Chapter 3 The Solar System
Mar 26, 2015
Chapter 3
The Solar System
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
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
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.
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
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
CopernicusPolish astronomerFound Earth and planets revolved around
sun In the same directionAt different speedsThought the orbits were circular
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
PlanetsMove in an elliptical orbit
PlanetsPeriod of revolution the time it takes to go once around the
sunone yearMercury 88 days, Pluto 248 years
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
What keeps them there?
Inertia
Gravit
y
RotationPlanets spin on their axesOne rotation is a dayMercury 58 days, Jupiter 10 hours
Special Features of the PlanetsMercury
Many Craters– no atmosphere– no erosion
Slow rotation makes it hot and cold
Venus Thick atmosphere of
carbon dioxide Sulfuric acid clouds Greenhouse effect
– carbon dioxide traps heat.
– Makes Venus hotter than Mercury
Retrograde rotation - rotates backward
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
Two moons of Mars
PhobosDeimos
Jupiter
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
JupiterGives off more heat than it receives from
the sun.By far the largest planet.
16 moons 4 seen by Galileo
helped change science
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
SaturnMany rings
– complex system– made of water– weave in and
out
SaturnMany moons - Titan- the largest is
like the early Earth.
UranusTwice as far from the
sun as Saturn.Covered with ocean
of superheated water
Tilted on axisRings of methane
iceMany moons
NeptuneLike UranusHydrogen and
helium atmosphere
Surface of water and methane
Rings made of dust
Eight moons
TritonLarge moonThought to be
capturedRetrograde
revolutionout of plane of
Neptune’s rotation
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
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
MeteoritesLeave a crater where they hit the groundMeteorite Crater in ArizonaEvidence of meteorites from the moon
and from Mars
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
Solar wind
Nucleus
Coma
Tail
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.
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
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.
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.
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
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.
SpacecraftProbes have gone past all the planets
except PlutoHave sampled comets tailsHave taken pictures of planets and
moons.