Natisinahikaniwoc:Dark Matter is Darker Than Once Thought (19057102495).jpg
E irikweckwemakisitc600 x 600 pixels Kotak erikokowactepiriki: 240 x 240 pixels | 480 x 480 pixels | 768 x 768 pixels | 1 024 x 1 024 pixels | 2 048 x 2 048 pixels | 3 600 x 3 600 pixels.
E otciparik masinahikaniwoc (3 600x3 600pixels, e irikweckamikak mawtockwemikan:1,08 Mionohwe MIME:image/jpeg)
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Nosem
| E witcikemakak |
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/ |
| Apitc | |
| Ite wetciparik | Dark Matter is Darker Than Once Thought |
| Ka ki masihiketc | Smithsonian Institution from United States |
| Niheritam (E koski apatak masinihikaniwoc) |
Smithsonian Institution @ Flickr Commons |
Orocowatcikan
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Cette image a été originellement postée sur Flickr par Smithsonian Institution à l'adresse https://flickr.com/photos/25053835@N03/19057102495. Elle a été passée en revue le 27 Kakone pisimw 2015 par le robot FlickreviewR, qui a confirmé qu'elle se trouvait sous licence No known copyright restrictions. |
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Ota ici nta makona e tatokonikisitc acitc e tato tipahikaneak kitci wapataman apitc ka masinatek.
| E tatokonakisitc acitc e tato tipahikaneak | Masinasowinicic | E iskwaki | Ka mitatc | E iteritaman | |
|---|---|---|---|---|---|
| mekwatc | 27 Kakone pisimw 2015 à 08:09 | | 3 600 × 3 600 (1,08 Mio) | Sumita Roy Dutta | Transferred from Flickr via Flickr2Commons |
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