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Euclid's sight has been restored

Written by  Tuesday, 26 March 2024 13:10
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Euclid's sight restored
The light is directed onto Euclid’s two scientific instruments: the visible camera VIS that will provide very sharp images, and the near-infrared spectrometer and photometer NISP which will provide both images and spectroscopic data, over the largest infrared field of view from space. ESA's Euclid mission is designed to explore the composition and evolution of the dark universe. The space telescope will create the largest, most accurate 3D map of the Universe across space and time by observing billions of galaxies out to 10 billion light-years, across more than a third of the sky. Euclid will explore how the Universe has expanded and how and how large-scale structure is distributed across space and time, revealing more about the role of gravity and the nature of dark energy and dark matter. Credit: ESA. Acknowledgement: Work performed by ATG under contract for ESA" width="800" height="450"/>
An artist impression of ESA’s Euclid mission in space. The spacecraft carries a 1.2-metre telescope that collect the light from sources in the sky such as far-away galaxies. The light is directed onto Euclid’s two scientific instruments: the visible camera VIS that will provide very sharp images, and the near-infrared spectrometer and photometer NISP which will provide both images and spectroscopic data, over the largest infrared field of view from space. ESA's Euclid mission is designed to explore the composition and evolution of the dark universe. The space telescope will create the largest, most accurate 3D map of the Universe across space and time by observing billions of galaxies out to 10 billion light-years, across more than a third of the sky. Euclid will explore how the Universe has expanded and how and how large-scale structure is distributed across space and time, revealing more about the role of gravity and the nature of dark energy and dark matter. Credit: ESA. Acknowledgement: Work performed by ATG under contract for ESA

A newly devised procedure to de-ice Euclid's optics has performed significantly better than hoped. Light coming in to the visible "VIS" instrument from distant stars was gradually decreasing due small amounts of water ice building up on its optics. Mission teams spent months devising a procedure to heat up individual mirrors in the instrument's complex optical system, without interfering with the finely tuned mission's calibration or potentially causing further contamination. After the very first mirror was warmed by just 34°, Euclid's sight was restored.

A little ice goes a long way

Euclid is on a mission to uncover the secrets of dark matter and dark energy, which are thought to make up 95% of the universe yet cannot be directly observed. But a few nanometers of ice—the width of a large molecule—have been accumulating on the mission's optics each month, causing a drop in the light coming in from distant galaxies.

ESA teams across Europe, at the agency's ESTEC technical heart in the Netherlands, ESOC mission control in Germany and ESAC science operations center in Spain, worked closely with the Euclid Consortium and industrial partners Thales Alenia Space and Airbus Space to investigate, research and come up with a potential solution.

"It was an enormous team effort over the last months to plan, execute and analyze the heating of selected mirrors onboard Euclid, resulting in the fantastic result we see now," explains Ralf Kohley, Euclid instrument scientist and in charge of the anomaly review board.

"The mirrors, and the amount of light coming in through VIS will continue being monitored, and the results from this first test will continue to be analyzed as we turn this experiment into a core part of flying and operating Euclid."

One by one, then group by group, they planned to heat up mirrors in Euclid's optics and test the effect on the light coming in. They had reason to believe, but couldn't know for sure, that the first mirror they would heat was causing most of the problems.

Euclid's sight restored
During ESA Euclid’s first months in space, some water molecules absorbed from the air, during assembly on Earth, by parts of the spacecraft were being gradually released. Cold surfaces like the mirrors in Euclid’s instruments tend to attract these molecules, where they formed a very thin layer of ice – the width of a DNA-strand. This thin layer was starting to hinder the satellite’s vision. That is why operation teams on the ground started a de-icing campaign. They sent commands to the satellite to heat the instrument mirrors individually and remove the layer of ice. This graph shows the impact of one of the first operations. It shows the percentage of light collected by Euclid’s VIS instrument during the heating of a mirror. After about 90 minutes, the sublimation temperature of ice was reached – the temperature at which ice can transform directly into water vapour in the vacuum of space. From this temperature onwards, the release of ice proceeded swiftly, and the layer was essentially removed after another 19 minutes, when the mirror reached a temperature of –117 °C. With Euclid's vision cleared at the very first stage of the procedure, scientists and engineers could tell where precisely the ice had formed, and where it is likely to form again. But it will be simple to repeat this targeted procedure every six to twelve months. Credit: ESA/Euclid/Euclid Consortium

Dark universe detective sees more of the light

"It was midnight at ESOC mission control when we de-iced the first two mirrors in the procedure. We were very careful with our timings, ensuring we had constant contact between the spacecraft and our in Malargüe, Argentina, so we could be ready to react in real time if there were any anomalies," explains Micha Schmidt, Euclid Spacecraft Operations Manager.

"Thankfully, it all went as planned. When we saw the first analysis provided by the science experts, we knew that they would be very happy—the result was significantly better than expected."

Mischa Schirmer, calibration scientist for the Euclid Consortium and one of the main designers of the de-icing plan, explains the results.

"Our primary suspect, the coldest mirror behind the main telescope optics, was heated from –147°C to –113°C. It didn't need to get hot, because in a vacuum this temperature is enough to quickly evaporate all the ice. And it worked like a charm! Almost immediately, we were receiving 15% more light from the universe. I was certain that we would see a considerable improvement, but not in such a spectacular way."

With Euclid's vision cleared at the very first stage of the procedure, scientists and engineers could tell where precisely the ice had formed, and where it is likely to form again. "Euclid's 'eye' has been cleared, allowing it to clearly see faint light from distant galaxies, and more of them than would otherwise be possible without this operation," explains Reiko Nakajima, VIS instrument scientist.

"We expect ice to cloud the VIS instrument's vision again in the future. But it will be simple to repeat this selective decontamination procedure every six to 12 months and with very little cost to science observations or the rest of the mission."

After months of research from scientists and engineers across Europe, late nights at ESA's ESOC mission control and 100 minutes of targeted warmth, Euclid's vision has been protected. These studies, and incredible result, will also help future satellites likely to face the same, common icy problem.

Citation: Euclid's sight has been restored (2024, March 26) retrieved 26 March 2024 from https://phys.org/news/2024-03-euclid-sight.html
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