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Chapter 3 The Solar System
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Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Mar 26, 2015

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Page 1: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Chapter 3

The Solar System

Page 2: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

How was it formedThe Nebular TheoryStarted as nebula about 5 billion years ago

– Composed of hydrogen and heliumNearby supernova sent shock waves

through galaxy– caused gases to be pulled inward– supplied new elements

Shrank to a spinning disk –10 billion kilometers across

Gravity heated center to protostar - the sun

Page 3: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

How was it formedOther matter spun around the new sungathered into clumps- protoplanetsNear the sun the light weight gases

boiled away– Mercury, Venus, Earth, Mars

In those far away the gases did not boil away

– Jupiter, Saturn, Uranus, Neptune– the gas giants

Page 4: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

How was it formedAround the protoplanets smaller clumps

formed moons or satellites.Pluto is thought to be a moon of Neptune

that broke away.Asteroid belt- clumps of rocks between

Mars and JupiterJupiter’s gravity stopped a planet from

formingOort Cloud- Near the edge clumps of

matter- home of comets.

Page 5: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

HistoryPeople have used the stars for ages.Used constellations to set planting timesUsed constellations to guide travelsSome lights in the sky wandered through

the constellationsCalled them “planets” which is Greek for

wanderers

Page 6: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

PtolemyGreek scientistPlaced earth at center of universeOther objects moved in orbits around the

earthBecause circle was considered a perfect

shape, thought they moved in circular paths

Page 7: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

CopernicusPolish astronomerFound Earth and planets revolved around

sun In the same directionAt different speedsThought the orbits were circular

Page 8: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

KeplerGerman mathematician and astronomerUsed others observations (Tycho Brahe)Calculated the orbits of planets were

ovals or ellipsesCloser to the sun - shortest time of orbitFarther from the sun - greater time

Page 9: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

PlanetsMove in an elliptical orbit

Page 10: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

PlanetsPeriod of revolution the time it takes to go once around the

sunone yearMercury 88 days, Pluto 248 years

Page 11: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

What keeps them there?Law of inertia - objects motion won’t

change unless acted upon by an outside force.

Won’t change speed or directionWhy do they curve?Gravity pulls them toward the sun

Page 12: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

What keeps them there?

Inertia

Gravit

y

Page 13: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

RotationPlanets spin on their axesOne rotation is a dayMercury 58 days, Jupiter 10 hours

Page 14: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Special Features of the PlanetsMercury

Many Craters– no atmosphere– no erosion

Slow rotation makes it hot and cold

Page 15: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Venus Thick atmosphere of

carbon dioxide Sulfuric acid clouds Greenhouse effect

– carbon dioxide traps heat.

– Makes Venus hotter than Mercury

Retrograde rotation - rotates backward

Page 16: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

MarsRed planet- covered by

iron oxide (rust)Mons Olympus - Largest volcano in the

solar systemTwo ice caps

– north - water -never melts– south -carbon dioxide

melts in summer

Page 17: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.
Page 18: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Two moons of Mars

PhobosDeimos

Page 19: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.
Page 20: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.
Page 21: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Jupiter

Page 22: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

JupiterLargest of the gas giantsHuge storms - red spotSmall solid coreLiquid metal layer makes a huge

magnetic fieldMagnetosphereGives off more heat than it receives from

the sunThin ring

Page 23: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

JupiterGives off more heat than it receives from

the sun.By far the largest planet.

Page 24: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

16 moons 4 seen by Galileo

helped change science

Page 25: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

SaturnSimilar to JupiterClouds, magnetosphere, gives off heatRotates in 10 hours - makes it bulge in

the middle and flat at the polesLow density- would float in water

Page 26: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

SaturnMany rings

– complex system– made of water– weave in and

out

Page 27: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

SaturnMany moons - Titan- the largest is

like the early Earth.

Page 28: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

UranusTwice as far from the

sun as Saturn.Covered with ocean

of superheated water

Tilted on axisRings of methane

iceMany moons

Page 29: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

NeptuneLike UranusHydrogen and

helium atmosphere

Surface of water and methane

Rings made of dust

Eight moons

Page 30: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

TritonLarge moonThought to be

capturedRetrograde

revolutionout of plane of

Neptune’s rotation

Page 31: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

PlutoMoon sizedMade of methane Pink atmosphere on the sunny sideMoon Charon 1/2 the size of PlutoScientists think it is a moon broken away

from Neptune– Orbit crosses Neptune– Orbit not in plane with other planets

Page 32: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Other StuffMeteor- the shooting star -the light you

see the skyMeteoroid- solid rocky objects circling the

sunMeteorite- When a meteor hits the groundMost don’t because they burn up in the

atmosphereSome meteoroids are iron and nickelSome are stonyOthers are combinations

Page 33: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

MeteoritesLeave a crater where they hit the groundMeteorite Crater in ArizonaEvidence of meteorites from the moon

and from Mars

Page 34: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

CometsChunks of dust and gas from the Oort

Cloud that orbit the sunWhen it gets close to the sun it gets

hotterSome of the gas and dust form a cloud

around the head called the comaSolar wind pushes the gases away from

the sun and make the tailTail is pushed by the solar windTail always points way from the sun

Page 35: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Solar wind

Nucleus

Coma

Tail

Page 36: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.
Page 37: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

CometsComets orbit the sunLong period comets take a long time to

go around– Thousands of years

Short period comets return every few years

– Halley’s every 75 to 79 years– Last time in 1986

Suspect a nearby star disrupts the Oort cloud to send more comets toward sun.

Page 38: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

AsteroidsChunks of planetlike material floating in

spaceMost between Mars and JupiterMost 1km in diameterCeres- 1000km in diameterSome pass near EarthCaused craters on moon, and inner

planets

Page 39: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Looking for lifeOn other planetsNeed liquid water and moderate

temperatures.Earth is just the right distance to have the

right temperaturesLooking for evidence of former life on

Mars- used to have water.On Titan atmosphere like early earth.

Page 40: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

RocketsRely on Netwon’s Third law of Motion

– For every action there is an equal and opposite reaction.

Reward blast of hot gases causes rocket to shoot forward.

First developed by Chinese in 1000– Tube full of gunpowder with cap on one

end.

Page 41: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Escape VelocityThe minimum speed needed to leave the

gravitational pull.Depends on mass of planet and distance

from the center of planet.– Earth 11.2 km/sec– Moon 2.3 km/sec– Jupiter 63.4 km/sec– Pluto 0.3 km/sec– Sun 616 km/sec

Page 42: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

Rockets and Escape Velocity

Solid rockets burn up fuel quickly– Large thrust early– Gravity eventually slows them down.

Liquid fuels provide continuous thrust.– Goddard- gasoline and liquid oxygen– Space shuttle liquid hydrogen and

liquid oxygenMultiple stages to reduce weight.

Page 43: Chapter 3 The Solar System. How was it formed l The Nebular Theory l Started as nebula about 5 billion years ago – Composed of hydrogen and helium l Nearby.

SpacecraftProbes have gone past all the planets

except PlutoHave sampled comets tailsHave taken pictures of planets and

moons.