File:Rosette Nebula (noao-rosette mulligan).tiff
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editDescriptionRosette Nebula (noao-rosette mulligan).tiff |
English: The appropriately named Rosette nebula is, not unlike a newly bloomed flower, a place of newfound life. Many of the stars within this wreath of gas have just formed. Their energetic winds and emissions of UV radiation are quickly blowing away the surrounding clouds of gas to reveal a new cluster of stars. Many thicker parts of the cloud resist their ultimate demise, and remain in radial structures stubborn to relent to the impressive forces arrayed against them. The initial mass of gas clouds such as this determine how many stars are formed within. A very massive cloud will likely form many stars. Here, the stars in the heart of the Rosette nebula are blowing away the building blocks of more stars and have halted most other star formation. However, there are many globules of gas (Bok Globules) that may contain individual stars still in the process of forming. A high resolution image of one of these regions in Hydrogen-alpha light can be seen by looking at this detail image of the Rosette nebula.This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
Date | 12 June 2014 (upload date) |
Source | Rosette Nebula |
Author | KPNO/NOIRLab/NSF/AURA/Walter Mulligan/Flynn Haase |
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editThis 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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current | 17:18, 23 October 2023 | 1,800 × 1,299 (5.11 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-rosette_mulligan.tif via Commons:Spacemedia |
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Image title | The appropriately named Rosette nebula is, not unlike a newly bloomed flower, a place of newfound life. Many of the stars within this wreath of gas have just formed. Their energetic winds and emissions of UV radiation are quickly blowing away the surrounding clouds of gas to reveal a new cluster of stars. Many thicker parts of the cloud resist their ultimate demise, and remain in radial structures stubborn to relent to the impressive forces arrayed against them. The initial mass of gas clouds such as this determine how many stars are formed within. A very massive cloud will likely form many stars. Here, the stars in the heart of the Rosette nebula are blowing away the building blocks of more stars and have halted most other star formation. However, there are many globules of gas (Bok Globules) that may contain individual stars still in the process of forming. A high resolution image of one of these regions in Hydrogen-alpha light can be seen by looking at this detail image of the Rosette nebula. This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
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Camera manufacturer | ST-10 |
Width | 1,800 px |
Height | 1,299 px |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 48 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 19:47, 30 August 2021 |
Exif version | 2.31 |
Color space | sRGB |