Comparative Study of Aerial Platforms for Mars Exploration
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NASA Mars Helicopter Team Striving for a “Kitty Hawk” Moment
NASA Mars Helicopter Team Striving for a “Kitty Hawk” Moment NASA’s next Mars exploration ground vehicle, Mars 2020 Rover, will carry along what could become the first aircraft to fly on another planet. By Richard Whittle he world altitude record for a helicopter was set on June 12, 1972, when Aérospatiale chief test pilot Jean Boulet coaxed T his company’s first SA 315 Lama to a hair-raising 12,442 m (40,820 ft) above sea level at Aérodrome d’Istres, northwest of Marseille, France. Roughly a year from now, NASA hopes to fly an electric helicopter at altitudes equivalent to two and a half times Boulet’s enduring record. But NASA’s small, unmanned machine actually will fly only about five meters above the surface where it is to take off and land — the planet Mars. Members of NASA’s Mars Helicopter team prepare the flight model (the actual vehicle going to Mars) for a test in the JPL The NASA Mars Helicopter is to make a seven-month trip to its Space Simulator on Jan. 18, 2019. (NASA photo) destination folded up and attached to the underbelly of the Mars 2020 Rover, “Perseverance,” a 10-foot-long (3 m), 9-foot-wide (2.7 The atmosphere of Mars — 95% carbon dioxide — is about one m), 7-foot-tall (2.13 m), 2,260-lb (1,025-kg) ground exploration percent as dense as the atmosphere of Earth. That makes flying at vehicle. The Rover is scheduled for launch from Cape Canaveral five meters on Mars “equal to about 100,000 feet [30,480 m] above this July on a United Launch Alliance Atlas V rocket and targeted sea level here on Earth,” noted Balaram. -
Infrared Experiments for Spaceborne Planetary Atmospheres Research Full Report
NASA Technical Memorandum 84414 Infrared Experiments for Spaceborne Planetary Atmospheres Research Full Report Infrared Experiments Working Group NOVEMBER 1981 NASA NASA Technical Memorandum 84414 Infrared Experiments for Spaceborne Planetary Atmospheres Research Full Report Infrared Experiments Working Group Jet Propulsion Laboratory Pasadena, California NASA National Aeronautics and Space Administration Scientific and Technical Information Branch 1981 TABLE OF CONTENTS Preface Summary of Principal Conclusions and Recommendations Chapter I The Role of Infrared Sensing in Atmospheric Science Chapter II Review of Existing Infrared Measurement Techniques Chapter III Critical Comparison of Proposed Measurement Techniques Chapter IV Conclusions and Recommended Instrument Developments Appendices: A Critical Technologies B Applicability of Atmospheric Infrared Instrumentation to Surface Science C Supporting Studies in Data Analysis and Numerical Modeling D Description of Planned Earth Orbital Platforms ii PREFACE Experiments conducted in the infrared spectral region provide a powerful tool for the study of the composition, structure and dynamics of planetary atmospheres. However, the field has become highly complex, especially that part associated with spacecraft sensing, and the range of technologies used so diverse that it is difficult to determine which of the available methods for making a particular measurement is to be preferred, even for those deeply involved in the field. Unfortunately, the realities of the age demand that some selectivity be employed; not all approaches can be supported. Furthermore, the chosen methods are generally sufficiently untried that long pre-flight developments are neces- sary if viable proposals are to be written for future flight opportunities. These considerations clearly lead to a program of developments which must be coordinated on a national scale. -
Mariner to Mercury, Venus and Mars
NASA Facts National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 Mariner to Mercury, Venus and Mars Between 1962 and late 1973, NASA’s Jet carry a host of scientific instruments. Some of the Propulsion Laboratory designed and built 10 space- instruments, such as cameras, would need to be point- craft named Mariner to explore the inner solar system ed at the target body it was studying. Other instru- -- visiting the planets Venus, Mars and Mercury for ments were non-directional and studied phenomena the first time, and returning to Venus and Mars for such as magnetic fields and charged particles. JPL additional close observations. The final mission in the engineers proposed to make the Mariners “three-axis- series, Mariner 10, flew past Venus before going on to stabilized,” meaning that unlike other space probes encounter Mercury, after which it returned to Mercury they would not spin. for a total of three flybys. The next-to-last, Mariner Each of the Mariner projects was designed to have 9, became the first ever to orbit another planet when two spacecraft launched on separate rockets, in case it rached Mars for about a year of mapping and mea- of difficulties with the nearly untried launch vehicles. surement. Mariner 1, Mariner 3, and Mariner 8 were in fact lost The Mariners were all relatively small robotic during launch, but their backups were successful. No explorers, each launched on an Atlas rocket with Mariners were lost in later flight to their destination either an Agena or Centaur upper-stage booster, and planets or before completing their scientific missions. -
