Cargando…

A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions

Mercury has a global dayside exosphere, with measured densities of 10(−2) cm(−3) at ~1500 km. Here we report on the inferred enhancement of neutral densities (<10(2) cm(−3)) at high altitudes (~5300 km) by the MESSENGER spacecraft. Such high-altitude densities cannot be accounted for by the typic...

Descripción completa

Detalles Bibliográficos
Autores principales: Jasinski, Jamie M., Regoli, Leonardo H., Cassidy, Timothy A., Dewey, Ryan M., Raines, Jim M., Slavin, James A., Coates, Andrew J., Gershman, Daniel J., Nordheim, Tom A., Murphy, Neil
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2020
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7525509/
https://www.ncbi.nlm.nih.gov/pubmed/32994408
http://dx.doi.org/10.1038/s41467-020-18220-2
_version_ 1783588745882107904
author Jasinski, Jamie M.
Regoli, Leonardo H.
Cassidy, Timothy A.
Dewey, Ryan M.
Raines, Jim M.
Slavin, James A.
Coates, Andrew J.
Gershman, Daniel J.
Nordheim, Tom A.
Murphy, Neil
author_facet Jasinski, Jamie M.
Regoli, Leonardo H.
Cassidy, Timothy A.
Dewey, Ryan M.
Raines, Jim M.
Slavin, James A.
Coates, Andrew J.
Gershman, Daniel J.
Nordheim, Tom A.
Murphy, Neil
author_sort Jasinski, Jamie M.
collection PubMed
description Mercury has a global dayside exosphere, with measured densities of 10(−2) cm(−3) at ~1500 km. Here we report on the inferred enhancement of neutral densities (<10(2) cm(−3)) at high altitudes (~5300 km) by the MESSENGER spacecraft. Such high-altitude densities cannot be accounted for by the typical exosphere. This event was observed by the Fast-Imaging Plasma Spectrometer (FIPS), which detected heavy ions of planetary origin that were recently ionized, and “picked up” by the solar wind. We estimate that the neutral density required to produce the observed pickup ion fluxes is similar to typical exospheric densities found at ~700 km altitudes. We suggest that this event was most likely caused by a meteroid impact. Understanding meteoroid impacts is critical to understanding the source processes of the exosphere at Mercury, and the use of plasma spectrometers will be crucial for future observations with the Bepi-Colombo mission.
format Online
Article
Text
id pubmed-7525509
institution National Center for Biotechnology Information
language English
publishDate 2020
publisher Nature Publishing Group UK
record_format MEDLINE/PubMed
spelling pubmed-75255092020-10-19 A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions Jasinski, Jamie M. Regoli, Leonardo H. Cassidy, Timothy A. Dewey, Ryan M. Raines, Jim M. Slavin, James A. Coates, Andrew J. Gershman, Daniel J. Nordheim, Tom A. Murphy, Neil Nat Commun Article Mercury has a global dayside exosphere, with measured densities of 10(−2) cm(−3) at ~1500 km. Here we report on the inferred enhancement of neutral densities (<10(2) cm(−3)) at high altitudes (~5300 km) by the MESSENGER spacecraft. Such high-altitude densities cannot be accounted for by the typical exosphere. This event was observed by the Fast-Imaging Plasma Spectrometer (FIPS), which detected heavy ions of planetary origin that were recently ionized, and “picked up” by the solar wind. We estimate that the neutral density required to produce the observed pickup ion fluxes is similar to typical exospheric densities found at ~700 km altitudes. We suggest that this event was most likely caused by a meteroid impact. Understanding meteoroid impacts is critical to understanding the source processes of the exosphere at Mercury, and the use of plasma spectrometers will be crucial for future observations with the Bepi-Colombo mission. Nature Publishing Group UK 2020-09-29 /pmc/articles/PMC7525509/ /pubmed/32994408 http://dx.doi.org/10.1038/s41467-020-18220-2 Text en © The Author(s) 2020 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 license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license 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 license, visit http://creativecommons.org/licenses/by/4.0/.
spellingShingle Article
Jasinski, Jamie M.
Regoli, Leonardo H.
Cassidy, Timothy A.
Dewey, Ryan M.
Raines, Jim M.
Slavin, James A.
Coates, Andrew J.
Gershman, Daniel J.
Nordheim, Tom A.
Murphy, Neil
A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions
title A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions
title_full A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions
title_fullStr A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions
title_full_unstemmed A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions
title_short A transient enhancement of Mercury’s exosphere at extremely high altitudes inferred from pickup ions
title_sort transient enhancement of mercury’s exosphere at extremely high altitudes inferred from pickup ions
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7525509/
https://www.ncbi.nlm.nih.gov/pubmed/32994408
http://dx.doi.org/10.1038/s41467-020-18220-2
work_keys_str_mv AT jasinskijamiem atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT regolileonardoh atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT cassidytimothya atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT deweyryanm atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT rainesjimm atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT slavinjamesa atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT coatesandrewj atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT gershmandanielj atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT nordheimtoma atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT murphyneil atransientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT jasinskijamiem transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT regolileonardoh transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT cassidytimothya transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT deweyryanm transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT rainesjimm transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT slavinjamesa transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT coatesandrewj transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT gershmandanielj transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT nordheimtoma transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions
AT murphyneil transientenhancementofmercurysexosphereatextremelyhighaltitudesinferredfrompickupions