4.6 Article

NEOWISE REACTIVATION MISSION YEAR TWO: ASTEROID DIAMETERS AND ALBEDOS

Journal

ASTRONOMICAL JOURNAL
Volume 152, Issue 3, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.3847/0004-6256/152/3/63

Keywords

minor planets, asteroids: general; surveys

Funding

  1. NASA
  2. Planetary Science Division of NASA
  3. JPL Office of the CIO
  4. U.S. Department of Energy
  5. U.S. National Science Foundation
  6. Ministry of Science and Education of Spain
  7. Science and Technology Facilities Council of the United Kingdom
  8. Higher Education Funding Council for England
  9. National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign
  10. Kavli Institute of Cosmological Physics at the University of Chicago
  11. Center for Cosmology and Astro-Particle Physics at the Ohio State University
  12. Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University
  13. Financiadora de Estudos e Projetos
  14. Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro
  15. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico
  16. Ministerio da Ciencia, Tecnologia e Inovacao
  17. Deutsche Forschungsgemeinschaft
  18. Collaborating Institutions in the Dark Energy Survey
  19. Ministerio da Ciencia, Tecnologia e Inovacao (Brazil) [GS-2015A-LP-3, GS-2015B-LP-3]

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The Near-Earth Object Wide-Field Infrared Survey Explorer (NEOWISE) mission continues to detect, track, and characterize minor planets. We present diameters and albedos calculated from observations taken during the second year since the spacecraft was reactivated in late 2013. These include 207 near-Earth asteroids (NEAs) and 8885 other asteroids. Of the NEAs, 84% NEAs did not have previously measured diameters and albedos by the NEOWISE mission. Comparison of sizes and albedos calculated from NEOWISE measurements with those measured by occultations, spacecraft, and radar-derived shapes shows accuracy consistent with previous NEOWISE publications. Diameters and albedos fall within +/-similar to 20% and +/-similar to 40%, 1-sigma, respectively, of those measured by these alternate techniques. NEOWISE continues to preferentially discover near-Earth objects which are large (>100 m), and have low albedos.

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