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Sources of cosmic dust in the Earth's atmosphere
There are four known sources of dust in the inner solar system: Jupiter Family comets, asteroids, Halley Type comets, and Oort Cloud comets. Here we combine the mass, velocity, and radiant distributions of these cosmic dust populations from an astronomical model with a chemical ablation model to est...
Autores principales: | , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
John Wiley and Sons Inc.
2016
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5319002/ https://www.ncbi.nlm.nih.gov/pubmed/28275286 http://dx.doi.org/10.1002/2016GL071697 |
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author | Carrillo‐Sánchez, J. D. Nesvorný, D. Pokorný, P. Janches, D. Plane, J. M. C. |
author_facet | Carrillo‐Sánchez, J. D. Nesvorný, D. Pokorný, P. Janches, D. Plane, J. M. C. |
author_sort | Carrillo‐Sánchez, J. D. |
collection | PubMed |
description | There are four known sources of dust in the inner solar system: Jupiter Family comets, asteroids, Halley Type comets, and Oort Cloud comets. Here we combine the mass, velocity, and radiant distributions of these cosmic dust populations from an astronomical model with a chemical ablation model to estimate the injection rates of Na and Fe into the Earth's upper atmosphere, as well as the flux of cosmic spherules to the surface. Comparing these parameters to lidar observations of the vertical Na and Fe fluxes above 87.5 km, and the measured cosmic spherule accretion rate at South Pole, shows that Jupiter Family Comets contribute (80 ± 17)% of the total input mass (43 ± 14 t d(−1)), in good accord with Cosmic Background Explorer and Planck observations of the zodiacal cloud. |
format | Online Article Text |
id | pubmed-5319002 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2016 |
publisher | John Wiley and Sons Inc. |
record_format | MEDLINE/PubMed |
spelling | pubmed-53190022017-03-06 Sources of cosmic dust in the Earth's atmosphere Carrillo‐Sánchez, J. D. Nesvorný, D. Pokorný, P. Janches, D. Plane, J. M. C. Geophys Res Lett Research Letters There are four known sources of dust in the inner solar system: Jupiter Family comets, asteroids, Halley Type comets, and Oort Cloud comets. Here we combine the mass, velocity, and radiant distributions of these cosmic dust populations from an astronomical model with a chemical ablation model to estimate the injection rates of Na and Fe into the Earth's upper atmosphere, as well as the flux of cosmic spherules to the surface. Comparing these parameters to lidar observations of the vertical Na and Fe fluxes above 87.5 km, and the measured cosmic spherule accretion rate at South Pole, shows that Jupiter Family Comets contribute (80 ± 17)% of the total input mass (43 ± 14 t d(−1)), in good accord with Cosmic Background Explorer and Planck observations of the zodiacal cloud. John Wiley and Sons Inc. 2016-12-14 2016-12-16 /pmc/articles/PMC5319002/ /pubmed/28275286 http://dx.doi.org/10.1002/2016GL071697 Text en ©2016. The Authors. This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs (http://creativecommons.org/licenses/by-nc-nd/4.0/) License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made. |
spellingShingle | Research Letters Carrillo‐Sánchez, J. D. Nesvorný, D. Pokorný, P. Janches, D. Plane, J. M. C. Sources of cosmic dust in the Earth's atmosphere |
title | Sources of cosmic dust in the Earth's atmosphere |
title_full | Sources of cosmic dust in the Earth's atmosphere |
title_fullStr | Sources of cosmic dust in the Earth's atmosphere |
title_full_unstemmed | Sources of cosmic dust in the Earth's atmosphere |
title_short | Sources of cosmic dust in the Earth's atmosphere |
title_sort | sources of cosmic dust in the earth's atmosphere |
topic | Research Letters |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5319002/ https://www.ncbi.nlm.nih.gov/pubmed/28275286 http://dx.doi.org/10.1002/2016GL071697 |
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