solid core surrounded by liquid hydrogen- mostly made of hydrogen & helium
63+ moons (more than any other planet), discovered by Galileo so the 4 largest are Galilean moons
Io, Europa, Ganymede, and Callisto  are all made of rock and ice
P. 778 See Red Tables
 
Saturn
 
6th planet, considered the ringed planet due to 7 bands of rings of chunky ice and stretched clouds
Least dense planet
Solid core with layer of liquid hydrogen and gas outer layer - mostly made of hydrogen and helium
60+ moons; largest is Titan and it is the only moon in the solar system with an atmosphere
P. 779 See Red Table
 
Uranus
 
7th planet, seems to orbit the sun like a rolling ball due to sideways tilt
So far away, only 1 space probe (Voyager 2) explored it in 1986
Thick atmosphere with thick, slushy layer of water and ammonia - mostly made of hydrogen & helium and
methane gas
We assume it has a core surrounded by water, ice and gases
27+ moons
P. 780 See Red Table
 
Neptune
 
8th planet with not as much knowledge due to lack of exploration
Voyager 2 explored it in 1989 (took 3 years to travel from Uranus to Neptune)
Huge storm (dark spot) was detected in 1989 but gone 5 years later
Atmosphere made of hydrogen, helium and methane gas
13+ moons
P. 781 See Red Table
 
21.4 Other Space Objects
 
Dwarf planets are objects that orbit the sun, has enough mass & gravity to form a sphere and has other
similar objects orbiting near it-new classification in 2006
Pluto, Ceres (smallest), Eris, (largest) MakeMake, and Haumea are dwarf planets
All are smaller than our moon
Pluto is ⅔ size of our moon, very cold (frozen), 3 moons, and takes 248 years to revolve around the sun
Explored by the Hubble Telescope
 
Asteroids & Comets
 
Most asteroids are located in the asteroid belt & orbit the sun; made of chunks of rock and ice tightly
clumped together
Some asteroids are larger than your school
Comets also orbit the sun but produce a coma (bright tail) of melting ice; tail burns on opposite side of sun
Comets are loosely clumps of ice and gas
See p. 787
 
Meteoroids
 
Small rocky object that moves through space; produces a streak of light in Earth’s atmosphere called
meteor; once it collides with another object/planet it is a meteorite
Most are the size of a grain of sand
The collision of meteorites forms an impact crater-round depression formed on the planet
More than 170 impact craters on Earth (Wetumpka, AL)
 
TEST TIME
 
Know vocab
Study main ideas on p, 792
Complete review p. 793-795
Read about the confusing topics in the textbook
Google confusing topics
Study highlighted bullets on Power Point
Slide Note
Embed
Share

Delve into the structure of the solar system, with the sun at its center surrounded by planets, asteroids, and comets. Learn about the inner rocky planets, outer gas giants, and tiny dwarf planets. Discover how distance is measured in space using astronomical units and unravel the motion of planets as they orbit the sun.

  • Solar System
  • Planets
  • Space Exploration
  • Astronomy
  • Sun

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  1. The Solar System Chapter 21

  2. 21.1 Structure of the Solar System The sun is the center of our solar system The sun and 9 planets make up our solar system Planets wander or orbit around the sun at different distances Sometimes when we view stars, we actually see planets that appear to be stars Venus is the closest planet to Earth and is easily seen most nights Stars are much farther away than planets so appear as tiny specks of light

  3. Objects in the Solar System Sun: largest star in the solar system-makes up 99%, 10x larger than Jupiter, made of gases (hydrogen) The sun produces energy through nuclear fusion and applies gravity to all planets Planets: reflect sunlight, spherical shaped object that orbits sun, classified/grouped as inner, outer, dwarf Asteroids: small rocky objects orbiting sun between Mars & Jupiter (belt), range in size Comets: Gas, dust, and ice orbiting sun and producing a glowing tail (melting), trillions in space

  4. Planets Inner: terrestrial/rocky: Mercury, Venus, Earth, Mars; smaller than outer planets Outer: gas giants: Jupiter, Saturn, Uranus, Neptune; larger than inner planets Dwarf: tiny mass, made of rock and ice: Pluto, Ceres, Eris, Makemake

  5. Measuring Space AU-astronomical unit is used to measure distance in space It is the average distance from Earth to the sun About 150 million kilometers Each planet s AU increases as it gets farther from the sun See Chart p. 764

