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Raumfahrt - ESA-Mission Euclid (2020) zur Erforschung des dunklen Universum -Update-2

21.09.2019

Euclid space telescope to study 'dark Universe' makes progress

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The Euclid STM stands outside the big thermal-vacuum chamber at Thales Alenia Space
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Europe's space mission to uncover the secrets of the "dark Universe" has reached a key milestone.

The test model of the Euclid telescope has just emerged from a chamber where it was subjected to the kind of conditions experienced in orbit.

It was a critical moment for engineers because the successful trial confirms the observatory's design is on track.

Euclid, due for launch in 2022, will map the cosmos for clues to the nature of dark matter and dark energy.

These phenomena appear to control the shape and expansion of the Universe but virtually nothing is known about them.

The €800m venture, led by the European Space Agency (Esa), will be one of a group of new experiments to come online in the next few years.

Scientists are hopeful these next-generation technologies will provide the insights that have so far eluded them.

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The finished observatory has a sunshield and white baffle to shade its observations
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The Structural and Thermal Model (STM) of Euclid is a near-clone of the real thing, or "flight model" (FM).

To the lay person, it's actually hard to tell the difference. But the telescope mirrors inside this copy, for example, are unpolished spares, and its "scientific instruments" don't contain the full complement of components and electronics.

An STM is, nonetheless, a very good representation.

Its job is to run ahead of the FM in the assembly process to find and fix any issues that might arise in the use of materials and the integration of equipment.

"I've seen many Structural and Thermal Models in my career and I think this is the most beautiful because it's actually nearly all made from flight hardware," Giuseppe Racca, Esa Euclid project manager, told BBC News.

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The STM contains many flight-worthy spare parts but it will not go into space

One of the most important stages for the test model is when it goes in a vacuum chamber and is confronted with the challenging temperatures - both hot and cold - that occur in space.

For the Euclid STM, this thermal-vac evaluation was conducted throughout August at a factory in Cannes, France, belonging to Thales Alenia Space (TAS).

TAS leads the industrial consortium that's building Euclid.

Engineers will now shake the model and blast it with noise to gain the additional assurance that the design can withstand a rocket ride to orbit.

"We should finish the campaign by the end of October and then we will take the lessons learned and apply those to the flight model," said TAS project manager Paolo Musi.

The observatory is currently running about a year-and-a-half behind schedule. Problems have arisen in a number of areas, but Esa now believes the path ahead looks robust.

TAS will spend most of next year assembling the flight model at its factory in Turin, Italy.

Sub-contractor Airbus is putting together the module that contains the mirrors and instruments. The company should deliver this no later than the beginning of 2021.

Another full round of environmental testing follows before the completed observatory is shipped to the launch pad.

Euclid is currently booked to ride a Russian Soyuz into space in 2022, but Esa is now looking closely at the possibility of using Europe's new Ariane-62 rocket - if it's available and deemed suitable.

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Once in orbit, the observatory will have two major goals.

One is to map the distribution of dark matter, the matter that cannot be detected directly but which astronomers know to be there because of its gravitational effects on the matter we can see.

Galaxies, for example, could not hold their shape were it not for the presence of some additional "scaffolding". This is presumed to be dark matter - whatever that is.

Euclid will aim to plot its distribution - and discern something of its properties - by looking for the subtle way its mass distorts the light coming from distant galaxies.

Dark energy represents an altogether different problem, and is arguably one of the major outstanding issues facing 21st-Century science.

This mysterious "force" appears to be accelerating the expansion of the Universe. Recognition of its existence and effect earned the 2011 Physics Nobel.

Euclid will investigate dark energy by mapping the three-dimensional distribution of galaxies.

There are patterns in the great voids that exist between these objects that can be used as a kind of "yardstick" to measure the expansion through time.

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The Large Synoptic Survey Telescope will use multiple techniques to study the sky

Euclid is just one in a series of new experiments that will tackle the dark conundrum.

