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Originele taal-2 | English |
---|---|
Pagina's (van-tot) | 1 |
Aantal pagina's | 24 |
Tijdschrift | The Planetary Science Journal |
Volume | 5 |
Nummer van het tijdschrift | 49 |
DOI's | |
Status | Published - 1 feb 2024 |
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Publisher Copyright:© 2024. The Author(s).
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Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission. / Chabot, Nancy; andrew, David; andrew, David; Barnouin, Olivier; Fahnestock, Eugene; Richardson, Derek C; Stickle, Angela; Thomas, Cristina; Ernst, Carolyn; Daly, Ronald; Dotto, Elisabetta; Angelo, ZINZI; Chesley, Steven; Moskovitz, Nicholas; Barbee, Brent; Abell, Paul; Agrusa, Harrison; Bannister, Michele; Beccarelli, Joel; Bekker, Dmitriy; Syal, Megan Bruck; Buratti, Bonnie; Busch, Michael W.; Bagatin, Adriano Campo; Chatelain, Joseph; Chocron, Isaias; Collins, Gareth; Conversi, Luca; Davison, Thomas; DeCoster, Mallory E.; Deshapriya, Jasinghege Don Prasanna; Eggl, Siegfried; Espiritu, Raymond; Farnham, Tony; Ferrais, Marin; Ferrari, Fabio; Föhring, Dora; Fuentes-Muñoz, Oscar; Gai, Igor; Giordano, Carmine; Glenar, David; Gomez, Edward; Graninger, Dawn; Green, Simon F.; Greenstreet, Sarah; Hasselmann, Pedro Henrique; Herreros, Isabel; Hirabayashi, Masatoshi; Husarik, Marek; (he/him), Simone Ieva; Senel, Cem Berk.
In: The Planetary Science Journal, Vol. 5, Nr. 49, 01.02.2024, blz. 1.Onderzoeksoutput: Article › peer review
TY - JOUR
T1 - Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
AU - Chabot, Nancy
AU - andrew, David
AU - andrew, David
AU - Barnouin, Olivier
AU - Fahnestock, Eugene
AU - Richardson, Derek C
AU - Stickle, Angela
AU - Thomas, Cristina
AU - Ernst, Carolyn
AU - Daly, Ronald
AU - Dotto, Elisabetta
AU - Angelo, ZINZI
AU - Chesley, Steven
AU - Moskovitz, Nicholas
AU - Barbee, Brent
AU - Abell, Paul
AU - Agrusa, Harrison
AU - Bannister, Michele
AU - Beccarelli, Joel
AU - Bekker, Dmitriy
AU - Syal, Megan Bruck
AU - Buratti, Bonnie
AU - Busch, Michael W.
AU - Bagatin, Adriano Campo
AU - Chatelain, Joseph
AU - Chocron, Isaias
AU - Collins, Gareth
AU - Conversi, Luca
AU - Davison, Thomas
AU - DeCoster, Mallory E.
AU - Deshapriya, Jasinghege Don Prasanna
AU - Eggl, Siegfried
AU - Espiritu, Raymond
AU - Farnham, Tony
AU - Ferrais, Marin
AU - Ferrari, Fabio
AU - Föhring, Dora
AU - Fuentes-Muñoz, Oscar
AU - Gai, Igor
AU - Giordano, Carmine
AU - Glenar, David
AU - Gomez, Edward
AU - Graninger, Dawn
AU - Green, Simon F.
