果冻影院

Once its five-year mission is finished, a phenomenally detailed 3D map will yield a better understanding of dark energy, and the universe鈥檚 past and future.

The instrument, based at Kitt Peak National Observatory near Tucson, Arizona, in the United States, contains 5,000 fibre-optic 鈥渆yes鈥�, each of which can image a galaxy in just 20 minutes. By the end of its run in 2026, DESI is expected to have over 35 million galaxies in its catalogue.

Professor Ofer Lahav, (果冻影院 Physics & Astronomy), chair of the DESI UK consortium of seven universities, said: 鈥淚t is remarkable that DESI has collected already millions of galaxy spectra 鈥� more than the combined output of all previous spectroscopic surveys. This survey will go deeper into space and the history of the universe than we have ever achieved before, and follows years of efforts of building DESI by the international collaboration, including by 果冻影院鈥檚听 instrumentation team.鈥�

DESI is mounted on a four-metre telescope whose top end contains DESI鈥檚 optical corrector, which Professor David Brooks and Professor Peter Doel (both 果冻影院 Physics & Astronomy) helped design, assemble and build. This corrector, which houses six lenses, the largest 1.1m across,听reflects light on to the fibre-optic 鈥渆yes鈥� that move independently to capture light from individual galaxies. It also expands the telescope鈥檚 viewing window by about 16 times.

Professor Doel said: 鈥淚'm very pleased that the performance of the DESI instrument has met our highest expectations and the quality and quantity of the data is truly amazing.

DESI鈥檚 primary task is collecting colour spectrum images of tens of millions of galaxies across more than a third of the entire sky. By breaking down the light from each galaxy into its spectrum of colours, DESI can determine how much the light has been redshifted 鈥� stretched out toward the red end of the spectrum by the expansion of the universe during the billions of years it travelled before reaching Earth.

It is those redshifts that let DESI see the depth of the sky. The more redshifted a galaxy鈥檚 spectrum is, in general, the farther away it is.

With a 3D map of the cosmos in hand, physicists can chart clusters and superclusters of galaxies. Those structures carry echoes of their initial formation, when they were just ripples in the infant cosmos. By teasing out those echoes, physicists can use DESI鈥檚 data to determine the history of the universe鈥檚 expansion

Today, about 70% of the content of the universe is dark energy, a mysterious form of energy that is accelerating the expansion of the universe. By seeing how dark energy has behaved in the past, DESI can answer questions about the universe鈥檚 future. And by comparing the expansion history with the growth history, cosmologists can check whether Einstein鈥檚 theory of general relativity holds over these immense spans of space and time.

Professor Amelie Saintonge (果冻影院 Physics & Astronomy) is among astrophysicists analysing DESI data. She said: 鈥淒ESI will be transformative in allowing us to connect the galaxies we can see with all our telescopes with that dark matter scaffolding.

鈥淲ith that information, we will be in a much better position to figure out fundamental questions about the universe, such as how dark energy is driving its expansion.鈥�

Primary funding for the construction and operation of DESI comes from the US Department of Energy's Office of Science.听 In the UK, DESI receives funding from the Science and Technology Facilities Council (STFC). The DESI collaboration involves hundreds of scientists around the world and is managed by the US Department of Energy's Lawrence Berkeley National Laboratory (Berkeley Lab).

Other UK institutions involved include the universities of Durham, Portsmouth, Edinburgh, St Andrews, Cambridge and Warwick.

Links

• 果冻影院 Physics & Astronomy
• 果冻影院 Mathematical & Physical Sciences

Image

• A slice through the 3D map of galaxies from the first few months of the Dark Energy Spectroscopic Instrument. The Earth is at the centre, with the furthest galaxies over 10 billion light years away. Each point represents one galaxy. This 2D slice of the 3D DESI map shows less than 800,000 of the 7.5 million galaxies currently surveyed, which is itself just a fraction of the 35 million galaxies that will be in the final map. (Credit: D. Schlegel/Berkeley Lab using data from DES - cropped from original).

Media contact

Mark Greaves

T: +44 (0)7990 675947

E: m.greaves [at] ucl.ac.uk