inventory of the solar system

28
Where did the solar system come from? Astr 221 2015 NW Chs. 8&9 Also: Sun – Moon -Eclipses

Upload: ezekiel-acevedo

Post on 03-Jan-2016

25 views

Category:

Documents


4 download

DESCRIPTION

Inventory of the Solar System. Astr 221 10/09/2013 Nightwatch Ch. 7 & 10. There are eight major planets with nearly circular orbits. Pluto and Eris are smaller than the major planets and have more elliptical orbits. What are the major features of the Sun and planets?. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Inventory of the Solar System

Where did the solar system come from?

Astr 2212015NW Chs. 8&9

Also:Sun – Moon -Eclipses

Page 2: Inventory of the Solar System

Evidence from Other Gas Clouds

• We can see stars forming in other interstellar gas clouds, lending support to the nebular theory.

Page 3: Inventory of the Solar System

Was our solar system destined to be?

• Formation of planets in the solar nebula seems inevitable.

• But details of individual planets could have been different.

Page 4: Inventory of the Solar System

• An oasis of life• The only surface liquid water in the solar system• A surprisingly large moon

Earth and Moon with sizes shown to scale

Earth

Page 5: Inventory of the Solar System

Giant Impact

Page 6: Inventory of the Solar System

First Quarter Second Quarter

Page 7: Inventory of the Solar System

Formation of Lunar Maria

Large impact Large impact crater crater weakens weakens crust.crust.

Heat build-Heat build-up allows up allows lava to well lava to well up to surface.up to surface.

Early surface Early surface is covered is covered with craters.with craters.

Cooled lava is Cooled lava is smoother and smoother and darker than darker than surroundings.surroundings.

Page 8: Inventory of the Solar System

Radius:

6.9 108 m

(109 times Earth)

Mass:

2 1030 kg

(300,000 Earths)

Luminosity:

3.8 1026 watts

Page 9: Inventory of the Solar System

Gravitational equilibrium:

Energy supplied by fusion maintains the pressure that balances the inward crush of gravity.

Page 10: Inventory of the Solar System

What is the Sun’s structure?

Insert TCP 6e Figure 14.3

Page 11: Inventory of the Solar System

The proton–proton chain is how hydrogen fuses into helium in Sun.

Page 12: Inventory of the Solar System

Sunspots

Are cooler than other parts of the Sun’s surface (4000 K)

Are regions with strong magnetic fields

Page 13: Inventory of the Solar System

Loops of bright gas often connect sunspot pairs.

Page 14: Inventory of the Solar System

The number of sunspots rises and falls in an 11-year cycle.

Insert TCP 6e Figure 14.21a unannotated

Insert TCP 6e Figure 14.21b unannotated

Page 15: Inventory of the Solar System

The sunspot cycle has something to do with winding and twisting of the Sun’s magnetic field.

Page 16: Inventory of the Solar System

Magnetic activity also causes solar prominences that erupt high above the Sun’s surface.

Page 17: Inventory of the Solar System

Charged particles streaming from the Sun can disrupt electrical power grids and can disable communications satellites.

Page 18: Inventory of the Solar System

AuroraBorealis

Page 19: Inventory of the Solar System

What causes eclipses?

• The Earth and Moon cast shadows.• When either passes through the other’s

shadow, we have an eclipse.

Page 20: Inventory of the Solar System

Lunar Eclipse

Page 21: Inventory of the Solar System

When can eclipses occur?

• Lunar eclipses can occur only at full moon.

• Lunar eclipses can be penumbral, partial, or total.

Page 22: Inventory of the Solar System

Solar Eclipse

Page 23: Inventory of the Solar System

When can eclipses occur?

• Solar eclipses can occur only at new moon.• Solar eclipses can be partial, total, or annular.

Page 24: Inventory of the Solar System

Why don’t we have an eclipse at every new and full moon? – The Moon’s orbit is tilted 5° to ecliptic plane.– So we have about two eclipse seasons each year, with a lunar

eclipse at new moon and solar eclipse at full moon.

Page 25: Inventory of the Solar System

Summary: Two conditions must be met to have an eclipse:

1. It must be full moon (for a lunar eclipse) or new moon (for a solar eclipse).

AND2. The Moon must be at or near one of the two points in its orbit where

it crosses the ecliptic plane (its nodes).

Page 26: Inventory of the Solar System
Page 27: Inventory of the Solar System

Predicting Eclipses• Eclipses recur with the 18-year, 11 1/3-day

saros cycle, but type (e.g., partial, total) and location may vary.

Page 28: Inventory of the Solar System