File:IC 1396 Portion (noao-ic1396tan).tiff
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![File:IC 1396 Portion (noao-ic1396tan).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/6/63/IC_1396_Portion_%28noao-ic1396tan%29.tiff/lossy-page1-800px-IC_1396_Portion_%28noao-ic1396tan%29.tiff.jpg?20231023172809)
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IC 1396 is another region full of molecular hydrogen gas and recent star formation.
Summary
[edit]DescriptionIC 1396 Portion (noao-ic1396tan).tiff |
English: IC 1396 is another region full of molecular hydrogen gas and recent star formation. Many stars in this area are less than a couple hundred thousand years old - very young in the grand scheme of astronomy, where stars live to be billions of years old! The hot young stars are in the process of ionizing and expelling the molecular hydrogen gas. At the same time, new stars are still being born in this nebula. For more information, check out this fantastic APOD taken in early 2014.This image was taken as part of Advanced Observing Program (AOP) program during 2014 at Kitt Peak Visitor Center. |
Date | 6 June 2014, 09:40:00 (upload date) |
Source | IC 1396 Portion |
Author | KPNO/NOIRLab/NSF/AURA/Johannes Tan/Adam Block |
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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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current | 17:28, 23 October 2023 | ![]() | 2,100 × 1,450 (6.53 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-ic1396tan.tif via Commons:Spacemedia |
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Image title | IC 1396 is another region full of molecular hydrogen gas and recent star formation. Many stars in this area are less than a couple hundred thousand years old - very young in the grand scheme of astronomy, where stars live to be billions of years old! The hot young stars are in the process of ionizing and expelling the molecular hydrogen gas. At the same time, new stars are still being born in this nebula. For more information, check out this fantastic APOD taken in early 2014. This image was taken as part of Advanced Observing Program (AOP) program during 2014 at Kitt Peak Visitor Center. |
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Camera manufacturer | ST-10 |
Width | 2,100 px |
Height | 1,450 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 | 41 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 16:21, 30 August 2021 |
Exif version | 2.31 |
Color space | sRGB |
Structured data
image/tiff
1,450 pixel
2,100 pixel
6,842,250 byte
776309d83e8da16c8ab7de0cc234edb32fce5278
6 June 2014
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