Russia and Germany have just launched the Spektr-RG space telescope which will do a similar job to Euclid but by studying X-ray light in the sky (Euclid will operate in the visible and the infrared).

The American Mid-Scale Dark Energy Spectroscopic Instrument (DESI) is a ground-based experiment due to begin initial operations in the coming weeks. Like Euclid, it will be using the yardstick technique.

And then there's the Large Synoptic Survey Telescope (LSST). Its full science observations should begin in 2022 also, using a range of methods, including mapping the positions of exploding stars to measure cosmic expansion.

Isobel Hook from Lancaster University, UK, worked in one of the Nobel-winning teams and is involved in both the Euclid and LSST projects.

"We need to be able to measure the effects of dark energy at different distances and at different times in the history of the Universe. That's what could reveal something really exciting," she told BBC News.

"It's the combination of all these experiments that will give us the maximum amount of information from the one sky that we've got."

Quelle: BBC

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Update: 23.09.2019

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Structural and thermal model of the Euclid satellite

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The structural and thermal model of the Euclid satellite recently completed its thermal qualification tests at Thales Alenia Space’s premises in Cannes, France. Integrated in near-flight configuration, including the payload and service modules, the satellite model is ready to undergo mechanical vibration tests in coming weeks.

Euclid is a medium-class mission in ESA's Cosmic Vision programme to investigate the expansion of our Universe over the past ten billion years, probing cosmic epochs from before the expansion started to accelerate, all the way to the present. To this aim, the mission will survey galaxies at a variety of distances from Earth, using a 1.2 m diameter telescope with two instruments – the visual imager (VIS) and the near-infrared spectrometer and photometer (NISP) – and covering an area of the sky equivalent to more than 35 percent of the celestial sphere.

By making use of both weak gravitational lensing, which measures the distortion of distant galaxies caused by intervening matter, and baryonic acoustic oscillations, based on measurements of the clustering of galaxies, Euclid will capture a 3D picture of the evolving distribution of both dark and ordinary (or baryonic) matter in the cosmos. This will enable scientists to reconstruct the past few billion years of the Universe's expansion history, estimating the acceleration caused by the mysterious dark energy to percent-level accuracy, and possible variations in the acceleration to 10 percent accuracy.

The satellite model shown in this photo is not the so-called flight model – the one that will be eventually launched – but it contains flight-worthy spare parts. From a mechanical point of view, it is identical to the flight model, and it allows engineers to apply extreme thermal and mechanical stresses during testing, without having to subject the delicate flight hardware to same processes. These tests, which will soon involve vibrations using a large shaker to simulate launch conditions, are performed to determine whether the thermal and mechanical properties of the actual hardware correspond to the predictions.

In order to reach Euclid’s ambitious science goals, the main design drivers include the quality and stability of the integrated optical system; the speed and completeness of its sky survey capability; accurate and stable pointing; and the ability to reliably transmit to the ground the huge volumes of scientific data that the satellite will gather. The design proposed by Thales Alenia Space, the mission’s prime contractor, is based on the experience gained with ESA’s Herschel and Planck missions, which both demonstrated excellent performance in orbit and delivered extraordinary data to delve into the mysteries of our Universe.

In addition to that, a peculiarity of Euclid is that the satellite will maintain a very stable optical performance under the most extreme attitude changes that will occur during slew manoeuvres. The recent thermal vacuum tests have simulated and successfully proven the capability to maintain the thermal stability in these conditions. The next step will be to confirm that also the optical stability will be ensured, but this will only happen during the end-to-end test of the payload module flight model next year.    

Meanwhile, integration and testing of the flight model of the Euclid telescope and service module have already started at the premises of Airbus in Toulouse, France and Thales Alenia Space in Turin, Italy, respectively. The two modules will be integrated in 2021, and the complete satellite will undergo final tests in preparation to launch, which is scheduled for 2022.

Credits: ESA–S. Corvaja
Quelle: ESA

 

 

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