NASA has delivered three detector for the spacecraft's near-infrared instrument.
"The delivery of these detector systems is a milestone for what we hope will be an extremely exciting mission, the first space mission dedicated to going after the mysterious dark energy," said Michael Seiffert, from the NASA's Jet Propulsion Laboratory in the US.
The Euclid will carry two instruments: a visible-light imager (VIS) and a near-infrared spectrometer and photometer (NISP).
A special light-splitting plate on the Euclid telescope enables incoming light to be shared by both instruments, so they can carry out observations simultaneously.
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Astrophysicists think dark energy is responsible for this effect, and Euclid will explore this hypothesis and help constrain dark energy models.
This census of distant galaxies will also reveal how galaxies are distributed in our universe, which will help astrophysicists understand how the delicate interplay of the gravity of dark matter, luminous matter and dark energy forms large-scale structures in the universe.
Additionally, the location of galaxies in relation to each other tells scientists how they are clustered.
Dark matter, an invisible substance accounting for over 80 per cent of matter in our universe, can cause subtle distortions in the apparent shapes of galaxies.
Euclid's combination of visible and infrared instruments will examine this distortion effect and allow astronomers to probe dark matter and the effects of dark energy.
Detecting infrared light, which is invisible to the human eye, is especially important for studying the universe's distant galaxies.
Each detector system consists of a detector, a cable and a "readout electronics chip" that converts infrared light to data signals read by an onboard computer and transmitted to Earth for analysis. Sixteen detectors will fly on Euclid, each composed of 2040x2040 pixels.
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