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Orbital period change of Dimorphos due to the DART kinetic impact

The Double Asteroid Redirection Test (DART) spacecraft successfully performed the first test of a kinetic impactor for asteroid deflection by impacting Dimorphos, the secondary of near-Earth binary asteroid (65803) Didymos, and changing the orbital period of Dimorphos. A change in orbital period of...

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Autores principales: Thomas, Cristina A., Naidu, Shantanu P., Scheirich, Peter, Moskovitz, Nicholas A., Pravec, Petr, Chesley, Steven R., Rivkin, Andrew S., Osip, David J., Lister, Tim A., Benner, Lance A. M., Brozović, Marina, Contreras, Carlos, Morrell, Nidia, Rożek, Agata, Kušnirák, Peter, Hornoch, Kamil, Mages, Declan, Taylor, Patrick A., Seymour, Andrew D., Snodgrass, Colin, Jørgensen, Uffe G., Dominik, Martin, Skiff, Brian, Polakis, Tom, Knight, Matthew M., Farnham, Tony L., Giorgini, Jon D., Rush, Brian, Bellerose, Julie, Salas, Pedro, Armentrout, William P., Watts, Galen, Busch, Michael W., Chatelain, Joseph, Gomez, Edward, Greenstreet, Sarah, Phillips, Liz, Bonavita, Mariangela, Burgdorf, Martin J., Khalouei, Elahe, Longa-Peña, Penélope, Rabus, Markus, Sajadian, Sedighe, Chabot, Nancy L., Cheng, Andrew F., Ryan, William H., Ryan, Eileen V., Holt, Carrie E., Agrusa, Harrison F.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10115635/
https://www.ncbi.nlm.nih.gov/pubmed/36858072
http://dx.doi.org/10.1038/s41586-023-05805-2
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author Thomas, Cristina A.
Naidu, Shantanu P.
Scheirich, Peter
Moskovitz, Nicholas A.
Pravec, Petr
Chesley, Steven R.
Rivkin, Andrew S.
Osip, David J.
Lister, Tim A.
Benner, Lance A. M.
Brozović, Marina
Contreras, Carlos
Morrell, Nidia
Rożek, Agata
Kušnirák, Peter
Hornoch, Kamil
Mages, Declan
Taylor, Patrick A.
Seymour, Andrew D.
Snodgrass, Colin
Jørgensen, Uffe G.
Dominik, Martin
Skiff, Brian
Polakis, Tom
Knight, Matthew M.
Farnham, Tony L.
Giorgini, Jon D.
Rush, Brian
Bellerose, Julie
Salas, Pedro
Armentrout, William P.
Watts, Galen
Busch, Michael W.
Chatelain, Joseph
Gomez, Edward
Greenstreet, Sarah
Phillips, Liz
Bonavita, Mariangela
Burgdorf, Martin J.
Khalouei, Elahe
Longa-Peña, Penélope
Rabus, Markus
Sajadian, Sedighe
Chabot, Nancy L.
Cheng, Andrew F.
Ryan, William H.
Ryan, Eileen V.
Holt, Carrie E.
Agrusa, Harrison F.
author_facet Thomas, Cristina A.
Naidu, Shantanu P.
Scheirich, Peter
Moskovitz, Nicholas A.
Pravec, Petr
Chesley, Steven R.
Rivkin, Andrew S.
Osip, David J.
Lister, Tim A.
Benner, Lance A. M.
Brozović, Marina
Contreras, Carlos
Morrell, Nidia
Rożek, Agata
Kušnirák, Peter
Hornoch, Kamil
Mages, Declan
Taylor, Patrick A.
Seymour, Andrew D.
Snodgrass, Colin
Jørgensen, Uffe G.
Dominik, Martin
Skiff, Brian
Polakis, Tom
Knight, Matthew M.
Farnham, Tony L.
Giorgini, Jon D.
Rush, Brian
Bellerose, Julie
Salas, Pedro
Armentrout, William P.
Watts, Galen
Busch, Michael W.
Chatelain, Joseph
Gomez, Edward
Greenstreet, Sarah
Phillips, Liz
Bonavita, Mariangela
Burgdorf, Martin J.
Khalouei, Elahe
Longa-Peña, Penélope
Rabus, Markus
Sajadian, Sedighe
Chabot, Nancy L.
Cheng, Andrew F.
Ryan, William H.
Ryan, Eileen V.
Holt, Carrie E.
Agrusa, Harrison F.
author_sort Thomas, Cristina A.
collection PubMed
description The Double Asteroid Redirection Test (DART) spacecraft successfully performed the first test of a kinetic impactor for asteroid deflection by impacting Dimorphos, the secondary of near-Earth binary asteroid (65803) Didymos, and changing the orbital period of Dimorphos. A change in orbital period of approximately 7 min was expected if the incident momentum from the DART spacecraft was directly transferred to the asteroid target in a perfectly inelastic collision(1), but studies of the probable impact conditions and asteroid properties indicated that a considerable momentum enhancement (β) was possible(2,3). In the years before impact, we used lightcurve observations to accurately determine the pre-impact orbit parameters of Dimorphos with respect to Didymos(4–6). Here we report the change in the orbital period of Dimorphos as a result of the DART kinetic impact to be −33.0 ± 1.0 (3σ) min. Using new Earth-based lightcurve and radar observations, two independent approaches determined identical values for the change in the orbital period. This large orbit period change suggests that ejecta contributed a substantial amount of momentum to the asteroid beyond what the DART spacecraft carried.
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spelling pubmed-101156352023-04-21 Orbital period change of Dimorphos due to the DART kinetic impact Thomas, Cristina A. Naidu, Shantanu P. Scheirich, Peter Moskovitz, Nicholas A. Pravec, Petr Chesley, Steven R. Rivkin, Andrew S. Osip, David J. Lister, Tim A. Benner, Lance A. M. Brozović, Marina Contreras, Carlos Morrell, Nidia Rożek, Agata Kušnirák, Peter Hornoch, Kamil Mages, Declan Taylor, Patrick A. Seymour, Andrew D. Snodgrass, Colin Jørgensen, Uffe G. Dominik, Martin Skiff, Brian Polakis, Tom Knight, Matthew M. Farnham, Tony L. Giorgini, Jon D. Rush, Brian Bellerose, Julie Salas, Pedro Armentrout, William P. Watts, Galen Busch, Michael W. Chatelain, Joseph Gomez, Edward Greenstreet, Sarah Phillips, Liz Bonavita, Mariangela Burgdorf, Martin J. Khalouei, Elahe Longa-Peña, Penélope Rabus, Markus Sajadian, Sedighe Chabot, Nancy L. Cheng, Andrew F. Ryan, William H. Ryan, Eileen V. Holt, Carrie E. Agrusa, Harrison F. Nature Article The Double Asteroid Redirection Test (DART) spacecraft successfully performed the first test of a kinetic impactor for asteroid deflection by impacting Dimorphos, the secondary of near-Earth binary asteroid (65803) Didymos, and changing the orbital period of Dimorphos. A change in orbital period of approximately 7 min was expected if the incident momentum from the DART spacecraft was directly transferred to the asteroid target in a perfectly inelastic collision(1), but studies of the probable impact conditions and asteroid properties indicated that a considerable momentum enhancement (β) was possible(2,3). In the years before impact, we used lightcurve observations to accurately determine the pre-impact orbit parameters of Dimorphos with respect to Didymos(4–6). Here we report the change in the orbital period of Dimorphos as a result of the DART kinetic impact to be −33.0 ± 1.0 (3σ) min. Using new Earth-based lightcurve and radar observations, two independent approaches determined identical values for the change in the orbital period. This large orbit period change suggests that ejecta contributed a substantial amount of momentum to the asteroid beyond what the DART spacecraft carried. Nature Publishing Group UK 2023-03-01 2023 /pmc/articles/PMC10115635/ /pubmed/36858072 http://dx.doi.org/10.1038/s41586-023-05805-2 Text en © The Author(s) 2023 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Article
Thomas, Cristina A.
Naidu, Shantanu P.
Scheirich, Peter
Moskovitz, Nicholas A.
Pravec, Petr
Chesley, Steven R.
Rivkin, Andrew S.
Osip, David J.
Lister, Tim A.
Benner, Lance A. M.
Brozović, Marina
Contreras, Carlos
Morrell, Nidia
Rożek, Agata
Kušnirák, Peter
Hornoch, Kamil
Mages, Declan
Taylor, Patrick A.
Seymour, Andrew D.
Snodgrass, Colin
Jørgensen, Uffe G.
Dominik, Martin
Skiff, Brian
Polakis, Tom
Knight, Matthew M.
Farnham, Tony L.
Giorgini, Jon D.
Rush, Brian
Bellerose, Julie
Salas, Pedro
Armentrout, William P.
Watts, Galen
Busch, Michael W.
Chatelain, Joseph
Gomez, Edward
Greenstreet, Sarah
Phillips, Liz
Bonavita, Mariangela
Burgdorf, Martin J.
Khalouei, Elahe
Longa-Peña, Penélope
Rabus, Markus
Sajadian, Sedighe
Chabot, Nancy L.
Cheng, Andrew F.
Ryan, William H.
Ryan, Eileen V.
Holt, Carrie E.
Agrusa, Harrison F.
Orbital period change of Dimorphos due to the DART kinetic impact
title Orbital period change of Dimorphos due to the DART kinetic impact
title_full Orbital period change of Dimorphos due to the DART kinetic impact
title_fullStr Orbital period change of Dimorphos due to the DART kinetic impact
title_full_unstemmed Orbital period change of Dimorphos due to the DART kinetic impact
title_short Orbital period change of Dimorphos due to the DART kinetic impact
title_sort orbital period change of dimorphos due to the dart kinetic impact
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10115635/
https://www.ncbi.nlm.nih.gov/pubmed/36858072
http://dx.doi.org/10.1038/s41586-023-05805-2
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