Touring Our Solar System

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Touring Our Solar System. Chapter 23. 23.1 The Solar System. 99.85% of the mass of our solar system is in the Sun, planets make up the rest. Gravity holds planets in orbit. Overview of the Planets Terrestrial planets : small and rocky Jovian planets : huge gas giants. - PowerPoint PPT Presentation

Transcript of Touring Our Solar System

Page 1: Touring Our Solar System
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Touring Our Solar System

Chapter 23

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23.1 The Solar System

99.85% of the mass of our solar system is in the Sun, planets make up the rest.

Gravity holds planets in orbit.A. Overview of the Planets

Terrestrial planets: small and rockyJovian planets: huge gas giants

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How long is Jupiter’s “year”? How long is Mercury’s “year?

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23.1 The Solar SystemInteriors of the PlanetsClasses: (based on melting

point)gases: H and He (-273oC)rocks: silicate and iron (> 700oC)ices: ammonia, methane, carbon dioxide, and water. (between others)

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23.1 The Solar System

Atmosphere of the Planets

Planets can only have an atmosphere if gravity is great enough.

Ex: Earth: 11 km/s escape velocity.

He and H escape from Earth.

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23.1 The Solar System

B. Formation of solar System.

Nebular TheorySun and planets formed from a rotating disk of gas and dust.

Planetesimals collided and built the planets and become round.

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23.2 Terrestrial Planets

A. Mercury:Smallest planet (no atmosphere)Dense with many cratersScraps from coolingTemperature:-173 to 427oC59 earth-day rotation88 earth-day revolution

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23.2 Terrestrial PlanetsB. Venus:255 Earth-day “year”Thick crushing atmosphere (97%

carbon dioxide) 90x pressure Temperture-475oC

Radar maps shows basaltic volcanism and tectonic activity.

Most flat plains with few mountains.

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23.2 Terrestrial PlanetsC. Mars:Polar caps made of CO2

Large long dust stormsMost atmosphere escapedOlympus Mons- 23 km highValles Marineris

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23.2 Terrestrial PlanetsC. Mars:Rovers discovered marks of liquid

water on Mars

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23.3 Outer Planets (and Pluto)Jupiter: Giant Among Planets1/800 of Sun Mass2.5x greater then all others

planets together.Great Red Spot- seen cyclonic

storm seen Giovanni Cassini about 1690.

Structure: pressure to make hydrogen into a liquid.

May have rocky core.

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23.3 Outer Planets (and Pluto)Jupiter:Moons:Io- volcanicEurpoa- fractured icy surfaceGanymede- largest, parallel

grovesCallisto- many craters

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23.3 Outer Planets (and Pluto)Jupiter:Rings:Very faint

Maybe fragments of 2 smaller moons

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23.3 Outer Planets (and Pluto)Saturn:Rings: Main feature100 m thick

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23.3 Outer Planets (and Pluto)Saturn:Moons:56 currentlyTitan – largest

Atmosphereand hydrocarbon seas

Enceladus-volcanic and water geysers

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23.3 Outer Planets (and Pluto)Uranus: Planet on its

side.

Winking star was a sign of a ring (9)

Miranda

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23.3 Outer Planets (and Pluto)Neptune: Windy Planet1000km/hrGreat Dark Spot: Storm

like Giant red Spot.Vanished! Repapered.Methane clouds.Triton –retrograde and

volcanic

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23.3 Outer Planets (and Pluto)Pluto: Dwarf PlanetFails to attract object

in its orbit. (clearing its orbit)

228 yearsCharon-moon

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23.4 Minor MembersNEAR ShoemakerLanded on asteroid

ErosVery low gravityMost asteroids are

between Mars and Jupiter.

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23.4 Minor MembersCometsMade of rocks, frozen

water, methane, carbon dioxide and carbon monoxide.

Very elongated orbits.Tail points away from

the sun.

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23.4 Minor MembersCometsMany short period

come from the Kuiper Belt

Long period come from the Oort Cloud

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23.4 Minor MembersCometsHalley’s Comet1986 Giotto probe

passed within 600 km

8 km x 16 km

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23.4 Minor MembersMeteoroidsAge of meteorites are

about 4.567 billion years old.

Made mostly of iron.Meteor Showers-

annual event from comet passes across Earth’s orbit.