Home | Site Map | What's New | Image Index | Copyright | Posters | ScienceViews | Science Fiction Timelines |

PHOTO INDEX OF
PRIMARY TARGETS
ASTEROIDS
COMETS
EARTH
JUPITER
KUIPER BELT
MARS
MERCURY
METEORITES
NEPTUNE
OORT CLOUD
PLUTO
SATURN
SOLAR SYSTEM
SPACE
SUN
URANUS
VENUS
ORDER PRINTS

OTHER PHOTO INDEXES
ALL TARGETS
PHOTO CATEGORIES

SCIENCEVIEWS
AMERICAN INDIAN
AMPHIBIANS
BIRDS
BUGS
FINE ART
FOSSILS
THE ISLANDS
HISTORICAL PHOTOS
MAMMALS
OTHER
PARKS
PLANTS
RELIGIOUS
REPTILES
SCIENCEVIEWS PRINTS

High Haze in Color (Close-up)

Target Name:  Titan
Spacecraft:  Cassini Orbiter
Instrument:  Imaging Science Subsystem - Narrow Angle
Produced by:  NASA/JPL/Space Science Institute
Copyright: NASA Copyright Free Policy
Cross Reference:  PIA06123
Date Taken:  24 October 2004

Related Documents
Download Options

NameTypeWidth x HeightSize
PIA06123.jpgJPEG640 x 27115K
PIA06123.jpgJPEG1182 x 50039K
PIA06123.tifTIFF1182 x 500611.6 kB

A global detached haze layer and discrete cloud-like features high above Titan's northern terminator (day-night transition) are visible in this close-up image acquired on October 24, 2004, as the Cassini spacecraft neared its first close encounter with Titan. This image is a colorized version of an ultraviolet image released on October 25, 2004 (PIA06120). The haze has been given colors that are close to what the natural colors are believed to be. The view was also sharpened to enhance the structure in the discrete features.

The image was acquired at a distance of about 1 million kilometers (621,371 miles) in a near ultraviolet filter that is sensitive to scattering by small particles. The Sun preferentially illuminates the southern hemisphere at this time; the north polar region is in darkness. The well-known global detached haze layer, hundreds of kilometers above Titan's surface, is produced by photochemical reactions and is visible as a thin ring of bright material around the entire planet. At the northern high-latitude edge of the image, additional striations are visible, caused by particulates that are high enough to be illuminated by the Sun even though the surface directly below is in darkness. These striations may simply be caused by a wave propagating through the detached haze, or they may be evidence of additional regional haze or cloud layers not present at other latitudes.

Copyright © 1995-2016 by Calvin J. Hamilton. All rights reserved.