Coprates quadrangle - Revision history

Suitupshowup at 14:08, 24 January 2025

2025-01-24T14:08:57Z

Suitupshowup: added image

2024-12-18T16:20:17Z

added image

Suitupshowup: /* Recurrent slope lineae */ added ref

2024-01-01T15:58:32Z

Recurrent slope lineae: added ref

Suitupshowup: /* Layers */

2023-12-26T18:54:07Z

Layers

Suitupshowup: /* Layers */ added image

2023-12-26T18:52:41Z

Layers: added image

Suitupshowup: /* Valles Marineris canyon system */

2023-12-24T22:44:14Z

Valles Marineris canyon system

Suitupshowup: /* Valles Marineris canyon system */

2023-12-24T22:43:22Z

Valles Marineris canyon system

Suitupshowup: /* Layers */

2023-11-17T23:11:07Z

Layers

Suitupshowup: /* Layers */ added image

2023-11-17T23:09:40Z

Layers: added image

Suitupshowup: /* Valles Marineris canyon system */ added images

2023-09-02T15:50:11Z

Valles Marineris canyon system: added images

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 |[[Mars Atlas|Atlas]]
 |}
 <gallery widths="400" heights="300">
 File:USGS-Mars-MC-18-CopratesRegion-mola.png

← Older revision		Revision as of 16:20, 18 December 2024
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	</gallery>		</gallery>
	[[Category: Mars Atlas]]		[[Category: Mars Atlas]]
		+
		+
		+	[[File:Collage coprates 01.jpg\|Features of Features of Coprates quadrangle, as seen by HiRISE under under HiWish program\|600pxr\| Features of Coprates quadrangle]]
		+
		+	Scenes of the Coprates quadrangle

← Older revision		Revision as of 15:58, 1 January 2024
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	Recurrent slope lineae (RSL) are small dark streaks on slopes that elongate in warm seasons. They may be evidence of liquid water.<ref>McEwen, A., et al. 2014. Recurring slope lineae in equatorial regions of Mars. Nature Geoscience 7, 53-58. doi:10.1038/ngeo2014</ref><ref>McEwen, A., et al. 2011. Seasonal Flows on Warm Martian Slopes. Science. 05 Aug 2011. 333, 6043,740-743. DOI: 10.1126/science.1204816</ref><ref>http://redplanet.asu.edu/?tag=recurring-slope-lineae</ref>		Recurrent slope lineae (RSL) are small dark streaks on slopes that elongate in warm seasons. They may be evidence of liquid water.<ref>McEwen, A., et al. 2014. Recurring slope lineae in equatorial regions of Mars. Nature Geoscience 7, 53-58. doi:10.1038/ngeo2014</ref><ref>McEwen, A., et al. 2011. Seasonal Flows on Warm Martian Slopes. Science. 05 Aug 2011. 333, 6043,740-743. DOI: 10.1126/science.1204816</ref><ref>http://redplanet.asu.edu/?tag=recurring-slope-lineae</ref>

−	[[File:49955 1665rslcolorarrows.jpg\|thumb\|400px\|left\|Close, color view of recurrent slope lineae, as seen by HiRISE under HiWish program Arrows point to some of the recurrent slope lineae]]	+	[[File:49955 1665rslcolorarrows.jpg\|thumb\|400px\|left\|Close, color view of recurrent slope lineae, as seen by HiRISE under HiWish program Arrows point to some of the recurrent slope lineae <ref>Stillman, D., et al. 2017. Characteristics of the numerous and widespread recurring slope lineae (RSL) in Valles Marineris, Mars. Icarus. Volume 285. Pages 195-210</ref>]]

@@ Line 73: / Line 73: @@
 <gallery class="center"  widths="380px" heights="360px">
-File:Wide view of layers in candor ESP 074432 1735.jpg|Wide view of layers in Candor, as seen by HiRISE.  This picture was named HiRISE picture of the day'
+File:Wide view of layers in candor ESP 074432 1735.jpg|Wide view of layers in Candor, as seen by HiRISE.  This picture was named HiRISE picture of the day for November 9, 2023.
 File:Layers in Candor, ESP 074432 1735-2.jpg|Close view of layers in Candor.  Image has been processed in color to bring out more detail.  It was named HiRISE picture of the day for November 9, 2023.

← Older revision		Revision as of 18:52, 26 December 2023
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	<gallery class="center" widths="380px" heights="360px">		<gallery class="center" widths="380px" heights="360px">
		+
		+	File:Wide view of layers in candor ESP 074432 1735.jpg\|Wide view of layers in Candor, as seen by HiRISE. This picture was named HiRISE picture of the day'
		+
		+	File:Layers in Candor, ESP 074432 1735-2.jpg\|Close view of layers in Candor. Image has been processed in color to bring out more detail. It was named HiRISE picture of the day for November 9, 2023.

	Image:Ganges Chasma Layers.JPG\|Ganges Chasma Layers, as seen by HiRISE.		Image:Ganges Chasma Layers.JPG\|Ganges Chasma Layers, as seen by HiRISE.

@@ Line 50: / Line 50: @@
 File: Ganges Chasma.JPG|Cliff in northern wall of Ganges Chasma, as seen by THEMIS.
 </gallery>
 ==Interior layered deposits and sulfate==

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 File:Layers and light-toned rocks 01.jpg|Wide view of layers in a crater and light-toned material, as seen by HiRISE under HiWish program.  Light-toned materials often contain water bearing minerals like sulfates.
 File:Layers in crater 03.jpg|Layers in crater, as seen by HiRISE
 File:Layers and light-toned rocks 04.jpg|Layers in crater, as seen by HiRISE  Light toned material is visible also.  Light-toned materials often contain water bearing minerals like sulfates.  Only part of the image is in color because the camera only takes a color strip in the center.

@@ Line 93: / Line 93: @@
 ESP 048057 1560crater.jpg|Layers near top of crater wall
 1560craterlayersclose.jpg|Close view of layers near top of crater wall
 </gallery>

← Older revision		Revision as of 15:50, 2 September 2023
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	[[File: Melas Chasma.JPG\|thumb\|400px\|center\|[[Melas Chasma]], as seen by THEMIS.]]		[[File: Melas Chasma.JPG\|thumb\|400px\|center\|[[Melas Chasma]], as seen by THEMIS.]]
		+
		+	[[File:ESP 013784 1710Valles Marineriswide.jpg\|thumb\|300px\|left\|Layers in south wall of Valles Marineris Wall shows many layers; some are from lava flows.]]
		+
		+	[[File:ESP 013784 1710Valles Marineriscolors.jpg\|thumb\|300px\|right\|Color image of part of south wall of Valles Marineris, as seen by HiRISE. Different minerals produce different colors.]]

	<gallery class="center" widths="380px" heights="360px">		<gallery class="center" widths="380px" heights="360px">