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OpenMARS: A global record of martian weather from 1999 to 2015
DOI: 10.1016/j.pss.2020.104962 Bibcode: 2020P&SS..18804962H

Holmes, James A.; Lewis, Stephen R.; Patel, Manish R.

The Open access to Mars Assimilated Remote Soundings (OpenMARS) dataset is a reanalysis product combining past spacecraft observations with a Mars Global Circulation Model (GCM). The OpenMARS product is a global surface/atmosphere reference database of surface and atmospheric properties for almost nine Mars years that can be used by Mars scientist…

2020 Planetary and Space Science
MEx 41
The Holy Grail: A road map for unlocking the climate record stored within Mars' polar layered deposits
DOI: 10.1016/j.pss.2020.104841 Bibcode: 2020P&SS..18404841S

Horgan, Briony; Byrne, Shane; Zacny, Kris +35 more

In its polar layered deposits (PLD), Mars possesses a record of its recent climate, analogous to terrestrial ice sheets containing climate records on Earth. Each PLD is greater than 2 km thick and contains thousands of layers, each containing information on the climatic and atmospheric state during its deposition, creating a climate archive. With …

2020 Planetary and Space Science
MEx 28
Implications for the origin and evolution of Martian Recurring Slope Lineae at Hale crater from CaSSIS observations
DOI: 10.1016/j.pss.2020.104947 Bibcode: 2020P&SS..18704947M

Pajola, M.; Cremonese, G.; Thomas, N. +9 more

Recurring Slope Lineae (RSL) are narrow, dark features that typically source from rocky outcrops, incrementally lengthen down Martian steep slopes in warm seasons, fade in cold seasons and recur annually. In this study we report the first observations of RSL at Hale crater, Mars, during late southern summer by the Color and Surface Science Imaging…

2020 Planetary and Space Science
ExoMars-16 25
3D digital outcrop model reconstruction of the Kimberley outcrop (Gale crater, Mars) and its integration into Virtual Reality for simulated geological analysis
DOI: 10.1016/j.pss.2019.104808 Bibcode: 2020P&SS..18204808C

Le Mouélic, Stéphane; Mangold, Nicolas; Le Deit, Laetitia +3 more

Structure-from-Motion photogrammetry has recently become a cheap and efficient method to reconstruct accurate and highly-resolved 3D Digital Outcrop Model (DOM) from a single set of images. This enables the 3D visualization of hardly accessible and/or remote geological scenes, which is of strong interest for planetary bodies. This paper focuses on…

2020 Planetary and Space Science
MEx 22
Layered mound, inverted channels and polygonal fractures from the Makgadikgadi pan (Botswana): Possible analogues for Martian aqueous morphologies
DOI: 10.1016/j.pss.2020.105048 Bibcode: 2020P&SS..19205048F

Franchi, Fulvio; MacKay, Ruaraidh; Selepeng, Ame Thato +1 more

Layered mounds and inverted channels with polygonal fractures from the Ntwetwe Pan in the Makgadikgadi Basin (central Botswana) have been herein investigated. These morphologies are from an evaporitic basin (the Makgadikgadi Basin) that is the remnant of an ancient Pleistocene lake and is currently part of the world's largest evaporitic system.

2020 Planetary and Space Science
MEx 12
Outbursts of comets at large heliocentric distances: Concise review and numerical simulations of brightness jumps
DOI: 10.1016/j.pss.2020.104867 Bibcode: 2020P&SS..18404867W

Wesołowski, M.; Gronkowski, P.; Tralle, I.

The outburst of comet brightness is spectacular and well-known manifestation of the physical activity of these relatively small cosmic bodies. The outbursts of brightness are observed for periodic comets, as well as for the comets moving along parabolic trajectories. The most known comet representing such kind of activity is the comet 29P/Schwassm…

2020 Planetary and Space Science
Rosetta 11
End-of-mission calibration of the Cassini Imaging Science Subsystem
DOI: 10.1016/j.pss.2020.104898 Bibcode: 2020P&SS..18504898K

Porco, Carolyn; West, Robert; Verbiscer, Anne +3 more

We provide an end-of-mission update to the in-flight calibration of the Imaging Science Subsystem cameras on the Cassini spacecraft, resolving discrepancies in our previous analyses from 2004 to 2010, incorporating data through the end of the mission, adding a correction for the weak but measurable camera sensitivity decline over time, and providi…

2020 Planetary and Space Science
Cassini eHST 11
Variability of spider spatial configuration at the Martian south pole
DOI: 10.1016/j.pss.2020.104848 Bibcode: 2020P&SS..18504848H

Jaumann, R.; Hauber, E.; Portyankina, G. +5 more

Araneiform terrain, or "spider" (spider-like surface modifications) is suggested to form through basal sublimation of seasonal translucent CO2 slab ice and subsequent gas jetting, and so far only known to occur at the Martian south pole. Their spatial configuration characteristics remain incompletely understood. We observed non-random s…

2020 Planetary and Space Science
MEx 11
Zodiacal light observations and its link with cosmic dust: A review
DOI: 10.1016/j.pss.2020.104973 Bibcode: 2020P&SS..19004973L

Lasue, Jeremie; Levasseur-Regourd, Anny-Chantal; Renard, Jean-Baptiste

The zodiacal light is a nightglow mostly visible along the plane of the ecliptic. It represents the background radiation associated with solar light scattered by the tenuous flattened interplanetary cloud of dust particles surrounding the Sun and the planets. It is an interesting subject of study, as the source of the micrometeoroids falling on Ea…

2020 Planetary and Space Science
Rosetta 11
Analogues of interplanetary dust particles to interpret the zodiacal light polarization
DOI: 10.1016/j.pss.2018.04.022 Bibcode: 2020P&SS..18304527H

Lasue, J.; Levasseur-Regourd, A. C.; Hadamcik, E. +1 more

2020 Planetary and Space Science
Rosetta 10