Skip to main content

Thank you for visiting You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.


New eyes on the Universe


This month marks the start of the Dark Energy Spectroscopic Instrument (DESI) survey, which will be mapping the distance to 35 million galaxies and 2.4 million quasars across one-third of the sky over the next 5 years. The expected 100 TB of data per year gathered by the survey is anticipated to improve our understanding of dark energy, the mysterious force driving the accelerated expansion of our Universe.

Credit: DESI Collaboration © 2019 The Regents of the University of California, Lawrence Berkeley National Laboratory

DESI is mounted on the 4 m Mayall Telescope at Kitt Peak National Observatory in Arizona. It is a complex instrument made of six large fused silica lenses to provide a larger field of view, a focal system and 10 spectrographs. The focal plane consists of 5,000 robotic positioners (pictured) each holding a 100 μm diameter optical fibre. The fibres are gathered into 10 groups of 500, each group feeding into one spectrograph. The robotic positioners automatically rearrange themselves in such a way that light is collected from a certain set of galaxies and quasars. This rearrangement only takes 10 s, providing DESI with unprecedented surveying speed and hence the ability to map 20 times more objects than was possible with previous instruments.

“The individual elements of DESI are complex in their own regard, but more so in the full assembly of the instrument. It has been wonderful to see the whole instrument come together after years of design and construction,” says Daniel Eisenstein co-spokesperson of DESI.

To learn more about dark energy, DESI will primarily measure baryon acoustic oscillations — baryonic matter density fluctuations caused by the primordial acoustic density waves — and redshift space distortions, the modifications in the spatial distribution of galaxies caused by the gravitational pull from the surrounding large-scale structure of the Universe. These should improve our understanding of the expansion history of our Universe. Beyond cosmology, DESI is expected to enhance our understanding of the physics of galaxies, quasars and intergalactic gas. With a planned public data release every year there is a lot of excitement in store for cosmologists and astrophysicists.

Author information

Authors and Affiliations


Corresponding author

Correspondence to Iulia Georgescu.

Rights and permissions

Reprints and Permissions

About this article

Verify currency and authenticity via CrossMark

Cite this article

Georgescu, I. New eyes on the Universe. Nat Rev Phys 2, 70 (2020).

Download citation

  • Published:

  • Issue Date:

  • DOI:


Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing