Euclid: Observing the unseen

October 30, 2015 by Tomasz Nowakowski, report
Artist's impression of the Euclid spacecraft. Credit: ESA/C. Carreau

(—In a notorious hunt for elusive dark matter, seeing the unseen is the key to scientific success. The latest addition to the fleet of probes searching for dark matter, European Space Agency's (ESA) Euclid spacecraft, is being designed to bring breakthrough results while observing the yet unobserved.

"Euclid will observe the unseen, meaning the part of the universe that does not emit or absorb light, but we know it is there because of the global properties of the universe, its geometrical properties and its expansion rate," Giuseppe D. Racca, ESA's Euclid Project Manager told

To find the traces of , the spacecraft will map the large-scale structure of the universe over the entire extragalactic sky. According to ESA, the probe will measure out to redshifts of about two, looking back in time 10 billion years as it covers the period over which dark energy accelerated the expansion of the universe. Dark matter is invisible, but has gravity and acts to slow the expansion. It is now assumed that ordinary matter makes up only about 4 percent of the universe; the rest is actually dominated by dark matter and .

To achieve its ambitious goals, besides a 1.2 m-diameter telescope, Euclid will be equipped with two powerful instruments designed to carry out scientific observations.

"We have two instruments, one visible imager, called VIS, capable to resolve images of galaxies in the 550 to 900 nm passband. The VIS nominal survey images are used to determine the shapes of at least 30 galaxies per arcmin, for a total of 1.5 billion galaxies," Racca said.

"The other instrument is NISP [an infrared instrument], designed to carry out slitless spectroscopy and imaging photometry in the near-infrared (NIR) wavelength. The NISP spectroscopy measures the redshifted H-alpha emission line of galaxies," he added.

VIS and NISP, large-format cameras, will be used to characterize the morphometric, photometric and spectroscopic properties of galaxies. Euclid will use two techniques to observe the invisible, called galaxy clustering (GC) and weak lensing (WL).

In Euclid's case, GC means performing a measurement of the redshift distribution of galaxies from their H-alpha emission line survey using near-infrared slitless spectroscopy. This method also provides direct information of the validity of general relativity because it enables monitoring the evolution of structures subject to the combined effects of gravity, which forces clumping of matter and the opposing force caused by the accelerated expansion.

The WL technique measures the distortion of the galaxy shapes due to the gravitational lensing caused by the predominantly dark matter distribution from the galaxies and the observer. The obtained galaxy shear field can be transformed into the matter distribution. WL requires extremely high image quality because possible image distortions by the optical system must be suppressed or calibrated out in order to measure the true distortions caused by gravity.

"It is important that the two techniques are performed at the same time. The complementarity of the two probes will, indeed, provide important additional information on possible systematics, which limit the accuracy of each of the probes," Racca noted.

The Euclid mission is currently on track for the planned launch in late 2020. It was selected for implementation as a Medium-class mission in ESA's Cosmic Vision program in October 2011 and formally adopted in June 2012. The mission will operate from the Sun–Earth Lagrangian point (L2), situated 1.5 million km from Earth. Science and spacecraft operations will be conducted by ESA. The Euclid Consortium, consisting of more than one hundred scientific institutes, is responsible for the development and delivery of the spacecraft's instruments and the scientific data processing.

Explore further: Euclid to probe dark Universe with Astrium science module

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1 / 5 (4) Oct 30, 2015
Always nice to see new technologies and techniques for the exploring of the universe.
Worryingly is, only, where they go to look for something (dark matter) which is 95% of the Universe? It would be logical to seek the the remaining less than 5%.
See: http://www.svemir...html#17b (Are we blind or we do not want to see the dark matter!).
2.3 / 5 (3) Oct 31, 2015
My understanding from reading the article is that an assumption is made that dark matter exists and is not an artifact of an inaccurate model.
It would be far more exciting if they got a null result.
My point is that all the information is conveyed by one medium, light. That is akin to believing the story of only one witness.
1 / 5 (3) Oct 31, 2015
The light is the product of the collision of radiation with matter, that is the reason why the universe is dark. Where no matter there is no light (radiation are ubiquitous).
3 / 5 (2) Oct 31, 2015
dark matter are neurtinos and dark energy is energy of quantum vacuum itself
2 / 5 (4) Oct 31, 2015
Many millions of dollars spent in searching in the wrong direction, as based on their flawed assumptions.
1 / 5 (6) Oct 31, 2015
The word vacuum forget. The vacuum would torn, all bodies within the universe, but it does not happen (the same is between water and air, etc.). No more types of of vacuum, just one. Vacuum replace with dark matter and energy.
The second question is what is the dark matter and which laws are related to it.
The area is unknown and ledger and old knowledge here, do not help.
5 / 5 (2) Oct 31, 2015
Quote from one middle paragraph: "..and the opposing force caused by the accelerated expansion" . states a backward conclusioin.. It should read: and the opposing force that caused the accelerated expansion!

It has been often posited that space contains an intrinsic expansion force. This would also imply that space has quanta as of a cellular nature. That may make sense from a quantum mechanical viewpoint. Matter particles such as protons originally were described as small spheres, but later this was held to be statistical probability densities governed by quantum mechanical higher order partial differential equations in many unknowns.

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