- The following is an archived discussion of the DYK nomination of the article below. Please do not modify this page. Subsequent comments should be made on the appropriate discussion page (such as this nomination's talk page, the article's talk page or Wikipedia talk:Did you know), unless there is consensus to re-open the discussion at this page. No further edits should be made to this page.
The result was: promoted by Cwmhiraeth (talk) 05:29, 18 August 2017 (UTC)
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Abalos Undae
edit- ... that the Martian dunes of the Abalos Undae (pictured) may have formed from erosion of Rupes Tenuis, the polar scarp? Source1: quote: "The Abalos Undae dune field stretches westward, away from a portion (Abalos Colles) of the ice-rich north polar layered deposits that is separated from the main Planum Boreum dome by two large chasms. These dunes are special because their sands may have been derived from erosion of the Rupes Tenuis unit (the lowest stratigraphic unit in Planum Boreum, beneath the icier layers during formation of the chasms.)" Source2: quote: "Today's image location is slightly east of Monday's image. In this image the polar scarp (called Tenuis Rupes) bisects the image."
Created by Dr.K. (talk). Self-nominated at 19:01, 23 July 2017 (UTC).