{"title":"Layered remnant deposits in Hellas Planitia, Mars as the remains of ancient ice mounds","authors":"Eva Z. Petrini , Michael M. Sori","doi":"10.1016/j.icarus.2025.116604","DOIUrl":null,"url":null,"abstract":"<div><div>Hellas Planitia is the site of many icy features in craters whose formation mechanisms offer insights into the climate processes of Mars. Layered remnant deposits (LRD) appear as crater deposits with distinct layers and have an unclear formation because of their frequent existence in the southern half of craters. We create an inventory of LRDs within Hellas Planitia using Thermal Emission Imaging System (THEMIS), Context Camera (CTX), and HiRISE images when available to measure key characteristics of LRDs and their host crater. We find 245 LRDs. Based on trends in our inventory, we propose LRDs result from old, crater-filling ice mounds that had preferential sublimation on the northern side leaving the present-day remnant in the southern portion of the crater. Understanding the formation of LRDs provides valuable insights into the broader narrative of Mars' climatic history, offering clues about past environmental conditions in the planet's Amazonian era.</div></div>","PeriodicalId":13199,"journal":{"name":"Icarus","volume":"436 ","pages":"Article 116604"},"PeriodicalIF":2.5000,"publicationDate":"2025-04-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Icarus","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0019103525001514","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Hellas Planitia is the site of many icy features in craters whose formation mechanisms offer insights into the climate processes of Mars. Layered remnant deposits (LRD) appear as crater deposits with distinct layers and have an unclear formation because of their frequent existence in the southern half of craters. We create an inventory of LRDs within Hellas Planitia using Thermal Emission Imaging System (THEMIS), Context Camera (CTX), and HiRISE images when available to measure key characteristics of LRDs and their host crater. We find 245 LRDs. Based on trends in our inventory, we propose LRDs result from old, crater-filling ice mounds that had preferential sublimation on the northern side leaving the present-day remnant in the southern portion of the crater. Understanding the formation of LRDs provides valuable insights into the broader narrative of Mars' climatic history, offering clues about past environmental conditions in the planet's Amazonian era.
期刊介绍:
Icarus is devoted to the publication of original contributions in the field of Solar System studies. Manuscripts reporting the results of new research - observational, experimental, or theoretical - concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our Solar System or extrasolar systems are welcome. The journal generally does not publish papers devoted exclusively to the Sun, the Earth, celestial mechanics, meteoritics, or astrophysics. Icarus does not publish papers that provide "improved" versions of Bode''s law, or other numerical relations, without a sound physical basis. Icarus does not publish meeting announcements or general notices. Reviews, historical papers, and manuscripts describing spacecraft instrumentation may be considered, but only with prior approval of the editor. An entire issue of the journal is occasionally devoted to a single subject, usually arising from a conference on the same topic. The language of publication is English. American or British usage is accepted, but not a mixture of these.