File:Krater mit Dünenfeld in der Nähe des Vulkans Aonia Tholus (23657058408).jpeg
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![File:Krater mit Dünenfeld in der Nähe des Vulkans Aonia Tholus (23657058408).jpeg](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d0/Krater_mit_D%C3%BCnenfeld_in_der_N%C3%A4he_des_Vulkans_Aonia_Tholus_%2823657058408%29.jpeg/800px-Krater_mit_D%C3%BCnenfeld_in_der_N%C3%A4he_des_Vulkans_Aonia_Tholus_%2823657058408%29.jpeg?20230212211716)
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[edit]DescriptionKrater mit Dünenfeld in der Nähe des Vulkans Aonia Tholus (23657058408).jpeg |
Deutsch: Die vom DLR betriebene HRSC auf Mars Express nimmt die Marsoberfläche gleichzeitig in hoher Auflösung, in 3D und mit vier Farbfiltern im sichtbaren Licht für die Farben Blau, Grün und Rot sowie in Wellenlängen des nahen Infrarot auf. Diese aus dem senkrecht auf den Mars gerichteten Nadirkanal und den Farbkanälen erzeugte, kontrastverstärkte Echtfarbendarstellung lässt gut Materialunterschiede in der sonst meist sehr eintönigen Marsoberfläche erkennen. Auffallend ist insbesondere das dunkle Dünenfeld innerhalb des 48 Kilometer großen Einschlagskraters (links). Der Krater befindet sich unweit des Vulkans Aonia Tholus. Frühere vulkanische Aktivität auf dem Mars erzeugte große Mengen feinkörniger Asche, die im Laufe der Zeit von anderem Gesteinsmaterial überdeckt wurde. Durch Einschlagskrater wurden diese verdeckten Schickten wieder freigelegt – sie gelten deshalb als wahrscheinliche Quelle für die dunklen Dünen. Norden liegt rechts im Bild.
Mehr dazu: www.dlr.de/dlr/desktopdefault.aspx/tabid-10333/623_read-2... Credit: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGOEnglish: The HRSC on Mars Express, operated by DLR, simultaneously records the Martian surface in high resolution, in 3D and with four color filters in visible light for the colors blue, green and red as well as in near-infrared wavelengths. This contrast-enhanced, true-color display, generated from the nadir channel, which is directed perpendicularly to Mars, and the color channels, makes it easy to see material differences in the otherwise mostly very monotonous surface of Mars. The dark dune field within the 48-kilometer impact crater (left) is particularly striking. The crater is located near the volcano Aonia Tholus. Previous volcanic activity on Mars produced large amounts of fine-grained ash, which over time became covered by other rocky material. These hidden layers were uncovered again by impact craters - they are therefore regarded as a probable source for the dark dunes. North is on the right in the picture. More on this: www.dlr.de/dlr/desktopdefault.aspx/tabid-10333/623_read-2... www.dlr.de/mars Credit: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO |
Date | Taken on 29 August 2017, 18:51:55 |
Source | Krater mit Dünenfeld in der Nähe des Vulkans Aonia Tholus |
Author | DLR_de |
Flickr set InfoField | Mars Express |
Flickr tags InfoField | roterplanet; marsexpress; mars; planet; stereokamera; hrsc; planetenforschung; kamera |
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This image was originally posted to Flickr by DLR_de at https://flickr.com/photos/48213136@N06/23657058408. It was reviewed on 12 February 2023 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-sa-2.0. |
12 February 2023
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