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Double Titan
Caption NASA:"These two views of Saturn's moon Titan exemplify how NASA's Cassini Spacecraft has revealed the Surface of this fascinating world.

Cassini carried several instruments to pierce the veil of hydrocarbon haze that enshrouds Titan. These include the Spacecraft's Radar and the Visual and InfraRed Mapping Spectrometer, or VIMS. The mission's imaging cameras also have several spectral filters sensitive to specific wavelengths of InfraRed Light that are able to make it through the Haze to the Surface and back into space. These "spectral windows" have enable the imaging cameras to map nearly the entire surface of Titan.

In addition to Titan's Surface, images from both the imaging cameras and VIMS have provided windows into the moon's ever-changing Atmosphere, chronicling the appearance and movement of Hazes and Clouds over the years. A large, bright and feathery band of Summer Clouds can be seen arcing across high Northern Latitudes in the view at right (Dx).

These views were obtained with the Cassini Spacecraft Narrow-Angle Camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the Natural-Color View on the left (Sx). 
The false-color view at right (Dx) was made by substituting an InfraRed image (centered at 938 nanometers) for the red color channel.

The views were acquired at a distance of approx. 613.000 miles (such as a little more than 986.000 Km) from Titan and the Image Scale is roughly 4 miles (such as approx. 6,437 Km) per pixel".
Parole chiave: Titan

Double Titan

Caption NASA:"These two views of Saturn's moon Titan exemplify how NASA's Cassini Spacecraft has revealed the Surface of this fascinating world.

Cassini carried several instruments to pierce the veil of hydrocarbon haze that enshrouds Titan. These include the Spacecraft's Radar and the Visual and InfraRed Mapping Spectrometer, or VIMS. The mission's imaging cameras also have several spectral filters sensitive to specific wavelengths of InfraRed Light that are able to make it through the Haze to the Surface and back into space. These "spectral windows" have enable the imaging cameras to map nearly the entire surface of Titan.

In addition to Titan's Surface, images from both the imaging cameras and VIMS have provided windows into the moon's ever-changing Atmosphere, chronicling the appearance and movement of Hazes and Clouds over the years. A large, bright and feathery band of Summer Clouds can be seen arcing across high Northern Latitudes in the view at right (Dx).

These views were obtained with the Cassini Spacecraft Narrow-Angle Camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the Natural-Color View on the left (Sx).
The false-color view at right (Dx) was made by substituting an InfraRed image (centered at 938 nanometers) for the red color channel.

The views were acquired at a distance of approx. 613.000 miles (such as a little more than 986.000 Km) from Titan and the Image Scale is roughly 4 miles (such as approx. 6,437 Km) per pixel".

Titan-W00074172-79-MF-EB-LXTT-IPF-3.jpg Titan-Regions-Belet_Region-PIA12647.jpg Titan-PIA21624.jpg Titan-MF-EB-LXTT-IPF.jpg Titan-PIA14913-0.jpg
Informazioni sul file
Nome del file:Titan-PIA21624.jpg
Nome album:MareKromium / Titan: The "Foggy" Moon
Valutazione (2 voti):55555(Mostra dettagli)
Parole chiave:Titan
Copyright:NASA/JPL-Caltech/Space Science Institute
Dimensione del file:727 KiB
Data di inserimento:Gen 23, 2020
Dimensioni:2024 x 1024 pixels
Visualizzato:139 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=31360
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