File:Infrared images of Titan (geminiann08014a).jpg
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
Infrared_images_of_Titan_(geminiann08014a).jpg (500 × 421 pixels, file size: 69 KB, MIME type: image/jpeg)
File information
Structured data
Captions
Summary[edit]
DescriptionInfrared images of Titan (geminiann08014a).jpg |
English: Infrared images of Titan observed on Feb. 2, 7, and 8, 2006 with the Near-infrared Integral Field Spectrograph (NIFS) on Gemini North. The images in the first row (a) are at 2.027-2.037 microns, where Titan’s atmosphere is nearly transparent and surface features are thought to be revealed clearly The second row of images (b) cover 2.060 -2.070 microns, where the atmosphere is less transparent and absorption by haze and liquid methane could be influential). The images in the third row (c), made from a Mercator map of observations by the Visual and Infrared Mapping Spectrometer (VIMS) (Barnes et al. 2008) correspond to views of the surface of Titan from Earth at the times of the Gemini observations. Major geologic features (marked by A, B, C, D, E, and F) on the NIFS images are seen to occur at the same places on the VIMS images. The pairs of images in the top two rows illustrate the difficulty of detecting temporal atmospheric effects such as variable haze and localized methane drizzle. |
Date | 16 May 2008 (upload date) |
Source | Infrared images of Titan |
Author | International Gemini Observatory/NOIRLab/NSF/AURA |
Other versions |
|
Licensing[edit]
This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 22:45, 23 October 2023 | 500 × 421 (69 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann08014a.jpg via Commons:Spacemedia |
You cannot overwrite this file.
File usage on Commons
The following page uses this file:
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Credit/Provider | International Gemini Observatory/NOIRLab/NSF/AURA |
---|---|
Source | NSF's NOIRLab |
Short title |
|
Image title |
|
Usage terms |
|
Date and time of data generation | 05:00, 16 May 2008 |
JPEG file comment | Infrared images of Titan observed on Feb. 2, 7, and 8, 2006 with the Near-infrared Integral Field Spectrograph (NIFS) on Gemini North. The images in the first row (a) are at 2.027-2.037 microns, where Titan’s atmosphere is nearly transparent and surface features are thought to be revealed clearly The second row of images (b) cover 2.060 -2.070 microns, where the atmosphere is less transparent and absorption by haze and liquid methane could be influential). The images in the third row (c), made from a Mercator map of observations by the Visual and Infrared Mapping Spectrometer (VIMS) (Barnes et al. 2008) correspond to views of the surface of Titan from Earth at the times of the Gemini observations. Major geologic features (marked by A, B, C, D, E, and F) on the NIFS images are seen to occur at the same places on the VIMS images. The pairs of images in the top two rows illustrate the difficulty of detecting temporal atmospheric effects such as variable haze and localized methane drizzle. |
Software used | GIMP 2.10.18 |
File change date and time | 14:02, 10 August 2020 |
Keywords | Titan (moon) |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |