Transcript Chapter 29 - solar system

Ch. 29 – The Solar System
The planets within the solar system have various sizes,
surface conditions, internal structures. They all orbit the
Sun in the same direction and similar planes.
Pluto
is no longer considered a planet.
Early astronomers assumed that the Sun, planets, and
stars orbited a stationary Earth in what is now known as
a geocentric model.
Planetary motion was difficult to explain with this
geocentric model.
Mars for example will undergo a retrograde motion,
where it moves in the opposite direction across the sky.
Fig. 29-1 (pg. 776)
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 Nicolaus Copernicus was the first to suggest that the
Sun was the center of the solar system, which is
referred to as a heliocentric model.
This would explain that the planets closer to the Sun orbit
quicker, thus when Earth moves past Mars’ orbit it appears
as though Mars is moving backwards in the sky – retrograde
motion.
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 Other scientists started to build on these astronomy
discoveries. Tyco Brahe made several accurate
observations of planetary positions during his time.
Johannes Kepler used Brahe’s data to explain that
planets orbit the Sun in an ellipse, rather than in a
circle. This is known as Kepler’s first law.
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Video
 An ellipse is an oval shape that is centered on 2 points
instead of a single fixed point.
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Minilab – pg. 777
 Each planet’s average distance between it and the
Sun is called astronomical units.

The Earth has a AU of 1, which is the standard of all the
other planets.
 When a planet is closest to the Sun in its orbit we call
this perihelion.
 When a planet is farthest away from the Sun we call
this aphelion.
 The shape of the planet’s elliptical orbit is defined as
eccentricity.

