Finding Hazardous Asteroids Using Infrared and Visible Wavelength Telescopes

Author:   National Academies of Sciences, Engineering, and Medicine ,  Division on Engineering and Physical Sciences ,  Space Studies Board ,  Committee on Near Earth Object Observations in the Infrared and Visible Wavelengths
Publisher:   National Academies Press
ISBN:  

9780309493987


Pages:   74
Publication Date:   09 November 2019
Format:   Paperback
Availability:   In Print   Availability explained
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Finding Hazardous Asteroids Using Infrared and Visible Wavelength Telescopes


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Overview

Near Earth objects (NEOs) have the potential to cause significant damage on Earth. In December 2018, an asteroid exploded in the upper atmosphere over the Bering Sea (western Pacific Ocean) with the explosive force of nearly 10 times that of the Hiroshima bomb. While the frequency of NEO impacts rises in inverse proportion to their sizes, it is still critical to monitor NEO activity in order to prepare defenses for these rare but dangerous threats. Currently, NASA funds a network of ground-based telescopes and a single, soon-to-expire space-based asset to detect and track large asteroids that could cause major damage if they struck Earth. This asset is crucial to NEO tracking as thermal-infrared detection and tracking of asteroids can only be accomplished on a space-based platform. Finding Hazardous Asteroids Using Infrared and Visible Wavelength Telescopes explores the advantages and disadvantages of infrared (IR) technology and visible wavelength observations of NEOs. This report reviews the techniques that could be used to obtain NEO sizes from an infrared spectrum and delineate the associated errors in determining the size. It also evaluates the strengths and weaknesses of these techniques and recommends the most valid techniques that give reproducible results with quantifiable errors. Table of Contents Front Matter Summary 1 Introduction and Background 2 The Components of Planetary Defense 3 Current and Near-Term NEO Observation Systems 4 The Advantages of Space-Based Infrared Platforms 5 Techniques to Obtain NEO Sizes 6 The Role of Archival Data 7 Impact Hazards Not Explicitly Considered by the George E. Brown, Jr. Act Appendixes Appendix A: Letter of Request Appendix B: Studies of the Accuracy of the Near Earth Asteroid Thermal Model Appendix C: Advantages and Disadvantages of Ground- and Space-Based Options for Infrared and Visible Observations of Near Earth Objects Appendix D: Committee and Staff Biographical Information Appendix E: Acronyms

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Author:   National Academies of Sciences, Engineering, and Medicine ,  Division on Engineering and Physical Sciences ,  Space Studies Board ,  Committee on Near Earth Object Observations in the Infrared and Visible Wavelengths
Publisher:   National Academies Press
Imprint:   National Academies Press
ISBN:  

9780309493987


ISBN 10:   0309493986
Pages:   74
Publication Date:   09 November 2019
Audience:   Professional and scholarly ,  Professional & Vocational
Format:   Paperback
Publisher's Status:   Active
Availability:   In Print   Availability explained
This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us.

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