File:RMC 136 (gemini-2013-rmc136-legacy).tiff
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Size of this JPG preview of this TIF file: 618 × 600 pixels. Other resolutions: 247 × 240 pixels | 495 × 480 pixels | 792 × 768 pixels | 1,055 × 1,024 pixels | 2,111 × 2,048 pixels | 4,611 × 4,474 pixels.
Original file (4,611 × 4,474 pixels, file size: 39.79 MB, MIME type: image/tiff)
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[edit]DescriptionRMC 136 (gemini-2013-rmc136-legacy).tiff |
English: This near-infrared image obtained with GeMS adaptive optics system resolves the stars inside RMC 136, a giant star cluster within the Tarantula Nebula in the Large Magellanic Cloud. The cluster produces most of the energy that energizes the Tarantula Nebula. The estimated mass of the cluster is about half a million times the mass of the sun, suggesting it will probably become a globular cluster in the future. |
Date | 30 June 2020, 21:55:00 (upload date) |
Source | RMC 136 |
Author | International Gemini Observatory, Robert Blum (National Optical Astronomy Observatory) and T.A. Rector (University of Alaska Anchorage) |
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[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.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 21:25, 2 September 2023 | 4,611 × 4,474 (39.79 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/gemini-2013-rmc136-legacy.tif via Commons:Spacemedia |
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Image title | This near-infrared image obtained with GeMS adaptive optics system resolves the stars inside RMC 136, a giant star cluster within the Tarantula Nebula in the Large Magellanic Cloud. The cluster produces most of the energy that energizes the Tarantula Nebula. The estimated mass of the cluster is about half a million times the mass of the sun, suggesting it will probably become a globular cluster in the future. |
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Author | Gemini Observatory/AURA |
Width | 4,611 px |
Height | 4,474 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 18 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS6 (Macintosh) |
File change date and time | 11:04, 12 June 2013 |
Exif version | 2.21 |
Color space | sRGB |