Complete List of Contents
Complete List of Contents Volume 1 Cape Canaveral and the Kennedy Space Center ......213 Publisher’s Note ......................................................... vii Chandra X-Ray Observatory ....................................223 Introduction ................................................................. ix Clementine Mission to the Moon .............................229 Preface to the Third Edition ..................................... xiii Commercial Crewed vehicles ..................................235 Contributors ............................................................. xvii Compton Gamma Ray Observatory .........................240 List of Abbreviations ................................................. xxi Cooperation in Space: U.S. and Russian .................247 Complete List of Contents .................................... xxxiii Dawn Mission ..........................................................254 Deep Impact .............................................................259 Air Traffic Control Satellites ........................................1 Deep Space Network ................................................264 Amateur Radio Satellites .............................................6 Delta Launch Vehicles .............................................271 Ames Research Center ...............................................12 Dynamics Explorers .................................................279 Ansari X Prize ............................................................19 Early-Warning Satellites ..........................................284 -
Planetary Exploration Using Biomimetics an Entomopter for Flight on Mars Phase II Project NAS5-98051
Planetary Exploration Using Biomimetics An Entomopter for Flight On Mars Phase II Project NAS5-98051 NIAC Fellows Conference June 11-12, 2002 Lunar and Planetary Institute Houston Texas Anthony Colozza Northland Scientific / Ohio Aerospace Institute Cleveland, Ohio Planetary Exploration Using Biomimetics Team Members • Mr. Anthony Colozza / Northland Scientific Inc. • Prof. Robert Michelson / Georgia Tech Research Institute • Mr. Teryn Dalbello / University of Toledo ICOMP • Dr.Carol Kory / Northland Scientific Inc. • Dr. K.M. Isaac / University of Missouri-Rolla • Mr. Frank Porath / OAI • Mr. Curtis Smith / OAI Mars Exploration Mars has been the primary object of planetary exploration for the past 25 years To date all exploration vehicles have been landers orbiters and a rover The next method of exploration that makes sense for mars is a flight vehicle Mars Exploration Odyssey Orbiter Viking I & II Lander & Orbiter Global Surveyor Pathfinder Lander & Rover Mars Environment Mars Earth Temp Range -143°C to 27°C -62°C to 50°C & Mean -43°C 15°C Surface 650 Pa 103300 Pa Pressure Gravity 3.75 m/s2 9.81 m/s2 Day Length 24.6 hrs 23.94 hrs Year Length 686 days 365.26 days Diameter 6794 km 12756 km Atmosphere CO2 N2, O2 Composition History of Mars Aircraft Concepts Inflatable Solar Aircraft Concept Hydrazine Power Aircraft Concept MiniSniffer Aircraft Long Endurance Solar Aircraft Concept Key Challenges to Flight On Mars • Atmospheric Conditions (Aerodynamics) • Deployment • Communications • Mission Duration Environment: Atmosphere • Very low atmospheric -
Galileo in 1610
Module 3 – Nautical Science Unit 4 – Astronomy Chapter 15 - The Planets Section 2 – Mars & Jupiter What You Will Learn to Do Demonstrate understanding of astronomy and how it pertains to our solar system and its related bodies: Moon, Sun, stars and planets Objectives 1. Describe the major features of Mars 2. Identify the principal characteristics of Jupiter Key Terms CPS Key Term Questions 1 - 5 Key Terms Nix Olympica - Snow of Olympus Galilean satellites - The four largest and brightest moons of Jupiter: Io, Europa, Ganymede and Callisto; discovered by Galileo in 1610 Prograde The counter-clockwise direction of motion - celestial bodies around the Sun as seen from above the north pole of the Sun; in the sky it is from west to east Key Terms Retrograde The clockwise direction of celestial motion - bodies around the Sun; in the sky it is from east to west Rotational axis - The straight line through all fixed points of a rotating rigid body around which all other points of the body move in circles Opening Question Discuss what types of exploration missions have occurred on Mars. (Use CPS “Pick a Student” for this question.) Mars Fourth from Mars the Sun and the next planet beyond Earth, Mars has aroused the greatest interest. Mars Mars Ares (Roman Mars) Mars Named for the Roman god of war, it is often called the “red planet.” Mars Mars’ red color and its rapid movement from west to east among the stars make it stand out in the sky. Mars Earth The best time to see Mars is when it is nearest to Earth in August and September, when the Earth is Sun between the Sun and Mars. -
Lunar and Planetary Information Bulletin, Issue
Jet Propulsion Laboratory: Where Planetary Exploration Began Note from the Editors: This issue’s lead article is the seventh in a series of reports describing the history and current activities of the planetary research facilities funded by NASA and located nationwide. This issue features the Jet Propulsion Laboratory (JPL), which since before World War II has been a leading engineering research and development center, creating America’s first satellite and most of its lunar and planetary spacecraft. It is now a major NASA center, focusing on robotic space exploration. While JPL is also very active in Earth observation and space technology programs, this article focuses on JPL’s planetary efforts. — Paul Schenk and Renee Dotson LFrom the roar of pioneering Space Age rockets to the soft whir of servos on twenty-first-century robot explorers on Mars, spacecraft designed and built at NASA’s Jet Propulsion Laboratory (JPL) have blazed the trail to the planets and into the universe beyond for nearly 60 years. The United States (U.S.) first entered space with the 1958 launch of the satellite Explorer 1, built and controlled by JPL. From orbit, Explorer 1’s voyage yielded immediate scientific results — the discovery of the Van Allen radiation belts — and led to the creation of NASA. Innovative technology from JPL has taken humanity far beyond regions of space where we can actually travel ourselves. The most distant human-made objects, Voyagers 1 and 2, were built at and are operated by JPL. From JPL’s labs and clean rooms come telescopes and cameras that have extended our vision to unprecedented depths and distances, Ppeering into the hearts of galactic clouds where new stars and planets are born, and even toward the beginning of time at the edge of the universe. -
Digital Processing of the Mariner 6 and 7 Pictures
VOL. 76, NO. 2 JOURNAL OF GEOPHYSICAL RESEARCH JANUARY 10, 1971 Digital Processing of the Mariner 6 and 7 Pictures T. C. RINDFLEISC H, J. A. DUNNE, H. ,J. FRIEDEN, W. D. STHOMBEHa, AND R. M. RUIZ Space Sciences D-ivision, J et Propttls'ion Laboratory Pasaaena, California 91103 The Mariner Mars 1969 t.elevision camera system was a vidicon-based digital system and in cluded a complex on-board video encoding and recording scheme. The spacecraft video processing was designed to maximize the volume of data returned and the encoded discriminability of the low-contrast surface detail of Mars. The ground-based photometric reconstruction of the Mariner photographs, as well as the correction of inherent vidicon camera distortion effects necessary to achieve television experiment objectives, required use of a digit.al computer to process the pictllres. The digital techniques developed to reconstl"Uct the spacecraft encoder effects and to correct for camera distortions are described and examples shown of the processed results. Specific distortion corrections that are considered include the removal of structured system noises, the removal of sensor residual image, the correction of photometric sensitivity nonunifonnit,ies and nonlinearities, the correction of geometric distortions, and the correctrn of modulat,ion transfer limitations. As all physically realizable instruments in_/ and interpretations of the imagery can be based fluence the data they collect, the Mariner Mars on information as representative of the Martian 1969 television cameras left their signatures on surface as possible. the imagery they returned to earth. Analyses The succeeding sections will describe, from of the Mariner photographs must be performed the point of view of image processing, the per with the knowledge that Mars was observed formance characteristics of the vidicon cameras through the spacecraft cameras, and any distor- and data-encoding electronics on board the tions introduced by the camera system processes spacecraft, the over-all flow of the various potentially affect the results. -
Moon-Miners-Manifesto-Mars.Pdf
http://www.moonsociety.org/mars/ Let’s make the right choice - Mars and the Moon! Advantages of a low profile for shielding Mars looks like Arizona but feels like Antarctica Rover Opportunity at edge of Endeavor Crater Designing railroads and trains for Mars Designing planes that can fly in Mars’ thin air Breeding plants to be “Mars-hardy” Outposts between dunes, pulling sand over them These are just a few of the Mars-related topics covered in the past 25+ years. Read on for much more! Why Mars? The lunar and Martian frontiers will thrive much better as trading partners than either could on it own. Mars has little to trade to Earth, but a lot it can trade with the Moon. Both can/will thrive together! CHRONOLOGICAL INDEX MMM THEMES: MARS MMM #6 - "M" is for Missing Volatiles: Methane and 'Mmonia; Mars, PHOBOS, Deimos; Mars as I see it; MMM #16 Frontiers Have Rough Edges MMM #18 Importance of the M.U.S.-c.l.e.Plan for the Opening of Mars; Pavonis Mons MMM #19 Seizing the Reins of the Mars Bandwagon; Mars: Option to Stay; Mars Calendar MMM #30 NIMF: Nuclear rocket using Indigenous Martian Fuel; Wanted: Split personality types for Mars Expedition; Mars Calendar Postscript; Are there Meteor Showers on Mars? MMM #41 Imagineering Mars Rovers; Rethink Mars Sample Return; Lunar Development & Mars; Temptations to Eco-carelessness; The Romantic Touch of Old Barsoom MMM #42 Igloos: Atmosphere-derived shielding for lo-rem Martian Shelters MMM #54 Mars of Lore vs. Mars of Yore; vendors wanted for wheeled and walking Mars Rovers; Transforming Mars; Xities -
