Results 101 to 110 of about 1,240 (223)

Variation of crater morphological parameters in the landing area of Tianwen-1: relationships with the geological environment and climate change

open access: yesEarth, Planets and Space
The Zhurong rover of the Tianwen-1 mission successfully landed in the southern part of the Utopian Planitia and the northern region of the dichotomy boundary.
Yu Yang   +6 more
doaj   +1 more source

Dust Devil Tracks [PDF]

open access: yes, 2016
Dust devils that leave dark- or light-toned tracks are common on Mars and they can also be found on the Earth’s surface. Dust devil tracks (hereinafter DDTs) are ephemeral surface features with mostly sub-annual lifetimes.
A. Spiga   +156 more
core   +1 more source

Planet Tours [PDF]

open access: yes, 2011
Introduction: Planning to take a vacation soon? Visit Phobos! Small and cozy, Phobos orbits the fourth planet from the Sun in less than eight hours. From your observation deck on Phobos, you will have a superb view of Mars. You will see its mountains,
McDonald Observatory   +1 more
core  

Martian impact crater ejecta morphologies as indicators of the distribution of subsurface volatiles [PDF]

open access: yes, 2003
Fresh Martian impact craters display a variety of ejecta blanket morphologies. The fluidized appearance of most fresh ejecta types is commonly ascribed to heating and vaporization of subsurface volatiles during crater formation.
Barlow, Nadine G., Perez, Carola B.
core   +2 more sources

An Inclusive Library for Quantitative Analysis of the Laser-induced Breakdown Spectra Acquired by the Zhurong Mars Rover

open access: yesThe Astrophysical Journal
Laser-induced breakdown spectroscopy (LIBS) is a critical tool for geochemical analysis in planetary science due to its ability to remotely detect a broad range of elements at submillimeter spatial resolution.
Shuai-Yi Qu   +10 more
doaj   +1 more source

Chemical evolution of the early Martian hydrosphere [PDF]

open access: yes
The chemical evolution of the early Martian hydrosphere is discussed. The early Martian ocean can be modeled as a body of relatively pure water in equilibrium with a dense carbon dioxide atmosphere. The chemical weathering of lavas, pyroclastic deposits,
Schaefer, M. W.
core   +1 more source

Geological analysis of the dome field in western Utopia Planitia, on Mars

open access: yesIcarus
Hundreds of domes are scattered over a plain composed of different geological units in the western margin of Utopia Planitia, near the northern martian dichotomy. These structures have traditionally been considered of igneous origin. In this work, we utilized recent data to study the geomorphological and compositional properties of this dome field.
Suárez-Valencia, Javier Eduardo   +4 more
openaire   +2 more sources

Evidence for glaciation in Elysium [PDF]

open access: yes
It is suggested that certain landforms in the Elysium region of Mars provide strong evidence for glaciation. Landscapes related to subglacial volcanism suggest that ice was a primary agent in the development of ...
Anderson, Duwayne M.   +1 more
core   +1 more source

Erosional and depositional history of central Chryse Planitia [PDF]

open access: yes
This map uses high resolution image data to assess the detailed depositional and erosional history of part of Chryse Planitia. This area is significant to the study of the global geology of Mars because it represents one of only two areas on the martian ...
Crumpler, L. S.
core   +1 more source

Martian Subsurface Properties and Crater Formation Processes Inferred From Fresh Impact Crater Geometries [PDF]

open access: yes, 2011
The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of ...
Stewart, Sarah, Valiant, Gregory J.
core  

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