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After DART: Using the first full-scale test of a kinetic impactor to inform a future planetary defense mission
by
Statler, Thomas S
, Dotto, Elisabetta
, Rahil Makadia
, Ferrari, Fabio
, Soldini, Stefania
, Jutzi, Martin
, Cambioni, Saverio
, Ivanovski, Stavro
, Agrusa, Harrison F
, Trigo-Rodríguez, Josep M
, Raducan, Sabina D
, Cheng, Andrew F
, Souami, Damya
, Schwartz, Stephen R
, Eggl, Siegfried
, Sánchez, Paul
, Fahnestock, Eugene G
, Michel, Patrick
, DeCoster, Mallory E
, Rivkin, Andrew S
, Pajola, Maurizio
, Barbee, Brent
, Venditti, Flaviane
, Marzari, Francesco
, Chesley, Steven R
, Luther, Robert
, Jean-Baptiste, Vincent
, Wünnemann, Kai
, Graninger, Dawn
, Herique, Alain
, Hirabayashi, Masatoshi
, Lucchetti, Alice
, Nakano, Ryota
, Barnouin, Olivier S
, Herreros, Isabel
, Murdoch, Naomi
, Tortora, Paolo
, Stickle, Angela
, Ormö, Jens
, Rossi, Alessandro
, Karatekin, Özgür
in
Asteroid deflection
/ Constraints
/ Earth
/ Ejecta
/ Figure of merit
/ Full scale tests
/ Hypervelocity impact
/ Impact prediction
/ Momentum transfer
/ Physical properties
/ Planetary defense
/ Reconnaissance
2022
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After DART: Using the first full-scale test of a kinetic impactor to inform a future planetary defense mission
by
Statler, Thomas S
, Dotto, Elisabetta
, Rahil Makadia
, Ferrari, Fabio
, Soldini, Stefania
, Jutzi, Martin
, Cambioni, Saverio
, Ivanovski, Stavro
, Agrusa, Harrison F
, Trigo-Rodríguez, Josep M
, Raducan, Sabina D
, Cheng, Andrew F
, Souami, Damya
, Schwartz, Stephen R
, Eggl, Siegfried
, Sánchez, Paul
, Fahnestock, Eugene G
, Michel, Patrick
, DeCoster, Mallory E
, Rivkin, Andrew S
, Pajola, Maurizio
, Barbee, Brent
, Venditti, Flaviane
, Marzari, Francesco
, Chesley, Steven R
, Luther, Robert
, Jean-Baptiste, Vincent
, Wünnemann, Kai
, Graninger, Dawn
, Herique, Alain
, Hirabayashi, Masatoshi
, Lucchetti, Alice
, Nakano, Ryota
, Barnouin, Olivier S
, Herreros, Isabel
, Murdoch, Naomi
, Tortora, Paolo
, Stickle, Angela
, Ormö, Jens
, Rossi, Alessandro
, Karatekin, Özgür
in
Asteroid deflection
/ Constraints
/ Earth
/ Ejecta
/ Figure of merit
/ Full scale tests
/ Hypervelocity impact
/ Impact prediction
/ Momentum transfer
/ Physical properties
/ Planetary defense
/ Reconnaissance
2022
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After DART: Using the first full-scale test of a kinetic impactor to inform a future planetary defense mission
by
Statler, Thomas S
, Dotto, Elisabetta
, Rahil Makadia
, Ferrari, Fabio
, Soldini, Stefania
, Jutzi, Martin
, Cambioni, Saverio
, Ivanovski, Stavro
, Agrusa, Harrison F
, Trigo-Rodríguez, Josep M
, Raducan, Sabina D
, Cheng, Andrew F
, Souami, Damya
, Schwartz, Stephen R
, Eggl, Siegfried
, Sánchez, Paul
, Fahnestock, Eugene G
, Michel, Patrick
, DeCoster, Mallory E
, Rivkin, Andrew S
, Pajola, Maurizio
, Barbee, Brent
, Venditti, Flaviane
, Marzari, Francesco
, Chesley, Steven R
, Luther, Robert
, Jean-Baptiste, Vincent
, Wünnemann, Kai
, Graninger, Dawn
, Herique, Alain
, Hirabayashi, Masatoshi
, Lucchetti, Alice
, Nakano, Ryota
, Barnouin, Olivier S
, Herreros, Isabel
, Murdoch, Naomi
, Tortora, Paolo
, Stickle, Angela
, Ormö, Jens
, Rossi, Alessandro
, Karatekin, Özgür
in
Asteroid deflection
/ Constraints
/ Earth
/ Ejecta
/ Figure of merit
/ Full scale tests
/ Hypervelocity impact
/ Impact prediction
/ Momentum transfer
/ Physical properties
/ Planetary defense
/ Reconnaissance
2022
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After DART: Using the first full-scale test of a kinetic impactor to inform a future planetary defense mission
Paper
After DART: Using the first full-scale test of a kinetic impactor to inform a future planetary defense mission
2022
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Overview
NASA's Double Asteroid Redirection Test (DART) is the first full-scale test of an asteroid deflection technology. Results from the hypervelocity kinetic impact and Earth-based observations, coupled with LICIACube and the later Hera mission, will result in measurement of the momentum transfer efficiency accurate to ~10% and characterization of the Didymos binary system. But DART is a single experiment; how could these results be used in a future planetary defense necessity involving a different asteroid? We examine what aspects of Dimorphos's response to kinetic impact will be constrained by DART results; how these constraints will help refine knowledge of the physical properties of asteroidal materials and predictive power of impact simulations; what information about a potential Earth impactor could be acquired before a deflection effort; and how design of a deflection mission should be informed by this understanding. We generalize the momentum enhancement factor \\(\\beta\\), showing that a particular direction-specific \\(\\beta\\) will be directly determined by the DART results, and that a related direction-specific \\(\\beta\\) is a figure of merit for a kinetic impact mission. The DART \\(\\beta\\) determination constrains the ejecta momentum vector, which, with hydrodynamic simulations, constrains the physical properties of Dimorphos's near-surface. In a hypothetical planetary defense exigency, extrapolating these constraints to a newly discovered asteroid will require Earth-based observations and benefit from in-situ reconnaissance. We show representative predictions for momentum transfer based on different levels of reconnaissance and discuss strategic targeting to optimize the deflection and reduce the risk of a counterproductive deflection in the wrong direction.
Publisher
Cornell University Library, arXiv.org
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