stsci_2018-56a December 20th, 2018
Credit: NASA, ESA, and M. Montes (University of New South Wales) Acknowledgment: J. Lotz (STScI) and the HFF team
Utilizing the powerful Hubble Frontier Fields observations of galaxy clusters, a study demonstrates that intracluster light — the light of stars orphaned in galaxy cluster mergers — aligns with dark matter, tracing its distribution more accurately than other methods. With broader use, astronomers think the technique could be a first step in exploring the nature of the unobservable, elusive dark matter that makes up the majority of the universe.
Provider: Space Telescope Science Institute
Image Source: https://hubblesite.org/contents/news-releases/2018/news-2018-56
Curator: STScI, Baltimore, MD, USA
Image Use Policy: http://hubblesite.org/copyright/
| Telescope | Spectral Band | Wavelength | |
|---|---|---|---|
|
Hubble (ACS/WFC) | Optical (B) | 435.0 nm |
|
Hubble (ACS/WFC) | Optical (V) | 606.0 nm |
|
Hubble (ACS/WFC) | Optical (R) | 814.0 nm |
|
Hubble (WFC3/IR) | Infrared (Y) | 1.1 µm |
|
Hubble (WFC3/IR) | Infrared (J) | 1.3 µm |
|
Hubble (WFC3/IR) | Infrared (JH) | 1.4 µm |
|
Hubble (WFC3/IR) | Infrared (H) | 1.6 µm |
Detailed color mapping information coming soon...
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