Inferior and superior planets
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In the Solar System,
- Inferior planets are the planets whose orbits lie within Earth's orbit around the Sun: Mercury and Venus.
- Superior planets are the planets whose orbits lie outside Earth's orbit around the Sun: Mars, Jupiter, Saturn, Uranus and Neptune. Dwarf planets like Ceres or Pluto and most asteroids are 'superior' in the sense that they almost all orbit outside the orbit of Earth.
History[edit]
These terms were originally used in the geocentric cosmology of Claudius Ptolemy to differentiate as inferior those planets (Mercury and Venus) whose epicycle remained co-linear with the Earth and Sun, and as superior those planets (Mars, Jupiter, and Saturn) that did not.[1]
In the 16th century, the terms were modified by Copernicus, who rejected Ptolemy's geocentric model, to distinguish a planet's orbit's size in relation to the Earth's.[2]
Planets in each category[edit]
When Earth is stated or assumed to be the reference point:
- "Inferior planet" is used in reference to Mercury and Venus, which are closer to the Sun than the Earth is.
- "Superior planet" is used in reference to Mars, Jupiter, Saturn, (and later additions Uranus and Neptune), which are farther from the Sun than the Earth is.
The terms are sometimes used more generally: for example, the Earth is an inferior planet as seen from Mars.
Other planetary terms[edit]
These terms are different from the terms inner planet and outer planet, which designate those planets which lie inside the asteroid belt and those that lie outside it, respectively. Inferior planet is also different from minor planet or dwarf planet. Superior planet is also different from gas giant.
References[edit]
- ^ Lakatos, Imre; Worrall, John; Currie, Gregory (1980). Worrall, John; Currie, Gregory, eds. The Methodology of Scientific Research Programmes. Cambridge University Press. p. 186. ISBN 0-521-28031-1.
- ^ Kuhn, Thomas S. (1985). The Copernican Revolution: Planetary Astronomy in the Development of Western Thought (4th ed.). Harvard University Press. p. 172. ISBN 0-674-17103-9.
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