Planetary Defense Exercise Uses Apophis as Hazardous Asteroid Stand-In
Over 100 participants from 18 countries – including NASA scientists and the agency’s NEOWISE mission – took part in the international exercise.
We know that asteroids have struck the Earth in the past with devastating consequences, such as the asteroid 66 million years ago that wiped out the dinosaur. In fact, new research found that early Earth may have had 10 times as many huge impactors as previously thought. Recently, the asteroid Apophis quickly gained notoriety as an asteroid that could pose a serious threat to Earth in 2029. Fortunately, new data ruled out an impact at that time, and further data has shown that Earth is safe from Apophis for at least the next 100 years.
Since the threat “planet killer” asteroid is real, space agencies have been increasing planetary defense efforts. A recent exercise that included over 100 astronomers from around the world used the aforementioned asteroid, Apophis, as a stand-in for a new potentially hazardous asteroid. The lessons learned could help reduce or avoid global destruction when the scenario turns real.
Watching the skies for large asteroids that could pose a hazard to the Earth is a global endeavor. So, to test their operational readiness, the international planetary defense community will sometimes use a real asteroid’s close approach as a mock encounter with a “new” potentially hazardous asteroid. The lessons learned could limit, or even prevent, global devastation should the scenario play out for real in the future.
To that end, more than 100 astronomers from around the world participated in an exercise last year in which a large, known, and potentially hazardous asteroid was essentially removed from the planetary defense-monitoring database to see whether it could be properly detected anew. Not only was the object “discovered” during the exercise, but its chances of hitting Earth were also continually reassessed as it was tracked, and the possibility of impact was ruled out.
Coordinated by the International Asteroid Warning Network (IAWN) and NASA’s Planetary Defense Coordination Office (PDCO), the exercise confirmed that, from initial detection to follow-up characterization, the international planetary defense community can act swiftly to identify and assess the hazard posed by a new near-Earth asteroid discovery. The results of the exercise are detailed in a study published in the Planetary Science Journal on Tuesday, May 31, 2022.
The exercise focused on the real asteroid Apophis. For a short while after its discovery in 2004, Apophis was assessed to have a significant chance of impacting Earth in 2029 or later. But based on tracking measurements taken during several close approaches since the asteroid’s discovery, astronomers have refined Apophis’ orbit and now know that it poses no impact hazard whatsoever for 100 years or more. Scientific observations of Apophis’ most recent close approach, which occurred between December 2020 and March 2021, were used by the planetary defense community for this exercise.
“This real-world scientific input stress-tested the entire planetary defense response chain, from initial detection to orbit determination to measuring the asteroid’s physical characteristics and even determining if, and where, it might hit Earth,” said Vishnu Reddy, associate professor at the University of Arizona’s Lunar and Planetary Laboratory in Tucson, who led the campaign.
Astronomers knew Apophis would approach Earth in early December 2020. But to make the exercise more realistic, the Minor Planet Center (MPC) – the internationally recognized clearinghouse for the position measurements of small celestial bodies – pretended that it was an unknown asteroid by preventing the new observations of Apophis from being connected with previous observations of it. When the asteroid approached, astronomical surveys had no prior record of Apophis.
On December 4, 2020, as the asteroid started to brighten, the NASA-funded Catalina Sky Survey in Arizona made the first detection and reported the object’s astrometry (its position in the sky) to the Minor Planet Center. Because there was no prior record of Apophis for the purpose of this exercise, the asteroid was logged as a brand-new detection. Other detections followed from the Hawaii-based, NASA-funded Asteroid Terrestrial-impact Last Alert System (ATLAS) and Panoramic Survey Telescope and Rapid Response System (Pan-STARRS).
As Apophis drifted into the field of view of NASA’s Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) mission, the MPC linked its observations with those made by ground-based survey telescopes to show the asteroid’s motion through the sky. On December 23, the MPC announced the discovery of a “new” near-Earth asteroid. Exercise participants quickly gathered additional measurements to assess its orbit and whether it could impact Earth.
“Even though we knew that, in reality, Apophis was not impacting Earth in 2029, starting from square one – with only a few days of astrometric data from survey telescopes – there were large uncertainties in the object’s orbit that theoretically allowed an impact that year,” said Davide Farnocchia, a navigation engineer at NASA’s Jet Propulsion Laboratory in Southern California, who led the orbital determination calculations for JPL’s Center for Near Earth Object Studies (CNEOS).
