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opposition (Definition)

In astronomy, two astronomical objects are said to be in opposition when they are on opposite sides of the Celestial Sphere, as observed from a given body (usually Earth).

A planet (or asteroid or comet) is said to be "in opposition" or "at opposition" when it is in opposition to the Sun. Because most orbits in the Solar system are nearly coplanar to the ecliptic, this occurs when the Sun, Earth, and the body are configured in an approximately straight line, or syzygy; that is, Earth and the body are in the same direction as seen from the Sun. Opposition occurs only for superior planets (see Figure 1).

The instant of opposition is defined as that when the apparent geocentric celestial longitude of the body differs by $180^{\circ}$ from the apparent geocentric longitude of the Sun.[1] At that time, a body is:

  • in apparent retrograde motion [2]
  • visible almost all night - rising around sunset, culminating around midnight, and setting around sunrise [3]
  • at the point in its orbit where it is roughly closest to Earth, making it appear larger and brighter [4]
  • nearly completely sunlit; the planet shows a full phase, analogous to a full moon [5]
  • at the place where the opposition effect increases the reflected light from bodies with unobscured rough surfaces

The Moon, which orbits Earth rather than the Sun, is in approximate opposition to the Sun at full moon.[6] A more exact opposition occasionally occurs with mathematical regularity if the Moon is at its usual sun and Earth-aligning point so that it appears full and happens to be aligning with the ecliptic (Earth's orbital plane) during the descending or ascending phase of its $5^{\circ}$ inclined (tilted) orbit, which is more concisely termed at a node of its orbit, in which case, a lunar eclipse occurs. A more exact, shaded form is when a central area of the earth aligns more precisely: a central lunar eclipse, of which there were14 in the 50 years to 2000, others being penumbral.

Seen from a superior planet, an inferior planet on the opposite side of the Sun is in superior conjunction with the Sun. An inferior conjunction occurs when the two planets align on the same side of the Sun. At inferior conjunction, the superior planet is "in opposition" to the Sun as seen from the inferior planet (see Figure 1).

Image Positional_astronomySmall
Figure 1: Planet confiugration and definitions.

Bibliography

This article is a derivative work of the creative commons share alike with attribution in [7].

[1] U.S. Naval Observatory Nautical Almanac Office (1992). P. Kenneth Seidelmann (ed.). Explanatory Supplement to the Astronomical Almanac. University Science Books, Mill Valley, CA. p. 733. ISBN 0-935702-68-7.

[2] Newcomb and Holden (1890), p. 115

[3] Newcomb, Simon; Holden, Edward S. (1890). Astronomy. pp. 115, 273.

[4] Moulton, Forest Ray (1918). An Introduction to Astronomy. pp. 255, 256.

[5] Newcomb and Holden (1890), p. 334

[6] Moulton (1918), p. 191

[7] Wikipedia contributors. Opposition (astronomy) [Internet]. Wikipedia, The Free Encyclopedia; 2025 Mar 29, 10:34 UTC [cited 2025 Mar 30].



"opposition" is owned by bloftin.
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See Also: retrograde motion


Cross-references: retrograde motion, ecliptic, system, Celestial Sphere, objects

This is version 13 of opposition, born on 2025-03-30, modified 2025-03-31.
Object id is 997, canonical name is Opposition.
Accessed 67 times total.

Classification:
Physics Classification95.10.Km (Ephemerides, almanacs, and calendars)
 45.50.Pk (Celestial mechanics )
 95.10.-a (Fundamental astronomy)
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