HiPOD: Sunday, 26 March 2023
North Polar Gypsum Dunes in Olympia Undae

North Polar Gypsum Dunes in Olympia Undae
These sand dunes are a type of aeolian bedform and partly encircle the Martian North Pole in a region called Olympia Undae.

Unlike most of the sand dunes on Mars that are made of the volcanic rock basalt, these are made of a type of sulfate mineral called gypsum. Whence the sand? Well, gypsum is a mineral that can often form from the evaporation of water that has sulfur and calcium dissolved in it. This sand was probably sourced from a northern region on Mars that used to be quite wet. The boxy gridding of the dunes indicates that the wind blows in multiple directions.

Note: “Aeolian” means wind-blown and “bedform” means piles of sediment shaped by a flowing fluid (liquid or gas).

ID: ESP_045501_2605
date: 10 April 2016
altitude: 319 km

https://uahirise.org/hipod/ESP_045501_2605
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

Black & white is less than 5 km across; enhanced color is less than 1 km. For full observation details, visit the ID link.