File:NGC4496 Potw2209a.jpg
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Summary
[edit]DescriptionNGC4496 Potw2209a.jpg |
English: The twin galaxies NGC 4496A and NGC 4496B dominate the frame in this image from the NASA/ESA Hubble Space Telescope. Both galaxies lie in the constellation Virgo, but despite appearing side-by-side in this image they are at vastly different distances from both Earth and one another. NGC 4496A is 47 million light-years from Earth while NGC 4496B is 212 million light-years away. The enormous distances between the two galaxies mean that the two cannot interact, and they only appear to overlap owing to a chance alignment. Chance galactic alignments such as this provide astronomers with the opportunity to delve into the distribution of dust in these galaxies. Galactic dust adds to the beauty of astronomical images — it can be seen in this image as the dark tendrils threading through both NGC 4496A and NGC 4496B —but it also complicates astronomers’ observations. Dust absorbs starlight, making stars seem dimmer and shifting their light towards longer wavelengths, a process that astronomers refer to as “reddening” (not the same thing as redshift). By carefully measuring how starlight from background galaxies is affected by dust in intervening galaxies, astronomers can map out where the dust is in the foreground galaxy’s spiral arms. The resulting “dust maps” help astronomers calibrate measurements of everything from cosmological distances to the types of stars populating galaxies.
Coordinates Position (RA): 12 31 39.34 Position (Dec): 3° 55' 41.10" Field of view: 2.61 x 2.63 arcminutes Orientation: North is 3.8° left of vertical Colours & filters Band Wavelength Telescope Optical u 354 nm SDSS Optical G 474 nm Víctor M. Blanco 4-meter Telescope DECam Optical G 477 nm SDSS Optical R 623 nm SDSS Optical R 644 nm Víctor M. Blanco 4-meter Telescope DECam Optical I 762 nm SDSS Optical Z 913 nm SDSS Optical Z 919 nm Víctor M. Blanco 4-meter Telescope DECam Optical V 606 nm Hubble Space Telescope WFC3. |
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Source | https://esahubble.org/images/potw2209a/ | |||
Author | ESA/Hubble & NASA, T. Boeker, B. Holwerda, Dark Energy Survey, DOE, FNAL/DECam, CTIO/NOIRLab/NSF/AURA, SDSS | |||
Permission (Reusing this file) |
This file is licensed under the Creative Commons Attribution 4.0 International license. Attribution: Credit:
ESA/Hubble & NASA, J. Dalcanton, Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA
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current | 10:01, 21 January 2023 | 3,944 × 3,977 (4.71 MB) | Loopjaw (talk | contribs) | Uploaded a work by ESA/Hubble & NASA, T. Boeker, B. Holwerda, Dark Energy Survey, DOE, FNAL/DECam, CTIO/NOIRLab/NSF/AURA, SDSS from https://esahubble.org/images/potw2209a/ with UploadWizard |
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Source | ESA/Hubble |
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Credit/Provider | ESA/Hubble & NASA, T. Boeker, B. Holwerda, Dark Energy Survey, DOE, FNAL/DECam, CTIO/NOIRLab/NSF/AURA, SDSS Acknowledgement: R. Colombari |
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Date and time of data generation | 06:00, 28 February 2022 |
Software used | Adobe Photoshop 23.0 (Windows) |
File change date and time | 15:50, 23 February 2022 |
Date and time of digitizing | 11:43, 5 January 2022 |
Date metadata was last modified | 16:50, 23 February 2022 |
Unique ID of original document | xmp.did:a99202ba-e0d3-3049-9225-8a36d8a48906 |
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Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |