Planetary Protection Independent Review Board Recommendations
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Using a Nuclear Explosive Device for Planetary Defense Against an Incoming Asteroid
Georgetown University Law Center Scholarship @ GEORGETOWN LAW 2019 Exoatmospheric Plowshares: Using a Nuclear Explosive Device for Planetary Defense Against an Incoming Asteroid David A. Koplow Georgetown University Law Center, [email protected] This paper can be downloaded free of charge from: https://scholarship.law.georgetown.edu/facpub/2197 https://ssrn.com/abstract=3229382 UCLA Journal of International Law & Foreign Affairs, Spring 2019, Issue 1, 76. This open-access article is brought to you by the Georgetown Law Library. Posted with permission of the author. Follow this and additional works at: https://scholarship.law.georgetown.edu/facpub Part of the Air and Space Law Commons, International Law Commons, Law and Philosophy Commons, and the National Security Law Commons EXOATMOSPHERIC PLOWSHARES: USING A NUCLEAR EXPLOSIVE DEVICE FOR PLANETARY DEFENSE AGAINST AN INCOMING ASTEROID DavidA. Koplow* "They shall bear their swords into plowshares, and their spears into pruning hooks" Isaiah 2:4 ABSTRACT What should be done if we suddenly discover a large asteroid on a collision course with Earth? The consequences of an impact could be enormous-scientists believe thatsuch a strike 60 million years ago led to the extinction of the dinosaurs, and something ofsimilar magnitude could happen again. Although no such extraterrestrialthreat now looms on the horizon, astronomers concede that they cannot detect all the potentially hazardous * Professor of Law, Georgetown University Law Center. The author gratefully acknowledges the valuable comments from the following experts, colleagues and friends who reviewed prior drafts of this manuscript: Hope M. Babcock, Michael R. Cannon, Pierce Corden, Thomas Graham, Jr., Henry R. Hertzfeld, Edward M. -
JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
View Conducted by Its Standing Review Board (SRB)
Science Committee Report Dr. Wes Huntress, Chair 1 Science Committee Members Wes Huntress, Chair Byron Tapley, (Vice Chair) University of Texas-Austin, Chair of Earth Science Alan Boss, Carnegie Institution, Chair of Astrophysics Ron Greeley, Arizona State University, Chair of Planetary Science Gene Levy, Rice University , Chair of Planetary Protection Roy Torbert, University of New Hampshire, Chair of Heliophysics Jack Burns, University of Colorado Noel Hinners, Independent Consultant *Judith Lean, Naval Research Laboratory Michael Turner, University of Chicago Charlie Kennel, Chair of Space Studies Board (ex officio member) * = resigned July 16, 2010 2 Agenda • Science Results • Programmatic Status • Findings & Recommendations 3 Unusual Thermosphere Collapse • Deep drop in Thermospheric (50 – 400 km) density • Deeper than expected from solar cycle & CO2 4 Aeronomy of Ice in the Mesosphere (AIM) unlocking the secrets of Noctilucent Clouds (NLCs) Form 50 miles above surface in polar summer vs ~ 6 miles for “norm79al” clouds. NLCs getting brighter; occurring more often. Why? Linked to global change? AIM NLC Image June 27, 2009 - AIM measured the relationship between cloud properties and temperature - Quantified for the first time, the dramatic response to small changes, 10 deg C, in temperature - T sensitivity critical for study of global change effects on mesosphere Response to Gulf Oil Spill UAVSAR 23 June 2010 MODIS 31 May 2010 ASTER 24 May 2010 Visible Visible/IR false color Satellite instruments: continually monitoring the extent of -
Planetary Protection Requirements for Human and Robotic Missions to Mars
Concepts and Approaches for Mars Exploration (2012) 4331.pdf PLANETARY PROTECTION REQUIREMENTS FOR HUMAN AND ROBOTIC MISSIONS TO MARS. R. Mogul1, P. D. Stabekis2, M. S. Race3, and C. A. Conley4, 1California State Polytechnic University, Pomona, 3801 W. Temple Ave, Pomona, CA 91768 ([email protected]), 2Genex Systems, 525 School St. SW, Suite 201, Washington D.C. 20224 ([email protected]), 3SETI Institute, Mountain View, CA 94043, 4NASA Head- quarters, Washington D.C. 20546 ([email protected]) Introduction: Ensuring the scientific integrity of mission. Hardware involved in the acquisition and Mars exploration, and protecting the Earth and the storage of samples from Mars must be designed to human population from potential biohazards, requires protect Mars material from Earth contamination, and the incorporation of planetary protection into human ensure appropriate cleanliness from before launch spaceflight missions as well as robotic precursors. All through return to Earth. Technologies needed to ensure missions returning samples from Mars are required to sample cleanliness at levels