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A €9M contract was announced recently for UK-based engineers and designers to build a unique and powerful instrument that aims to tackle some of the most compelling astronomical puzzles – such as how stars and galaxies form and evolve, and probing the structure of our own Milky Way.

A project team from the UK Astronomy Technology Centre (UK ATC) in Edinburgh will lead this international project to develop and build MOONS for the European Southern Observatory’s (ESO) Very Large Telescope (VLT) in northern Chile, already the world’s most productive ground-based astronomical facility.

MOONS (Multi-Object Optical and Near-infrared Spectrograph) will allow astronomers to see obscured areas in the Milky Way at a distance of around 40,000 light years away, and enable them to create a 3D map of our galaxy. This is difficult to do as the Earth is in the middle of the Milky Way’s disc, so the process is like trying to map a forest of densely-packed trees from the inside.

Director of the UK ATC, Professor Gillian Wright, said “The team at UK ATC in Scotland have an opportunity with this project to enable all of us to understand why the Milky Way looks the way it does. This instrument will act as an intergalactic GPS to help us to navigate through the billions of stars in our galaxy and create a comprehensive map of its structure.”

Conceived at the UK ATC – part of the Science and Technology Facilities Council (STFC) – MOONS is scheduled to become operational by 2019. Building such an ambitious and powerful new device – which will be about the size of a transit van – will take around 200 staff-years of effort, with the hardware alone costing €9M. The full project will cost around €23M. The UK ATC will lead the Project Office managing the multinational consortium that will construct MOONS, and will also play a vital design role for key components and ensure the project’s benefits extend throughout UK industry.

Like any spectrograph, MOONS will use the colour of light emitted by objects to reveal their chemical composition, mass, speed and other properties. Breaking new ground by simultaneously observing 1000 objects using fibre-optic cables to feed their visible and infrared light into the instrument, it will survey large samples of objects far faster than any existing instrument and conduct surveys that would be virtually impossible using today’s technologies. Not surprisingly, the design will pose extraordinary technical demands. For example, each of the 1000-plus fibres will have to move into position very quickly, with great accuracy and without colliding with each other.

In collaboration with the University of Cambridge and other UK universities, the UK ATC’s world-leading expertise in fields such as miniaturised mechanics and precision optics will be harnessed on key aspects of the project. The UK ATC will develop the most innovative component, the individual motorised systems allowing each fibre to move rapidly into position; it will also develop the cryostat system (used to cool MOONS down to -170°C) vital to enabling the infrared observations needed to penetrate galactic and intergalactic dust clouds. The University of Cambridge will develop complex cameras capable of meeting the instrument’s demanding performance requirements.

Partnerships with a range of UK equipment suppliers will also contribute across the project, helping the UK to further strengthen its cutting-edge scientific capabilities in the relevant fields.

Once MOONS is up and running, the international consortium will receive 300 nights of observations using the instrument. In particular, this will benefit two ground-breaking projects: one to produce an unprecedented sophisticated survey of the centre of the Milky Way; the other to look far back in time at ultra-distant galaxies to uncover the secrets of their early evolution. For more information, visit the ROE website.

Dr Michele Cirasuolo of the UK ATC, Principal Investigator on the project, says: “MOONS is a unique instrument able to pioneer a wide range of galactic, extragalactic and cosmological studies and provide crucial follow-up for major facilities such as Gaia, the Visible and Infrared Survey Telescope for Astronomy (VISTA), Euclid and the Large Synoptic Survey Telescope (LSST). I am hugely proud of the dedication and skill demonstrated over the project’s selection stages by our engineers and scientists at the UK ATC and across the consortium. We look forward to building this exceptional piece of technology and paving the way for many discoveries.”

Professor Roberto Maiolino from the University of Cambridge, Project Scientist for MOONS, says: “MOONS will vastly expand our knowledge of the mechanisms responsible for galaxy evolution across the life of the Universe. It will be possible to characterise the properties of millions of distant galaxies – for instance, by identifying the signatures of ongoing star formation and black hole accretion – and how galaxies’ evolution depends on their large-scale environment. Cambridge will play an essential role designing and assembling key optical subsystems, as well as in defining the science programme.”

More Information

STFC Press Office:

Marion O'Sullivan 
Mob: 07824 888990

Corinne Mosese 
Mob: 07557 317200

Notes for Editors

1. An artistic impression of the MOONS instrument on the VLT is available: Please credit STFC
   Images of the VLT are available from the ESO website.
    
2. The six countries involved in the MOONS project, alongside ESO, are: Chile, France, Italy, Portugal, Switzerland and the UK.
    
3. UK ATC 

   Based at the Royal Observatory in Edinburgh and operated by STFC, the UK Astronomy Technology Centre (UK ATC) is the national centre for astronomical technology. The UK ATC designs and builds instruments for many of the world’s major telescopes. It also project manages UK and international collaborations and its scientists carry out observational and theoretical research into questions such as the origins of planets and galaxies. The UK ATC has been at the forefront of previous key initiatives at the VLT, including the construction of KMOS (K-band Multi-Object Spectrograph) which enables 24 objects to be observed simultaneously in infrared light.

4. Very Large Telescope 

   The Very Large Telescope (VLT) is the world's most advanced optical instrument, consisting of four Unit Telescopes with main mirrors 8.2m in diameter and four movable 1.8m diameter Auxiliary Telescopes. The telescopes can work together to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer (VLTI), allowing astronomers to see details up to 25 times finer than with the individual telescopes. The Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure, corresponding to seeing objects four billion times fainter than can be seen with the unaided eye.

   VLT brochure (PDF)

5. ESO 

   The European Southern Observatory (ESO) is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the UK. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising co-operation in astronomical research. It operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. ESO is currently planning the 39m European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.

6. The University of Cambridge 

   The University of Cambridge, through the Cavendish Laboratory and the Institute of Astronomy, will contribute to MOONS with various activities. For example, the design and manufacturing of some key opto-mechanical parts of the spectrograph, which will result in the delivery of some high precision and high accuracy mechanical elements (specifically the mechanical mounts of the cameras of the spectrometer). Cambridge will also be responsible for the assembly, alignment and testing of three of the six cameras of the spectrometer. These tasks will be achieved by leveraging on the expertise in the area of high precision optical instrumentation in which Cambridge has worked extensively in the past.

   The University of Cambridge also hosts the Project Scientist as well as numerous astronomers (both observers and theoreticians) who are experts in the field of galaxy formation and evolution and Galactic astro-archeology, which are the main scientific themes of MOONS.

   Simulations developed in Cambridge are contributing to the instrument design and requirements, as well as identifying the optimal observing modes and strategies required to achieve the major science cases.

   The astronomers in Cambridge will also contribute to the detailed planning of the observations, and to the data analysis.

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