ስዕል:Dark Matter is Darker Than Once Thought (19057102495).jpg
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ዋና ፋይል (3,600 × 3,600 ፒክስል፤ መጠን፦ 1.08 MB፤ የMIME ዓይነት፦ image/jpeg)
ይህ ፋይል ከWikimedia Commons የተቀሰመ ነው እና በሌላ ዊኪ ላይ ሊጠቅም ይችላል። በhttps://commons.wikimedia.org/wiki/File:Dark_Matter_is_Darker_Than_Once_Thought_(19057102495).jpg ላይ የሚገኘው የፋይሉ መግለጫ ከዚህ በታች ቀርቧል።
ማጠቃለያ
ማጠቃለያDark Matter is Darker Than Once Thought (19057102495).jpg |
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/ |
ቀን | |
ምንጭ | Dark Matter is Darker Than Once Thought |
አቅራቢው | Smithsonian Institution from United States |
የማብዛት ፈቃድ (Reusing this file) |
Smithsonian Institution @ Flickr Commons |
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This image was taken from Flickr's The Commons. The uploading organization may have various reasons for determining that no known copyright restrictions exist, such as: No known copyright restrictionsNo restrictionshttps://www.flickr.com/commons/usage/false
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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 27 ሴፕቴምበር 2015 by FlickreviewR and was confirmed to be licensed under the terms of the No known copyright restrictions. |
27 ሴፕቴምበር 2015
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9 ማርች 2015
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የቀድሞው ዕትም ካለ ቀን/ሰዓቱን በመጫን መመልከት ይቻላል።
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ያሁኑኑ | 13:09, 27 ሴፕቴምበር 2015 | 3,600 × 3,600 (1.08 MB) | Sumita Roy Dutta | Transferred from Flickr via Flickr2Commons |
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ይህ ፋይል በውስጡ ተጨማሪ መረጃ ይይዛል። መረጃውም በዲጂታል ካሜራ ወይም በኮምፒውተር ስካነር የተጨመረ ይሆናል። ይህ ከኦሪጂናሉ ቅጅ የተለወጠ ከሆነ፣ ምናልባት የመረጃው ዝርዝር ለውጦቹን የማያንጸባረቅ ይሆናል።
JPEG file comment | 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. |
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