AU - Greenstreet, Sarah
AU - Hasselmann, Pedro Henrique
AU - Herreros, Isabel
AU - Hirabayashi, Masatoshi
AU - Husarik, Marek
AU - (he/him), Simone Ieva
AU - Senel, Cem Berk
N1 - Funding Information: Additional support from a number of sources for individuals is also acknowledged here. For R.L., D.A.G., T.J.S.: this work was supported by the NASA/GSFC Internal Scientist Funding Model (ISFM) Exospheres, Ionospheres, Magnetospheres Modeling (EIMM) team. The work done through the Center for Research and Exploration in Space Science and Technology (CRESST-II) is supported by NASA award No. 80GSFC21M0002. N.X.R. acknowledges support by the Planetary Science Division Internal Scientist Funding Program through the Fundamental Laboratory Research (FLaRe) work package. P.M. acknowledges funding from ESA, CNES, the CNRS through the MITI interdisciplinary programs. For P.M., R.L., K.W., T.S.-R., C.B.S., and A.C.B.: funding from the European Union's Horizon 2020 research and innovation program under grant agreement No. 870377, through Near Earth Object Modelling and Payloads for Protection (NEO-MAPP) project (H2020-EU-2-1-6/870377, EC H2020-SPACE-718 2018-2020, H2020-SPACE-2019). R.M. and S.E. acknowledge funding from a NASA Space Technology Graduate Research Opportunities (NSTGRO) award, contract No. 80NSSC22K1173. For P.P. and P.S: this work was supported by the Grant Agency of the Czech Republic, grant 20-04431S. A.M. acknowledges the Italian Space Agency (ASI) for financial support through agreement No. 2022-8-HH.0 for ESA's Hera mission. I.H. acknowledges the Spanish Research Council (CSIC) support for international cooperation I-LINK project ILINK22061. For J.O.: this work was supported by the Spanish Ministry of Science and Innovation/State Agency of Research MCIN/AEI by grant PID2021-125883NB-C22 and by “ERDF A way of making Europe.” For M.H.: this work was supported by the Slovak Grant Agency for Science VEGA (grant No. 2/0059/22) and by the Slovak Research and Development Agency under contract No. APVV-19-0072. G.S.C. and T.M.D. acknowledge funding from the UK Science and Technology Facilities Council, grant ST/S000615/1. For L.M.P.: contribution was supported by the Margarita Salas postdoctoral grant funded by the Spanish Ministry of Universities—NextGenerationEU. F.F. acknowledges funding from the European Research Council (ERC) under the European Union's Horizon Europe research and innovation program (grant agreement No. 101077758). For T.S.-R.: this work was also partially supported by the Spanish MICIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe” by the “European Union” through grant PID2021-122842OB-C21, and the Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia ’Marıa de Maeztu’) through grant CEX2019-000918-M. For J.M.: funding support acknowledged from the DART Participating Scientist Program ( \#80NSSC21K1048). For A.P.: financial support from Academy of Finland grant No. 1345115. For A.C.B.: funding support from MICINN (Spain) PGC2021, PID2021-125883NB-C21. R.N. acknowledges support from NASA/FINESST (NNH20ZDA001N). J.-Y.L. acknowledges grants HST-GO-16674, HST-GO-17292, and HST-GO-17330 from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, under NASA contract NAS 5-26555. Funding Information: The DART mission is a result of the dedicated efforts of more than a thousand people working for years to make the mission successful. DART Investigation Team and LICIACube Team members beyond those listed as coauthors are thanked for their contributions to the discussions that led to the results summarized in this paper. This work was supported by the DART mission, NASA contract 80MSFC20D0004, and by the Italian Space Agency, Agenzia Spaziale Italiana (ASI) within the LICIACube project (ASI-INAF agreement AC n. 2019-31-HH.0). Funding Information: Additional support from a number of sources for individuals is also acknowledged here. For R.L., D.A.G., T.J.S.: this work was supported by the NASA/GSFC Internal Scientist Funding Model (ISFM) Exospheres, Ionospheres, Magnetospheres Modeling (EIMM) team. The work done through the Center for Research and Exploration in Space Science and Technology (CRESST-II) is supported by NASA award No. 80GSFC21M0002. N.X.R. acknowledges support by the Planetary Science Division Internal Scientist Funding Program through the Fundamental Laboratory Research (FLaRe) work package. P.M. acknowledges funding from ESA, CNES, the CNRS through the MITI interdisciplinary programs. For P.M., R.L., K.W., T.S.-R., C.B.S., and A.C.B.: funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No. 870377, through Near Earth Object Modelling and Payloads for Protection (NEOMAPP) project (H2020-EU-2-1-6/870377, EC H2020-SPACE-718 2018-2020, H2020-SPACE-2019). R.M. and S. E. acknowledge funding from a NASA Space Technology Graduate Research Opportunities (NSTGRO) award, contract No. 80NSSC22K1173. For P.P. and P.S: this work was supported by the Grant Agency of the Czech Republic, grant 20-04431S. A.M. acknowledges the Italian Space Agency (ASI) for financial support through agreement No. 2022-8-HH.0 for ESA’s Hera mission. I.H. acknowledges the Spanish Research Council (CSIC) support for international cooperation I-LINK project ILINK22061. For J.O.: this work was supported by the Spanish Ministry of Science and Innovation/State Agency of Research MCIN/AEI by grant PID2021-125883NB-C22 and by “ERDF A way of making Europe.” For M.H.: this work was supported by the Slovak Grant Agency for Science VEGA (grant No. 2/0059/22) and by the Slovak Research and Development Agency under contract No. APVV-19-0072. G.S.C. and T.M.D. acknowledge funding from the UK Science and Technology Facilities Council, grant ST/ S000615/1. For L.M.P.: contribution was supported by the Margarita Salas postdoctoral grant funded by the Spanish Ministry of Universities—NextGenerationEU. F.F. acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon Europe research and innovation program (grant agreement No. 101077758). For T. S.-R.: this work was also partially supported by the Spanish MICIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe” by the “European Union” through grant PID2021-122842OB-C21, and the Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia’Marıa de Maeztu’) through grant CEX2019-000918-M. For J.M.: funding support acknowledged from the DART Participating Scientist Program (\#80NSSC21K1048). For A.P.: financial support from Academy of Finland grant No. 1345115. For A.C.B.: funding support from MICINN (Spain) PGC2021, PID2021-125883NB-C21. R.N. acknowledges support from NASA/FINESST (NNH20ZDA001N). J.-Y.L. acknowledges grants HST-GO-16674, HST-GO-17292, and HST-GO-17330 from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, under NASA contract NAS 5-26555. Funding Information: A portion of this work was conducted at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Lawrence Livermore National Laboratory is operated by Lawrence Livermore National Security, LLC, for the U.S. Department of Energy, National Nuclear Security Administration under contract DE-AC5207NA27344. LLNL-JRNL-854115. We appreciate the time and effort of two anonymous reviewers to review this paper. Publisher Copyright: © 2024. The Author(s).