similar to those maintained comply with stringent planetary protection require- by the Viking project, in the context of modern space- ments for this purpose, recent refinements to which are craft materials, are yet to be developed. reported here. The objectives of planetary protection policy are As indicated in NASA Policy Directive NPD the same for both human and robotic missions; howev- 8020.7G (section 5c), to ensure compliance with the er, the specific implementation requirements will nec- Outer Space Treaty planetary protection is a mandatory essarily be different. Human missions will require component for all solar system exploration, including additional planetary protection approaches that mini- human missions. -
Astronomy News KW RASC FRIDAY JANUARY 8 2021
Astronomy News KW RASC FRIDAY JANUARY 8 2021 JIM FAIRLES What to expect for spaceflight and astronomy in 2021 https://astronomy.com/news/2021/01/what-to-expect-for- spaceflight-and-astronomy-in-2021 By Corey S. Powell | Published: Monday, January 4, 2021 Whatever craziness may be happening on Earth, the coming year promises to be a spectacular one across the solar system. 2020 - It was the worst of times, it was the best of times. First landing on the lunar farside, two impressive successes in gathering samples from asteroids, the first new pieces of the Moon brought home in 44 years, close-up explorations of the Sun, and major advances in low-cost reusable rockets. First Visit to Jupiter's Trojan Asteroids First Visit to Jupiter's Trojan Asteroids In October, NASA is set to launch the Lucy spacecraft. Over its 12-year primary mission, Lucy will visit eight different asteroids. One target lies in the asteroid belt. The other seven are so-called Trojan asteroids that share an orbit with Jupiter, trapped in points of stability 60 degrees ahead of or behind the planet as it goes around the sun. These objects have been trapped in their locations for billions of years, probably since the time of the formation of the solar system. They contain preserved samples of water-rich and carbon-rich material in the outer solar system; some of that material formed Jupiter, while other bits moved inward to contribute to Earth's life-sustaining composition. As a whimsical aside: When meteorites strike carbon-rich asteroids, they create tiny carbon crystals. -
PLANETARY PROTECTION and REGULATING HUMAN HEALTH: a RISK THAT IS NOT ZERO Victoria Sutton1
(3) FINAL MACRO VERSION - VICTORIA SUTTON ARTICLE (PP. 71-102) (DO NOT DELETE) 3/9/2020 9:40 AM 19 Hous. J. Health L. & Policy 71 Copyright © 2019 Victoria Sutton Houston Journal of Health Law & Policy PLANETARY PROTECTION AND REGULATING HUMAN HEALTH: A RISK THAT IS NOT ZERO Victoria Sutton1 INTRODUCTION ............................................................................................ 73 I. LESSONS FROM HUMAN HISTORY ........................................................... 75 II. U.S. LEADERSHIP, INTERNATIONAL LAW, AND GUIDELINES FOR BACK CONTAMINATION—A SHORT HISTORY OF PLANETARY PROTECTION AND BIOCONTAINMENT ................................................... 79 A. International Law and Biocontainment Binding All Nations .......................................................................................... 82 B. Private Space Travel Must Comply with Planetary Protection ...................................................................................... 84 C. Enforceability is a Weakness ......................................................... 85 III. POLICY INDICATIONS THAT A RENEWED FOCUS IS NEEDED FOR BACK CONTAMINATION ........................................................................ 86 A. The Elimination of Human Health and Quarantine from U.S. Planetary Protection Protocols ........................................... 86 1 Victoria Sutton, MPA, PhD, JD, is the Paul Whitfield Horn Professor at Texas Tech University School of Law. Dr. Sutton is the former Assistant Director at the White House Science Office -
Lunar & Planetary Surface Power Management & Distribution
NASA SBIR 2020 Phase I Solicitation Z1.05 Lunar & Planetary Surface Power Management & Distribution Lead Center: GRC Participating Center(s): GSFC, JSC Technology Area: TA3 Space Power and Energy Storage Scope Title Innovative ways to transmit high power for lunar & Mars surface missions Scope Description The Global Exploration Roadmap (January 2018) and the Space Policy Directive (December 2017) detail NASA’s plans for future human-rated space missions. A major factor in this involves establishing bases on the lunar surface and eventually Mars. Surface power for bases is envisioned to be located remotely from the habitat modules and must be efficiently transferred over significant distances. The International Space Station (ISS) has the