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MSC View Program / Exhibit

Figure 7 · The Moon on the approach, 70–72 h GET

The Moon as the program drew it on the way in, and why the recreation cannot match it at the times printed on the figure.

Panel
View
Style
CopernicusArchimedesSpacecraft relative to Moonh_M = 17 077 stat. mi.V_i = 4 001 fps = 2 728 mphField of view = 6°X, nondimensionalY, nondimensional

What the original shows

A 6° field on the Moon, mostly in “lunar darkness” (hatched), with a lit crescent along the bottom. The 1969 program drew craters as ellipses, rays around Copernicus, and part of the outline of the Sea of Serenity.

Recomputed

The command module’s position comes from the Mission Report’s trajectory, propagated from the first midcourse correction to the printed time. The Moon’s features are from the IAU gazetteer (craters of 40 km and more) and the LROC mare outlines, and are labelled as reconstructed: the program’s crater models do not survive. “Up” is the spacecraft’s direction of travel, the rule recovered from Figure 6.

Why it does not match

Thresholds were set before measuring: disc and terminator within 2% of the diameter, features within 3%. Neither panel comes close.

Features and the terminator are not compared at these misfits. Everything above is recorded as measured; nothing was adjusted to make it fit.

Limits