PY - 2024/2/1
Y1 - 2024/2/1
N2 - NASA's Double Asteroid Redirection Test (DART) mission was the first to demonstrate asteroid deflection, and the mission's Level 1 requirements guided its planetary defense investigations. Here, we summarize DART's achievement of those requirements. On 2022 September 26, the DART spacecraft impacted Dimorphos, the secondary member of the Didymos near-Earth asteroid binary system, demonstrating an autonomously navigated kinetic impact into an asteroid with limited prior knowledge for planetary defense. Months of subsequent Earth-based observations showed that the binary orbital period was changed by –33.24 minutes, with two independent analysis methods each reporting a 1σ uncertainty of 1.4 s. Dynamical models determined that the momentum enhancement factor, β, resulting from DART's kinetic impact test is between 2.4 and 4.9, depending on the mass of Dimorphos, which remains the largest source of uncertainty. Over five dozen telescopes across the globe and in space, along with the Light Italian CubeSat for Imaging of Asteroids, have contributed to DART's investigations. These combined investigations have addressed topics related to the ejecta, dynamics, impact event, and properties of both asteroids in the binary system. A year following DART's successful impact into Dimorphos, the mission has achieved its planetary defense requirements, although work to further understand DART's kinetic impact test and the Didymos system will continue. In particular, ESA's Hera mission is planned to perform extensive measurements in 2027 during its rendezvous with the Didymos–Dimorphos system, building on DART to advance our knowledge and continue the ongoing international collaboration for planetary defense.
AB - NASA's Double Asteroid Redirection Test (DART) mission was the first to demonstrate asteroid deflection, and the mission's Level 1 requirements guided its planetary defense investigations. Here, we summarize DART's achievement of those requirements. On 2022 September 26, the DART spacecraft impacted Dimorphos, the secondary member of the Didymos near-Earth asteroid binary system, demonstrating an autonomously navigated kinetic impact into an asteroid with limited prior knowledge for planetary defense. Months of subsequent Earth-based observations showed that the binary orbital period was changed by –33.24 minutes, with two independent analysis methods each reporting a 1σ uncertainty of 1.4 s. Dynamical models determined that the momentum enhancement factor, β, resulting from DART's kinetic impact test is between 2.4 and 4.9, depending on the mass of Dimorphos, which remains the largest source of uncertainty. Over five dozen telescopes across the globe and in space, along with the Light Italian CubeSat for Imaging of Asteroids, have contributed to DART's investigations. These combined investigations have addressed topics related to the ejecta, dynamics, impact event, and properties of both asteroids in the binary system. A year following DART's successful impact into Dimorphos, the mission has achieved its planetary defense requirements, although work to further understand DART's kinetic impact test and the Didymos system will continue. In particular, ESA's Hera mission is planned to perform extensive measurements in 2027 during its rendezvous with the Didymos–Dimorphos system, building on DART to advance our knowledge and continue the ongoing international collaboration for planetary defense.
UR - http://dx.doi.org/10.3847/psj/ad16e6
UR - http://www.scopus.com/inward/record.url?scp=85188202563&partnerID=8YFLogxK
U2 - 10.3847/psj/ad16e6
DO - 10.3847/psj/ad16e6
M3 - Article
VL - 5
SP - 1
JO - The Planetary Science Journal
JF - The Planetary Science Journal
SN - 2632-3338
IS - 49
ER -