Revealing a filament from the cosmic web
Is there an invisible web of dark matter surrounding us? Its influence can be observed across the cosmos, but the web remains unseen… for the most part. This Picture of the Week shows the clearest image yet of a filament from this cosmic web. The filament was imaged with ESO’s Very Large Telescope, and is shown here in purple overlaid on a background image from the NASA/ESA Hubble Space Telescope. Made of gas clumped together by the influence of dark matter, the filament stretches out for 3 million light-years, connecting two distant galaxies in the early Universe.
Around 85% of all matter in the Universe is actually dark matter. Dark matter is invisible, but the gas around it is not. This gas glows extremely faintly though, making these structures very difficult to observe. But after about 150 hours of observations, a team of astronomers led by Davide Tornotti, a PhD student at the University of Milano-Bicocca in Italy, managed to take this sharp image of a cosmic filament. This was possible thanks to the exceptional sensitivity of the MUSE instrument at the VLT, which has become a workhorse instrument at imaging the cosmic web.
The light from this filament took 11 billion years to reach us, and it shows exactly what theory predicted. In the early Universe, filaments of dark matter could have created a large web that entangled gas through their gravitational pull. Once gas accumulated at the intersection between filaments, it would have provided the fuel necessary to form galaxies. As we observe more of these mysterious filaments, what else will we find trapped within this dark web?
Links
Credit:ESO/D. Tornotti et al./Hubble: M. Revalski, P. Francis et al.
About the Image
Id: | potw2504a |
Type: | Observation |
Release date: | 29 January 2025, 11:00 |
Size: | 1945 x 1915 px |
About the Object
Type: | Early Universe : Cosmology : Morphology : Large-Scale Structure Early Universe : Cosmology : Phenomenon : Dark Matter |
Constellation: | Grus |
Category: | Cosmology |
Wallpapers
Coordinates
Position (RA): | 21 42 25.54 |
Position (Dec): | -44° 19' 48.20" |
Field of view: | 1.95 x 1.92 arcminutes |
Orientation: | North is 35.4° left of vertical |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical Ly-alpha (redshifted) | 513 nm | Very Large Telescope MUSE |
Ultraviolet F336W | 335 nm | Hubble Space Telescope WFC3 |
Optical F450W | 448 nm | Hubble Space Telescope WFPC2 |
Optical F702W | 681 nm | Hubble Space Telescope WFPC2 |
Infrared F125W+F140W | 130 nm | Hubble Space Telescope WFC3 |