Evidence map›Paper›PMID 34770727›Full record

ArticleSensors (Basel, Switzerland)2021

Experimental Investigation of the Atmosphere-Regolith Water Cycle on Present-Day Mars.

Abhilash Vakkada Ramachandran, María-Paz Zorzano, Javier Martín-Torres

Abstract read
In one paragraph

Article in Sensors (Basel, Switzerland), 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 3 papers.

0numbers the graph read from it
0cells of the map it votes in
3citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

3 citing papers in PubMed.

  1. Article
  2. Review
  3. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

3 authors.

Abhilash Vakkada RamachandranGroup of Atmospheric Science, Department of Computer Science, Electrical and Space Engineering, Luleå University of Technology, 97187 Luleå, Sweden.ORCID 0000-0003-0499-6370
María-Paz ZorzanoCentro de Astrobiología (CSIC-INTA), Torrejón de Ardoz, 28850 Madrid, Spain.ORCID 0000-0002-4492-9650
Javier Martín-TorresSchool of Geosciences, University of Aberdeen, Aberdeen AB24 3FX, UK.ORCID 0000-0001-6479-2236

Funding

Kempe Foundation SMK-1934Knut and Alice Wallenberg Foundation KAW 2016.0346Spanish State Research Agency MDM-2017-0737
6 · The paper itself

Abstract

The water content of the upper layers of the surface of Mars is not yet quantified. Laboratory simulations are the only feasible way to investigate this in a controlled way on Earth, and then compare it with remote and in situ observations of spacecrafts on Mars. Describing the processes that may induce changes in the water content of the surface is critical to determine the present-day habitability of the Martian surface, to understand the atmospheric water cycle, and to estimate the efficiency of future water extraction procedures from the regolith for In Situ Resource Utilization (ISRU). This paper illustrates the application of the SpaceQ facility to simulate the near-surface water cycle under Martian conditions. Rover Environmental Monitoring Station (REMS) observations at Gale crater show a non-equilibrium situation in the atmospheric H

Indexed as

Extraterrestrial EnvironmentMarsAtmosphereSpacecraftWaterWater CycleWaterhabitabilityISRUMarsplanetary protectionpure liquid waterwater cycle simulation

Identifiers

PMID34770727
PMCPMC8588207

What OpenQuestion holds

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LicenceCC BY
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Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.