Lance, I appreciate the discussion. Please see below.
I'm sorry Tom but that libration timeframe is wildly out whack.
I spent four hours observing the south pole on april 20 & 21st/2024 and in that short period the moon nodded in and out so quickly that if you weren't watching continuously you'd have missed the Leibonitz mtn and several south pole peaks.
The very rapid changes you are describing are caused by changes in solar illumination, not libration. Sorry if my statement in the previous post was unclear. I was referring to changes in perspective of features on the sunlit limb, not to changes in illumination near the terminator (because your feature in question is not near the terminator). Illumination changes can indeed be very dramatic and rapid near the terminator as the sunlight and shadows move quickly. Libration, on the other hand, is the wobbling of the Moon due to parallax, or the apparent shift in an object that occurs when changing viewing angles. This is caused by the movement of the Moon relative to the Earth. Changes in libration are much slower to be perceived than changes in illumination. In fact, we can look up the exact values at any given time. Libration is typically reported by providing the coordinates of the sub-Earth point, and at the time of your image, the sub-Earth point was located at -1.564 S, -0.596 W (values in degrees). Four hours later, the sub-Earth point was -1.333 S, -0.821 W. This is a very small change that would not be perceived at the image scales you are sharing with us.
I believe that this is not an artifact and in my high resolution map Oken and a crater between Gum s and Abel b have mtns on their rim edges and is not so flat.
Your hypotheses are very reasonable. The way to test them is to determine if such craters do in fact project above the limb at the time of your image. The NASA Dial-A-Moon images I posted yesterday indicate that they do not. But if you don't like that reference, we can also look to LTVT (more on that below) to produce a simulated image at the same time. This is reproduced below, with a few landmark craters labeled. The image indicates a relatively smooth lunar limb, with some very slight irregularities, but nothing that corresponds to the peak shown in your image. Some of the difficulty is due to the limitations of resolution in your image.
The gold standard for identifying features along the lunar limb is to use software that simulates the view from Earth and provides a mechanism to take accurate latitude and longitude measurements that may be cross referenced with LROC data. The best example of such software is LTVT, although the software does require considerable practice in order to use effectively. As it turns out, I'm very familiar with the Mare Australe region, having done an analysis several years ago posted here, as well as in an image I captured of the region during an occultation of Mars. All the crater identifications were performed by matching precise locations in the images to latitude and longitude coordinates (with the help of LTVT) that could then be looked up using the LRO Quickmap for verification. Peaks are sometimes visible along the limb in this region, although they tend to be very subtle ones, and conclusive identification is not always easy without some of the methods mentioned above.
Edited by Tom Glenn, 19 February 2025 - 05:03 AM.