Temperatures of the Lacus Mortis region of the Moon

Earth and Space Science
By: , and 

Links

Abstract

Over 11 years of data acquired by the Diviner Lunar Radiometer Experiment instrument aboard Lunar Reconnaissance Orbiter have been compiled into a comprehensive data set of surface temperatures in the Lacus Mortis region which includes the landing ellipse of the Astrobotic Mission One lander mission. These data provide diurnal brightness temperatures at 128 pixels per degree (ppd) spatial resolution and 0.1 hr of local time resolution. From this data set, we highlight several features that display variations in radiative and thermophysical properties in the Lacus Mortis region and characterize the temperatures of the Astrobotic Mission One landing ellipse. We identify distinctly contrasting properties of materials in the walls of Bürg crater, hummocks of materials on the southeast margin of the mare basalts, and materials exposed or excavated by impacts. Additionally, we describe an exceptionally rocky fault scarp that predates the formation of Bürg crater suggesting the observed boulders are replenished on a timescale <1 Ga. Within the Astrobotic landing ellipse, temperatures are observed to range from ∼88 to ∼359 K with sunrise and sunset local times constrained to 5.8–6.3 hr and 17.8 and 18.1 hr respectively.

Publication type Article
Publication Subtype Journal Article
Title Temperatures of the Lacus Mortis region of the Moon
Series title Earth and Space Science
DOI 10.1029/2021EA001966
Volume 9
Issue 2
Year Published 2022
Language English
Publisher American Geophysical Union
Contributing office(s) Astrogeology Science Center
Description e2021EA001966, 17 p.
Other Geospatial Lacus Mortis region, Moon
Google Analytic Metrics Metrics page
Additional publication details