Astro Class Home

Introduction

Constellations
& Observing

Missions/ Spacecraft

History

Solar System

Stars

Stellar Evolution

Milky Way

Galaxies

Universe

Cosmology

Relativity   

Tests

 

The Sun-Earth-Moon System

   Planet Earth

     LUNA: Earth's Moon

     Eclipses

     Lunar Structures

    Current Exploration

     Origin of Our Moon

Earth Science:

Vocabulary and Review

Index

Astronomy class:

The Solar System

ASTRONOMY Home Page
ASTRONOMY Class Syllabus

 Planet Earth

    Objectives

    Describe earth's shape and list physical data about Earth

    Compare and contrast the rotation and revolution of Earth

    Relate Earth's tilt and revolution to the change of seasons

 

Earth's Shape

  A sphere is what the earth is almost shaped like

It's rotating at around 1,000 miles per hour (at the equator), so naturally it bulges a little there.

Evidence

Before telescopes and space travel, how did people know the earth was a sphere? This was, in fact, well known, by Columbus' time.

  for example,
Aristotle, 384 - 322 B.C.
, noted that the shadow cast by the earth on the moon during a lunar eclipse was always rounded, never square or a line, so he reasoned that the earth must be spherical.

The moon during Lunar Eclipse: 

Rotation

Earth rotates on its axis,

like a wheel rotates on its axle.

About one rotation in 24 hours.

Sun, stars appear to move because of this rotation, but it's Earth that is moving relative to the heavens.

Magnetic Field
  [A Beginner's Guide to the Earth's Magnetosphere]
   [The Magnetosphere]

Same force (electromagnetic field) as that produced by a magnet.

Earth has North and South magnetic poles, like a magnet!

 Because: Earth has an iron core.

Note: The magnetic poles are not in exactly the same place
as the geographic N and S poles.

Other planets have magnetic fields:

- Jupiter's is very large, and very strong:

View the Magnetic Field of Jupiter at Views of the Solar System
(This is a large .avi movie.  This link will open it in a new browser window)

- The Voyagers' and Galileo's instruments had to be specially protected against damage from it!

- Saturn's is much weaker than Jupiter's.

SEASONS

  Factors determining the changes in earth's seasons:

Revolution: Around the sun, (our Year) coupled with the:

TILT Of the earth's Axis of Rotation,

and it is NOT related to the fact that:

  • In fact, the Earth is farther from the sun during the Northern Hemisphere summer than during the Northern Hemisphere winter.

 

ANGLE OF INCIDENCE:

  The angle at which the sun's rays strike the earth's surface.

  • The higher the angle, the stronger the sunshine per unit area. Also, the sun is up longer in summer than in winter.

  • EQUINOX

      When the sun is directly above the equator [SEE IT]

  • Length of day = Length of night
  • Start of spring/fall
  • ~20 March, ~21 September
  • SOLSTICE

      When the sun is farthest north or south of the equator.

      • Day is either longest or shortest of year.
      • Start of winter/summer
      • ~21 June, ~21 December

    Go to: LUNA: Earth's Moon to continue with this lesson.

      On to The Solar System, or Other Solar System Objects, or Eclipses

    Back to ASTRONOMY Home Page,
     ASTRONOMY Class Syllabus

    Last Updated 03/03/2008