View allAll Photos Tagged hellas
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Colour-coded topography map of the Hellas Chaos region found in the Hellas Basin in the southern hemisphere of Mars. White and red show the highest terrains, while blue and purple show the deepest.
This region was imaged by the High Resolution StereoCamera on ESA’s Mars Express on 23 January 2014 during orbit 12 785. The image is centred on 46ºS / 69ºE and has a ground resolution of about 18 m per pixel. North is to the right and west is at the top.
Read more: www.esa.int/Our_Activities/Space_Science/Mars_Express/Fro...
Credit: ESA/DLR/FU Berlin (G. Neukum), CC BY-SA 3.0 IGO
Copyright Notice:
This work is licenced under the Creative Commons Attribution-ShareAlike 3.0 IGO (CC BY-SA 3.0 IGO) licence. The user is allowed to reproduce, distribute, adapt, translate and publicly perform this publication, without explicit permission, provided that the content is accompanied by an acknowledgement that the source is credited as 'ESA/DLR/FU Berlin’, a direct link to the licence text is provided and that it is clearly indicated if changes were made to the original content. Adaptation/translation/derivatives must be distributed under the same licence terms as this publication. To view a copy of this license, please visit creativecommons.org/licenses/by-sa/3.0/igo/
[C.YFashion] *HELLA*
EXCLUSIVE FOR EVENT*ASTROPHE*
SET:JACKET-TOP-PASTIES-PANTS-PANTIES BOM-GARTE MAZE-HEELS
OPEN EVENT 05/03-CLOSED 25/03/2025
LM IN STORE
Scarring the southern highlands of Mars is one of the Solar System’s largest impact basins: Hellas, with a diameter of 2300 km and a depth of over 7 km.
Hellas is thought to have formed between 3.8 and 4.1 billion years ago, when a large asteroid hit the surface of Mars. Since its formation, Hellas has been subject to modification by the action of wind, ice, water and volcanic activity.
Impact craters have also since pock-marked this vast basin floor, two of which are the focus of this image, taken by the High Resolution Stereo Camera on ESA’s Mars Express on 17 December 2013. The ground resolution is about 15 metres per pixel.
These craters lie in the deepest, western portion of Hellas, and such a clear view is unusual because dust clouds typically obscure the basin floor. Indeed, this region seems to be covered by a thick blanket of dust.
The larger of the two craters is about 25 km across. A flow of material appears to have been transported from the top left of the scene and into the crater. Zooming in to the smooth mound and the area immediately around it reveals interesting textures that likely resulted from this flow.
Flow features are also seen outside of the craters, and in particular, at the centre left of the image near the top of the frame. Material also seems to have cascaded from the larger crater’s rim and into a neighbouring smaller crater, at the far left of the image.
The morphology of many features in the Hellas Basin and its surroundings strongly suggests the presence of ice and glaciers.
For example, in the foreground and around the crater rim, polygons of patterned ground are visible which indicates the presence of water – this pattern occurs when fine grained and porous wet soil freezes.
Indeed, in the deepest parts of the basin, the atmospheric pressure is about 89% higher than at the surface, which may even offer conditions suitable for water. Radar images from NASA’s Mars Reconnaissance Orbiter suggest that some craters in Hellas might contain water-ice glaciers several hundred metres thick, buried under layers of dust.
Credit: ESA/DLR/FU Berlin (G. Neukum), CC BY-SA 3.0 IGO
Copyright Notice:
This work is licenced under the Creative Commons Attribution-ShareAlike 3.0 IGO (CC BY-SA 3.0 IGO) licence. The user is allowed to reproduce, distribute, adapt, translate and publicly perform this publication, without explicit permission, provided that the content is accompanied by an acknowledgement that the source is credited as 'ESA/DLR/FU Berlin’, a direct link to the licence text is provided and that it is clearly indicated if changes were made to the original content. Adaptation/translation/derivatives must be distributed under the same licence terms as this publication. To view a copy of this license, please visit creativecommons.org/licenses/by-sa/3.0/igo/
LEATHER WALK 2018 ! !
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THANK YOU for visiting my virtual art gallery! Enjoy my social documentary photos of various events !
ADDA DADA's photography presents a variety of adults at different public events . These photos do NOT imply the person's sexual orientation in any way. Everyone was asked and they consented to be photographed and posted.
Photos are properly marked SAFE or RESTRICTED ( 18+ only / nudity). There is NO porn, and, NO stolen photos on my site!
Viewers should be aware that these photos are viewed by a wide variety of folks . Inappropriate, RUDE, 'X' or 'R' rated comments shall be removed forthwith & you will be blocked.
MY photos are NOT to be reproduced, COPIED, BLOGGED, USED in any way shape or form. Use of them by anyone is an infringement of copyright ! © All rights reserved. Use without permission is illegal.
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On the way to Klima village from the Catacombs of Milos island and after an hour's worth of steep and quite a dangerous descent under the blistering August sun, on a path seemingly God forsaken, we realized it was anything BUT forsaken. A small clearing, a tiny Chapel built in the mountain's rock, an olive tree, some longed-for shade... Refuge, with view to the majestic Aegean blue.
The Chapel is dedicated to St. Paraskevi, patron Saint of eyes and sight. Summer of 2012, Milos Island.