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Near-Earth object surveys

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Near-Earth object surveys
NameNear-Earth object surveys
TypeAstronomical survey
Established20th century
FocusAsteroid detection, comet detection, planetary defense

Near-Earth object surveys Near-Earth object surveys are coordinated observational efforts to detect, track, and characterize asteroids and comets whose orbits bring them into proximity with Earth. These efforts involve a network of observatories, space missions, and research institutions such as NASA, European Space Agency, SpaceX, and Roscosmos collaborating with universities like Massachusetts Institute of Technology, California Institute of Technology, University of Arizona, and University of Hawaii. Surveys support initiatives linked to United Nations Office for Outer Space Affairs, Spaceguard Foundation, White House directives, and international agreements such as the Outer Space Treaty.

Overview

Surveys combine telescopes at facilities like Kitt Peak National Observatory, Mauna Kea Observatories, Palomar Observatory, and La Silla Observatory with space assets including NEOWISE, Gaia (spacecraft), and James Webb Space Telescope to discover and follow up objects cataloged in databases managed by Minor Planet Center, Jet Propulsion Laboratory, and European Space Agency centers. Data pipelines developed at institutions such as Harvard University, University of Cambridge, Max Planck Society, Smithsonian Astrophysical Observatory, and Jet Propulsion Laboratory enable orbit determination using software from projects at Lawrence Livermore National Laboratory and Los Alamos National Laboratory. Funding and oversight often involve agencies like National Science Foundation, European Research Council, Canadian Space Agency, Japan Aerospace Exploration Agency, and Indian Space Research Organisation.

Historical development

Early photographic campaigns at Yerkes Observatory and Royal Greenwich Observatory preceded modern digital surveys such as LINEAR (Lincoln Near-Earth Asteroid Research), Catalina Sky Survey, Spacewatch, and Pan-STARRS. Key figures and programs include astronomers at Smithsonian Institution, pioneers like Eugene Shoemaker, Gene Shoemaker, Clyde Tombaugh, and institutions such as Lincoln Laboratory and Jet Propulsion Laboratory that advanced automated detection. Events such as the discovery of (433) Eros and impacts like the 2013 Chelyabinsk meteor and Tunguska event spurred policy responses involving Congress of the United States hearings, European Parliament resolutions, and collaboration through organizations like International Astronomical Union and United Nations Committee on the Peaceful Uses of Outer Space.

Survey techniques and instrumentation

Techniques employ wide-field CCD cameras, cryogenic infrared detectors, adaptive optics from facilities like Keck Observatory and Very Large Telescope, and radar imaging from Arecibo Observatory (formerly), Goldstone Deep Space Communications Complex, and Green Bank Observatory. Instrumentation projects are led by laboratories including Jet Propulsion Laboratory, Los Alamos National Laboratory, Sandia National Laboratories, and companies such as Ball Aerospace and Lockheed Martin. Methods integrate photometry, spectroscopy with instruments on Subaru Telescope and Gemini Observatory, astrometry using Hubble Space Telescope and Gaia (spacecraft), and spacecraft rendezvous exemplified by missions like OSIRIS-REx, Hayabusa2, DART (spacecraft), and NEAR Shoemaker.

Major survey programs and observatories

Prominent programs include LINEAR (Lincoln Near-Earth Asteroid Research), Catalina Sky Survey, Pan-STARRS, Spacewatch, NEOWISE, and projects at Kitt Peak National Observatory and Palomar Observatory. International partners include Siding Spring Observatory, Mount Lemmon Observatory, La Silla Observatory, Mt. Stromlo Observatory, SAAO (South African Astronomical Observatory), and arrays like Vera C. Rubin Observatory (LSST) and networks such as International Scientific Optical Network. Collaborative consortia involve European Southern Observatory, National Astronomical Observatory of Japan, China National Space Administration, Russian Academy of Sciences, and universities including University of Oxford, Princeton University, Stanford University, University of Tokyo, and Peking University.

Discoveries and statistics

Surveys have discovered major bodies such as (101955) Bennu, (162173) Ryugu, (99942) Apophis, and large samples cataloged by the Minor Planet Center. Statistical catalogs produced by teams at Jet Propulsion Laboratory, NASA Ames Research Center, European Space Agency, and International Astronomical Union reveal size-frequency distributions, orbital elements, and impact probability estimates that inform models developed at Caltech, MIT, University of California, Berkeley, and Carnegie Institution for Science. Discoveries include thousands of near-Earth asteroids, comets like Comet Encke, and bodies targeted by missions from NASA, JAXA, ESA, and Roscosmos.

Risk assessment and planetary defense

Risk assessment frameworks used by NASA Planetary Defense Coordination Office, European Space Agency's NEO Coordination Centre, and advisory panels such as National Research Council (United States) rely on tools from Jet Propulsion Laboratory including the Sentry (monitoring system), impact effect models developed with input from Los Alamos National Laboratory and Sandia National Laboratories, and international coordination through United Nations Office for Outer Space Affairs. Deflection concepts tested by missions such as DART (spacecraft) and studies at Aerospace Corporation, Blue Origin, Northrop Grumman, and research groups at Cornell University address kinetic impactors, gravity tractors, and nuclear options debated in forums including NATO and United Nations General Assembly. Response planning involves emergency agencies like Federal Emergency Management Agency and civil protection authorities in nations such as Japan, United States, Russia, and India.

Future plans and technologies

Planned facilities and missions include Vera C. Rubin Observatory, expanded campaigns by Pan-STARRS, follow-up networks using James Webb Space Telescope and proposed missions such as NEO Surveyor, ESA Hera, and concepts studied at NASA Jet Propulsion Laboratory, European Space Agency, ISRO, and private firms like SpaceX and Blue Origin. Emerging technologies involve machine learning research at Google DeepMind and OpenAI collaborations with universities, quantum sensors explored at MIT, and commercial partnerships with companies such as Maxar Technologies and Planet Labs to enhance detection, characterization, and mitigation capabilities. International frameworks under development involve United Nations Office for Outer Space Affairs, International Astronomical Union, Group of Twenty, and transnational research supported by Horizon Europe and the National Science Foundation.

Category:Astronomical surveys