The lunar limb is the edge of the visible surface (disc) of the Moon as viewed from Earth.[1] Seen from afar, it looks like a circular arc, but with higher resolution, it can be seen that the Moon’s surface is not flat and therefore its profile is irregular.
The lunar limb is not always the same: because of the libration of the Moon, i.e. small rotational movements as seen from Earth, its profile changes; this complicates the task of precisely calculating eclipse times and durations.[2] However, with elevation data from the mapping of the lunar surface, a three-dimensional model including mountains and valleys can be created and the lunar profile for any given time predicted with a high degree of accuracy.[3] The irregularity of the lunar limb is the cause of Baily's beads, which are collimated rays of sunlight that shine through in some places while not in others during a solar eclipse.
The contrast of the bright lunar disc against a black night sky makes the lunar limb a popular target when testing telescope optics (including binoculars).
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Why is the Moon wobbling like that? Libration Explained!
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Baily's beads
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References
- ^ "List of basic lunar features". Archived from the original on 2006-02-03.
- ^ O'Byrne, Chris. "Lunar Limb Corrections". Archived from the original on 2008-01-13.
- ^ Watts, C. B. (1963). "The Marginal Zone of the Moon". Astronomical Papers. 17 (1). U.S. Nautical Almanac Office: 951. Bibcode:1963USNAO..17....1W.
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This page was last edited on 7 April 2024, at 20:43