|
Collection:
|
|
NASA Cassini-Huygens Collection
Collection
NASA Cassini-Huygens Collection
Collection
|
|
Title:
|
|
High Haze in Color (Close-up)
Title
High Haze in Color (Close-up)
Title
|
|
Description:
|
|
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn.
description
Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn.
Description
|
|
Full Description:
|
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 (PIA 06120). 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 feature. 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. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.n
and the Cassini imaging team home page, http://ciclops.org. Image Credit: NASA/JPL/Space Science Institute
Full_Description
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 (PIA 06120). 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 feature. 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. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. For more information about the Cassini-Huygens mission, visit http://saturn.jpl.n
and the Cassini imaging team home page, http://ciclops.org. Image Credit: NASA/JPL/Space Science Institute
Full Description
|
|
Keywords:
|
|
gallery
keywords
gallery
Keywords
|
|
Keywords:
|
|
images
|
|
Keywords:
|
|
Cassini
keywords
Cassini
Keywords
|
|
Keywords:
|
|
mission
keywords
mission
Keywords
|
|
Keywords:
|
|
Huygens
keywords
Huygens
Keywords
|
|
Keywords:
|
|
probe
|
|
Keywords:
|
|
Saturn
|
|
Keywords:
|
|
explore
keywords
explore
Keywords
|
|
Keywords:
|
|
videos
|
|
Keywords:
|
|
movies
|
|
Keywords:
|
|
Jupiter
keywords
Jupiter
Keywords
|
|
Keywords:
|
|
flyby
|
|
Keywords:
|
|
spacecraft
keywords
spacecraft
Keywords
|
|
Keywords:
|
|
assembly
keywords
assembly
Keywords
|
|
Keywords:
|
|
launch
|
|
Keywords:
|
|
flight
|
|
Keywords:
|
|
operations facilities
keywords
operations facilities
Keywords
|
|
Keywords:
|
|
mpeg
|
|
Keywords:
|
|
Quicktime
keywords
Quicktime
Keywords
|
|
facet_what:
|
|
Saturn
facet_what
Saturn
facet_what
|
|
facet_what:
|
|
Cassini
facet_what
Cassini
facet_what
|
|
facet_what:
|
|
Jupiter
facet_what
Jupiter
facet_what
|
|
facet_what:
|
|
Cassini-Huygens
facet_what
Cassini-Huygens
facet_what
|
|
facet_what:
|
|
Huygens Probe
facet_what
Huygens Probe
facet_what
|
|
facet_what:
|
|
Titan
facet_what
Titan
facet_what
|
|
facet_what:
|
|
Cassini Orbiter
facet_what
Cassini Orbiter
facet_what
|
|
facet_what:
|
|
Sun
facet_what
Sun
facet_what
|
|
facet_what:
|
|
Polar
facet_what
Polar
facet_what
|
|
facet_where:
|
|
Saturn
facet_where
Saturn
facet_where
|
|
facet_where:
|
|
Jupiter
facet_where
Jupiter
facet_where
|
|
facet_where:
|
|
Jet Propulsion Laboratory
facet_where
Jet Propulsion Laboratory
facet_where
|
|
facet_where:
|
|
California
facet_where
California
facet_where
|
|
facet_where:
|
|
Washington
facet_where
Washington
facet_where
|
|
facet_where:
|
|
Jet Propulsion Laboratory (JPL)
facet_where
Jet Propulsion Laboratory (JPL)
facet_where
|
|
facet_where:
|
|
Washington, D.C.
facet_where
Washington, D.C.
facet_where
|
|
facet_when:
|
|
October 24, 2004
facet_when
October 24, 2004
facet_when
|
|
facet_when:
|
|
October 25, 2004
facet_when
October 25, 2004
facet_when
|
|
facet_when_year:
|
|
2004
facet_when_year
2004
facet_when_year
|
|
UID:
|
|
SPD-SATRN-1142
|
|
original url:
|
original_url
original url
|