This value ranges from 0 to 1
• O being a perfect circle & 1 being a parabola.
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 Kepler’s 2nd law described that an imaginary line
between the Sun and a planet sweeps out equal
of area in equal amounts of time. Fig. 29-4
`amounts
(pg. 778)
 Kepler’s 3rd law found that the sqaure of the orbital
period equals the cube of the semimajor axis. P2 = a3.
 Galileo used the first telescope to view many celestial
bodies in the solar system during this time.
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Jupiter’s 4 moons provide that not all objects orbit the Earth.
 Newton then proved the discoveries mathematically by
stating 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 distances between them
Universal Gravitation F = G (M1*M2/r2).
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The Terrestrial Planets
 Terrestrial Planets are the inner 4 planets,
which are close in size and have solid, rocky
surfaces.
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 Mercury – closest to the Sun.
 1/3 the size of Earth
 No moons
 Slow rotation – 1407.6 hours
 Orbit – 87.969 days
 In 2 of Mercury’s years, 3 of Mercury’s days have
passed.
 No Atmosphere – primarily oxygen & sodium
• Surface temp. of 427°C (day) & -173°C (night)
 Mercury (Cont.)
 Surface is covered with craters and plains
• Surface gravity is much greater than the Moon.
 Observation
suggest that Mercury may have been
much bigger in size (Earth-like). It is similar to
Earth without a mantle or crust.
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 Venus
 No Moons
 Brightest planet in Earth’s nighttime sky.
• Albedo of .75
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Venus day is 243 Earth days  Clockwise spin
• The Sun would rise in the West and set in the East
 Venus
is most similar to Earth with diameter, mass,
and density.
 Venus (Cont.)
 Average surface temp. = 464°C
 The atmospheric pressure is 92 atm., compared to Earth’s 1
atm. at sea level.
 Atmosphere is mainly carbon dioxide and nitrogen.
• Lots of clouds with sulfuric acid instead of water.
Hottest planet
 Smooth surface with volcanic flows .
 The interior of Venus is most likely similar to Earth because
of similar densities and size.
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 Mars
 4th from the Sun
 Called the red planet
• High Iron content
 Mars (Cont.)
 Smaller and less dense than Earth.
 2 irregularly shaped moons
• Phobos and Deimos
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Atmosphere similar to Venus
• The density and pressure are much lower than Venus.
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Thin atmosphere with constant wind.
• Dust storms that can last for weeks.
The southern hemisphere surface is covered in craters,
while the northern hemisphere is plains.
 The largest volcano is Olympus Mons
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• This is the largest mountain in the solar system.
Several erosion features suggests that liquid water once
existed on the surface of Mars.
 If Mars had a thicker atmosphere it would hold liquid water.
 Both poles have caps of “dry ice” – solid carbon dioxide.
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The Gas Giant Planets
 The gas giant planets are much larger, more
gaseous, and lack solid surfaces.
 Jupiter
planet & 5th from the Sun
 11 times larger than Earth
 Has 4 major satellites & several smaller ones
 Largest
• Io actually had volcanic activity.
 Jupiter
has a low density (lightweight elements)
 The atmosphere is mainly H & He.
 Has a layer of liquid metallic hydrogen.
 Jupiter spins on it’s axis every 10 hours.
• Shortest rotation in the solar system.
 Jupiter (Cont.)
 Jupiter’s Great Red Spot is an atmospheric storm
that has been rotating around Jupiter for more than
300 years.
 All 4 major moons have composed of ice and rock
mixtures.
• Europa is thought to still have a subsurface ocean of
liquid water.
 Jupiter’s
ring is 6400 km wide.
• All four gas giant planets.
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 Saturn
 6th planet from the Sun.
 2nd largest planet
 Atmosphere is primarily H & He.
 Saturn (Cont.)
 Broadest rings for among the planets.
• There are 7 major rings which are made of ringlets.
 Titan
is the largest moon of Saturn.
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 Uranus
 7th planet from the Sun.
 Discovered accidentally in 1781.
 Uranus is 4 times as large and 15 times as massive
as Earth.
 Most of Uranus’ atmosphere is He & H, but the
methane reflects light which cause a bluish
appearance.
 The rotation axis of Uranus is tipped over so far that
the north pole almost lies in its orbital plane.
 Uranus (Cont.)
 Each pole spends 42 Earth years in darkness and 42 years
in sunlight due to this tilt and Uranus’s long trip around the
Sun.
 The planet’s temp. is around -215° C.
 New moons are frequently being discovered just like Jupiter
and Saturn, so the moon count constantly changes.
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 Neptune
 Neptune was predicted to be present before it was ever
observed due to the law of gravitation.
 Neptune is slightly smaller and denser than Uranus.
 Neptune is very similar to Uranus, except for an atmosphere
with clouds and belts.
 Neptune had a persistent storm, the Great Dark Spot, but it
disappeared in 1994.
 Triton, Neptune’s moon, orbits backward unlike virtually
every other satellite in the solar system.
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Formation of Our Solar System
 Scientists use observations and data from
probes to take a look at the formation of the
solar system in regard to the shape of our solar
system, the differences among the planets, and
the oldest planetary surfaces, asteroids,
meteorites, and comets.
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 Stars and planets form from clouds of gas and
dust called interstellar clouds.
 Made
primarily of He & H.
 Interstellar clouds may start to condense as a result
of gravity and become concentrated enough to form
a star and possibly planets.
 As a collapsing cloud spins, the cloud flattens
and the cloud concentration becomes dense at
the center.
 The disk of dust and gas has now formed a
solar nebula – a beginning star.
 The
temps reach 2000 K.
 Jupiter was the first large planet to develop.
 There re 1000s of bodies that orbit the Sun within the
planetary orbits – these are called asteroids.
They range from a few Km to 1000 Km in diameter.
 Most are located between Mars and Jupiter.
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 When any interplanetary material enters Earth’s
atmosphere it is called a meteoroid.
 The streak of light produced by this is called a meteor,
as the meteoroid burns up.
 If it doesn’t burn up completely and collides with the
ground its then called a meteorite.
 There are impact craters on Earth.
Meteor Crater – Arizona
 Gosses Bluff in Central Australia
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 Comets are small, icy bodies that have highly
eccentric orbits around the Sun.
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When comets are within 3 AU of the Sun, it begins to
evaporate, becomes brighter, and forms a head and one or
more tails.
• Hale-Bopp (fig. 29-30)
The coma is the head of the comet.
 The nucleus is the solid core.
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• It releases gas and dust when heat – thus forming a tail.
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The tails are pushed away from the coma by particles, ions,
and radiation coming from the Sun.
• Tails always point away from the Sun because of this.
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Each time a comet pass the Sun it vaporizes some of the
comet’s ice and it loses some of its matter.
• I may eventually break apart completely as the remaining ice
evaporates.
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Video