Space telescope Euclid was launched successfully - it traces the dark energy
The objective of Euclid is to help us understand two of the most enigmatic, yet key phenomena in the universe; dark matter and dark energy.
“The gravity of dark matter and dark energy affects the movements of galaxies and the expansion of the universe. Though we cannot see either of them directly, they make up some 95% of the universe,” says Professor Hannu Kurki-Suonio from the University of Helsinki.
Euclid will produce a three-dimensional map of the universe with billions of galaxies. The map will cover over one third of space, up to 10 billion light years away. The further away an observed galaxy is, the further we can see into the past – all the way to 10 billion years ago.
The part of space to be mapped has been selected because that is where the furthermost galaxies are most clearly discernible, avoiding the plane of the Milky Way and our own solar system. Euclid will also measure the gravitational lens effect; how the gravitation of dark matter bends the trajectory of light so that it distorts how we see far-away galaxies. In this way we will be able to map the distribution of dark matter.
“In order to collate all this data, we need long-term collaboration between observatories and data centres around the world, but once it is finished, it will also offer scientists the best material for research into the structure of the universe,” says University Lecturer Aku Venhola from the University of Oulu.
The three-dimensional map produced by Euclid will help us study how the universe has expanded and how large-scale structures, like galaxies, have developed during cosmic history. This, in turn, depends on the characteristics of dark matter and dark energy.
Many Finns participating in the endeavour
Euclid was launched from Cape Canaveral in Florida with a SpaceX Falcon 9 rocket to 1.5 million kilometres from Earth, where it will be able to make observations without interference. There is a telescope on Euclid with a diameter of 1.2 metres, along with two instruments: one for taking sharp images in visual light, the other one for taking spectra and images in infrared.
Both instruments on Euclid contain a large camera. The images from visible light contain over 600 million pixels and the ones from infrared over 60 million pixels. Euclid differs from previous space telescopes specifically in that it can take in a much larger portion of space at one time – the portion of space covered by one image is larger than the full moon can conceal.
Over 300 research institutes and 2,000 researchers from 21 countries are participating in Euclid. The Finnish scientists have collaborated in developing computing methods, producing simulated data, and developing data quality-assurance methods for Euclid. The Finnish members also hold a strong position in combining observations made from Earth with Euclid data. In addition to the data gathered by the space telescope, we also need a huge amount of data collected from Earth in order to determine the distances of galaxies.
“Data-intensive computation is a swiftly growing field within science. The Finnish Euclid science data centre is a spearhead example of this,” says Director Janne Ignatius from CSC, the IT Center for Science.
“The development of efficient methods of data analysis poses cross-discipline challenges between cosmology and IT,” adds IT Professor Maarit Korpi-Lagg from Aalto University.
Finnish researchers have especially developed methods for computing statistical measures like correlation functions to describe the structure of the universe. After the launch, the Finnish computing centre will be responsible for processing 5% of the data from Euclid.
Finnish partners in Euclid are the University of Helsinki, the University of Turku, the University of Oulu, the University of Jyväskylä, Aalto University, and CSC Ltd.
The first results from the Euclid project are expected by the end of 2025.