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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.
Afiliação
  • Jasinski JM; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA. jasinski@jpl.nasa.gov.
  • Regoli LH; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA.
  • Cassidy TA; Applied Physics Laboratory, The John Hopkins University, Laurel, MD, USA.
  • Dewey RM; Laboratory of Atmospheric and Space Sciences, University of Colorado Boulder, Boulder, CO, USA.
  • Raines JM; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA.
  • Slavin JA; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA.
  • Coates AJ; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA.
  • Gershman DJ; Mullard Space Science Laboratory, UCL, Dorking, UK.
  • Nordheim TA; Center for Planetary Sciences, UCL/Birkbeck, London, UK.
  • Murphy N; NASA Goddard Space Flight Center, Greenbelt, MD, USA.
Nat Commun ; 11(1): 4350, 2020 09 29.
Article em En | MEDLINE | ID: mdl-32994408
ABSTRACT
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 (<102 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.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article