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Vol 49, No 4, April 2012 - BAA Lunar Section

Vol 49, No 4, April 2012 - BAA Lunar Section

Vol 49, No 4, April 2012 - BAA Lunar Section

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The usual figures for selenographic colongitude given in an ephemeris are defined with respect to the mean<br />

centre of the lunar disk (and so is 90 degrees exactly at exactly first quarter). Owing to libration in longitude,<br />

a feature can actually be up to 3.5 degrees either east or west of the terminator at the time when the ephemeris<br />

predicts that the feature should be on it. So the usual tabulated figures of selenographic colongitude only give<br />

the approximate position of a feature in relation to the terminator. After correcting for libration in longitude<br />

it might be that Molesworth really did observe earlier than the time of first appearance of the interior<br />

illumination of Plato.<br />

I am grateful to Gerald for the additional comments and the copy of his original observing notes and drawing.<br />

It is clear that the floor of Plato presents a number of unusual scenarios of light and shade under early sunrise<br />

and sunset and that the ephemeris might not tell the whole story in terms of what might be visible at the<br />

eyepiece.<br />

6<br />

<strong>BAA</strong> <strong>Lunar</strong> <strong>Section</strong> Circular <strong>Vol</strong>. <strong>49</strong> <strong>No</strong>. 4 <strong>April</strong> <strong>2012</strong>

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