Reconstruction of Bennu Particle Events From Sparse Data

Abstract OSIRIS‐REx began observing particle ejection events shortly after entering orbit around near‐Earth asteroid (101955) Bennu in January 2019. For some of these events, the only observations of the ejected particles come from the first two images taken immediately after the event by OSIRIS‐REx...

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Main Authors: John Y. Pelgrift, Erik J. Lessac‐Chenen, Coralie D. Adam, Jason M. Leonard, Derek S. Nelson, Leilah McCarthy, Eric M. Sahr, Andrew Liounis, Michael Moreau, Brent J. Bos, Carl W. Hergenrother, Dante S. Lauretta
Format: Article
Language:English
Published: American Geophysical Union (AGU) 2020-08-01
Series:Earth and Space Science
Online Access:https://doi.org/10.1029/2019EA000938
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spelling doaj-a6cfc71e631244598869fa7baa0de2982020-11-25T03:51:34ZengAmerican Geophysical Union (AGU)Earth and Space Science2333-50842020-08-0178n/an/a10.1029/2019EA000938Reconstruction of Bennu Particle Events From Sparse DataJohn Y. Pelgrift0Erik J. Lessac‐Chenen1Coralie D. Adam2Jason M. Leonard3Derek S. Nelson4Leilah McCarthy5Eric M. Sahr6Andrew Liounis7Michael Moreau8Brent J. Bos9Carl W. Hergenrother10Dante S. Lauretta11KinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USAKinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USAKinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USAKinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USAKinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USAKinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USAKinetX, Inc., Space Navigation and Flight Dynamics Practice Simi Valley CA USANASA Goddard Spaceflight Center Greenbelt MD USANASA Goddard Spaceflight Center Greenbelt MD USANASA Goddard Spaceflight Center Greenbelt MD USALunar and Planetary Laboratory University of Arizona Tucson AZ USALunar and Planetary Laboratory University of Arizona Tucson AZ USAAbstract OSIRIS‐REx began observing particle ejection events shortly after entering orbit around near‐Earth asteroid (101955) Bennu in January 2019. For some of these events, the only observations of the ejected particles come from the first two images taken immediately after the event by OSIRIS‐REx's NavCam 1 imager. Without three or more observations of each particle, traditional orbit determination is not possible. However, by assuming that the particles all ejected at the same time and location for a given event, and approximating that their velocities remained constant after ejection (a reasonable approximation for fast‐moving particles, i.e., with velocities on the order of 10 cm/s or greater, given Bennu's weak gravity), we show that it is possible to estimate the particles' states from only two observations each. We applied this newly developed technique to reconstruct the particle ejection events observed by the OSIRIS‐REx spacecraft during orbit about Bennu. Particles were estimated to have ejected with inertial velocities ranging from 7 cm/s to 3.3 m/s, leading to a variety of trajectory types. Most (>80%) of the analyzed events were estimated to have originated from midlatitude regions and to have occurred after noon (local solar time), between 12:44 and 18:52. Comparison with higher‐fidelity orbit determination solutions for the events with sufficient observations demonstrates the validity of our approach and also sheds light on its biases. Our technique offers the capacity to meaningfully constrain the properties of particle ejection events from limited data.https://doi.org/10.1029/2019EA000938
collection DOAJ
language English
format Article
sources DOAJ
author John Y. Pelgrift
Erik J. Lessac‐Chenen
Coralie D. Adam
Jason M. Leonard
Derek S. Nelson
Leilah McCarthy
Eric M. Sahr
Andrew Liounis
Michael Moreau
Brent J. Bos
Carl W. Hergenrother
Dante S. Lauretta
spellingShingle John Y. Pelgrift
Erik J. Lessac‐Chenen
Coralie D. Adam
Jason M. Leonard
Derek S. Nelson
Leilah McCarthy
Eric M. Sahr
Andrew Liounis
Michael Moreau
Brent J. Bos
Carl W. Hergenrother
Dante S. Lauretta
Reconstruction of Bennu Particle Events From Sparse Data
Earth and Space Science
author_facet John Y. Pelgrift
Erik J. Lessac‐Chenen
Coralie D. Adam
Jason M. Leonard
Derek S. Nelson
Leilah McCarthy
Eric M. Sahr
Andrew Liounis
Michael Moreau
Brent J. Bos
Carl W. Hergenrother
Dante S. Lauretta
author_sort John Y. Pelgrift
title Reconstruction of Bennu Particle Events From Sparse Data
title_short Reconstruction of Bennu Particle Events From Sparse Data
title_full Reconstruction of Bennu Particle Events From Sparse Data
title_fullStr Reconstruction of Bennu Particle Events From Sparse Data
title_full_unstemmed Reconstruction of Bennu Particle Events From Sparse Data
title_sort reconstruction of bennu particle events from sparse data
publisher American Geophysical Union (AGU)
series Earth and Space Science
issn 2333-5084
publishDate 2020-08-01
description Abstract OSIRIS‐REx began observing particle ejection events shortly after entering orbit around near‐Earth asteroid (101955) Bennu in January 2019. For some of these events, the only observations of the ejected particles come from the first two images taken immediately after the event by OSIRIS‐REx's NavCam 1 imager. Without three or more observations of each particle, traditional orbit determination is not possible. However, by assuming that the particles all ejected at the same time and location for a given event, and approximating that their velocities remained constant after ejection (a reasonable approximation for fast‐moving particles, i.e., with velocities on the order of 10 cm/s or greater, given Bennu's weak gravity), we show that it is possible to estimate the particles' states from only two observations each. We applied this newly developed technique to reconstruct the particle ejection events observed by the OSIRIS‐REx spacecraft during orbit about Bennu. Particles were estimated to have ejected with inertial velocities ranging from 7 cm/s to 3.3 m/s, leading to a variety of trajectory types. Most (>80%) of the analyzed events were estimated to have originated from midlatitude regions and to have occurred after noon (local solar time), between 12:44 and 18:52. Comparison with higher‐fidelity orbit determination solutions for the events with sufficient observations demonstrates the validity of our approach and also sheds light on its biases. Our technique offers the capacity to meaningfully constrain the properties of particle ejection events from limited data.
url https://doi.org/10.1029/2019EA000938
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