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Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover
Observations by several cameras on the Perseverance rover showed a 22° scattering halo around the Sun over several hours during northern midsummer (solar longitude 142°). Such a halo has not previously been seen beyond Earth. The halo occurred during the aphelion cloud belt season and the cloudiest...
Autores principales: | , , , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
John Wiley and Sons Inc.
2022
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9539710/ https://www.ncbi.nlm.nih.gov/pubmed/36245894 http://dx.doi.org/10.1029/2022GL099776 |
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author | Lemmon, M. T. Toledo, D. Apestigue, V. Arruego, I. Wolff, M. J. Patel, P. Guzewich, S. Colaprete, A. Vicente‐Retortillo, Á. Tamppari, L. Montmessin, F. de la Torre Juarez, M. Maki, J. McConnochie, T. Brown, A. Bell, J. F. |
author_facet | Lemmon, M. T. Toledo, D. Apestigue, V. Arruego, I. Wolff, M. J. Patel, P. Guzewich, S. Colaprete, A. Vicente‐Retortillo, Á. Tamppari, L. Montmessin, F. de la Torre Juarez, M. Maki, J. McConnochie, T. Brown, A. Bell, J. F. |
author_sort | Lemmon, M. T. |
collection | PubMed |
description | Observations by several cameras on the Perseverance rover showed a 22° scattering halo around the Sun over several hours during northern midsummer (solar longitude 142°). Such a halo has not previously been seen beyond Earth. The halo occurred during the aphelion cloud belt season and the cloudiest time yet observed from the Perseverance site. The halo required crystalline water‐ice cloud particles in the form of hexagonal columns large enough for refraction to be significant, at least 11 μm in diameter and length. From a possible 40–50 km altitude, and over the 3.3 hr duration of the halo, particles could have fallen 3–12 km, causing downward transport of water and dust. Halo‐forming clouds are likely rare due to the high supersaturation of water that is required but may be more common in northern subtropical regions during northern midsummer. |
format | Online Article Text |
id | pubmed-9539710 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2022 |
publisher | John Wiley and Sons Inc. |
record_format | MEDLINE/PubMed |
spelling | pubmed-95397102022-10-14 Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover Lemmon, M. T. Toledo, D. Apestigue, V. Arruego, I. Wolff, M. J. Patel, P. Guzewich, S. Colaprete, A. Vicente‐Retortillo, Á. Tamppari, L. Montmessin, F. de la Torre Juarez, M. Maki, J. McConnochie, T. Brown, A. Bell, J. F. Geophys Res Lett Research Letter Observations by several cameras on the Perseverance rover showed a 22° scattering halo around the Sun over several hours during northern midsummer (solar longitude 142°). Such a halo has not previously been seen beyond Earth. The halo occurred during the aphelion cloud belt season and the cloudiest time yet observed from the Perseverance site. The halo required crystalline water‐ice cloud particles in the form of hexagonal columns large enough for refraction to be significant, at least 11 μm in diameter and length. From a possible 40–50 km altitude, and over the 3.3 hr duration of the halo, particles could have fallen 3–12 km, causing downward transport of water and dust. Halo‐forming clouds are likely rare due to the high supersaturation of water that is required but may be more common in northern subtropical regions during northern midsummer. John Wiley and Sons Inc. 2022-09-09 2022-09-16 /pmc/articles/PMC9539710/ /pubmed/36245894 http://dx.doi.org/10.1029/2022GL099776 Text en © 2022. The Authors. https://creativecommons.org/licenses/by/4.0/This is an open access article under the terms of the http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. |
spellingShingle | Research Letter Lemmon, M. T. Toledo, D. Apestigue, V. Arruego, I. Wolff, M. J. Patel, P. Guzewich, S. Colaprete, A. Vicente‐Retortillo, Á. Tamppari, L. Montmessin, F. de la Torre Juarez, M. Maki, J. McConnochie, T. Brown, A. Bell, J. F. Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover |
title | Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover |
title_full | Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover |
title_fullStr | Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover |
title_full_unstemmed | Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover |
title_short | Hexagonal Prisms Form in Water‐Ice Clouds on Mars, Producing Halo Displays Seen by Perseverance Rover |
title_sort | hexagonal prisms form in water‐ice clouds on mars, producing halo displays seen by perseverance rover |
topic | Research Letter |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9539710/ https://www.ncbi.nlm.nih.gov/pubmed/36245894 http://dx.doi.org/10.1029/2022GL099776 |
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