Jump to content

Opposition effect

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by 209.146.90.157 (talk) at 12:44, 4 June 2009. The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

The opposition effect brightens the area around Buzz Aldrin's shadow due to retroreflective properties of lunar regolith.

The opposition effect (also opposition spike, or opposition surge) is the brightening of a rough surface, or an object with many particles, when illuminated from directly behind the observer. It is so named because the reflected light from the Moon and Mars appeared significantly brighter than predicted when at astronomical opposition, giving rise to an opposition spike.

The effect is pacrly pronounced on regolith surfaces of airless bodies in the solar system. The usual major cause of the effect is that a surface's small pores and pits that would otherwise be in shadow at other incidence angles become lit up when the observer is almost in the same line as the source of illumination. The effect is usually only visible for a very small range of phase angles near zero. For bodies whose reflectance properties have been quantitatively studied, details of the opposition effect — its strength and angular extent — are described by two of the Hapke parameters. In the case of planetary rings (such as Saturn's), an opposition effect is due to the covering of shadows on the ring particles.

The opposition effect does not arise on smooth mirror-like surfaces, which give rise to a different anti-solar brightening, nor from completely cloudy planets such as Jupiter.[citation needed]

See also

References