17 Mar

File:Curiosity's 'Rocknest' Workplace.jpeg

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The drift consists of sand trapped on the downwind side of a group of dark cobbles the team named Rocknest. This mosaic of 55 images from the Mars Hand Lens Imager (MAHLI) shows the first four of five places from which the rover’s scoop obtained sand to clean the sample handling and processing system. The scooped material was ultimately delivered to the Chemistry and Mineralogy Experiment (CheMin) and the Sample Analysis at Mars (SAM) laboratory instruments housed inside the rover’s body. The annotated version of this figure shows the location of a scoop taken at a later date -- the fifth and final scoop, and the only one that provided grains delivered to SAM.

The drift consists of sand trapped on the downwind side of a group of dark cobbles the team named Rocknest. This mosaic of 55 images from the Mars Hand Lens Imager (MAHLI) shows the first four of five places from which the rover’s scoop obtained sand to clean the sample handling and processing system. The scooped material was ultimately delivered to the Chemistry and Mineralogy Experiment (CheMin) and the Sample Analysis at Mars (SAM) laboratory instruments housed inside the rover’s body. The annotated version of this figure shows the location of a scoop taken at a later date -- the fifth and final scoop, and the only one that provided grains delivered to SAM.

Before scooping, the rover team put an approximately 20-inch-wide (about 50- centimeter-wide) wheel print on the Rocknest wind drift. This allowed MAHLI and the Alpha Particle X-Ray Spectrometer (APXS) to determine whether the drift really consisted of sand with small enough sizes to clean the Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) instrument and be delivered to CheMin and SAM. The drift material at the center of the wheel print, named "Portage" by the rover team, was examined by the APXS.}}

Before scooping, the rover team put an approximately 20-inch-wide (about 50- centimeter-wide) wheel print on the Rocknest wind drift. This allowed MAHLI and the Alpha Particle X-Ray Spectrometer (APXS) to determine whether the drift really consisted of sand with small enough sizes to clean the Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) instrument and be delivered to CheMin and SAM. The drift material at the center of the wheel print, named "Portage" by the rover team, was examined by the APXS.}}
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{{pl|1=Należący do {{w|NASA|NASA|pl}} łazik {{w|Curiosity Rover|Curiosity|pl}} przedstawia swój autoportret, a w kontekście jego miejsca pracy, obszar zwany "Rocknest Drift wiatru", w 84 dniu misji na Marsie, albo w {{w|Curiosity Rover#Sol|Sol|pl}}
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{{pl|1=Rocknest — miejsce pracy łazika Curiosity

Na zdjęciu, należący do {{w|NASA|NASA|pl}} łazik {{w|Curiosity Rover|Curiosity|pl}} przedstawia swój autoportret, a w kontekście jego miejsca pracy, obszar zwany "Rocknest Drift wiatru", w 84 dniu misji na Marsie, albo w {{w|Curiosity Rover#Sol|Sol|pl}} 84, (na Ziemi był wtedy 31 października 2012). Łazik pracował w tej lokalizacji od Sol 56 (2 października 2012) do Sol 100 (16 listopada 2012).

Wydma składa się z piasku uwięzionego na {{w|Strona zawietrzna|zawietrznej stronie|pl}} grupy ciemnych kamieni nazwanych Rocknest.

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84, (na Ziemi był wtedy 31 października 2012). Łazik pracował w tej lokalizacji od Sol 56 (2 października 2012) do Sol 100 (16 listopada 2012).}}

|date=2010-10-20 10:14:34

|date=2010-10-20 10:14:34

|source=http://www.nasa.gov/mission_pages/msl/multimedia/pia16468.html

|source=http://www.nasa.gov/mission_pages/msl/multimedia/pia16468.html

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