File:Webb captures detailed beauty of Ring Nebula (NIRCam and MIRI images) (weic2320a).jpg
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Summary
DescriptionWebb captures detailed beauty of Ring Nebula (NIRCam and MIRI images) (weic2320a).jpg |
English: The NASA/ESA/CSA James Webb Space Telescope has observed the well-known Ring Nebula with unprecedented detail. Formed by a star throwing off its outer layers as it runs out of fuel, the Ring Nebula is an archetypal planetary nebula. Also known as M57 and NGC 6720, it is both relatively close to Earth at roughly 2,500 light-years away.The new images provide unprecedented spatial resolution and spectral sensitivity, which also reveal unique details across both infrared observations. For example, the new image from Webb’s NIRCam (Near-InfraRed Camera) shows the intricate details of the filament structure of the inner ring (left), while the new image from Webb’s MIRI (Mid-InfraRed Instrument) reveals particular details in the concentric features in the outer regions of the nebulae’s ring (right).There are some 20,000 dense globules in the nebula, which are rich in molecular hydrogen. In contrast, the inner region shows very hot gas. The main shell contains a thin ring of enhanced emission from carbon-based molecules known as polycyclic aromatic hydrocarbons (PAHs). Roughly ten concentric arcs are located just beyond the outer edge of the main ring. The arcs are thought to originate from the interaction of the central star with a low-mass companion orbiting at a distance comparable to that between the Earth and the dwarf planet Pluto. In this way, nebulae like the Ring Nebula reveal a kind of astronomical archaeology, as astronomers study the nebula to learn about the star that created it.[Image description: This visual shows two images side by side of the Ring Nebula. The image on the left shows Webb’s NIRCam view and the image on the right shows Webb’s MIRI image. The left image shows the planetary nebula as a distorted donut with a rainbow of colours with a blue/green inner cavity and clear filamental structure in the inner region of the ring. The right image shows the nebula with a red/orange central cavity with a ring structure that transitions from colours of yellow to purple/blue.] |
Date | 21 August 2023 (upload date) |
Source | Webb captures detailed beauty of Ring Nebula (NIRCam and MIRI images) |
Author | ESA/Webb, NASA, CSA, M. Barlow, N. Cox, R. Wesson |
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ESA/Webb images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the webbtelescope.org website, use the {{PD-Webb}} tag.
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Attribution: ESA/Webb, NASA, CSA, M. Barlow, N. Cox, R. Wesson
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Captions
The NASA/ESA/CSA James Webb Space Telescope has observed the well-known Ring Nebula with unprecedented detail. Formed by a star throwing off its outer layers as it runs out of fuel, the Ring Nebula is an archetypal planetary nebula.
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image/jpeg
3,428 pixel
4,097 pixel
2,857,986 byte
12bda2f4b0779c52801e7d2348618ec90693edef
21 August 2023
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 10:01, 22 August 2023 | ![]() | 4,097 × 3,428 (2.73 MB) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esawebb.org/archives/images/large/weic2320a.jpg via Commons:Spacemedia |
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Metadata
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Source | ESA/Webb |
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Credit/Provider | ESA/Webb, NASA, CSA, M. Barlow, N. Cox, R. Wesson |
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Date and time of data generation | 16:00, 21 August 2023 |
Software used | Adobe Photoshop 24.4 (Windows) |
File change date and time | 14:52, 15 August 2023 |
Date and time of digitizing | 10:45, 3 August 2023 |
Date metadata was last modified | 16:52, 15 August 2023 |
Unique ID of original document | xmp.did:f7a9539d-3295-ba48-a823-46a275445401 |
Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |