• LOGIN
    Login with username and password
Repository logo

BORIS Portal

Bern Open Repository and Information System

  • Publications
  • Theses
  • Research Data
  • Projects
  • Organizations
  • Researchers
  • More
  • Collections
  • Statistics
  • LOGIN
    Login with username and password
Repository logo
Unibern.ch
  1. Home
  2. Publications
  3. Seasonal low albedo streaks at the edge of the Martian south polar layered deposits

Seasonal low albedo streaks at the edge of the Martian south polar layered deposits

Details
Files
DOI
10.48620/97324
Publisher DOI
10.1016/j.icarus.2023.115790
Abstract
Low Albedo Streaks (LAS) are narrow dark streaks observed at the edges of the South Polar Layered Deposits (SPLD) on Mars. We investigate the seasonal morphology, surface topography of LAS-rich areas using monochrome and multiband images from both the High Resolution Imaging Science Experiment (HiRISE) and the Color and Stereo Surface Imaging System (CaSSIS). We complement the image analysis with spectral data from the Compact Reconnassiance Imaging Spectrometer (CRISM). In addition, we analyze the thermal environment of LAS-rich areas with data from a Martian global climatological model. Our analysis suggests that streaks (i) originate from similar scarps and outcrops on the edge of layered structures at the end of local winter during different Martian years, (ii) lengthening in spring forming sinuous branches on terrain with rippled ridges, and (iii) eventually fade leaving distinguishable bright deposits within the streaked area. The surface topography analysis indicates that streaks advance on slopes between 4° and 34°, while the dust flows emanated from mass-wasting scars propagate on the slope steeper than 20°. Our spectral data analysis suggests that pyroxene- or basaltic-bearing materials are deposited on the surface mainly composed of dust by LAS. Thermal analysis indicates that LAS are active when the surface temperature rises from 145.5 K to 162 K, fading when the temperature increases suddenly and significantly. Finally, we evaluate several possible mechanisms to explain the formation of LAS. LAS might be formed by liquids, and such liquids might be brines. However, the presence of salts with lower eutectic temperatures seems to be necessary for the existence of brine on the Martian surface, and should be investigated at the target area in the future.
Date Issued
2024-01
Publication Type
Article
Subject(s)
500 Science > 530 Physics
Language(s)
en
Author(s)
Peng, Jimin
Munaretto, Giovanni
Tornabene, Livio
Lucchetti, Alice
Cremonese, Gabriele
Pajola, Maurizio
Re, Cristina
Becerra, Patricio  
Physics Institute, Space Research and Planetary Sciences  
Thomas, Nicolas  
Physics Institute, Space Research and Planetary Sciences  
Space Research and Planetology Physics - Remote Sensing  
Additional Credits
Physics Institute, Space Research and Planetary Sciences  
Space Research and Planetology Physics - Remote Sensing  
Journal
Icarus
Publisher
Elsevier
ISSN
0019-1035
Access(Rights)
restricted
Show full item
BORIS Portal
Bern Open Repository and Information System
Build: 0eaa7c [ 7.08. 11:06]
Explore
  • Projects
  • Funding
  • Publications
  • Research Data
  • Organizations
  • Researchers
  • Audiovisual Material
  • Software & other digital items
  • Events
More
  • About BORIS Portal
  • BORIS Portal & Open Science
  • Send Feedback
  • Cookie settings
  • Service Policy
Follow us on
  • Mastodon
  • YouTube
  • LinkedIn
UniBe logo
Repository logo COAR Notify