2017 IEEE Aerospace Conference 2017
DOI: 10.1109/aero.2017.7943906
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Development of Venus drill

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Cited by 6 publications
(2 citation statements)
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“…Some older soviet landers as Luna 16, 20 and 24 reached 1.6 m below the lunar surface [69], while Lunokhod 1 and 2 rovers carried a cone-vane penetrometer to access distances of up to 0.1 m [70]. Drills mounted on landers or robotic equipment have made some tasks at shallow depths on Venus (Venera 13-14 and Vega 2 landers [71]), or performed scooping on the Moon (Surveyor 3 and 7 [50]) or Mars (Viking landers [72]). More recently, space drilling activities took place onboard the Rosetta [73] and Beagle 2 [74] landers and in the Curiosity rover [75].…”
Section: Subsurface Locomotionmentioning
confidence: 99%
“…Some older soviet landers as Luna 16, 20 and 24 reached 1.6 m below the lunar surface [69], while Lunokhod 1 and 2 rovers carried a cone-vane penetrometer to access distances of up to 0.1 m [70]. Drills mounted on landers or robotic equipment have made some tasks at shallow depths on Venus (Venera 13-14 and Vega 2 landers [71]), or performed scooping on the Moon (Surveyor 3 and 7 [50]) or Mars (Viking landers [72]). More recently, space drilling activities took place onboard the Rosetta [73] and Beagle 2 [74] landers and in the Curiosity rover [75].…”
Section: Subsurface Locomotionmentioning
confidence: 99%
“…The global radar images reveal an array of landforms, some of which appear to be the result of tectonism while others are proposed to be volcanic features produced by a variety of magma types with different viscosities [6][7][8]. The highland tesserae, from which we do not have geochemical data, may contain more felsic compositions hinting at similarities to terrestrial-style continental crust building [9,10]. The tesserae regions are thought to be ancient, and are likely either granitic in composition or represent heavily altered basalt, both pointing to an epoch long since passed in Venus' history.…”
mentioning
confidence: 99%