|... in the solar system|
|... different surfaces|
|Fields (not ordered)||0.26|
(angle of inclination> 45 °)
(angle of inclination> 30 °)
(angle of inclination> 20 °)
(angle of inclination> 10 °)
The albedo ( Latin albedo 'white' ; from Latin albus 'white' ) is a measure of the reflectivity ( reflection radiation ) of diffusely reflective , i.e. non-luminous surfaces. It is given as a dimensionless number and corresponds to the ratio of reflected to incident light (an albedo of 0.9 corresponds to 90% reflection). For a given surface, the albedo depends on the wavelength of the incident light and can be used for wavelength ranges - e.g. B. the solar spectrum or visible light - can be specified. It is particularly important in meteorology , as it enables statements to be made about how much a surface heats up - and thus also the air in contact with the surface.
In astronomy , the albedo plays an important role as they (z. B. diameter, apparent / absolute magnitude) with basic parameters of celestial bodies related.
There are different types of albedo:
- The spherical albedo (also called planetary albedo and Bond's albedo ) is the ratio of the light reflected from a spherical surface in all directions to the radiation incident on the spherical cross-section. In the case of the planetary albedo, the surface is the upper edge of the atmosphere. The spherical albedo is always between 0 and 1. The value 0 corresponds to complete absorption and 1 to complete reflection of the incident light.
- The geometric albedo is the ratio of the radiation current reaching the observer from a fully irradiated area to that which would reach the observer from a diffusely reflecting, absolutely white disc (a so-called Lambert radiator ) of the same size with perpendicular light incidence. In rare cases, the geometric albedo can also have values greater than 1, because real surfaces do not reflect ideally diffusely.
The relationship between spherical albedo and geometric albedo is the so-called phase integral (see phase ), which takes into account the angle-dependent reflectivity of each surface element.
The albedo is measured using an albedometer and is given in percent. In astronomy, albedometers cannot be used because of the great distances. The geometric albedo can be calculated from the apparent brightness and the radius of the celestial body and the distances between earth, object and sun. In order to determine the spherical albedo, the phase integral (and thus the phase function) must also be known. However, this is only fully known for those celestial bodies that move within the earth's orbit ( Mercury , Venus ). The phase function can only be partially determined for the upper planets , which means that the values for their spherical albedo are not exactly known.
NASA satellites have been measuring the albedo of the earth since around 2004. Overall, apart from short-term fluctuations, this has remained constant over the past two decades; regionally, on the other hand, there were changes of more than 8%. In the Arctic z. B. the reflection is lower, in Australia higher.
The Deep Space Climate Observatory has been measuring the Earth's albedo at a distance of 1.5 million kilometers from the Lagrange point L1 since 2015 . At this point the probe has a permanent view of the sunlit side of the earth.
The surface quality of a celestial body determines its albedo. The comparison with the albedo values of earthly substances makes it possible to draw conclusions about the nature of other planetary surfaces. According to the definition of the spherical albedo, the prerequisite for parallel incident light is very well given because of the great distances of the reflecting celestial bodies from the sun as a light source. The always closed cloud cover of Venus reflects back much more light than the basalt-like surface parts of the moon . Venus therefore has a very high reflectivity with a mean spherical albedo of 0.76, and the Moon has a very low reflectance with an average of 0.12. The earth has a mean spherical albedo of 0.3. Due to global warming, the regional albedo values are shifting on earth. By shifting the cloud bands, the albedo sank z. B. in the northern temperate zone , but rose further north. The highest values measured so far fall on the Saturn moons Telesto (0.994) and Enceladus (0.99). The lowest mean value was found at comet Borrelly with only 0.03 .
Smooth surfaces such as water, sand or snow have a relatively high proportion of specular reflection , so their albedo is strongly dependent on the angle of incidence of the solar radiation (see table).
The albedo also depends on the wavelength of the light that is being examined, which is why the corresponding wavelength range should always be specified when specifying the albedo values.
- Joachim Gürtler , Johann Dorschner : The solar system. Barth, 1993, ISBN 3-335-00281-4 .
- J. Bennett, M. Donahue, N. Schneider, M. Voith: Astronomy. Ed. Harald Lesch , 5th edition (1170 pages). Pearson-Studienverlag, Munich 2010.
- H. Zimmermann, A. Weigert: Lexicon of Astronomy. Spectrum academ. Publishing house, Heidelberg / Berlin.
- NASA: Lunar and Planetary Science ; see fact sheets
- Anne Verbiscer, Richard French, Mark Showalter, Paul Helfenstein: Enceladus: Cosmic Graffiti Artist Caught in the Act . In: Science . tape 315 , no. 5813 , 2007, doi : 10.1126 / science.1134681 , PMID 17289992 (English,  [accessed on August 2, 2013]).
- NASA: Saturnian Satellite Fact Sheet. October 13, 2015, accessed July 16, 2015
- Phase Integral - from Eric Weisstein's World of Physics. In: scienceworld.wolfram.com. Retrieved February 28, 2015 .
- Monika Seynsche : The Arctic is absorbing more and more heat , Deutschlandfunk , Forschung Aktuell , February 18, 2014, accessed on February 20, 2014.
- Measuring Earth's Albedo. Image of the day. October 21, 2014 @ earthobservatory.nasa.gov; FAZ November 5, 2014, p. N1.
- PR Goode et al .: Earthshine Observations of the Earth's Reflectance. In: Geophysical Research Letters. Volume 28, No. 9, 2001, pp. 1671-1674
- Cloud changes further heat up the warming through positive feedback. In: scinexx.de. July 12, 2016, accessed March 1, 2019 .