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You may have seen MRK’s amazing videos, but did you know that you can buy prints of his digital creations?
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Posted on April 6, 2013 via thinx with 5,013 notes
Source: staceythinx
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Berlin was rad
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Posted on April 3, 2013 via The Landscape of Logan with 1,025 notes
Source: logans818
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Tatiana Plakhova and Leandro Sanchez - Another California
“Photographer Leandro Sanchez captures unique visuals of flooded beaches in Southern California and deep desert that only a few human beings will ever see, to them unite forces with Tatiana Plakhova and her extraordinary delicate designs.”
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Posted on April 1, 2013 via arpeggia with 3,984 notes
Source: arpeggia
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welp
Posted on March 26, 2013 via bonbonAficionado with 170,964 notes
Source: misskerryberry
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Posted on March 9, 2013 via R.S. with 1,106 notes
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Amazing Volcanic Photography of Martin Rietze
Posted on March 6, 2013 via Scinerds with 36,488 notes
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HiRISE Updates From February 27th
Note: Images described in the order they appear from top down.
Cratered Cones in the Cydonia Region
This observation focuses on an unusually high density of cratered cones, imaged previously by the Mars Orbiter Camera. These cones could possibly be mud volcanos. On Earth, a large number of these formations are located in Gobustan, Azerbaijan and the Caspian Sea.
This image in Ius Chasma, a portion of the massive canyon system Vallis Marineris, draws our attention because a fault previously imaged by the Mars Orbiter Camera.
A valley cuts also cuts across the ridge. Is this the result of some tectonic process? A study in 2012 suggested that Mars possesses tectonic plates, but if so, how these processes work is still an area of study.
The Mars Science Laboratory mission released a total of 8 tungsten masses for balance purposes during entry and descent. Two 75-kilogram masses were released at the top of the atmosphere, and the resultant craters were probably imaged in ESP_029245_1755.
Delta Structure in Eberswalde Crater
Eberswalde Crater contains layered rocks about 100-meters thick exposed in a a well-preserved delta (Malin and Edgett 2003, Moore et al. 2003).
This sedimentary deposit contains dozens of shallowly tilted, alternating bright and dark layers of varying thickness (1–10 meters). HiRISE terrain models reveal structures in these layers which are interpreted as lake-floor deposits (Lewis and Aharonson 2006, Pondrelli et al. 2008).
This delta is distinguished from other fan-shaped deposits on Mars by the presence of a preserved distributary network including lobes, inverted channels, and meander cutoffs. Another example of a fan with a distributary network can be found in Jezero Crater, which may represent a more degraded version of the same kind of system.
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Posted on March 3, 2013 via CWL with 175 notes
Source: kenobi-wan-obi
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Posted on January 28, 2013 via OOBLIVM with 6,100 notes
Source: brettkingery

