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Planetary surface dating from crater size-frequency distribution measurements: Poisson timing analysis
DOI: 10.1016/j.icarus.2016.05.019 Bibcode: 2016Icar..277..279M

Michael, G. G.; Kneissl, T.; Neesemann, A.

The predictions of crater chronology models have customarily been evaluated by dividing a crater population into discrete diameter intervals, plotting the crater density for each, and finding a best-fit model isochron, with the uncertainty in the procedure being assessed using 1/√n estimates, where n is the number of craters in an interval. This a…

2016 Icarus
MEx 131
Sequence and relative timing of large lakes in Gale crater (Mars) after the formation of Mount Sharp
DOI: 10.1002/2015JE004905 Bibcode: 2016JGRE..121..472P

Mangold, Nicolas; Williams, Rebecca M. E.; Palucis, Marisa C. +6 more

The quantification of lake levels in Gale crater is important to define the hydrologic and climatic history experienced by the sedimentary deposits found by Curiosity. We propose that there were at least three major lake stands within Gale, each persisted >1000 years, and all occurred after Mount Sharp reached close to its current topographic f…

2016 Journal of Geophysical Research (Planets)
MEx 81
Observations of an aeolian landscape: From surface to orbit in Gale Crater
DOI: 10.1016/j.icarus.2015.09.042 Bibcode: 2016Icar..280...37D

Day, Mackenzie; Kocurek, Gary

Landscapes derived solely from aeolian processes are rare on Earth because of the dominance of subaqueous processes. In contrast, aeolian-derived landscapes should typify Mars because of the absence of liquid water, the long exposure times of surfaces, and the presence of wind as the default geomorphic agent. Using the full range of available orbi…

2016 Icarus
MEx 79
The High Resolution Stereo Camera (HRSC) of Mars Express and its approach to science analysis and mapping for Mars and its satellites
DOI: 10.1016/j.pss.2016.02.014 Bibcode: 2016P&SS..126...93G

Jaumann, R.; Oberst, J.; Preusker, F. +32 more

The High Resolution Stereo Camera (HRSC) of ESA's Mars Express is designed to map and investigate the topography of Mars. The camera, in particular its Super Resolution Channel (SRC), also obtains images of Phobos and Deimos on a regular basis. As HRSC is a push broom scanning instrument with nine CCD line detectors mounted in parallel, its unique…

2016 Planetary and Space Science
MEx 75
Insights into surface runoff on early Mars from paleolake basin morphology and stratigraphy
DOI: 10.1130/G37734.1 Bibcode: 2016Geo....44..419G

Mustard, John F.; Goudge, Timothy A.; Head, James W. +2 more

2016 Geology
MEx 70
Observations and modeling of northern mid-latitude recurring slope lineae (RSL) suggest recharge by a present-day martian briny aquifer
DOI: 10.1016/j.icarus.2015.10.007 Bibcode: 2016Icar..265..125S

Michaels, Timothy I.; Hanley, Jennifer; Grimm, Robert E. +1 more

Recurring slope lineae (RSL) are narrow (0.5-5 m) dark features on Mars that incrementally lengthen down steep slopes, fade in colder seasons, and recur annually. These features have been identified from the northern to southern mid-latitudes. Here, we describe how observations of northern mid-latitude RSL in northern Chryse Planitia and southwest…

2016 Icarus
MEx 60
Mars Express 10 years at Mars: Observations by the Mars Express Radio Science Experiment (MaRS)
DOI: 10.1016/j.pss.2016.02.013 Bibcode: 2016P&SS..127...44P

Pätzold, M.; Hahn, M.; Rosenblatt, P. +17 more

The Mars Express spacecraft is operating in Mars orbit since early 2004. The Mars Express Radio Science Experiment (MaRS) employs the spacecraft and ground station radio systems (i) to conduct radio occultations of the atmosphere and ionosphere to obtain vertical profiles of temperature, pressure, neutral number densities and electron density, (ii…

2016 Planetary and Space Science
MEx VenusExpress 58
Annual variations in the Martian bow shock location as observed by the Mars Express mission
DOI: 10.1002/2016JA023316 Bibcode: 2016JGRA..12111474H

Holmström, M.; Fränz, M.; Lester, M. +12 more

The Martian bow shock distance has previously been shown to be anticorrelated with solar wind dynamic pressure but correlated with solar extreme ultraviolet (EUV) irradiance. Since both of these solar parameters reduce with the square of the distance from the Sun, and Mars' orbit about the Sun increases by ∼0.3 AU from perihelion to aphelion, it i…

2016 Journal of Geophysical Research (Space Physics)
MEx 54
Discovery of alunite in Cross crater, Terra Sirenum, Mars: Evidence for acidic, sulfurous waters
DOI: 10.2138/am-2016-5574 Bibcode: 2016AmMin.101.1527E

Murchie, Scott L.; Ehlmann, Bethany L.; Mustard, John F. +11 more

2016 American Mineralogist
MEx 54
Geologic context of recurring slope lineae in Melas and Coprates Chasmata, Mars
DOI: 10.1002/2015JE004991 Bibcode: 2016JGRE..121.1204C

McEwen, Alfred; Chojnacki, Matthew; Ojha, Lujendra +3 more

One of the major Mars discoveries of recent years is the existence of recurring slope lineae (RSL), which suggests that liquid water occurs on or near the surface of Mars today. These dark and narrow features emerge from steep, rocky exposures and incrementally grow, fade, and reform on a seasonal basis and are detected in images from the High Res…

2016 Journal of Geophysical Research (Planets)
MEx 53