Skip to ContentSkip to Navigation
Part of University of Groningen
Science LinX Science Linx News

We’re going to put a radio telescope on the back side of the Moon

25 September 2023
Impression of ESA’s Moon lander Argonaut | © ESA

One day, the European Space Agency (ESA) asked Professor Léon Koopmans from the University of Groningen: ‘Would you like to put a radio telescope on the Moon?’ His telescope will tag along on ESA’s Moon lander Argonaut , but first, a lot of things need to be developed.

FSE Science Newsroom | Charlotte Vlek

With a radio telescope on the Moon, Koopmans wants to find out what the Universe looked like during the Cosmic Dark Ages: the period just after the Big Bang, before the first stars were formed. At that time, everything was dark and covered in a mist of hydrogen. This darkness makes it a particularly interesting period: it can give us insight into fundamental physics, while observations are not dominated by starlight.

Not measurable from Earth

It is obvious that a regular, optical telescope cannot be used to inspect this early, dark Universe. A radio telescope, however, can. The hydrogen atoms sent out a radio signal, the 21-centimetre signal, named after the wavelength of the 21-centimetre line. The radiation that reaches us now has travelled a long distance, which makes it possible to ‘look back in time’.

Those signals are largely deflected by the outer layer of our atmosphere and what is left is drowned out by the radio signals that we emit from Earth.

Koopmans was already working with telescopes on Earth that detect the 21-centimetre signal, such as LOFAR (spread across Europe and centred in Drenthe) and NenuFAR (France). But these telescopes cannot pick up radiation from the Dark Ages: those signals are largely deflected by the outer layer of our atmosphere and what is left is drowned out by the radio signals that we emit from Earth.

Koopmans explains: ‘The older these signals are, the longer their wavelengths are.’ While they were travelling in our direction, they were stretched due to the expansion of the Universe; similar to the pitch of a police siren that becomes lower as it moves away from you. These signals have stretched to several meters, up to tens of metres long, which means that they are now in the same range as a lot of other signals. This makes them hard to detect, precisely because they are so old. However, detection should be easier on the Moon. 

Léon Koopmans. © Emiel Lops
Léon Koopmans. © Emiel Lops

What do we need to build?

The question for Koopmans and his team is now: what do we need to build to be able to do something like this? Koopmans sums up: ‘Such a radio telescope needs to be compact, simple, and light. We need to develop good algorithms to process the data, but also a good system that can withstand the extreme temperatures, fluctuating between –170 °C and +100 °C.

In an elaborate study with forty engineers from ESA, Koopmans has already identified which aspects need to be considered. These need to be worked out in the near future with colleagues from across Europe. Koopmans: ‘We are thinking about energy sources. Solar panels seem like a good idea, but a battery cannot withstand these low temperatures. You could use energy to keep the battery warm, but then you won’t have energy to do any measurements and to send data to Earth. You could bury everything underground to dampen the fluctuations in temperature, but how would you get that to happen?’

Processing large amounts of data

Léon Koopmans was the first to introduce the use of graphical processing units (GPUs) from Nvidia in the Netherlands, to process the enormous amounts of data from these kinds of radio telescopes. He had heard about them from a friend, a scientist whom he knew from his time as a PhD student.

Telescopes as described in this article gather large amounts of data: LOFAR and NenuFAR gather in the order of petabytes. For comparison: at home we might use a terabyte for large backups; a petabyte is a thousand times more.

Nvidia initially developed their graphical processing units for game consoles; by now, the company has grown to one of the five largest tech companies and their chips are often used for heavy computational work, such as data processing and AI applications.

I’m going to put a radio telescope on the back side of the Moon. How many people can say such a thing?

To the Moon, and soon!

There is enough for the team to work on. The current plan is that the ESA’s Moon lander Argonaut will go to the Moon in 2030, delivering some material for testing. The full telescope will follow around 2035. In terms of space missions, this is extremely fast, although obtaining the results from this research will need a bit more time. At least 10 years of measurements will be needed before any conclusions can be drawn.

How does Koopmans stay motivated for such a large project? He finds all aspects of it mighty interesting. And, says Koopmans: ‘If I talk to a neighbour about our work, I can say: I’m going to put a radio telescope on the back side of the Moon. How many people can say such a thing?’

Reference

Astronomical Lunar Observatory

Last modified:02 November 2023 1.14 p.m.
View this page in: Nederlands

More news

  • 10 June 2024

    Swarming around a skyscraper

    Every two weeks, UG Makers puts the spotlight on a researcher who has created something tangible, ranging from homemade measuring equipment for academic research to small or larger products that can change our daily lives. That is how UG...

  • 24 May 2024

    Lustrum 410 in pictures

    Lustrum 410 in pictures: A photo report of the lustrum 2024

  • 21 May 2024

    Results of 2024 University elections

    The votes have been counted and the results of the University elections are in!