During the asteroid’s March 2021 close approach, JPL astronomers used NASA’s 230-foot (70-meter) Goldstone Solar System Radar in California to image and precisely measure the asteroid’s velocity and distance. These observations, combined with measurements from other observatories, enabled astronomers to refine Apophis’ orbit and rule out a 2029 impact for the purpose of the exercise. (Beyond the exercise, they also were able to rule out any chance of impact for 100 years or more.)
Orbiting far above Earth’s atmosphere, NEOWISE provided infrared observations of Apophis that would be not have been possible from the ground because moisture in the Earth’s atmosphere absorbs light at these wavelengths.
“The independent infrared data collected from space greatly benefited the results from this exercise,” said Akash Satpathy, an undergraduate student who led a second paper with NEOWISE Principal Investigator Amy Mainzer at the University of Arizona, describing the results with inclusion of their data in the exercise. “NEOWISE was able to confirm Apophis’ rediscovery while also rapidly gathering valuable information that could be used in planetary defense assessments, such as its size, shape, and even clues as to its composition and surface properties.”
By better understanding the asteroid’s size, participating scientists at NASA’s Ames Research Center in Silicon Valley, California, could also estimate the impact energy that an asteroid like Apophis would deliver. And the participants simulated a swath of realistic impact locations on Earth’s surface that, in a real situation, would help disaster agencies with possible evacuation efforts.
“Seeing the planetary defense community come together during the latest close approach of Apophis was impressive,” said Michael Kelley, a program scientist with PDCO, within NASA’s Planetary Science Division at NASA Headquarters in Washington, who provided guidance to the exercise participants. “Even during a pandemic, when many of the exercise participants were forced to work remotely, we were able to detect, track, and learn more about a potential hazard with great efficiency. The exercise was a resounding success.”
Additional key planetary defense exercise working group leads included Jessie Dotson at NASA Ames, Nicholas Erasmus at the South African Astronomical Observatory, David Polishook at the Weizmann Institute in Israel, Joseph Masiero at Caltech-IPAC in Pasadena, and Lance Benner at JPL, a division of Caltech.
NEOWISE’s successor, the next-generation NEO Surveyor, is scheduled to launch no earlier than 2026 and will greatly expand the knowledge NEOWISE has amassed about the near-Earth asteroids that populate our solar system.
Reference: “Apophis Planetary Defense Campaign” by Vishnu Reddy, Michael S. Kelley, Jessie Dotson, Davide Farnocchia, Nicolas Erasmus, David Polishook, Joseph Masiero, Lance A. M. Benner, James Bauer, Miguel R. Alarcon, David Balam, Daniel Bamberger, David Bell, Fabrizio Barnardi, Terry H. Bressi, Marina Brozovic, Melissa J. Brucker, Luca Buzzi, Juan Cano, David Cantillo, Ramona Cennamo, Serge Chastel, Omarov Chingis, Young-Jun Choi, Eric Christensen, Larry Denneau, Marek Drózdz, Leonid Elenin, Orhan Erece, Laura Faggioli, Carmelo Falco, Dmitry Glamazda, Filippo Graziani, Aren N. Heinze, Matthew J. Holman, Alexander Ivanov, Cristovao Jacques, Petro Janse van Rensburg, Galina Kaiser, Krzysztof Kaminski, Monika K. Kaminska, Murat Kaplan, Dong-Heun Kim, Myung-Jin Kim, Csaba Kiss, Tatiana Kokina, Eduard Kuznetsov, Jeffrey A. Larsen, Hee-Jae Lee, Robert C. Lees, Julia de León, Javier Licandro, Amy Mainzer, Anna Marciniak, Michael Marsset, Ron A. Mastaler, Donovan L. Mathias, Robert S. McMillan, Hissa Medeiros, Marco Micheli, Artem Mokhnatkin, Hong-Kyu Moon, David Morate, Shantanu P. Naidu, Alessandro Nastasi, Artem Novichonok, Waldemar Ogloza, András Pál, Fabricio Pérez-Toledo, Alexander Perminov, Elisabeta Petrescu, Marcel Popescu, Mike T. Read, Daniel E. Reichart, Inna Reva, Dong-Goo Roh, Clemens Rumpf, Akash Satpathy, Sergei Schmalz, James V. Scotti, Aleksander Serebryanskiy, Miquel Serra-Ricart, Eda Sonbas, Robert Szakáts, Patrick A. Taylor, John L. Tonry, Andrew F. Tubbiolo, Peter Veres, Richard Wainscoat, Elizabeth Warner, Henry J. Weiland, Guy Wells, Robert Weryk, Lorien F. Wheeler, Yulia Wiebe, Hong-Suh Yim, Michal Zejmo, Anastasiya Zhornichenko, Stanislaw Zola and Patrick Michel, 31 May 2022, Planetary Science Journal.