Contains:  Solar system body or event
Lunar libration : conclusion, MAILLARD

Lunar libration : conclusion

Acquisition type: Lucky imaging
Lunar libration : conclusion, MAILLARD

Lunar libration : conclusion

Acquisition type: Lucky imaging

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Description

In 2019, I published an image that presents the phenomenon of lunar libration.

Version B takes up this view as well as the explanation of the subject.

However, this was the lunar north pole and I had kept the plan to simultaneously show the effect on the south pole.

The astronomical news (especially the Martian opposition, the purchase of new equipment, the succession of periods conducive to image the Moon and Uranus etc.) made me put aside this project.

So I end this study with a new image that reveals what happens in the south on the same dates of course.

I think it's even easier to check the libration on this image.

The reference here is the famous crater Clavius known to all. Starting from it on the left image, it is enough to go up and see, compared to the right, the appearance of new reliefs and especially at the top the crater Drygalski can only be observed by a favorable libration.

Finally, by comparing the two North and South versions to the same dates, you can check that the surface gained on one side and of course lost on the other confirming this movement of oscillations called libration.

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  • Final
    Lunar libration : conclusion, MAILLARD
    Original
  • Lunar libration : conclusion, MAILLARD
    B

B

Description: Here are two views of the same region of the lunar North Pole that allow us to visualize this phenomenon called lunar libration.
I deliberately aligned these two images on the same horizontal plane with the north materialized by an N, to be able to compare them more easily.

We might think that 50% of the lunar surface is available to our gaze, since it always presents us with the same face. That is not entirely accurate. The Moon is animated by slight periodic oscillations, called librations, which allow us to observe up to 59% of its surface (but of course never more than 50% simultaneously).

The case presented here is a latitude libration. It is due to the fact that the moon's rotational axis is not exactly perpendicular to the plane of its orbit. As a result, the Earth observer can successively see a thin additional net of lunar surface beyond the average limits of the North and South limbs. This libration in latitude reaches about 6°50' (on the right view it is about 5°).

There is also a longitude libration that reveals a thin additional band of lunar surface to the west or east.

All of these successively revealed areas represent 18% of the lunar surface.
You may notice the distorting effect due to perspective. A circular crater in this libration zone looks like a heavily flattened ellipse.

Finally, it should be noted that the study of libration zones depends on three simultaneous conditions: that the libration is indeed taking place, a favourable lighting angle and a calm and transparent atmosphere.
An attractive subject more for the amateur astronomer..

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Lunar libration : conclusion, MAILLARD