Right angles are not common in nature. They are almost always formed by tectonic forces. This right angle on Mars is part of Sacra Fossae. This image is from NASA's 2001 Mars Odyssey spacecraft.

Right angles are not common in nature. They are almost always formed by tectonic forces. This right angle on Mars is part of Sacra Fossae. This image is from NASA's 2001 Mars Odyssey spacecraft.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of Right angles are not common in nature. They are almost always formed by tectonic forces. This right angle on Mars is part of Sacra Fossae. This image is from NASA's 2001 Mars Odyssey spacecraft. by Piemags/PL Photography Limited is available for licensing today.

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This VIS image is located in the region between northern Terra Sabaea and Utopia Planitia. This unnamed crater contains a small dune field. The crater rim is heavily eroded and it appears that some downslope movement on the interior of the rim may have included a volatile component such as ice. Orbit Number 72636 Latitude 42.2873 Longitude 66.9553 Instrument VIS Captured 2018-04-30 01 22
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Reull Vallis. This VIS image shows a short section of Reull Vallis. Reull Vallis starts in Promethei Terra and empties into Hellas Plainitia. In other regions of the channel the floor contains ridged and grooved materials. In some sections of the channel these materials appear to deflect around obstacles. These features are proposed to be ice-rich materials similar to glaciers on Earth. Reull Vallis is 1051km (653 miles) long. Orbit Number 92980 Latitude -39.6307 Longitude 110.597 Instrument VIS Captured 2022-11-30 05 57 https //photojournal.jpl.nasa.gov/catalog/PIA25803
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Image Number: 6145-45038579Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Martian Terrain and Geological FeaturesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1392×2765
2001 Mars Odyssey
Mars|