1.2 Evidence for continental drift
Plate tectonics is an earth sciences topic that attracts a good deal of interest, given that it a topic very often featured in popular science programmes on TV and radio. It is a subject that have strong visual appeal. The coverage is S279 is self-contained, up to date and is written in a way that will be accessible to those with interest and motivation, all the more so for those who have some pre-existing scientific understanding.
Author(s): The Open University

1.1 Continental drift
Plate tectonics is an earth sciences topic that attracts a good deal of interest, given that it a topic very often featured in popular science programmes on TV and radio. It is a subject that have strong visual appeal. The coverage is S279 is self-contained, up to date and is written in a way that will be accessible to those with interest and motivation, all the more so for those who have some pre-existing scientific understanding.
Author(s): The Open University

Preamble: the moving Earth
Plate tectonics is an earth sciences topic that attracts a good deal of interest, given that it a topic very often featured in popular science programmes on TV and radio. It is a subject that have strong visual appeal. The coverage is S279 is self-contained, up to date and is written in a way that will be accessible to those with interest and motivation, all the more so for those who have some pre-existing scientific understanding.
Author(s): The Open University

Introduction
Plate tectonics is an earth sciences topic that attracts a good deal of interest, given that it a topic very often featured in popular science programmes on TV and radio. It is a subject that have strong visual appeal. The coverage is S279 is self-contained, up to date and is written in a way that will be accessible to those with interest and motivation, all the more so for those who have some pre-existing scientific understanding.
Author(s): The Open University

Introduction
This unit lays the foundation of Newtonian mechanics and in particular the procedure for solving dynamics problems. The preresquisite skills needed for this unit are the ability to solve first and second-order differential equations, a knowledge of vectors, and an understanding of the concept of a force
Author(s): The Open University

Introduction
This unit is intended to further develop your understanding of Newtonian mechanics in relation to oscillating systems. In addition to a basic grounding in solving systems of differential equations, this unit assumes that you have some understanding of eigenvalues and eigenvectors.
Author(s): The Open University

1.4 Stellar masses and stellar evolution
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

The H–R diagram
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

2.5 Using stars to probe the interstellar medium
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

2.4 The effect of interstellar dust
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

2.3 The effect of interstellar gas
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

2.1 Introduction
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

1.4 Stellar masses and stellar evolution
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

1.2 The main classes of stars
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

1.1 Constructing the H–R diagram
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

Introduction
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
Author(s): The Open University

Social care, social work and the law - England and Wales
This unit is made up of four extracts related to social care, social work and the law. The extracts are stand-alone sections but follow on from each other to make up this unit. You will be introduced to five main themes that shape practice in the field of social care and social work. The aim of this unit is to enhance your understanding of the relationship between social work practice and the law.
Author(s): The Open University

Introduction

This unit will examine some of the key ideas connected with innovation in organisations. You will be introduced to some important concepts which are used to analyse innovation, in particular the distinction between innovation and invention. In exploring the theme of innovation, general links will be made to the implications for the business functions.

This material is from our archive and is an adapted extract from Understanding Business Functions (B202) which is n
Author(s): No creator set

Summary of Part E
Rules affect us all, and the way they are made and interpreted could effect how we live. This unit explores how we could interpret and apply rules, and provides you with a basic understanding of rules and rule making within the English legal system.
Author(s): The Open University

Introduction
Rules affect us all, and the way they are made and interpreted could effect how we live. This unit explores how we could interpret and apply rules, and provides you with a basic understanding of rules and rule making within the English legal system.
Author(s): The Open University