Related Experiment Video
Updated: May 5, 2026

09:12
Production of Single Tracks of Ti-6Al-4V by Directed Energy Deposition to Determine the Layer Thickness for Multilayer Deposition
Published on: March 13, 2018
8.5K
Martian stepped-delta formation by rapid water release
Erin R Kraal1, Maurits van Dijk, George Postma
1Faculty of Geosciences, Utrecht University, Postbus 80115, 3508 TC, Utrecht, The Netherlands. ekraal@vt.edu
Nature
|February 22, 2008
Summary
Martian stepped deltas suggest surface water flowed for only tens of years, not millions. This finding provides new constraints on Mars
Area of Science:
- Planetary Science
- Geology
- Hydrology
Background:
- Deltas and alluvial fans on Mars are key indicators of past surface water flow.
- Previous morphological studies offered broad time estimates (decades to millions of years) for Martian hydrologic events.
- Understanding the formation of Martian deltas is crucial for reconstructing the planet's water history.
Purpose of the Study:
- To investigate the formation timescale of distinct Martian stepped (terraced) deltas.
- To constrain the duration and magnitude of past surface water flow events on Mars.
Main Methods:
- Utilized sand flume experiments to simulate delta formation.
- Analyzed the resulting morphology to infer formation processes and timescales.
Main Results:
- Martian stepped deltas likely formed from a single basin-filling event.
- This event occurred over a short timescale, estimated to be tens of years.
- The water volume required is comparable to large terrestrial rivers like the Mississippi.
Conclusions:
- Stepped deltas provide both minimum and maximum constraints on the duration of some Martian surface flows.
- The findings support a hypothesis of sudden water release from subsurface storage.
- This rapid release likely formed terraced delta deposits over alluvial fans.
Related Concept Videos
States of Water
46.5K
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.
Water freezes when the intermolecular forces are greater than the kinetic energy. Unlike most other substances, water is less dense in its solid state than in its liquid state. This is because each water molecule can form...
Water freezes when the intermolecular forces are greater than the kinetic energy. Unlike most other substances, water is less dense in its solid state than in its liquid state. This is because each water molecule can form...
46.5K
The Water Cycle
23.1K
The Earth’s hydrosphere includes all of the areas where the storage and movement of water occurs. Since water is the basis of all living processes, the cycling of water is extremely important to ecosystem dynamics.
23.1K
Speciation Rates
18.8K
Overview
18.8K
Hess's Law
44.1K
There are two ways to determine the amount of heat involved in a chemical change: measure it experimentally, or calculate it from other experimentally determined enthalpy changes. Some reactions are difficult, if not impossible, to investigate and make accurate measurements for experimentally. And even when a reaction is not hard to perform or measure, it is convenient to be able to determine the heat involved in a reaction without having to perform an experiment.
44.1K
Nuclear Fusion
33.2K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
33.2K
Escape Velocities of Gases
1.5K
To escape the Earth's gravity, an object near the top of the atmosphere at an altitude of 100 km must travel away from Earth at 11.1 km/s. This speed is called the escape velocity. The temperature at which gas molecules attain the rms speed, which is equal to the escape velocity, can be estimated by using the equation for the average kinetic energy of the gas molecules. According to the kinetic theory of gas, the average kinetic energy of the gas molecules is proportional to its...
1.5K

