1. Understanding martian gullies Howe, K. L. 1,2, Coleman, K. S. A. 2,3, Dixon, J.C 2,3 1 Department of Geological Sciences, State University of New York at Geneseo, Geneseo, NY 14454; 2 Arkansas Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, AR 72701; 3 Department of Geosciences, University of Arkansas, Fayetteville, AR 72701 INTRODUCTIONRESULTS CONCLUSIONS METHODOLOGY Malin and Edgett (2000) identified martian features that resemble earth gullies Questions as to the formation of martian gullies exist since gullies are often located in areas with surface temperatures below water’s freezing point Objective of this study: simulate gully formation with morphologies similar to those observed on Mars and use the results to identify potential fluid and formation characteristics The alcove, channel and apron measurements (length, width, depth) are taken and sand saturation is measured (Figure 2) Parameters are recorded and graphed (Figure 3) for 4 different flows (445, 705, 965, 1260 ml/s) at 3 different slopes (10°, 20°, 30°) FUTURE RESEARCH Detailed morphometric analysis of gullies will be conducted using GIS and similar resources REFERENCES Malin, M. C. and Edgett, K. S., 2000, Evidence for recent ground water seepage and surface runoff on Mars: Science, v. 288, no. 5475, p. 2330-2336. ACKNOWLEDGEMENTS Arkansas Center for Space and Planetary Sciences for funding Walter Graupner for technical assistance DISCUSSION Simulations in flume show three distinct sections of the gully Some gully parameters show a stronger relationship than others to the changing flow rate and/or changing slope Gully response to flow rate changes are visually more obvious than slope changes Many of the high, isolated points on graphs can be attributed to high sand saturation during run Most noticeable in the apron, saturation has a relationship with measurements and shape of gully sections Gully formation simulated in the flume can be used to study martian gullies Both slope and flow rate have noticeable effects on alcove, channel and apron measurements Parameter most impacted by changing slope and flow rate was the total gully volume Least effected parameters are the depths, especially at base of the channels Aprons of saturated runs tend to be thinner and more triangular shaped than the thicker, lobate aprons of less saturated runs Figure 3: Graphs show that length, width and depth of the gully alcoves are affected by changes in flow rate (top) and changes in slope (bottom) Figure 4: Differences in shape of gully sections are apparent with different saturations. Both pictures at slope 20 ° and flow 705 ml/s. High saturation on left; lower saturation on right. Figure 1: The flume allows for the process of gully formation to be studied Figure 2: Measurement of gully parameters allows for analysis of gully morphology Alcove Volume Dimensions vs. Flow Rate Alcove Volume Dimensions vs. Slope Flow Rate (ml/s) at 10 ° Slope Alcove Measurements (mm) Slope (degrees) Alcove Measurements (mm) Alcove Volume Dimensions vs. Slope Alcove Length Alcove Width Alcove Depth 4 mm Alcove Channel Apron WidthsDepthsLengths Saturation 4 mm Simulations run in 1x1.5 meter flume (Figure 1) Water flows from overhead bucket, through flow meter into tubing sunk below the sand surface and emerges at the break in slope