PPT-MARS HABITAT – SURFACE MATERIALS ISRU

Mars Sustainability Workshop Buzz Aldrin Space Institute Feb 89 2018 Jean Bigoney The Essentials Part 1 Materials seek a state of minimum energy Natural state of materials usually as oxides. Have you ever wanted to see strange photos from Mars? I made this so people could see what’s actually happening on mars and what is strange that scientists have found. Some of these pics could help us find us find out if we can live there and if there is life on mars. These photos could shape our future. So these are the top 5 most mysterious photos from mars.. Other processes on Mars. Dendritic. (tree-like) drainage valleys. Earth. Mars. Stream-lined islands. Fluting – Longitudinal lines caused by fluid flow. Fluting – Longitudinal lines caused by fluid flow. Topical Analyses of . Gap-Filling Activities. CL#12-3066. SKG breakdown. Atmospheric SKGs. 2. Large uncertainties in atmospheric models directly increase mission risk, reduce payload margins by increasing entry system mass, limit landing sites, and may force non-optimal technology choices. 10.1 Orbital Properties. 10.2 Physical Properties. 10.3 Long-Distance Observations of Mars. 10.4 The Martian Surface. 10.5 Water on Mars. Life on Mars?. 10.6 The Martian Atmosphere. 10.7 Martian Internal Structure. Martian geology: a rapid summary. Mars is geologically distinctive at the large scale. The southern hemisphere is made of ancient cratered terrain and the northern hemisphere flat, more recent (less impacted) terrain that is at lower elevation. This distinctive geology is called the . The orbits of Venus and Mercury show that these planets never appear far from the Sun.. Orbital and Physical Properties. The . terrestrial planets have similar densities and roughly similar sizes. , but their rotation periods, surface temperatures, and atmospheric pressures vary widely.. With its next . lander. , NASA plans to discover what turned Mars from a warm, wet place to the cold, arid planet we see today.. Long ago, the Red Planet was very different from the frozen, barren desert we have seen on our TV screens courtesy of Pathfinder. . Perspective from Atmospheric Science Stakeholders. Scot Rafkin. Southwest Research Institute. Boulder, CO. r. afkin.swri@gmail.com. Image Credit: MSSS/NASA/JPL. AMIII 2-4 Dec 2015. S. Rafkin -- Atmospheric Science. cool surface features. Lets look at some!. (all images credit: Mike . Sussman. ). The famous “Face on Mars”. Now don’t get all excited…. How Come We Missed These?. Look harder!. The Panda!. George Washington Screaming!. Kristopher A. Lee. 1. Why Water Electrolysis?. Electrolysis is a straightforward way to make oxygen on Mars or the Moon if you can obtain water.. 2. Sabatier: CO. 2. + 4H. 2. CH. 4. +. 2H. Gap-Filling Activities. CL#12-3066. SKG breakdown. Atmospheric SKGs. 2. Large uncertainties in atmospheric models directly increase mission risk, reduce payload margins by increasing entry system mass, limit landing sites, and may force non-optimal technology choices. As a group we have designed our functional space shuttle what will use to get to Mars. This design will be able to transport around 160 people. This number is very special as it is the repopulation number, this will help to colonies Mars. Our ship will contains hundreds of rooms all serving a different purpose, such as: a command post, hydroponic farms, research module, housing, designing room, fitness area and rooms to relax in.. Mars is the forth planet from the . sun. Mars has two moons in orbit. The names of the moons are called Phobos and Deimos. Mars is currently 218.27 million KMs from the sun. Mars’ diameter is 6,779kms. Introduction. Named after: . the Roman God of War. Visible to the naked eye. Earliest record of observation: . circa 1534 BCE, by the Ancient Egyptians .