The fraction of the total light or other radiation which falls on a
non-luminous body, such as a → planet,
→ satellite, or → asteroid,
and which is reflected by it. Generally, the albedo is equal to the ratio
between the light quantity reflected and the light quantity received.
The albedo values range between 0.0 (0%), for a perfectly black area,
which absorbs all incident light, and 1.0 (100%) for a perfect
reflector. The planets or planetary satellites with dense atmospheres
have greater albedos than those of transparent atmospheres or of no
atmospheres. The albedo can vary from one surface point to another, so
that a mean albedo is given for practical purposes. The natural
surfaces reflect different light quantities in different directions
and the albedo can be expressed in several ways, depending on the way
in which the measurement was made: in one direction or, on the average,
in all directions (M.S.: SDE). See also → Bond albedo,
→ geometric albedo.
Etymology (EN): Albedo, L. “whiteness,” from albus “white,”
from PIE base *albho- “white”.
Compare with Gk. alphos “white leprosy,”
O.H.G. albig, O.E. elfet “swan, the white bird”.
The idea of whiteness derives from the fact that whiter bodies
have a higher reflective power, while opaque objects are more absorptive.
Etymology (PE): Sepidâ, from sepid, →, white, + -â
noun-forming prefix from certain adjectives.