Rings, Moons and Pluto, Schemes and Mind Maps of Astronomy

All of the gas giants have rings. ▫ Composed of lots of small particles. ▫ From tiny moons to dust. ▫ Orbit planet because of its gravity.

Typology: Schemes and Mind Maps

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Rings, Moons and Pluto
September 30, 2002
1) Introduction
2) Rings
3) Moons
4) Pluto
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Rings, Moons and Pluto

September 30, 2002

Introduction

2) Rings 3) Moons 4) Pluto

Review

„

Outer Planets

„ Interior/Exterior „ Gas Giants „ Jupiter & Saturn „ Ice Giants „ Uranus & Neptune „

Tides

„ Forces „ Tidal Resonances

Saturn’s Rings

„

Complicated, intense ring system

„ Ring A – bright, narrow, with gaps „ Ring B – very wide with no gaps „ Rings C&D – close to the planet „ Rings E&G – very large, diffuse outer rings „

Cassini Division – separates the A&B rings

Other Rings

„

Jupiter

„ best seen lit from behind „ diffuse „

Uranus

„ 10 narrow rings „ one wide ring close to planet „

Neptune

„ 3 narrow, 3 wide „ arc-like segments within rings

Ring Stability

„

Rings want to spread out and disappear

„

Can be held together by gravity andcollisions

„ Temporary „

Can be held together by moons

„ Remember shepherd moons in

To Boldly Go

Moons

„ There are more than 90 moons – mostly in theouter Solar System „ Only 3 around the inner planets, Earth & Mars (2) „ Wide range of sizes „ Generally low mass and little or noatmosphere „ Categories – Geological Activity „ Currently active (confirmed) „ May be active „ Probably was active at one time „ Dead Moons

„

Moon of Jupiter

„ Very close to Jupiter „ Tidal forces heat the interior „

Very volcanically active

„ Most volcanically active object in the SolarSystem „ Several plumes observed by Voyager „ More than 300 volcanic sites have beenidentified „ Probably has turned itself inside out at leastonce

Io

May Be Active

„ No observed activity, but evidence of activity atone time „ less craters, more smooth surfaces „ Europa (Jupiter) „ rock with icy crust „ may contain liquid water below surface „ evidence of internal heating „ Titan (Saturn) „ dense atmosphere (35% denserthan Earth’s) „ evidence of water ice and liquidmethane

Dead Moons

„

No signs of geological activity sinceformation

„ lots of craters „

Include:

„ irregular moons „ often captured or remnants of older moons „ Callisto (Saturn) „ confusing data on formation/history „ Umbriel (Uranus) „ why wasn’t it active?

Pluto

„ Farthest of the planets (most of the time) „ Occasionally is closer than Neptune (elliptical orbit) „ Orbit takes 248 Earth years „ Charon „ Moon with 1/2 mass of Pluto „ Pluto and Charon are tidal locked „ Mass of Pluto + Charon is 1/ th that of Earth „ Rock, ice and methane „ Similar to Europa „ Like other objects in Kuiper Belt… „ Today, would not be classified a planet

Meteors

„

Parts of the Solar System that come tous

„ some of the moststudied astronomicalobjects „

Categories

„ stony meteorites „ iron meteorites „ stony-iron meteorites „ category depends upon source of meteor

Asteroids

„

Classification depends upon formation

„

C-type

„ cooled without differentiation „ snapshot of material of early Solar System „

S-type

„ differentiated – iron core, silicate crust „

M-type

„ iron core without crust