Datei:M51 (MIRI image) (potm2308c).jpg
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Beschreibung
BeschreibungM51 (MIRI image) (potm2308c).jpg |
English: The graceful winding arms of the grand-design spiral galaxy M51 stretch across this image from the NASA/ESA/CSA James Webb Space Telescope. Unlike the menagerie of weird and wonderful spiral galaxies with ragged or disrupted spiral arms, grand-design spiral galaxies boast prominent, well-developed spiral arms like the ones showcased in this image. This galactic portrait was captured by Webb’s Mid-InfraRed Instrument (MIRI).In this image the reprocessed stellar light by dust grains and molecules in the medium of the galaxy illuminate a dramatic filamentary medium. Empty cavities and bright filaments alternate and give the impression of ripples propagating from the spiral arms. The yellow compact regions indicate the newly formed star clusters in the galaxy.M51 — also known as NGC 5194 — lies about 27 million light-years away from Earth in the constellation Canes Venatici, and is trapped in a tumultuous relationship with its near neighbour, the dwarf galaxy NGC 5195. The interaction between these two galaxies has made these galactic neighbours one of the better-studied galaxy pairs in the night sky. The gravitational influence of M51’s smaller companion is thought to be partially responsible for the stately nature of the galaxy’s prominent and distinct spiral arms. If you would like to learn more about this squabbling pair of galactic neighbours, you can explore earlier observations of M51 by the NASA/ESA Hubble Space Telescope here. This Webb observation of M51 is one of a series of observations collectively titled Feedback in Emerging extrAgalactic Star clusTers, or FEAST. The FEAST observations were designed to shed light on the interplay between stellar feedback and star formation in environments outside of our own galaxy, the Milky Way. Stellar feedback is the term used to describe the outpouring of energy from stars into the environments which form them, and is a crucial process in determining the rates at which stars form. Understanding stellar feedback is vital to building accurate universal models of star formation.The aim of the FEAST observations is to discover and study stellar nurseries in galaxies beyond our own Milky Way. Before Webb became operative, other observatories such as the Atacama Large Millimetre Array in the Chilean desert and Hubble have given us a glimpse of star formation either at the onset (tracing the dense gas and dust clouds where stars will form) or after the stars have destroyed with their energy their natal gas and dust clouds. Webb is opening a new window into the early stages of star formation and stellar light, as well as the energy reprocessing of gas and dust. Scientists are seeing star clusters emerging from their natal cloud in galaxies beyond our local group for the first time. They will also be able to measure how long it takes for these stars to pollute with newly formed metals and to clean out the gas (these time scales are different from galaxy to galaxy). By studying these processes, we will better understand how the star formation cycle and metal enrichment are regulated within galaxies as well as what are the time scales for planets and brown dwarfs to form. Once dust and gas is removed from the newly formed stars, there is no material left to form planets.[Image Description: A large spiral galaxy takes up the entirety of the image. The core is mostly bright white, but there are also swirling, detailed structures that resemble water circling a drain. There is white and pale blue light that emanates from stars and dust at the core’s centre, but it is tightly limited to the core. The detailed rings feature bands of deep orange and cloudy grey, which are interspersed by darker empty regions throughout.]Links |
Datum | 29. August 2023 (Hochladedatum) |
Quelle | M51 (MIRI image) |
Urheber | ESA/Webb, NASA & CSA, A. Adamo (Stockholm University) and the FEAST JWST team |
Andere Versionen |
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Lizenz
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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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Namensnennung: ESA/Webb, NASA & CSA, A. Adamo (Stockholm University) and the FEAST JWST team
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The graceful winding arms of the grand-design spiral galaxy M51 stretch across this image from the NASA/ESA/CSA James Webb Space Telescope.
L'une des galaxies de M51, prise par l'instrument MIRI du télescope spatial James Webb.
In dieser Datei abgebildete Objekte
Motiv
image/jpeg
1.551 Pixel
4.137 Pixel
2.997.301 Byte
b01f2ec7685263de69ef731f457eedd271cddd45
29. August 2023
pHash checksum Englisch
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aktuell | 12:00, 29. Aug. 2023 | ![]() | 4.137 × 1.551 (2,86 MB) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esawebb.org/archives/images/large/potm2308c.jpg via Commons:Spacemedia |
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Metadaten
Diese Datei enthält weitere Informationen (beispielsweise Exif-Metadaten), die in der Regel von der Digitalkamera oder dem verwendeten Scanner stammen. Durch nachträgliche Bearbeitung der Originaldatei können einige Details verändert worden sein.
Quelle | ESA/Webb |
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Namensnennung/Veröffentlicher | ESA/Webb, NASA & CSA, A. Adamo (Stockholm University) and the FEAST JWST team |
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Bildtitel |
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Nutzungsbedingungen |
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Erfassungszeitpunkt | 10:00, 29. Aug. 2023 |
Software | Adobe Photoshop 24.7 (Windows) |
Speicherzeitpunkt | 16:10, 22. Aug. 2023 |
Digitalisierungszeitpunkt | 20:03, 4. Aug. 2023 |
Datum, zu dem die Metadaten letztmalig geändert wurden | 18:10, 22. Aug. 2023 |
Eindeutige Kennung des ursprünglichen Dokuments | xmp.did:4d454c70-acf3-c042-b5d0-1b465b0af6a7 |
Kontaktinformationen |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM-Version | 4 |
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