File:PIA21482 - Curiosity Observes Whirlwinds Carrying Martian Dust.gif

From Wikimedia Commons, the free media repository
Jump to navigation Jump to search

Original file(1,650 × 550 pixels, file size: 1.87 MB, MIME type: image/gif, looped, 17 frames, 8.5 s)

Captions

Captions

Add a one-line explanation of what this file represents

Summary

[edit]
Description
English: Dust devils dance in the distance in this sequence of images taken by the Navigation Camera on NASA's Curiosity Mars rover on Feb. 12, 2017, during the summer afternoon of the rover's 1,607th Martian day, or sol.

Within a broader context view, the rectangular area outlined in black was imaged multiple times over a span of several minutes to check for dust devils. Images from the period with most activity are shown in the inset area. The images are in pairs that were taken about 12 seconds apart, with an interval of about 90 seconds between pairs. Timing is accelerated and not fully proportional in this animation.

One dust devil appears at the right edge of the inset -- toward the south from the rover -- in the first few frames. Another appears on the left -- toward south-southeast -- later in the sequence. Contrast has been modified to make frame-to-frame changes easier to see. A black frame is added between repeats of the sequence.

Portions of Curiosity are visible in the foreground. The cylindrical UHF (ultra-high frequency) antenna on the left is used for sending data to Mars orbiters, which relay the data to Earth. The angled planes to the right of this antenna are fins of the rover's radioisotope thermoelectric generator, which provides the vehicle's power. The post with a knob on top at right is a low-gain, non-directional antenna that can be used for receiving transmissions from Earth, as backup to the main high-gain antenna (not shown here) used for that purpose.

On Mars as on Earth, dust devils are whirlwinds that result from sunshine warming the ground, prompting convective rising of air that has gained heat from the ground. Observations of Martian dust devils provide information about wind directions and interaction between the surface and the atmosphere.

Curiosity's Sol 1607 location, reached by a drive that was completed two sols earlier, is mapped at http://mars.jpl.nasa.gov/multimedia/images/2017/curiosity-rovers-location-for-sol-1605.

NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Science Laboratory Project for the NASA Science Mission Directorate, Washington. JPL designed and built the project's Curiosity rover and the rover's Navcam.

For more information about Curiosity, visit http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl.
Date 12 February 2017 (published 27 February 2017)
Source Catalog page · Full-res (GIF)
Author NASA/JPL-Caltech/TAMU
Location on Mars4° 42′ 37.43″ S, 137° 21′ 27.93″ E View this and other nearby images on: Google Mapsinfo
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA21482.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
Other languages:
This media is a product of the
Mars Science Laboratory mission
Credit and attribution belongs to the mission team, if not already specified in the "author" row

Licensing

[edit]
Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current23:12, 27 February 2017Thumbnail for version as of 23:12, 27 February 20171,650 × 550 (1.87 MB)PhilipTerryGraham (talk | contribs)User created page with UploadWizard

Metadata