|
Collection:
|
|
NASA Cassini-Huygens Collection
Collection
NASA Cassini-Huygens Collection
Collection
|
|
Title:
|
|
Titan's Whispers
Title
Titan's Whispers
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:
|
This image shows Titan data from the passive radiometer mode of Cassini's radar instrument overlaid onto a visible-light image mosaic from the spacecraft's imaging science subsystem. The contours and colors show Titan's radiation at microwave wavelengths (about two centimeters or 0.79 inch), while the light and dark shading is from the optical image. This microwave radiation comes directly from Titan itself, rather than being a reflection from the Sun as detected in visible-light images. The microwave brightness tells us about surface properties such as temperature composition and roughness. The brightness decreases when the angle of the surface is tilted from the viewer, causing the edges of Titan's disc to look dark relative to the center even though they are probably at the same temperature. Since the variations in brightness are likely larger than variations in physical temperature, they are probably due to compositional or structural properties of the surface. There is a significant correlation between areas that are bright in the microwave and dark in the optical, and vice versa. Comparison of data sets will help determine the causes of these variations. The radar data was taken on Oct. 26, 2004, during Cassini's first close encounter with Titan. The imaging science subsystem data was acquired on approach to the moon. 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 instrument team is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. For the latest news about the Cassini-Huygens mission visit http://www.nasa.gov
For more information about the mission visit http://saturn.jpl.n
. Image Credit: NASA/JPL
Full_Description
This image shows Titan data from the passive radiometer mode of Cassini's radar instrument overlaid onto a visible-light image mosaic from the spacecraft's imaging science subsystem. The contours and colors show Titan's radiation at microwave wavelengths (about two centimeters or 0.79 inch), while the light and dark shading is from the optical image. This microwave radiation comes directly from Titan itself, rather than being a reflection from the Sun as detected in visible-light images. The microwave brightness tells us about surface properties such as temperature composition and roughness. The brightness decreases when the angle of the surface is tilted from the viewer, causing the edges of Titan's disc to look dark relative to the center even though they are probably at the same temperature. Since the variations in brightness are likely larger than variations in physical temperature, they are probably due to compositional or structural properties of the surface. There is a significant correlation between areas that are bright in the microwave and dark in the optical, and vice versa. Comparison of data sets will help determine the causes of these variations. The radar data was taken on Oct. 26, 2004, during Cassini's first close encounter with Titan. The imaging science subsystem data was acquired on approach to the moon. 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 instrument team is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. For the latest news about the Cassini-Huygens mission visit http://www.nasa.gov
For more information about the mission visit http://saturn.jpl.n
. Image Credit: NASA/JPL
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:
|
|
Moon
facet_what
Moon
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:
|
|
Imaging Science Subsystem (ISS)
facet_what
Imaging Science Subsystem (ISS)
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
|
|
UID:
|
|
SPD-SATRN-1169
|
|
original url:
|
original_url
original url
|