चित्र:Dark Matter is Darker Than Once Thought (19057102495).jpg
यै पूर्व रुपको आकार: ६०० × ६०० पिक्सल। और रिजोल्युशनहरु: २४० × २४० पिक्सल • ४८० × ४८० पिक्सल • ७६८ × ७६८ पिक्सल • १,०२४ × १,०२४ पिक्सल • २,०४८ × २,०४८ पिक्सल • ३,६०० × ३,६०० पिक्सल।
खास फाइल (३,६०० × ३,६०० पिक्सेलहरु, फाइल आकार: १.०८ मेगाबाइट, MIME प्रकार: image/jpeg)
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सारांश:
| बेलिविस्तार |
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/ |
| मिति | |
| स्रोत | Dark Matter is Darker Than Once Thought |
| लेख्यामान्सु | Smithsonian Institution from United States |
| छुटकारा (यो चित्र पुनप्रयोग गद्द) |
Smithsonian Institution @ Flickr Commons |
आज्ञापत्र दिन्नाछ़
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More information can be found at https://flickr.com/commons/usage/. Please add additional copyright tags to this image if more specific information about copyright status can be determined. See Commons:Licensing for more information. |
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This image was originally posted to Flickr by Smithsonian Institution at https://flickr.com/photos/25053835@N03/19057102495. It was reviewed on २७ सेप्टेम्बर २०१५ by FlickreviewR and was confirmed to be licensed under the terms of the No known copyright restrictions. |
फाइल इतिहास
तिथि/बेलामी क्लिक अरि तैबेला(समय) यो फाइल कसो थ्यो भणी हेद्द सकिन्याछ ।
| तिथि/बेला | थम्बनेल | आयाम | प्रयोगकर्ता | टिप्पणी | |
|---|---|---|---|---|---|
| यैलको | १८:५४, २७ सेप्टेम्बर २०१५ | | ३,६०० × ३,६०० (१.०८ मेगाबाइट) | Sumita Roy Dutta | Transferred from Flickr via Flickr2Commons |
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निम्न और विकिहरुमि यै फाइलको प्रयोग:
- sd.wikipedia.org मि उपयोग
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