The Chief Scientist for NASA’s Mars Program, David Beaty, has spent more than 20 years searching the Earth for metals and oil, and this makes the right man to help future astronauts survive off-Earth.Ĭhecking Out ‘Cheyenne’ and Testing Relay for Phoenix How to Open a THEMIS QUB File In ENVI and MultiSpec Prospecting the Moon and Mars for Supplies Voyager Image DisplayĪn easy to use shareware Windows 95/98/NT/2000 based image processing program that can read and enhance images from various NASA spacecraft. The downloaded products are fully functional and they run in a restricted mode for seven-minute sessions. ENVI FreeLookĮNVI FreeLook is designed to provide basic viewing, data selection, and data quality assessment capabilities for a wide variety of image data. ImageJ is the world’s fastest pure Java image processing program. ImageJ runs on Linux, Mac OS 9, Mac OS X and Windows. ImageJįree Image Processing and Analysis Tool in Java. UTHSCSA ImageTool (IT) is a free image processing and analysis program for Microsoft Windows 9x, Windows ME or Windows NT. MultiSpec© with its documentation© is distributed without charge. MultiSpec©Ī Multispectral Image Data Analysis System. NASAView is a Free Planetary Data System archive product display tool that runs on Sun/Solaries, Windows/NT/95, and PowerMac platforms with a common look-and-feel Graphical User Interface (GUI). Moon’ Phobos and Deimos Downloads NASAVIEW™ SOFTWARE Mars Desert Research Station Past Missions The older flows are most likely also from Arsia Mons The upper part of the image shows the relatively young volcanic flows from Arsia Mons, while the bottom exhibits the flow front texture of older flows. This daytime infrared image was collected Aug. The picture is located near 83.4°S, 8.1°W. This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows evidence of wind deposition of fine sediment in the form of drifts in the lee of obstacles in the martian south polar region. The picture is certainly far from optimum but the best shot I found of this region. Pictures allows filling most of the gaps. Lines separated by dark bars three pixel wide. The picture was reconstructed by using three very garbled pictureįrames sent back to Earth in 1976 by Viking Orbiter 1 (photos: 489a06,Ġ8, 10) only containing 25 to 33 percent information in form of single I think it is the result of a oblique impact 3.0 billion years This “Easter Egg” is a oval shaped crater around 33.21 S / 173.95 W.
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