Bond albedo oor Spaans
Bond albedo
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albedo de Bond
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The rings are extremely dark—the Bond albedo of the rings' particles does not exceed 2%.
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The predicted Bond albedo of a class V planet around a Sun-like star is 0.55, due to reflection by the cloud decks.
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Water clouds are more reflective than ammonia clouds, and the predicted Bond albedo of a class II planet around a Sun-like star is 0.81.
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Because of the lack of a reflective cloud layer, the Bond albedo is low, around 0.12 for a class-III planet around a Sun-like star.
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The Bond albedo of a class IV planet around a Sun-like star is predicted to be very low, at 0.03 because of the strong absorption by alkali metals.
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The predicted Bond albedo of a class I planet around a star like the Sun is 0.57, compared with a value of 0.343 for Jupiter and 0.342 for Saturn.
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Because bodies in the outer Solar System are always observed at very low phase angles from the Earth, the only reliable data for measuring their Bond albedo comes from spacecraft.
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Analysis of these images allowed derivation of the phase function (dependence of the ring's reflectivity on the angle between the observer and Sun), and geometrical and Bond albedo of ring particles.
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Assuming the planet is perfectly grey with no greenhouse or tidal effects, and a Bond albedo of 0.1, the temperature would be close to 1600 K. Although it has not been detected directly, it is certain that the planet is a gas giant.
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It is estimated that the average global equilibrium temperature (the temperature in the absence of atmospheric effects) of Gliese 581g would range from 209 to 228 K (−64 to −45 °C, or −84 to −49 °F) for Bond albedos (reflectivities) from 0.5 to 0.3 (with the latter being more characteristic of the inner Solar System).
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Bond albedo - Wikipedia, the free encyclopedia
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The rings are extremely dark—the Bond albedo of the rings' particles does not exceed 2%.
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The Bond albedo (A) is related to the geometric albedo (p) by the expression
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The bond albedo is the total radiation reflected from an object compared to the total incident radiation from the Sun.
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The geometric albedo of the ring particles does not exceed 5–6%, while the Bond albedo is even lower—about 2%.
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The geometric albedo of the ring particles does not exceed 5–6%, while the Bond albedo is even lower—about 2%.
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The geometric albedo may be greater or smaller than the Bond albedo, depending on surface and atmospheric properties of the body in question.
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The Bond albedo is the fraction of power in the total electromagnetic radiation hitting an astronomical body which is scattered back out into space.
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The Bond albedo is the fraction of power in the total electromagnetic radiation incident on an astronomical body that is scattered back out into space.
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In general, though, the Bond albedo may be greater or smaller than the geometric albedo, depending on surface and atmospheric properties of the body in question.
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In general, though, the Bond albedo may be greater or smaller than the geometric albedo, depending on surface and atmospheric properties of the body in question.
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The evolution of the earthshine albedo is in remarkable agreement with that from the CERES instruments, although each method measures different slices of the Earth’s Bond albedo.
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Because bodies in the outer Solar System are always observed at very low phase angles from the Earth, the only reliable data for measuring their Bond albedo comes from spacecraft. Contents
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The Bond albedo, named after the American astronomer George Phillips Bond (1825–1865), who originally proposed it, is the fraction of power in the total electromagnetic radiation incident on an astronomical body that is scattered back out into space.
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