File:Martian CO2 gas venting.jpg
Martian_CO2_gas_venting.jpg (501 × 351 pixels, file size: 41 KB, MIME type: image/jpeg)
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Summary
DescriptionMartian CO2 gas venting.jpg |
English: Schematic sketch of the CO2 geyser hypothesis. Martian south polar layered terrain is overlain by seasonal ice of ~1 m in thickness. Penetration of sunlight to the base of the seasonal deposit causes sublimation from the bottom, leading to a buildup of pressurized CO2 gas. The gas eventually bursts out, entraining dust and leading to the dark fan-shaped deposits. Repeated outbursts from year to year erode the underlying polar layered deposits, leading to the development of "Martian spiders".
Polski: Schematyczny szkic hipotezy gejzera CO2 Marsjańskie czapy polarne są przykryte przez suchy lód grubości ~ 1 m. Przenikanie światła słonecznego do podstawy podłoża poprzez taflę lodu (na wiosnę) powoduje sublimację CO2 od dołu, co prowadzi do tworzenia się gazowego CO2 poddawanemu coraz to większemu ciśnieniu. Gaz w końcu wybucha, porywając piasek i kurz, co prowadzi do tworzenia się na powierzchni lodu ciemnych osadów, najczęściej wachlarzowatych. Powtarzające się wybuchy z roku na rok, zaburzają/rozwijają podstawowe polarne warstwy osadowe, co prowadzi do rozwoju "marsjańskich pająków". Romkur 21:32, 16 August 2013 (UTC) |
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Date | |||||
Source | Own work by uploader: I scanned, cropped and resized the original image from paper by Sylvain Piqueux. JGR, VOL. 108, no. E8, 5084, doi:10.1029/2002JE002007, 2003 | ||||
Author | BatteryIncluded | ||||
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
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Kierunek wiatru
Dwutlenek węgla z porwanym piaskiem i kurzem
Osad piasku i kurzu na tafli zestalonego dwutlenku węgla, zanikający po nadejściu zimy
Sezonowa pokrywa lodowa
Polarne osady warstwowe
Termiczna izolacja
Captions
Items portrayed in this file
depicts
some value
5 September 2009
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 04:47, 5 September 2009 | ![]() | 501 × 351 (41 KB) | commons>BatteryIncluded | {{Information |Description={{en|1=Schematic sketch of the CO2 geyser hypothesis. Martian south polar layered terrain is overlain by seasonal ice of ~1 m in thickness. Penetration of sunlight to the base of the seasonal deposit causes sublimation from the |
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