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I was originally talking about the difference in temperature between the North Summer and the South Summer because of the talk about the bigger possibility of finding life near the South pole.
Originally posted by blue bird
* there is a big variation in temparature
Originally posted by zorgon
Originally posted by bigfatfurrytexan
NASA, that is who. Well...they say that the atmoshpere is thin.
OH THOSE GUYS
Clouds on Mars drifting by....
Shall we recognize in Mars all that makes our own world so well fitted for our wants – land and water, mountain and valley, cloud and sunshine, rain and ice, and snow, rivers and lakes, ocean currents and wind currents, without believing further in the existence of those forms of life without which all of these things would be wasted? ... it is yet to speculate ten thousand times more rashly to assert ... that Mars is a barren waste, either wholly untenanted by living creatures, or inhabited by beings belonging to the lowest orders of animated existence.
Aptly-named Mojave crater in the Xanthe Terra region has alluvial fans that look remarkably similar to landforms in the Mojave Desert of southeastern California and portions of Nevada and Arizona. Alluvial fans are fan-shaped deposits of water-transported material (alluvium). They typically form at the base of hills or mountains where there is a marked break, or flattening of slope. They typically deposit big rocks near their mouths (close to the mountains) and smaller rocks at greater distances. Alluvial fans form as a result of heavy desert downpours, typically thundershowers. Because deserts are poorly vegetated, heavy and short-lived downpours create a great deal of erosion and nearby deposition. There are fans inside and around the outsides of Mojave crater on Mars that perfectly match the morphology of alluvial fans on Earth, with the exception of a few small impact craters dotting this Martian landscape. Channels begin at the apex of topographic ridges, consistent . This remarkable landscape was first discovered from Mars Orbital Camera images. Mars researchers have suggested that impact-induced atmospheric precipitation may have created these unique landscapes.
Formation of Martian Gullies by the Action of Liquid Water Flowing under Current Martian Environmental Conditions
J.L. Heldmann (NASA Ames Research Center), O.B. Toon (University of Colorado), W.H. Pollard (McGill University), M.T. Mellon, J. Pitlick (University of Colorado), C.P. McKay (NASA Ames Research Center), D.T. Andersen (SETI)
Geomorphic evidence suggests that recent gullies on Mars were formed by fluvial activity. Irrespective of the ultimate source of the fluid carving the gullies, we seek to understand the behavior of this fluid after it reaches the Martian surface. We numerically simulate the flow of liquid water within gully channels to determine whether liquid water can flow over sufficient distances to carve the observed channels and to place constraints on the flow rate and salinity of the water. This model is first developed to simulate a well-observed terrestrial example of channel flow in the High Canadian Arctic. This model is then applied to Mars.
We find that, contrary to popular belief, the fluvially-carved Martian gullies are consistent with formation conditions such as now occur on Mars, outside of the temperature-pressure stability regime of liquid water. Our model of the action of flowing pure liquid water produces the observed gully length distribution only at surface pressures and temperatures below the triple point where liquid water simultaneously boils and freezes and thus suggests that gullies were formed under conditions similar to present-day Mars. Numerical simulations show that pure liquid water flowing at rates of 15-60 m3/s is consistent with the observations of the gullies. The formation of gullies on Mars is inconsistent with briny fluid flows with significant flow rates because inhibiting rapid evaporation by vapor pressure suppression (or other means such as ice sheets capping the flow, or a higher pressure climate state) results in channels that are much longer than those observed on Mars. Instead, our model indicates that these fluvially-carved gullies formed in the low temperature and low pressure conditions of present day Mars by the action of relatively pure liquid water.
A circular pattern can be seen at the center of this image, made by the Spirit rover's Microscopic Imager. Compare its appearance with the earthly lichen pictured below.
The first impression I got — based on the morphology alone — was how similar it looked to a common terrestrial foliose lichen," said Barry DiGregorio, a research associate for the Cardiff Centre for Astrobiology in the United Kingdom
This Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) "targeted image" shows a region of sand dunes surrounding the Martian north polar cap. CRISM, an instrument on NASA's Mars Reconnaissance Orbiter, acquired the image at 1811 UTC (2:11 p.m. EDT) on Oct. 1, 2006. The imaged site is near 80.0 degrees north latitude, 240.7 degrees east longitude. It covers an area about 12 kilometers (7.5 miles) square. At the center of the image, the spatial resolution is as good as 20 meters (65 feet) per pixel. The image was taken in 544 colors covering 0.36 to 3.92 micrometers.
Gypsum is a very soft mineral composed of calcium sulfate dihydrate............Gypsum is deposited in lake and sea water, as well as in hot springs, from volcanic vapors, and sulfate solutions in veins. Hydrothermal anhydrite in veins is commonly hydrated to gypsum by groundwater in near surface exposures..............................Because gypsum dissolves over time in water, gypsum is rarely found in the form of sand. However, the unique conditions of the White Sands National Monument in the US state of New Mexico
Originally posted by blue bird
Colonies of cyanobacteria on stromatolites!?
* Mars
source
*Earth
source
This band combination shows rock in blue, water in black and vegetated areas in browns, oranges and light greens.
Originally posted by bigfatfurrytexan
the question i have about this image:
Is where does the stuff that makes up the ice go, and how does it return? Without an atmosphere one would expect that it would dissipate into space, correct?
Originally posted by MicheleLee
I did enjoy the below video (presentation is nice) and hope you enjoy it to.
Maximize it to see it better.
Originally posted by zorgon
But that picture above I am REALLY curious about that black ring!!! In the center image you can see it just below the ice, then it really stands out in the last image
Originally posted by Gonjo
Yeah ofcourse its most likely something like that will be around the steamvents linked earlier in this thread I think atleast... I just kinda found it odd when you had an orbital pictures colored to match the colors on a single rock.
Wasnt trying to say it was impossible just that the scale of the mars example picture was so off it was silly. Its pretty much impossible to say for sure anything about the form of life but it would make sense for the kind of plantlife like you said, lichen and so on, to be the ones who would be most likely to blame for the different shades of the "rocks" in the meltdown areas.
But in a recent study by European scientists, lichen survived a trip in space even better than bacteria do.
All the lichen we have subjected to space or to space-simulated conditions have survived. After we put them in favorable conditions where they could recuperate, they exhibited high photosynthetic activity. We were surprised that the lichen reactivate so soon after exposure, and that there were no significant changes in the photosynthetic activity before and after exposure.
Originally posted by Gonjo
Also I took a part in the "mission" to mark some pictures for HiRISE and found few interesting ones to say the least.