File:Diagrama de Hubble para Supernova (noirlab2401h).jpg
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DescriptionDiagrama de Hubble para Supernova (noirlab2401h).jpg |
English: La historia de la expansión del Universo se puede rastrear mediante la comparación de velocidades de recesión (corrimiento al rojo) con las distancias determinadas para cada supernova. Los resultados del Estudio de Energía Oscura muestran que la expansión se ha ido acelerando con el tiempo cósmico, la firma de energía oscura. |
Date | 8 January 2024 (upload date) |
Source | Diagrama de Hubble para Supernova |
Author | NOIRLab |
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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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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 08:05, 9 January 2024 | 16,000 × 9,000 (9.78 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/noirlab2401h.jpg via Commons:Spacemedia |
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Source | NSF's NOIRLab |
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Credit/Provider | NOIRLab |
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Date and time of data generation | 13:00, 8 January 2024 |
Software used | Adobe Illustrator 28.0 (Macintosh) |
File change date and time | 23:41, 4 January 2024 |
Date and time of digitizing | 09:49, 20 December 2023 |
Date metadata was last modified | 00:41, 5 January 2024 |
Unique ID of original document | uuid:65E6390686CF11DBA6E2D887CEACB407 |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |
IIM version | 4 |