Melbourne - Oct. 19, 2000
A few paradoxes remain about this new Mars. Chief amongst these is the Carbonate Paradox. Basic chemistry requires that if Mars had liquid water at surface for any reasonable period of time, then rapid chemical reactions between the atmospheric CO2 dissolved in the water, and the rocks of Mars, would produce copious quantities of carbonate rock. The process should be so efficient that almost no CO2 should remain, and thick deposits of carbonates should fill all the lake and ocean beds of Mars.
Despite decades of orbital and Earth-based imaging and spectroscopy, and 3 Landers, no trace of surface carbonates can be found. Plenty of young impact craters have drilled into and exposed the lake beds, yet no carbonates are seen. The only carbonates that we know of on Mars come from ALH84001, the infamous "Life on Mars" meteorite". This contains carbonate globules that defy analysis. Some investigators are adamant that they are high temperature hydrothermal carbonates formed as the original heat of the igneous rock dissipated, and water circulated through the grains. Others suggest a low-temperature and presumed near-surface origin.
There is a Volumetric Paradox associated with the outburst floods. There is only a small amount of space available between the grains of a rock, even for a loose aggregate of grains. In order to flow catastrophically across the surface, many times more water than rock is required, otherwise a thick sluggish slurry develops, with very different flow duration and deposit morphology. In order to reproduce the observed features, about 10 times as much water is required, as the volume of the chaotic zone. It is hard to store and then release this amount of water - hence the complex recycling scenarios with many smaller floods, each tapping an enlarged aquifer.
We also have to remember the Faint Young Sun Paradox. Our knowledge of stellar evolution and fusion processes suggests that the Sun has warmed over geologic time. When it was first born, it only produced 70% of its present output, increasing steadily with time. The young planets would have been colder than they now are and even more extreme greenhouse atmospheres are required to compensate for this.
Perhaps we should take a note from history and see if we are not inadvertently starting down the same road of interpreting imperfect data about Mars to get the answer we would like, rather that which is most likely. Everything about Mars agrees that it is cold and dry, except for those outburst flood channels. Is there any other way to interpret them?
The role of CO2 on Mars
Because of this, liquid CO2 cannot exist on Mars' surface despite the fact that the temperature range for Mars is perfect for liquid CO2 (except in polar regions where it is too cold). However, it is a well known fact that underground the pressure increases due to the weight of rocks overhead. One does not need to go down more than a few hundred metres before the pressure is sufficient for liquid CO2 to be stable. Of course, some sort of seal is required, otherwise the CO2 will escape up cracks and between the individual grains of Mars' regolith, but a thin layer of impervious rock, or more probably a clotting layer of water ice can easily provide such a seal.
These flows are part of a suite of "Density Flows", so named because they consist of a dense fluidised cloud that flows downhill as if it were a fluid. They have interesting properties since they are compressible, travel at very high speeds, and can also move up and over large obstacles. On Earth, giant flows of this type have crossed ranges of hills nearly 1 km high and reformed on the far side to continue their destructive advance. Other examples are Snow Avalanches, Submarine Turbidites, and Long Run-Out Rock Avalanches. These flows are capable of travelling long distances if they are either initially very large, or if they contain a source of volatiles to sustain their fluidity. Boulders of metre scale or more are easily carried for many kilometres on a cushion of hot air!
Subscribe To SpaceDaily Express
|The content herein, unless otherwise known to be public domain, are Copyright 1995-2016 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement All images and articles appearing on Space Media Network have been edited or digitally altered in some way. Any requests to remove copyright material will be acted upon in a timely and appropriate manner. Any attempt to extort money from Space Media Network will be ignored and reported to Australian Law Enforcement Agencies as a potential case of financial fraud involving the use of a telephonic carriage device or postal service.|