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2023 DZ2 Planetary Defense Campaign

Authors :
Vishnu Reddy
Michael S. Kelley
Lance Benner
Jessie Dotson
Nicolas Erasmus
Davide Farnocchia
Tyler Linder
Joseph R. Masiero
Cristina Thomas
James Bauer
Miguel R. Alarcon
Paolo Bacci
Daniel Bamberger
Adam Battle
Zouhair Benkhaldoun
Guido Betti
Mirel Birlan
Marina Brozovic
Brian Burt
David C. Cantillo
Sunil Chandra
Gregoire Chomette
Ashley Coates
Francesca DeMeo
Maxime Devogèle
Petr Fatka
Marin Ferrais
Paolo Fini
Carel van Gend
Jon D. Giorgini
Dmitry Glamazda
Robert Holmes
Joseph L. Hora
Shinji Horiuchi
Kamil Hornoch
Marco Iozzi
Cristóvão Jacques
Emmanuel Jehin
Hai Jiang
Galina Kaiser
Peter Kušnirák
Eduard Kuznetsov
Julia de León
Alexios Liakos
Javier Licandro
Tim Lister
Jing Liu
Andy Lopez-Oquendo
Martina Maestripieri
Donovan Mathias
Marco Micheli
Shantanu P. Naidu
Alessandro Nastasi
Alin Nedelcu
Elisabeta Petrescu
Marcel Popescu
Stephen B. Potter
Petr Pravec
Juan Sanchez
Toni Santana-Ros
Miquel Serra-Ricart
Nick Sioulas
Adrian Sonka
Alessio Squilloni
Maura Tombelli
Madalina Trelia
David E. Trilling
Elizabeth Warner
Guy Wells
Lorien Wheeler
Mike Wiles
Source :
The Planetary Science Journal, Vol 5, Iss 6, p 141 (2024)
Publication Year :
2024
Publisher :
IOP Publishing, 2024.

Abstract

We present the results of a fourth planetary defense exercise, focused this time on the small near-Earth asteroid (NEA) 2023 DZ2 and conducted during its close approach to the Earth in 2023 March. The International Asteroid Warning Network (IAWN), with support from NASA's Planetary Defense Coordination Office (PDCO), has been coordinating planetary defense observational campaigns since 2017 to test the operational readiness of the global planetary defense capabilities. The last campaign focused on the NEA Apophis, and an outcome of that exercise was the need for a short burst campaign to replicate a real-life near-Earth object impact hazard scenario. The goal of the 2023 DZ2 campaign was to characterize the small NEA as a potential impactor and exercise the planetary defense system including observations, hypothetical risk assessment and risk prediction, and hazard communication with a short notice of just 24 hr. The entire campaign lasted about 10 days. The campaign team was divided into several working groups based on the characterization method: photometry, spectroscopy, thermal IR photometry and optical polarimetry, radar, and risk assessment. Science results from the campaign show that 2023 DZ2 has a rotation period of 6.2745 ± 0.0030 minutes; visible wavelength color photometry/spectroscopy/polarimetry and near-IR spectroscopy all point to an E-type taxonomic classification with surface composition analogous to aubrite meteorites; and radar observations show that the object has a diameter of 30 ± 10 m, consistent with the high albedo (0.49) derived from polarimetric and thermal IR observations.

Details

Language :
English
ISSN :
26323338
Volume :
5
Issue :
6
Database :
Directory of Open Access Journals
Journal :
The Planetary Science Journal
Publication Type :
Academic Journal
Accession number :
edsdoj.5803dc0c1d9f4ae3b0af7b6a2cfe0c0b
Document Type :
article
Full Text :
https://doi.org/10.3847/PSJ/ad4a6d