highest power (100kW), and largest space power distribution system with eight interleaved micro-grids providing power functions similar to a terrestrial power utility. Planetary bases will be similar to the ISS with expectations of multiple power sources, storage, science, and habitation modules, but at higher power levels and with longer distribution networks providing interconnection. In order to enable high power (>100kW) and longer distribution systems on the surface of the moon or Mars, NASA is in need of innovative technologies in the areas of lower mass/higher efficiency power electronic regulators, switchgear, cabling, connectors, wireless sensors, power beaming, power scavenging, and power management control. The technologies of interest would need to operate in extreme temperature environments, including lunar night, and could experience temperature changes from -153C to 123C for lunar applications, and -125C to 80C for Mars bases. In addition to temperature extremes, technologies would need to withstand (have minimal degradation from) lunar dust/regolith, Mars dust storms, and space radiation levels. -
Biological Planetary Protection for Human Missions to Mars
NASA NID 8715.129 Interim Effective Date: July 9, 2020 Directive Expiration Date: July 9, 2021 Subject: Biological Planetary Protection for Human Missions to Mars Responsible Office: Office of Safety and Mission Assurance Table of Contents Preface P.1 Purpose P.2 Applicability P.3 Authority P.4 Applicable Documents P.5 Measurement/Verification P.6 Cancellation Chapter 1. Mitigating Backward and Forward Harmful Biological Contamination from Human Missions to Mars 1.1 Overview 1.2 Guidance for Biological Planetary Protection for Human Missions to Mars 1.3 NASA Policy on Biological Planetary Protection for Human Missions to Mars Appendix A. References 1 Preface P.1 Purpose a. This directive defines NASA’s obligation to avoid harmful forward and backward biological contamination under Article IX of the Treaty on Principles Governing the Activities of States in the Exploration and Use of Outer Space, including the Moon and Other Celestial Bodies (the "Outer Space Treaty"), October 19, 1967. b. This directive specifically addresses the control of forward biological contamination of Mars and backward biological contamination of the Earth-Moon system associated with human presence in space vehicles intended to land, orbit, flyby, and return from Mars. c. The 1967 Outer Space Treaty provides in relevant part: “States Parties to the Treaty shall pursue studies of outer space, including the Moon and other celestial bodies, and conduct exploration of them so as to avoid their harmful contamination and also adverse changes in the environment of the Earth resulting from the introduction of extraterrestrial matter and, where necessary, shall adopt appropriate measures for this purpose.” NASA recognizes that the 1967 Outer Space Treaty (OST) sets forth legal requirements on U.S. -
09 September 2019 the Hindu Editorials Update Lqc G% 8 Cts# Mahendra's Youtube Channel
09 September 2019 The Hindu Editorials Update lqcg% 8 cts # Mahendra's YouTube Channel . The Sentinelese, a negrito tribe that lives on the North Sentinel Island of the Andamans, remains hostile to outsiders. Based on carbon dating by the Anthropological Survey of India, Sentinelese presence was confirmed in the islands to 2,000 years ago. The Govt. of India issued the Andaman and Nicobar Islands (Protection of Aboriginal Tribes) Regulation, 1956 to declare the traditional areas occupied by the tribes as reserves, and prohibited entry of all persons except those with authorisation. Photographing or filming the tribe members is also an offence. The rules were amended later to enhance penalties. But restricted area permits were relaxed for some islands . Almost nine months after American national John Allen Chau was recently. allegedly killed by the Sentinelese on the North Sentinel Island of Andaman and Nicobar islands, a recent publication by the Anthropological Survey of India (AnSI) throws more light on the incident and also the ways of one of the most isolated tribes in the world. Titled The Sentinelese of the North Sentinel Island: A reprisal of Tribal Scenario in an Andaman Island in context of Killing of an American Preacher. “On November 14, Chau left Port Blair and reached the island at night. He spent the entire day of November 15 with the Sentinelese and on the night when he met the fishermen who had transported him to the island, he gave them the dairy in which he had recorded his experience of the day,” the director said. The orbiter is safe in the intended orbit around the moon. -
Venus: Global Warming Gone Bad Earth & Venus: Sister Planets? Venus Earth