2016 Publication Year 2020-06-03T14:13:16Z Acceptance
Publication Year 2016 Acceptance in OA@INAF 2020-06-03T14:13:16Z Title Small Mars satellite: a low-cost system for Mars exploration Authors Pasolini, Pietro; Aurigemma, Renato; Causa, Flavia; Dell'Aversana, Pasquale; de la Torre Sangrà, David; et al. Handle http://hdl.handle.net/20.500.12386/25908 67th International Astronautical Congress (IAC), Guadalajara, Mexico, 26-30 September 2016. Copyright ©2016 by the International Astronautical Federation (IAF). All rights reserved. IAC-16-A3.3A.6 SMALL MARS SATELLITE: A LOW-COST SYSTEM FOR MARS EXPLORATION Pasolini P.*a, Aurigemma R.b, Causa F.a, Cimminiello N.b, de la Torre Sangrà D.c, Dell’Aversana P.d, Esposito F.e, Fantino E.c, Gramiccia L.f, Grassi M.a, Lanzante G.a, Molfese C.e, Punzo F.d, Roma I.g, Savino R.a, Zuppardi G.a a University of Naples “Federico II”, Naples (Italy) b Eurosoft srl, Naples (Italy) c Space Studies Institute of Catalonia (IEEC), Barcelona (Spain) d ALI S.c.a.r.l., Naples (Italy) e INAF - Astronomical Observatory of Capodimonte, Naples (Italy) f SRS E.D., Naples (Italy) g ESA European Space Agency, Nordwijk (The Netherlands) * Corresponding Author Abstract The Small Mars Satellite (SMS) is a low-cost mission to Mars, currently under feasibility study funded by the European Space Agency (ESA). The mission, whose estimated cost is within 120 MEuro, aims at delivering a small Lander to Mars using an innovative deployable (umbrella-like) heat shield concept, known as IRENE (Italian ReEntry NacellE), developed and patented by ALI S.c.a.r.l., which is also the project's prime contractor. -
§130.417. Scientific Research and Design TEKS Overview 2020 Texas High School Aerospace Scholars Online Curriculum
§130.417. Scientific Research and Design TEKS Overview 2020 Texas High School Aerospace Scholars Online Curriculum # of Activities Standard # Standa rd Aligned (c)(2) The student, for at least 40% of instructional time, conducts laboratory and field investigations using safe, environmentally appropriate, and ethical practices. The student is expected to: 130.417.c2A (2A) demonstrate safe practices during laboratory and field investigations; and 18 (2B) demonstrate an understanding of the use and conservation of resources and the proper disposal 130.417.c2B or recycling of materials. 18 (c)(3) The student uses scientific methods and equipment during laboratory and field investigations. The student is expected to: (3A) know the definition of science and understand that it has limitations, as specified in subsection 130.417.c3A (b)(4)* of this section; 29 (3B) know that scientific hypotheses are tentative and testable statements that must be capable of being supported or not supported by observational evidence. Hypotheses of durable explanatory power 130.417.c3B which have been tested over a wide variety of conditions are incorporated into theories; 29 (3C) know that scientific theories are based on natural and physical phenomena and are capable of being tested by multiple independent researchers. Unlike hypotheses, scientific theories are well- established and highly-reliable explanations, but may be subject to change as new areas of science and 130.417.c3C new technologies are developed; 10 130.417.c3D (3D) distinguish between scientific -
Tesi Di Laurea Magistrale
POLITECNICO DI TORINO Corso di Laurea Magistrale in Ingegneria per l’Ambiente e il Territorio Tesi di Laurea Magistrale Automated Landing Site Optimisation Model for Human Mission to Mars Relatore Prof. Marilena Cardu Candidata Costanza Caruzzo Marzo 2018 To my grandfather Gian Carlo ABSTRACT Successfully sending humans to Mars will represent one of the greatest achievements of the mankind. To ensure the crews’ safety and ongoing mission success the selection of an optimised landing site for the construction of a human base is highly critical. Site selection will require a multidisciplinary effort with significant planning to implement a successful strategy that is both flexible and adaptable. In this research, the development of a tool constructed in ArcGIS ModelBuilder which seeks to automate and optimise the landing site selection process for the first human mission to Mars will be discussed. The core focus of this work is to improve the selection process replacing time consuming and subjective manual analysis of datasets with an automated flexible model based on defined engineering constraints. To test and validate the effectiveness of the model, the constraints used for the landing of the Mars Science Laboratory (MSL) rover Curiosity at Gale Crater were incorporated into the tool. After workflow validation, the model was run on other proposed human exploration zones. The model works by integrating images analysis tools and provides an output map that reflects the desired engineering constraint requirements. The workflow is structured into three main phases, which consists of: (1) Data processing, (2) Engineering parameter map layer development, (3) Raster reclassification. The reclassified output maps are then combined into a single map, which summarises all the properties analysed.