File:Calypso crop resize sharp.jpg

Calypso_crop_resize_sharp.jpg(560 × 400 pixels, file size: 46 KB, MIME type: image/jpeg)

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Summary

Description
English: This raw, unprocessed image of Calypso was taken by Cassini on Feb. 13, 2010.

The image was taken with the Cassini spacecraft narrow-angle camera on Feb. 13, 2010 using a spectral filter sensitive to wavelengths of ultraviolet light centered at 338 nanometers. The view was obtained at a distance of approximately 23,000 kilometers (14,000 miles) from Calypso. Image scale is 135 meters (443 feet) per pixel.

The Cassini Equinox Mission is a joint United States and European endeavor. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini Equinox Mission visit http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

The original NASA image has been modified by cropping, doubling the linear pixel density, sharpening and removal of a cosmic ray artifact.
Date
Source http://ciclops.org/view/6204/Calypso_Rev_126_Flyby_Raw_Preview_1
Author NASA / JPL / Space Science Institute

Licensing

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.)
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13 February 2010

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current19:34, 20 February 2010560 × 400 (46 KB)WolfmanSF{{Information |Description={{en|1=This raw, unprocessed image of Calypso was taken by Cassini on Feb. 13, 2010. The image was taken with the Cassini spacecraft narrow-angle camera on Feb. 13, 2010 using a spectral filter sensitive to wavelengths of ultra

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