This page is regularly updated to track progress on a project to research mountains and craters of the Moon with a prominence or depth of 1000 metres or more. Given that the current publication covering Earth is titled The Relative Mountains of Earth: The Ribus, the working title for what is hoped to be a second publication is Relative Mountains of the Moon: Lunar Ribus.
Latest update: 28/10/2024 by Daniel Quinn
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28/10/2024:
An early preliminary test analysis of Lunar Ribus and Negative Ribus (craters) has been conducted by Oscar Argudo in order to provide a provisional expected size of the research project. He has found that there are likely to be very approximately 3000 Lunar Ribus (comfortably less than half of the 7150 Ribus found on Earth) and more than double that number of craters with a depth of 1000 metres or more (of which there are no known naturally-occurring examples on Earth but a handful of humanmade ones such as boreholes and mines). There are probably over 6500 craters on the Moon with a depth of 1000 metres or more.
The lunar surface
Preliminary analysis of Lunar Ribus (orange dot = P900 peak, red lines connect the peaks via the key cols)
Preliminary analysis of Negative Ribus (blue dot = crater with depth of 900m or more)
Preliminary analysis of Lunar Ribus and Negative Ribus – orange dots (P900 peaks) plus blue dots (craters with a depth of at least 900 metres)
This means the entire project will involve researching 10000 distinct lunar features, to take account of additional Sub-Ribus (P990-P999.9) that almost qualify as Ribus (P1000). 3000 Lunar Ribus plus 6500 craters plus at least 500 Lunar Sub-Ribus (negative and positive) equals 10000. It also means that approximately two-thirds of the entries in the Lunar Ribus database will be craters (negative) as opposed to mountains (positive).
As planned, the brief test was done using Andrew Kirmse’s code for analysing prominence in conjunction with the Lunar Orbiter Laser Altimeter digital elevation model from NASA / USGS.
On the same day I received an email from the Paul Hamlyn Foundation stating that I had not been successful in my application for funding for this project, primarily because it is viewed as academic research. Never mind. More soon.
The Moon photographed during the Apollo 12 mission in November 1969.
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05/10/2024:
Very early steps have been taken to commence a project to identify and name all of the Ribus on the Moon. This will include negative Ribus (craters with a depth of 1000 metres or more) and Lunar Sub-Ribus.
The project will begin in earnest towards the end of 2024 and most likely take a year to complete. I, Daniel Quinn, am looking for a data science student (or similar) who would be interested in working on this project. He or she needs to be capable of quite complex coding in order to create an online editing site with a representation of the Moon’s surface based on an available dataset. Plus lots of other stuff. At present there is no funding, but such a project would constitute a genuinely unique academic work. Depending on availability of time, co-authorship of a Lunar Ribus publication is up for grabs.
If you are interested in discussing this project in more detail please email dan@gunung.org
Dan, October 2024
