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Water exists in any one of the three classical states: solid (ice), liquid (water), and gas (steam or water vapor). The state of water depends on i) the intermolecular forces that draw molecules together and ii) the kinetic energy that leads to movements that pull them apart.
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Concrete's susceptibility to frost damage during freeze-thaw cycles demands strategic measures to enhance its frost resistance. Employing techniques like air entrainment, adjusting the water-cement ratio, proper curing, and selecting appropriate aggregates are essential.
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The experimental conditions in a gravimetric analysis should be optimized to maximize the particle size and purity of the obtained precipitate. Ideally, the concentration of the precipitating reagent should be low with effective stirring to maintain low relative supersaturation for the growth of large crystals. In homogeneous precipitation, the precipitant is slowly generated by a chemical reaction in the solution to avoid local reagent excesses. For example, urea decomposes gradually to...
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Manufacturing Simple and Inexpensive Soil Surface Temperature and Gravimetric Water Content Sensors
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Warm early Mars surface enabled by high-altitude water ice clouds.

Edwin S Kite1, Liam J Steele2, Michael A Mischna3

  • 1Department of the Geophysical Sciences, University of Chicago, Chicago, IL 60615; kite@uchicago.edu.

Proceedings of the National Academy of Sciences of the United States of America
|April 27, 2021
PubMed
Summary

Early Mars may have been warmed by water ice clouds, creating lakes. This global climate model study shows clouds can sustain warm, arid conditions for centuries, supporting the cloud greenhouse hypothesis.

Keywords:
Marspaleoclimateplanetary habitability

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Area of Science:

  • Planetary Science
  • Climate Modeling
  • Astrobiology

Background:

  • Early Mars received less solar radiation than present-day Earth.
  • Evidence suggests the presence of liquid water (lakes, rivers) on early Mars.
  • An unknown warming mechanism is required to explain these past warm, wet conditions.

Purpose of the Study:

  • To investigate the cloud greenhouse hypothesis as a warming mechanism for early Mars.
  • To determine if water ice clouds can create sustained warm climates capable of supporting lakes.
  • To reconcile climate model results with geological evidence of a warm, arid early Mars.

Main Methods:

  • Utilized a global climate model (GCM) to simulate Mars-like planetary conditions.
  • Incorporated radiative transfer effects of water ice clouds.
  • Varied surface water distribution to assess its impact on climate stability.

Main Results:

  • A cloud greenhouse effect can warm a Mars-like planet to approximately 265 K, enabling low-latitude lakes.
  • Warm, stable climates can persist for centuries under specific conditions.
  • Spatially patchy surface water and high-altitude clouds are crucial for sustained warming.
  • The model predicts arid conditions (25% relative humidity) consistent with geological interpretations.
  • Cloud persistence is maintained by sublimation of falling ice particles, moistening the atmosphere.

Conclusions:

  • The cloud greenhouse hypothesis is a viable explanation for sustained warm, lake-forming climates on early Mars.
  • The model supports a warm, arid climate scenario for early Mars, with lakes potentially fed by groundwater or melting ice.
  • This research provides a potential mechanism for reconciling past water presence with lower solar insolation.