ಮೂಲ ಕಡತ(೩,೬೦೦ × ೩,೬೦೦ ಚಿತ್ರಬಿಂದು, ಫೈಲಿನ ಗಾತ್ರ: ೧.೦೮ MB, MIME ಪ್ರಕಾರ: image/jpeg)

ಈ ಕಡತವು Wikimedia Commons ಇಂದ ಬಂದಿದ್ದು, ಬೇರೆ ಯೋಜನೆಗಳಲ್ಲೂ ಉಪಯೋಗಿಸಲ್ಪಡಬಹುದು. [ಕಡತ ವಿವರಣಾ ಪುಟ]ದಲ್ಲಿರುವ ವಿವರಣೆಯನ್ನು ಕೆಳಗೆ ಕೊಡಲಾಗಿದೆ.

ಸಾರಾಂಶ

ವಿವರ
English: These galaxy clusters are part of a large study using Chandra and Hubble that sets new limits on how dark matter - the mysterious substance that makes up most of the matter in the Universe - interacts with itself. The hot gas that envelopes the clusters glows brightly in X-rays detected by Chandra (pink). When combined with Hubble's visible light data, astronomers can map where the stars and hot gas are after the collision, as well as the inferred distribution of dark matter (blue) through the effect of gravitational lensing.

Creator: Chandra X-ray Observatory Center

Record URL: chandra.harvard.edu/photo/2015/dark/
ದಿನಾಂಕ
ಆಕರ Dark Matter is Darker Than Once Thought
ಕರ್ತೃ Smithsonian Institution from United States
ಅನುಮತಿ
(ಈ ಕಡತವನ್ನು ಮರುಬಳಕೆ ಮಾಡಲಾಗುತ್ತಿದೆ)
Smithsonian Institution @ Flickr Commons

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ಸೆಪ್ಟೆಂಬರ್ ೨೭, ೨೦೧೫

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Flickr user ID ಇಂಗ್ಲಿಷ್: 25053835@N03
author name string ಇಂಗ್ಲಿಷ್: Smithsonian Institution

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೯ ಮಾರ್ಚ್ 2015

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ಕಡತದ ಇತಿಹಾಸ

ದಿನ/ಕಾಲ ಒತ್ತಿದರೆ ಆ ಸಮಯದಲ್ಲಿ ಈ ಕಡತದ ವಸ್ತುಸ್ಥಿತಿ ತೋರುತ್ತದೆ.

ದಿನ/ಕಾಲಕಿರುನೋಟಆಯಾಮಗಳುಬಳಕೆದಾರಟಿಪ್ಪಣಿ
ಪ್ರಸಕ್ತ೧೮:೩೯, ೨೭ ಸೆಪ್ಟೆಂಬರ್ ೨೦೧೫೧೮:೩೯, ೨೭ ಸೆಪ್ಟೆಂಬರ್ ೨೦೧೫ ವರೆಗಿನ ಆವೃತ್ತಿಯ ಕಿರುನೋಟ೩,೬೦೦ × ೩,೬೦೦ (೧.೦೮ MB)Sumita Roy DuttaTransferred from Flickr via Flickr2Commons

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