Chapter 29 – The Solar System - Grygla Public School · Structure Liquid hydrogen ocean Halfway...
Transcript of Chapter 29 – The Solar System - Grygla Public School · Structure Liquid hydrogen ocean Halfway...
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CHAPTER 29 – THE SOLAR SYSTEM
Section 1 – Wrote notes on board
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SECTION 2 – THE INNER PLANETS
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The inner planets are also referred to as Terrestrial planets (Earth-like)
Mercury, Venus, Earth, Mars
Small, dense, rocky
Metal core
No rings
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Mercury Closest to the sun
Smallest planet now that Pluto is not a planet
Orbit period = 88 days
Planetary day = 59 days
Almost no atmosphere
Cold nights (-280 F)
Hot days (800 F)
Very dense, thought to have large iron core
No moons
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Venus Second planet from the sun
Orbit period = 225 days
Planetary day = 243 days
Rotates opposite on its axis
Second to the Moon in brilliance
Similar to Earth in
Size, Density, and Location
Shrouded in thick clouds of sulfuric acid
Atmosphere is 97% carbon dioxide
Surface atmospheric pressure is 100 times that of Earth’s
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Venus
The clouds of Venus do not allow visible light through
The Magellan orbiter produced radar images of the surface of Venus from 1990 to 1994
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Earth
Third planet from the sun
Fifth largest planet
One moon
Life is possible because of distance from sun
Venus to close…to hot for liquid water
Mars to far…to cold for liquid water
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Planets – A Brief Tour Mars
The “Red Planet”
Orbit period = 687 days
Planetary day = 24 hours 37 minutes
Cold polar temps (-193 F)
Polar caps of water ice, covered by thick layer of frozen carbon dioxide
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Mars Numerous large
volcanoes
Largest is Olympus Mons
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Mars Several canyons
Some larger than Earth’s Grand Canyon
Calles Marineras – The largest canyon
Almost 5000 km long
That’s as long as the U.S.
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Mars “Stream drainage”
patterns
Found in some valleys
No bodies of surface water on the planet
Possible origins
Past rainfall
Surface material collapses as the subsurface ice melts
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Planets – A Brief Tour Moons of Mars
Two moons
Phobos
Deimos
Captured asteroids
The fourth planet out from the Sun, Mars, has two moons. The are named Phobos (meaning "fear") and Deimos (meaning "panic"); appropriate companions for Mars, the God of War.
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SECTION 3 – THE OUTER PLANETS
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The outer planets are also referred to as the Jovian planets (Jupiter-like)
Jupiter, Saturn, Uranus, Neptune
Large, low-density, gaseous
Massive
Referred to as “Gas Giants”
All have rings, but Saturn's are the most prevalent
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Jupiter
5th planet from sun
Largest planet
Orbit period = 12 years
Very massive 2.5 times more massive
than combined mass of all the planets, satellites, and asteroids
If it had been ten times larger, it would have been a small star
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Jupiter
Rapid rotation
Slightly less than 10 hours
Slightly bulged equatorial regions
Banded appearance
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Jupiter
Great Red Spot
In planet’s southern hemisphere
Like a giant hurricane, has been going for hundreds of years
600 km/hr winds
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Jupiter
Structure
Liquid hydrogen ocean
Halfway into the interior, pressure causes liquid hydrogen to turn into metallic hydrogen
Core of rock and metallic minerals
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Jupiter
At least 28 moons
Four largest moons
Discovered by Galileo
Called Galilean satellites
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Saturn
Sixth planet from sun
Second largest planet
At least 20 moons
Orbit period = 29.5 years
Planetary day = 10 hours 40 minutes
Also has banded appearance
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Saturn
Saturn has such a low density (0.7 g/cm3) it would actually float in water!
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Uranus
7th planet from sun
3rd largest
Orbit period = 84 years
Planetary day = 17 hours
Uranus and Neptune are nearly twins
Rotates “on its side”
At least 15 moons
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Neptune
8th planet from sun
Orbit period = 165 years
Planetary day = 16 hours
Dynamic atmosphere
1,000 km/hr winds!
Great Dark Spot
Storm the size of Earth
White cirrus-like clouds above the main cloud deck
Eight moons
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Pluto
Now a “minor planet” or “planetoid”
Not visible with the unaided eye
Orbit period = 250 years
Planetary day = 6 days
Highly elongated orbit cases it to occasionally travel inside the orbit of Neptune, where it resided from 1979-1999
1 Moon (Charon)
The moon is half the size of Pluto
Average temp is -210 C
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Planets – A Brief Tour
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29.4 – ASTEROIDS, COMETS, AND METEOROIDS
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There are millions of smaller bodies of matter flying all around the solar system
Some are just bits of dust or ice, others are as large as small moons
They are leftover material from the nebula that formed our solar system
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Asteroids
Asteroids are the largest of the smaller bodies in the solar system
Fragments of rock that orbit the sun
More than 50,000 asteroids for sure, possible millions
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Asteroids have impacted the Earth, causing mass extinctions in the past
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Asteroids
Most lie between Mars and Jupiter in what is known as the Asteroid Belt
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Asteroids
Three main types of asteroids
1.) Made of carbon materials
Dark in appearance
2.) Made of iron and nickel
Metallic appearance
3.) Made of silicate minerals
Looks like ordinary earth rocks
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Asteroids
Some asteroids are not in the asteroid belt
Trojan Asteroids are in groups just ahead of and just behind Jupiter
Earth-grazers have very elongated orbits which brings them close to Earth at times
They can, and have, collide with Earth
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Planets – A Brief Tour
Comets Often compared to large “dirty
snowballs”
Composition Frozen Gases (water, methane, ammonia)
Rocky and metallic materials
Frozen gases vaporize when near the sun Produces a glowing head called the coma
Some develop a tail that points away from the Sun due to radiation pressure and solar wind
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Comets
Three main parts
1.) Nucleus
2.) Coma
3.) Tail
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Comets
Scientists think that comets come from a very distant cloud of dust and ice called the Oort Cloud
They are so far away from the sun that many take millions of years to orbit
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Comets
Long-period Comets – Periods of several thousands or even millions of years
Short-period Comets – Periods of around 100 years Halley’s Comet appears
every 76 years
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Meteoroids
Meteoroids are smaller bits of rock or metal
Called meteors when they enter Earth’s atmosphere
A meteor shower is when Earth encounters a swarm of meteoroids
Meteoroids are referred to as meteorites when they are found on Earth
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Meteoroids
Most are less than 1 mm in diameter
A large one would be greater than 1 cm in diameter
Can be produced by collisions between asteroids
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Meteoroids Most meteoroids burn up when entering
Earth’s atmosphere
This is what you are seeing when you see a “shooting star”
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Meteoroids
Three basic types of meteorites
1.) Stony Meteorites Similar to Earth rocks
2.) Iron Meteorites Metallic appearance
3.) Stony-iron Meteorites Contain both iron and stone (very rare)
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Meteorites from Mars?
Meteorite found in Antarctica in 1984
Thought to have come from Mars!
In 1996 scientists discovered fossil evidence of microorganisms
How could it have reached Earth? Why is this significant?
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