File:NGC4495 - Iotw2241a.jpg
Size of this preview: 800 × 589 pixels. Other resolutions: 320 × 236 pixels | 640 × 471 pixels | 1,024 × 754 pixels | 1,280 × 943 pixels | 2,035 × 1,499 pixels.
Original file (2,035 × 1,499 pixels, file size: 1.28 MB, MIME type: image/jpeg)
Summary
DescriptionNGC4495 - Iotw2241a.jpg | English: The constellation Coma Berenices hosts the galaxy NGC 4495 among myriad other astronomical objects. This galaxy has a tumultuous history: several supernovae have been recorded over the years, including the three named 1994S, 2010lo, and 2011ca. This last burst of energy from a dying star can be triggered by a number of different processes. 1994S, for example, was triggered by interactions between a white dwarf and another star, which reignited the core of the stellar remnant— a Type Ia supernova. 2011ca on the other hand is a Type Ic supernova, triggered by the core collapse of a single massive star. This image was captured by the DOE-built Dark Energy Camera (DECam) on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) as partof the DESI Legacy Imaging Surveys. The DESI Legacy Imaging Surveys were conducted to identify targets for the Dark Energy Spectroscopic Instrument (DESI) operations. These surveys comprise a unique blend of three projects that have observed a third of the night sky. DESI is an international sciencecollaboration managed by the US Department of Energy's (DOE) Lawrence Berkeley National Laboratory with primary funding for construction and operations from DOE’s Office of Science. |
Date | |
Source | https://noirlab.edu/public/images/iotw2241a/ |
Author |
Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA Image processing: Travis Rector (University of Alaska Anchorage/NSF’s NOIRLab), Jen Miller (Gemini Observatory/NSF’s NOIRLab), Mahdi Zamani & Davide de Martin (NSF’s NOIRLab) |
Other versions |
|
Licensing
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.
|
Items portrayed in this file
depicts
copyright status
copyrighted
copyright license
Creative Commons Attribution-ShareAlike 4.0 International
Creative Commons Attribution 4.0 International
media type
image/jpeg
checksum
0fd9bb5ce06fadb568bf7bbcb7f3cbb098d6b282
determination method or standard: SHA-1
data size
1,340,756 byte
height
1,499 pixel
width
2,035 pixel
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:22, 13 October 2022 | 2,035 × 1,499 (1.28 MB) | Fabian RRRR | Uploaded a work by Noirlab from Noirlab with UploadWizard |
File usage
The following 2 pages use this file:
Global file usage
The following other wikis use this file:
- Usage on de.wikipedia.org
Metadata
This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
If the file has been modified from its original state, some details may not fully reflect the modified file.
Credit/Provider | Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA Image processing: Travis Rector (University of Alaska Anchorage/NSF’s NOIRLab), Jen Miller (Gemini Observatory/NSF’s NOIRLab), Mahdi Zamani & Davide de Martin (NSF’s NOIRLab) |
---|---|
Source | NSF's NOIRLab |
Short title |
|
Image title |
|
Usage terms |
|
Date and time of data generation | 12:00, 12 October 2022 |
JPEG file comment | The constellation Coma Berenices hosts the galaxy NGC 4495 among myriad other astronomical objects. This galaxy has a tumultuous history: several supernovae have been recorded over the years, including the three named 1994S, 2010lo, and 2011ca. This last burst of energy from a dying star can be triggered by a number of different processes. 1994S, for example, was triggered by interactions between a white dwarf and another star, which reignited the core of the stellar remnant — a Type Ia supernova. 2011ca on the other hand is a Type Ic supernova, triggered by the core collapse of a single massive star. This image was captured by the DOE-built Dark Energy Camera (DECam) on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) as part of the DESI Legacy Imaging Surveys. The DESI Legacy Imaging Surveys were conducted to identify targets for the Dark Energy Spectroscopic Instrument (DESI) operations. These surveys comprise a unique blend of three projects that have observed a third of the night sky. DESI is an international science collaboration managed by the US Department of Energy's (DOE) Lawrence Berkeley National Laboratory with primary funding for construction and operations from DOE’s Office of Science. |
Software used | Adobe Photoshop 23.5 (Windows) |
Date and time of digitizing | 19:34, 19 March 2021 |
Date metadata was last modified | 23:10, 11 October 2022 |
File change date and time | 23:10, 11 October 2022 |
Unique ID of original document | xmp.did:4bda2c66-a9d0-4841-89af-a07e6e77135a |
Keywords | NGC 4495 |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |