Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia

Abstract Interest in impact craters on the earth's surface has increased worldwide and is being investigated by using remote sensing, geological, boreholes, geophysical, and laboratory measurements. These measurements are used to build dynamic models to study crater formation. In this work, the...

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Main Authors: Sherif M. Hanafy, Pantelis Soupios, Alexandros Stampolidis, Christian Bender Koch, Khalid Al‐Ramadan, Abdullatif Al‐Shuhail, Theis Solling, Ignatius Argadestya
Format: Article
Language:English
Published: American Geophysical Union (AGU) 2021-09-01
Series:Earth and Space Science
Subjects:
TEM
GPR
Online Access:https://doi.org/10.1029/2020EA001432
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spelling doaj-78bbcbfe42bb4f7e93ef1a96333694992021-09-27T21:10:34ZengAmerican Geophysical Union (AGU)Earth and Space Science2333-50842021-09-0189n/an/a10.1029/2020EA001432Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi ArabiaSherif M. Hanafy0Pantelis Soupios1Alexandros Stampolidis2Christian Bender Koch3Khalid Al‐Ramadan4Abdullatif Al‐Shuhail5Theis Solling6Ignatius Argadestya7College of Petroleum Engineering and Geosciences King Fahd University of Petroleum and Minerals Dhahran Saudi ArabiaCollege of Petroleum Engineering and Geosciences King Fahd University of Petroleum and Minerals Dhahran Saudi ArabiaSchool of Geology Aristotle University of Thessaloniki Thessaloniki GreeceDepartment of Chemistry University of Copenhagen Copenhagen DenmarkCollege of Petroleum Engineering and Geosciences King Fahd University of Petroleum and Minerals Dhahran Saudi ArabiaCollege of Petroleum Engineering and Geosciences King Fahd University of Petroleum and Minerals Dhahran Saudi ArabiaCollege of Petroleum Engineering and Geosciences King Fahd University of Petroleum and Minerals Dhahran Saudi ArabiaCollege of Petroleum Engineering and Geosciences King Fahd University of Petroleum and Minerals Dhahran Saudi ArabiaAbstract Interest in impact craters on the earth's surface has increased worldwide and is being investigated by using remote sensing, geological, boreholes, geophysical, and laboratory measurements. These measurements are used to build dynamic models to study crater formation. In this work, the near‐crater sediments at the young Wabar crater field in Saudi Arabia have been investigated using magnetic, transient electromagnetic (TEM), seismic, and ground‐penetrating radar (GPR) methods. The main objectives of this research were to (a) explore the possibility of any remnant major pieces of the meteorite, (b) investigate the meteoroid direction, and (c) map the deformational structures associated with the meteorite impact. Our results show five different magnetic anomaly types and three layers in the subsurface. The maximum depth of deformation due to the impact of the meteorite is about 25 m as shown by the seismic travel time tomogram, the quasi‐2D TEM, and the 3D GPR model. TEM survey confirmed the geometrical characteristics of the major crater and located another small crater (known as Philby‐A). The magnetic survey shows no evidence of any remnant major pieces of the meteorite; however, it was used to trace ejecta material containing highly dilute magnetic material. The magnetic carrier is most likely spheres of metal incorporated in the black/green glasses. During the expedition, many small pieces of the meteoroid were found and collected for further geochemical analysis. Based on the geophysical findings, the meteorite direction was found to be from north to south.https://doi.org/10.1029/2020EA001432magneticTEMseismicGPR
collection DOAJ
language English
format Article
sources DOAJ
author Sherif M. Hanafy
Pantelis Soupios
Alexandros Stampolidis
Christian Bender Koch
Khalid Al‐Ramadan
Abdullatif Al‐Shuhail
Theis Solling
Ignatius Argadestya
spellingShingle Sherif M. Hanafy
Pantelis Soupios
Alexandros Stampolidis
Christian Bender Koch
Khalid Al‐Ramadan
Abdullatif Al‐Shuhail
Theis Solling
Ignatius Argadestya
Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia
Earth and Space Science
magnetic
TEM
seismic
GPR
author_facet Sherif M. Hanafy
Pantelis Soupios
Alexandros Stampolidis
Christian Bender Koch
Khalid Al‐Ramadan
Abdullatif Al‐Shuhail
Theis Solling
Ignatius Argadestya
author_sort Sherif M. Hanafy
title Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia
title_short Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia
title_full Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia
title_fullStr Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia
title_full_unstemmed Comprehensive Geophysical Study at Wabar Crater, Rub Al‐Khali Desert, Saudi Arabia
title_sort comprehensive geophysical study at wabar crater, rub al‐khali desert, saudi arabia
publisher American Geophysical Union (AGU)
series Earth and Space Science
issn 2333-5084
publishDate 2021-09-01
description Abstract Interest in impact craters on the earth's surface has increased worldwide and is being investigated by using remote sensing, geological, boreholes, geophysical, and laboratory measurements. These measurements are used to build dynamic models to study crater formation. In this work, the near‐crater sediments at the young Wabar crater field in Saudi Arabia have been investigated using magnetic, transient electromagnetic (TEM), seismic, and ground‐penetrating radar (GPR) methods. The main objectives of this research were to (a) explore the possibility of any remnant major pieces of the meteorite, (b) investigate the meteoroid direction, and (c) map the deformational structures associated with the meteorite impact. Our results show five different magnetic anomaly types and three layers in the subsurface. The maximum depth of deformation due to the impact of the meteorite is about 25 m as shown by the seismic travel time tomogram, the quasi‐2D TEM, and the 3D GPR model. TEM survey confirmed the geometrical characteristics of the major crater and located another small crater (known as Philby‐A). The magnetic survey shows no evidence of any remnant major pieces of the meteorite; however, it was used to trace ejecta material containing highly dilute magnetic material. The magnetic carrier is most likely spheres of metal incorporated in the black/green glasses. During the expedition, many small pieces of the meteoroid were found and collected for further geochemical analysis. Based on the geophysical findings, the meteorite direction was found to be from north to south.
topic magnetic
TEM
seismic
GPR
url https://doi.org/10.1029/2020EA001432
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