The European Space Agency's (ESA) Euclid space telescope successfully blasted off from Cape Canaveral, Florida, on July 1, 2023. The groundbreaking space telescope will hunt for clues about two of the universe's greatest mysteries: dark matter and dark energy.
Despite making up an estimated 95% of the universe, dark matter and dark energy cannot be detected directly. Instead, scientists observe them in the gravitational warping effects seen in many galaxies across the universe. Euclid's enormous field of view will significantly expand this search for warped space-time.
Here's everything you need to know about Euclid and its search for the universe's most mysterious components.
Taken on their own, Euclid's cameras are common among space telescopes. What makes Euclid groundbreaking is these instruments' field of view, with a third of the entire night sky and over a billion galaxies expected to be cataloged by the time the telescope has finished its planned six years of scanning. The telescope should be able to peer up to 10 billion years into the past — slightly less than the James Webb Space Telescope, which has looked back more than 13 billion years.
An image taken with Euclid's Near-Infrared Spectrometer and Photometer (NISP) revealed a dazzling starscape of billions of stars and galaxies. Before reaching the instrument's detector, light from the distant objects passed through a filter that splits the light of every star and galaxy according to wavelength, allowing astronomers to determine what each object is made of and, in turn, how far it is from Earth.
The researchers also tested Euclid's VISible instrument (VIS), to capture the cosmos in visible light (the same type of light that we can see with our unaided eyes). This dense starscape took Euclid 566 seconds to collect, according to ESA. Both test images are largely unprocessed, and only offer a hint at what Euclid will be capable of delivering when fully operational.
The second will use so-called baryon acoustic oscillations, gigantic matter shock waves created when the universe was hot and now frozen in time, as cosmic tree rings to study the universe's accelerating growth and its suspected cause: dark energy.
So how do we know dark matter is there? While dark matter itself is invisible, the gravitational interactions it has with its surroundings are not — making its presence apparent in its extreme gravitational warping of galaxies, or in how it accelerates stars to otherwise inexplicable speeds as they orbit galactic centers.
The composition of dark matter isn't known. Some theories suggest that hypothetical particles called weakly interacting massive particles (WIMPs), each weighing 10 to 100 times the mass of a proton, could be ideal candidates to fill the theoretical gaps. Others have proposed that a minuscule particle less than a billionth the size of an electron — called an axion — could be the substance's primary candidate.
NASA has estimated that 68% of the universe is composed of dark energy; 27% is dark matter, and visible matter makes up just 5%.
Editor's note: This article was updated on July 31st to include Euclid's first two test images.