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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2020-08-01
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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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