Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus
Venus and Earth share key similarities yet differ fundamentally. It is uncertain how Venus's evolution diverged from Earth's and if its past was significantly different from its present state. Despite the interest in Venus since the dawn of planetary missions, orbiters could only use radar...
Main Authors: | , , , , |
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Format: | Conference Object |
Language: | English |
Published: |
2024
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Subjects: | |
Online Access: | https://elib.dlr.de/209895/ https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-1152.html |
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author | Domac, Akin Adeli, Solmaz Kenkmann, Thomas Arnold, Gabriele Helbert, Jörn |
author_facet | Domac, Akin Adeli, Solmaz Kenkmann, Thomas Arnold, Gabriele Helbert, Jörn |
author_sort | Domac, Akin |
collection | Unknown |
description | Venus and Earth share key similarities yet differ fundamentally. It is uncertain how Venus's evolution diverged from Earth's and if its past was significantly different from its present state. Despite the interest in Venus since the dawn of planetary missions, orbiters could only use radar waves to observe the surface due to its dense and opaque atmosphere. Subsequent research revealed that Venus's atmosphere permits the transmission of electromagnetic waves emitted from its hot surface through six spectral bands centered at 0.86 μm, 0.91 μm, 0.99 μm, 1.02 μm, 1.11 μm and 1.18 μm within five atmospheric windows [1]. Advances in near-infrared imagers and laboratory measurements of the emissivity of rocks have spurred a new era of Venus exploration. In June 2021, two orbiters were announced as part of a fleet of Venus missions: NASA’s VERITAS and ESA’s EnVision. Both orbiters will be equipped with emissivity mappers designed and built by the German Aerospace Center (DLR) and aim to use these six bands to map the surface globally: Venus Emissivity Mapper (VEM) and VenSpec-M, respectively. [2, 3]. Here, we inquire into the potential of near-infrared remote sensing observations to investigate recent or active volcanic activity by employing machine learning methods for classifying surface units and change detection in preparation for future Venus missions. Iceland serves as a primary analog for Venus in addressing the research questions of this study. This is because Iceland has a young, mostly vegetation-free surface that is formed by ongoing volcanic activity. Reykjanes Peninsula has been experiencing frequent fissure eruptions for the last 4 years. Two of these eruptions, known as the 2021 and 2022 Fagradalsfjall eruptions, resulted in the formation of a 5.01 km2 flow field called Fagradalshraun [4, 5, 6]. The study investigated the Reykjanes Peninsula, focusing on Fagradalshraun, using near-infrared bands in the spectral range of VEM of pre- and post-eruption Sentinel-2A datasets. The imagery dataset was selected ... |
format | Conference Object |
genre | Iceland |
genre_facet | Iceland |
geographic | Reykjanes Venus |
geographic_facet | Reykjanes Venus |
id | ftdlr:oai:elib.dlr.de:209895 |
institution | Open Polar |
language | English |
long_lat | ENVELOPE(-22.250,-22.250,65.467,65.467) ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
op_collection_id | ftdlr |
op_doi | https://doi.org/10.5194/epsc2024-1152 |
op_relation | https://elib.dlr.de/209895/1/EPSC2024-1152-print.pdf Domac, Akin und Adeli, Solmaz und Kenkmann, Thomas und Arnold, Gabriele und Helbert, Jörn (2024) Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus. Europlanet Science Congress 2024, 2024-09-08 - 2024-09-13, Berlin, Germany. doi:10.5194/epsc2024-1152 <https://doi.org/10.5194/epsc2024-1152>. |
op_rights | cc_by |
publishDate | 2024 |
record_format | openpolar |
spelling | ftdlr:oai:elib.dlr.de:209895 2025-06-15T14:30:15+00:00 Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus Domac, Akin Adeli, Solmaz Kenkmann, Thomas Arnold, Gabriele Helbert, Jörn 2024-07-03 application/pdf https://elib.dlr.de/209895/ https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-1152.html en eng https://elib.dlr.de/209895/1/EPSC2024-1152-print.pdf Domac, Akin und Adeli, Solmaz und Kenkmann, Thomas und Arnold, Gabriele und Helbert, Jörn (2024) Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus. Europlanet Science Congress 2024, 2024-09-08 - 2024-09-13, Berlin, Germany. doi:10.5194/epsc2024-1152 <https://doi.org/10.5194/epsc2024-1152>. cc_by Planetare Labore Konferenzbeitrag NonPeerReviewed 2024 ftdlr https://doi.org/10.5194/epsc2024-1152 2025-06-04T04:58:09Z Venus and Earth share key similarities yet differ fundamentally. It is uncertain how Venus's evolution diverged from Earth's and if its past was significantly different from its present state. Despite the interest in Venus since the dawn of planetary missions, orbiters could only use radar waves to observe the surface due to its dense and opaque atmosphere. Subsequent research revealed that Venus's atmosphere permits the transmission of electromagnetic waves emitted from its hot surface through six spectral bands centered at 0.86 μm, 0.91 μm, 0.99 μm, 1.02 μm, 1.11 μm and 1.18 μm within five atmospheric windows [1]. Advances in near-infrared imagers and laboratory measurements of the emissivity of rocks have spurred a new era of Venus exploration. In June 2021, two orbiters were announced as part of a fleet of Venus missions: NASA’s VERITAS and ESA’s EnVision. Both orbiters will be equipped with emissivity mappers designed and built by the German Aerospace Center (DLR) and aim to use these six bands to map the surface globally: Venus Emissivity Mapper (VEM) and VenSpec-M, respectively. [2, 3]. Here, we inquire into the potential of near-infrared remote sensing observations to investigate recent or active volcanic activity by employing machine learning methods for classifying surface units and change detection in preparation for future Venus missions. Iceland serves as a primary analog for Venus in addressing the research questions of this study. This is because Iceland has a young, mostly vegetation-free surface that is formed by ongoing volcanic activity. Reykjanes Peninsula has been experiencing frequent fissure eruptions for the last 4 years. Two of these eruptions, known as the 2021 and 2022 Fagradalsfjall eruptions, resulted in the formation of a 5.01 km2 flow field called Fagradalshraun [4, 5, 6]. The study investigated the Reykjanes Peninsula, focusing on Fagradalshraun, using near-infrared bands in the spectral range of VEM of pre- and post-eruption Sentinel-2A datasets. The imagery dataset was selected ... Conference Object Iceland Unknown Reykjanes ENVELOPE(-22.250,-22.250,65.467,65.467) Venus ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
spellingShingle | Planetare Labore Domac, Akin Adeli, Solmaz Kenkmann, Thomas Arnold, Gabriele Helbert, Jörn Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus |
title | Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus |
title_full | Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus |
title_fullStr | Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus |
title_full_unstemmed | Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus |
title_short | Remote Sensing Investigation of Recent Volcanic Activity on Reykjanes Peninsula, Iceland, as an Analog for Venus |
title_sort | remote sensing investigation of recent volcanic activity on reykjanes peninsula, iceland, as an analog for venus |
topic | Planetare Labore |
topic_facet | Planetare Labore |
url | https://elib.dlr.de/209895/ https://meetingorganizer.copernicus.org/EPSC2024/EPSC2024-1152.html |