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English: This is the first image taken by NASA's InSight lander on the surface of Mars. The instrument context camera (ICC) mounted below the lander deck obtained this image on Nov. 26, 2018, shortly after landing. The transparent lens cover was still in place to protect the lens from any dust kicked up during landing.
Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."
The thrusters of the InSight lander dug pits during landing beneath it at its landing site.. For landers that are even heavier than the Curiosity rover (which required a 4.5 meter (15 feet) diameter aeroshell), engineers are developing a combination rigid-inflatable Low-Density Supersonic Decelerator that could be 8 meters (26 feet) in diameter.
Here we report on the geology and subsurface structure of the landing site to aid in situ geophysical investigations. InSight landed in a degraded impact crater in Elysium Planitia on a smooth sandy, granule- and pebble-rich surface with few rocks. Superposed impact craters are common and eolian bedforms are sparse.
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Cropped version of the original batch-processed image (#035A72) of the "Face on Mars". The black dots that give the image a speckled appearance are data errors (salt-and-pepper noise). [10] Second Viking 1 image of the Cydonia region on Mars. Labeled 070A13. Cydonia was first imaged in detail by the Viking 1 and Viking 2 orbiters.
The landing occurred in the late afternoon, with the first images taken at 15:53:58 on the mission clock (local mean solar time). [83] The landing took place shortly after Mars passed through its northern vernal equinox ( Ls = 5.2°), at the start of the astronomical spring, the equivalent of the end of March on Earth.
Apollo 7 slow-scan TV, transmitted by the RCA command module TV camera. NASA decided on initial specifications for TV on the Apollo command module (CM) in 1962. [2] [ Note 1] Both analog and digital transmission techniques were studied, but the early digital systems still used more bandwidth than an analog approach: 20 MHz for the digital system, compared to 500 kHz for the analog system. [2]