PPT-Evolvable Mars Campaign

Presentation to Affordable Mars Workshop Pat Troutman December 2015 Pioneering Space Goals Fifty years after the creation of NASA our goal is no longer just a destination to reach Our goal is the capacity for people to work and learn and operate and live safely beyond the Earth for extended periods of time ultimately in ways that are more sustainable and even indefinite . These values our Five Principles set us apart from others requiring that we think and act differently towards our associates our brands and our business These principles have always been demanding and are an essential part of our heritage We belie MARS MARS MOBILEAUTOMATIC RECHARGE SYSTEM ComputerisedSoftware& Hardwaretorechargeall Mobile& Dth(Tv) Operators DistributorDealerRetailer-01Retailer-02Retailer-03Retailer-04 IP GSM Terminals with E-re evolvability. Vitaly. Feldman . Almaden. Research Center. Learning from examples vs . evolvability. Learnable from examples. Evolvable. Parity functions. The core model: PAC . [Valiant . 84. ]. Learner observes random examples: . Figure 2: Mars Mission Precursor Design Methodolog Nuclear Thermal Propulsion 4. Chemical Propulsion 5. Life Support Systems 6. In Situ Resource Utilization (ISRU) 7. Low-Gravity Threat Mitigation Future In-Space Operations (FISO) Working Group. Telecon. . Presentation. Sept 14, 2011. Gordon Woodcock. Huntsville Alabama. 1. Historical Note. In the 1960s, . Wernher. Von . Braun had a well thought-out overall approach to space exploration, sometimes known as the . Advisory Group. Matt Wallace . Mars 2020 Deputy Project Manager. February 22, 2017. © 2016 California Institute of Technology. Government sponsorship acknowledged.. Project Overview. Salient Features. H. å. kan. . Svedhem. Project Scientist. MEPAG, Monrovia, . Ca. , 22 February 2017. NOTE ADDED BY JPL WEBMASTER: This content has not been approved or adopted by NASA, JPL, or the California Institute of Technology. This document is being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology. . Lisbon, Portugal; June 16, 2011. Dave Des Marais, MEPAG Chair. MEPAG E2E-iSAG. Pre-decisional: for discussion purposes only. 6/10/2011. 1. Package 1 of 5. Sample Return is the Next Step. 2. Pre-decisional: for discussion purposes only. Launch in July-August 2020 from Cape Canaveral Air Force Station, FloridaLaunching on a ULA Atlas 541 procured under NASA’s Launch Services Programlled Jezero Craterexploring the landing sit 1 National Space Report Pursuant to Section 432(b) of the NASA Transition Authorization Act of 2017 (P.L. 115 - 10) September 2018 2 Table of Contents Section 1 Forward to the Moon , Mars and Bey 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!. Size & Distance. Smaller than Earth (0.532x). Mars . diam. ~ 6779 km (4212 miles). Earth . diam. ~ 12,742 km (7918 miles). 8 Mars would fit inside the Earth!. 1.5 AU from the sun (~140 million miles). Sample Return (MSR). E2E-iSAG: Phase I Analysis. Scott McLennan, Mark . Sephton. , and the E2E-iSAG team. AGU Town Hall, Dec. 15, 2010. MEPAG E2E-iSAG. Pre-decisional: for discussion purposes only. 2. 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.