A background to Mars exploration and research

Author:

Bargery Alistair S.1,Balme Matthew R.2,Warner Nicholas3,Gallagher Colman J.4,Gupta Sanjeev3

Affiliation:

1. Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UK

2. Department of Earth Science, Open University, Walton Hall, Milton Keynes MK7 6AA, UK

3. Department of Earth Science and Engineering, Imperial College, Prince Consort Road, London SW7 2PB, UK

4. Geography, Planning & Environmental Policy, Newman Building, University College Dublin, Belfield, Dublin 4, Ireland

Abstract

AbstractMars is the fourth planet in our Solar System and orbits roughly 230×106 km from the Sun. It has an orbital period of 687 Earth days and a solar day that is approximately 40 min longer than an Earth day. Mars is less dense and has half the radius of the Earth, and so has about one-tenth the mass; hence, the surface gravity of Mars is about four-tenths that of the Earth. Mars has no oceans and its surface area is therefore almost as large as that of Earth's continents. In this chapter, we present a summary of the Martian environment, global geography and geology, and provide some background on the missions and instruments that have played a role in developing our current understanding. Our aim is to provide a broad overview for those unfamiliar with Mars, rather than providing an exhaustive summary of every aspect of the planet's evolution.

Publisher

Geological Society of London

Subject

Geology,Ocean Engineering,Water Science and Technology

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