ESA Hubble Science Release | 2015 Mar 26
Astronomers using observations from the NASA/ESA Hubble Space Telescope and NASA’s Chandra X-ray Observatory have studied how dark matter in clusters of galaxies behaves when the clusters collide. The results, published in the journal Science on 27 March 2015, show that dark matter interacts with itself even less than previously thought, and narrows down the options for what this mysterious substance might be.
- [url=http://www.spacetelescope.org/images/heic1506h/][b][i]Collage of six cluster collisions, with dark-matter maps and X-ray data[/i][/b][/url] [b][i]Credit: X-ray: NASA/CXC/Ecole Polytechnique Federale de Lausanne, Switzerland/D.Harvey & NASA/CXC/Durham Univ/R.Massey; Optical & Lensing Map: NASA, ESA, D. Harvey (Ecole Polytechnique Federale de Lausanne, Switzerland) and R. Massey (Durham University, UK)[/i][/b]
Dark matter is a giant question mark looming over our knowledge of the Universe. There is more dark matter in the Universe than visible matter, but it is extremely elusive; it does not reflect, absorb or emit light, making it invisible. Because of this, it is only known to exist via its gravitational effects on the visible Universe (heic1215a).
To learn more about this mysterious substance, researchers can study it in a way similar to experiments on visible matter — by watching what happens when it bumps into things. For this reason, researchers look at vast collections of galaxies, called galaxy clusters, where collisions involving dark matter happen naturally and where it exists in vast enough quantities to see the effects of collisions. ...
Dark Matter Is Not as Sticky as Once Thought
NASA | STScI | HubbleSite | 2015 Mar 26
Dark Matter is Darker Than Once Thought
NASA | MSFC | SAO | Chandra | 2015 Mar 26
The nongravitational interactions of dark matter in colliding galaxy clusters - David Harvey et al
- Science 347(6229) 1462 (27 Mar 2015) DOI: 10.1126/science.1261381
arXiv.org > astro-ph > arXiv:1503.07675 > 26 Mar 2015