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  2. Albedo - Wikipedia

    en.wikipedia.org/wiki/Albedo

    When seen from a distance, the ocean surface has a low albedo, as do most forests, whereas desert areas have some of the highest albedos among landforms. Most land areas are in an albedo range of 0.1 to 0.4. [14] The average albedo of Earth is about 0.3. [15] This is far higher than for the ocean primarily because of the contribution of clouds.

  3. Classical albedo features on Mars - Wikipedia

    en.wikipedia.org/wiki/Classical_albedo_features...

    The first astronomer to name Martian albedo features systematically was Richard A. Proctor, who in 1867 created a map (based in part on the observations of William Rutter Dawes) in which several features were given the names of astronomers who had been involved in mapping Mars. In some cases, the same names were used for multiple features.

  4. Albedo feature - Wikipedia

    en.wikipedia.org/wiki/Albedo_feature

    In planetary geology, an albedo feature is a large area on the surface of a planet (or other Solar System body) which shows a contrast in brightness or darkness with adjacent areas. Historically, albedo features were the first (and usually only) features to be seen and named on Mars and Mercury .

  5. List of trans-Neptunian objects - Wikipedia

    en.wikipedia.org/wiki/List_of_trans-Neptunian...

    The first image compares some of the largest TNOs in terms of size, color and albedo. This is a list of trans-Neptunian objects (TNOs), which are minor planets in the Solar System that orbit the Sun at a greater distance on average than Neptune , that is, their orbit has a semi-major axis greater than 30.1 astronomical units (AU).

  6. Ascraeus Mons - Wikipedia

    en.wikipedia.org/wiki/Ascraeus_Mons

    The volcano's location corresponds to the classical albedo feature Ascraeus Lacus.. Ascraeus Mons was discovered by the Mariner 9 spacecraft in 1971. The volcano was originally called North Spot [2] because it was the northernmost of only four spots visible on the surface due to a global dust storm that was then enshrouding the planet.

  7. Tethys (moon) - Wikipedia

    en.wikipedia.org/wiki/Tethys_(moon)

    This very high albedo is the result of the sandblasting of particles from Saturn's E-ring, a faint ring composed of small, water-ice particles generated by Enceladus's south polar geysers. [9] The radar albedo of the Tethyan surface is also very high. [26] The leading hemisphere of Tethys is brighter by 10–15% than the trailing one. [27]

  8. Sednoid - Wikipedia

    en.wikipedia.org/wiki/Sednoid

    The sednoids' orbits cannot be explained by perturbations from the giant planets, [9] nor by interaction with the galactic tides. [4] If they formed in their current locations, their orbits must originally have been circular; otherwise accretion (the coalescence of smaller bodies into larger ones) would not have been possible because the large relative velocities between planetesimals would ...

  9. Bond albedo - Wikipedia

    en.wikipedia.org/wiki/Bond_albedo

    The Bond albedo is a value strictly between 0 and 1, as it includes all possible scattered light (but not radiation from the body itself). This is in contrast to other definitions of albedo such as the geometric albedo, which can be above 1. In general, though, the Bond albedo may be greater or smaller than the geometric albedo, depending on ...