  6. Motion of Planets Sun s gravitational pull on each planet prevents planets from drifting apart and keeps each planet on a curved path around the sun Revolution/revolve-is the time it takes a planet to travel once around the sun (year) Rotation/spinning on axis-is the time it takes planet to spin once on the axis (day) Copernicus proposed the idea that Earth and other planets orbit the sun (heliocentric model) instead of Earth being in the center (geocentric model) in 1500 s Kepler discovered in 1600 s that planet s orbit is an ellipse and not a perfect circle and speed increases near the sun

  7. 21.2 Inner Planets Terrestrial planets are closest to the sun and made of rock/metal; have solid outer layers Different sizes, atmospheres, and surfaces See p. 769

  8. Mercury Smallest and closest to the sun No atmosphere/wind, extreme changes in temps, many craters due to no erosion, solidified lava, cliffs Very little change over time Core, mantle, and crust Largest impact crater in solar system: Caloris Basin 1550 km across formed billions of years ago P. 770 See Red Table

  9. Venus Second closest to sun, hottest, about same size as Earth, many probes and landers visited Dense atmosphere of CO2 & thick acidic clouds cover the planet Greenhouse effect traps energy 80% is covered with solidified lava A day is longer than a year due to slow rotation; rotates east to west Core, mantle, and crust p. 771 See Red Table

  10. Earth third rock from the sun Third planet from the sun; has a moon Protective atmosphere provides water and temps to support life Greenhouse effect traps energy Only planet with liquid water on the surface Core, mantle, crust Crust is broken into pieces/ plates that constantly move to create and destroy more crust P. 772 See Red Table

  11. Mars Fourth from the sun; reddish color due to iron oxide (rust) in the soil; many probes have visited No water or life; polar ice caps hint to water once being available Thin atmosphere of CO2, extreme temps, Covered with craters and solidified lava; large & long lasting dust storms Valles Marineris- largecanyon; larger that the U.S. Martian Olympus volacano- largest mountain in solar system; wide as Arizona and higher than Everest P. 773 See Red Table

  12. 21.3 Outer Planets Gas giants with liquid interiors-hydrogen and helium Small solid cores Strong gravitational pull due to large mass/size All have a rings

  13. Jupiter 5th planet, largest-twice the mass of all other planets combined, thick atmosphere of clouds Rotates faster than any other planet causing dense, colorful clouds to stretch out and appear as rings Solid core surrounded by liquid hydrogen- mostly made of hydrogen & helium 63+ moons (more than any other planet), discovered by Galileo so the 4 largest are Galilean moons Io, Europa, Ganymede, and Callisto are all made of rock and ice P. 778 See Red Tables

  14. Saturn 6th planet, considered the ringed planet due to 7 bands of rings of chunky ice and stretched clouds Least dense planet Solid core with layer of liquid hydrogen and gas outer layer - mostly made of hydrogen and helium 60+ moons; largest is Titan and it is the only moon in the solar system with an atmosphere P. 779 See Red Table

  15. Uranus 7th planet, seems to orbit the sun like a rolling ball due to sideways tilt So far away, only 1 space probe (Voyager 2) explored it in 1986 Thick atmosphere with thick, slushy layer of water and ammonia - mostly made of hydrogen & helium and methane gas We assume it has a core surrounded by water, ice and gases 27+ moons P. 780 See Red Table

  16. Neptune 8th planet with not as much knowledge due to lack of exploration Voyager 2 explored it in 1989 (took 3 years to travel from Uranus to Neptune) Huge storm (dark spot) was detected in 1989 but gone 5 years later Atmosphere made of hydrogen, helium and methane gas 13+ moons P. 781 See Red Table

  17. 21.4 Other Space Objects Dwarf planets are objects that orbit the sun, has enough mass & gravity to form a sphere and has other similar objects orbiting near it-new classification in 2006 Pluto, Ceres (smallest), Eris, (largest) MakeMake, and Haumea are dwarf planets All are smaller than our moon Pluto is size of our moon, very cold (frozen), 3 moons, and takes 248 years to revolve around the sun Explored by the Hubble Telescope

  18. Asteroids & Comets Most asteroids are located in the asteroid belt & orbit the sun; made of chunks of rock and ice tightly clumped together Some asteroids are larger than your school Comets also orbit the sun but produce a coma (bright tail) of melting ice; tail burns on opposite side of sun Comets are loosely clumps of ice and gas See p. 787

  19. Meteoroids Small rocky object that moves through space; produces a streak of light in Earth s atmosphere called meteor; once it collides with another object/planet it is a meteorite Most are the size of a grain of sand The collision of meteorites forms an impact crater-round depression formed on the planet More than 170 impact craters on Earth (Wetumpka, AL)

  20. TEST TIME Know vocab Study main ideas on p, 792 Complete review p. 793-795 Read about the confusing topics in the textbook Google confusing topics Study highlighted bullets on Power Point

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