Venus: Global warming gone bad Earth & Venus: Sister planets? Venus Earth Mass 5x1024 kg 6x1024 kg a (semi- 0.7 AU 1 AU major axis) What is T at surface ~750 K ~300 K the boiling Temp of water? P at surface ~90 atm ~1 atm atm N2 and H2O CO2 and composition clouds H2SO4 clouds How do we know Venus’s surface temperature? How do we know Venus’s surface temperature? high energy low energy short wavelength long wavelength “bluer” “redder” hot cold How do we know Venus’s surface temperature? the Sun emits light Earth emits light here. T=6000 K here. T=300 K Venus emits light here. T=750 How do we know what the clouds are made of? Spectrum of planet with no atmosphere Amountof light observed above the atmosphere Wavelength of light (in the infrared) How do we know what the clouds are made of? Spectrum of Spectrum of planet with no planet with atmosphere atmosphere Wavelength at which a molecule in the atmosphere absorbs light Amountof light observed above the atmosphere Amountof light observed above the atmosphere Wavelength of light (in the Wavelength of light (in the infrared) infrared) How do we know what the clouds are made of? (Infrared light) How did Venus get so hot? Remember - all gases absorb light at specific wavelengths. “Greenhouse” gases (like carbon dioxide, water and methane) like to absorb in the infrared wavelengths. Planets emit light at infrared wavelengths (same as human bodies). Conclusio n? “Greenhouse” gases don’t lett the heat from the planet escape. -
Why Pluto Is Not a Planet Anymore Or How Astronomical Objects Get Named
3 Why Pluto Is Not a Planet Anymore or How Astronomical Objects Get Named Sethanne Howard USNO retired Abstract Everywhere I go people ask me why Pluto was kicked out of the Solar System. Poor Pluto, 76 years a planet and then summarily dismissed. The answer is not too complicated. It starts with the question how are astronomical objects named or classified; asks who is responsible for this; and ends with international treaties. Ultimately we learn that it makes sense to demote Pluto. Catalogs and Names WHO IS RESPONSIBLE for naming and classifying astronomical objects? The answer varies slightly with the object, and history plays an important part. Let us start with the stars. Most of the bright stars visible to the naked eye were named centuries ago. They generally have kept their old- fashioned names. Betelgeuse is just such an example. It is the eighth brightest star in the northern sky. The star’s name is thought to be derived ,”Yad al-Jauzā' meaning “the Hand of al-Jauzā يد الجوزاء from the Arabic i.e., Orion, with mistransliteration into Medieval Latin leading to the first character y being misread as a b. Betelgeuse is its historical name. The star is also known by its Bayer designation − ∝ Orionis. A Bayeri designation is a stellar designation in which a specific star is identified by a Greek letter followed by the genitive form of its parent constellation’s Latin name. The original list of Bayer designations contained 1,564 stars. The Bayer designation typically assigns the letter alpha to the brightest star in the constellation and moves through the Greek alphabet, with each letter representing the next fainter star. -
Planetary Geology: Goals, Future Directions, and Recommendations
NASA Conference Publication 3005 Planetary Geology: Goals, Future Directions, and Recommendations Proceedings of a workshop held at Arizona State University Tempe, Arizona January 1987 NASA Conference Publication 3005 Planetary Geology: Goals, Future Directions, and Recommendations NASA Office of Space Science and Applications Washington, D. C. Proceedings of a workshop held at Arizona State University Tempe, Arizona January 1987 National Aeronautics and Space Administration Scientific and Technical Information Division Preface This report gives results of a workshop on planetary geology held in January, 1987, at Arizona State University at the request of Dr. David Scott, Discipline Scientist, Planetary Geology and Geophysics, NASA. In addition to reviews by the workshop members, it was reviewed by the Planetary Geology and Geophysics Working Group and incorporated comments from Dr. James Underwood, current Discipline Scientist for the program. R. Greeley, January 1988 TABLE OF CONTENTS Page 1.0 Executive Summary ............................................................................... 1 2.0 Introduction ........................................................................................ 3 3.0 Workshop Conclusions ........................................................................... 5 3.1 Planetary geology studies are in transition from a descriptive phase to prcxess-oriented research .................................................. 5 3.2 Quantitative techniques can be applied to existing data. but there is a need for