Abstract
Beyond the Earth’s orbit, at a mean distance of228million km from the Sun, lies the orbit of the planet Mars. Mars is thus the first of thesuperior planets(planets which orbit the Sun at greater distances from it than the Earth does). Mars has the highest orbital eccentricity of all the major planets. The radius of Mars’s orbit varies from208million km at perihelion to250million km at aphelion. The planet’s sidereal period (the time taken for Mars to go once round the Sun) is687Earth-days.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Rights and permissions
Copyright information
© 2003 Springer-Verlag London
About this chapter
Cite this chapter
North, G. (2003). The Planet Mars. In: Astronomy in Depth. Springer, London. https://doi.org/10.1007/978-0-85729-426-5_6
Download citation
DOI: https://doi.org/10.1007/978-0-85729-426-5_6
Publisher Name: Springer, London
Print ISBN: 978-1-85233-580-9
Online ISBN: 978-0-85729-426-5
eBook Packages: Springer Book Archive