Standard Handbook for Aeronautical and Astronautical Engineers

Chapter 16: Earth's Environment and Space

Section Editor: Michael J. Rycroft

PART 1. THE EARTH AND ITS ATMOSPHERE

Michael J. Rycroft

16.1. THE EARTH IN SPACE

The Universe began with the Big Bang, about 14 billion years ago. About 4.6 billion years ago, the Sun formed during the gravitational collapse of an enormous cloud of gas and dust. Rotating around the Sun was a disk of material out of which the planets grew. These planets now orbit the Sun in the ecliptic plane. Our Earth is the third planet away from the Sun.

The different materials within the Earth gradually separated, with the densest (iron) forming an electrically conductive core. Dynamo action in the core generates the geomagnetic field. Above is the mantle, a region which convects very slowly. The Earth has a relatively thin crust, a few tens of kilometres thick, compared with the Earth's equatorial radius of 6,378 km. The crust and uppermost mantle are made up of 12 tectonic plates, hundreds of kilometers or so thick, which move relative to each other at up to one centimeter per year.

The Earth's atmosphere has evolved through outgassing from the interior via volcanoes. Oxygen was generated by dissociation of water vapor; the hydrogen that was also formed gravitationally escaped into space. Oxygen is also generated via photosynthesis by plants.

The Earth's hydrosphere (oceans), atmosphere, biosphere and solid surface interact with each other in many complex ways. This area of science is now termed Earth Systems Science (Ernst 2000).

16.2. PROPERTIES OF THE EARTH'S ATMOSPHERE

This...

UNLIMITED FREE
ACCESS
TO THE WORLD'S BEST IDEAS

SUBMIT
Already a GlobalSpec user? Log in.

This is embarrasing...

An error occurred while processing the form. Please try again in a few minutes.

Customize Your GlobalSpec Experience

Category: Satellites
Finish!
Privacy Policy

This is embarrasing...

An error occurred while processing the form. Please try again in a few minutes.