New Technologies for Astronomical Research
Operating principle of a photonic reformer. (Full caption in the main text.) Image: Dr Robert Harris, Königstuhl State Observatory, Centre for Astronomy of Heidelberg University
The “Novel Astronomical Instrumentation through Photonic Reformatting” (NAIR) project is being funded by the DFG within the “New Instrumentation for Research” call for proposals. The researchers in Heidelberg, Cologne and Potsdam will design and test components that can efficiently rearrange the light of stars and galaxies to enable high-precision measurements of cosmic objects. This new technology is targeted for use on large telescopes in order to, for example, search for earth-like planets of nearby stars and determine their atmospheric composition.
“When building spectrographs for modern telescopes, we increasingly encounter technical and financial limitations,” explains Prof. Dr Andreas Quirrenbach, Head of the Königstuhl State Observatory. “However, in the coming decade telescopes with mirrors up to 40 meters in diameter will be placed in operation. We need new concepts to exploit the potential of these giant telescopes.” One of these innovative approaches is the reformatting of light: for example, a light beam with a cross-section in the shape of a thin line is formed from a circular beam. According to Prof. Quirrenbach, it is also possible to use relatively small spectrographs with very large telescopes if they are fed these “squeezed” light bundles.
Heidelberg researcher Dr Robert Harris already worked with the rearrangement of starlight while preparing his doctoral dissertation. He came across micro-optic devices used by the telecommunications industry in switching centres for fibre-optic networks. They have complex functions in a minimum amount of space and are therefore suitable for reformatting light. Now Dr Harris is developing components specifically tailored to the needs of astronomy. There is a further application for these photonic systems, according to Prof. Dr Lucas Labadie of Cologne. “If several telescopes are connected to a so-called interferometer, we get sharper images than would be possible with a single telescope. For this purpose, all light bundles must be combined and superimposed with the highest precision.” Achieving this requires optimising the components and better understanding their physical properties in order to minimise light losses, as Dr Stefano Minardi and Dr Roger Haynes from Potsdam emphasise.
The DFG funding provides for staff and laboratory equipment to develop and test new micro-optic systems concepts for use in astronomical instruments. The technology should also be made available to others working in basic scientific research. Dr Minardi is research group leader at the centre for innovation competence innoFSPEC Potsdam.
Press Release of the University of Heidelberg:
Dr Stefano Minardi, innoFSPEC Potsdam, Leibniz Institute for Astrophysics Potsdam, +49 331-7499 687, firstname.lastname@example.org
Dr Roger Haynes, Leibniz Institute for Astrophysics Potsdam, +49 331-7499 654, email@example.com
Prof. Dr Andreas Quirrenbach, Centre for Astronomy of Heidelberg University – Königstuhl State Observatory, +49 6221-54 1792, firstname.lastname@example.org
Dr Robert Harris, Centre for Astronomy of Heidelberg University – Königstuhl State Observatory, +49 6221-54 1733, email@example.com
Prof. Dr Lucas Labadie, University of Cologne, Institute of Physics I, +49 221-470 3493, firstname.lastname@example.org
Media contact: Katrin Albaum, +49 331-7499 803, email@example.com
Figure 1: Operating principle of a photonic reformer. In this example, a squared field of view is converted into a thin line, which can be very effectively coupled into an astronomical spectrograph.
Image: Dr Robert Harris, Königstuhl State Observatory, Centre for Astronomy of Heidelberg University
Figure 2: Multicore optical fibre for use in high-precision spectrographs. The different colours and shapes show that the optical fibre mixes the incident white light and thus greatly reduces unwanted interference effects observed by the spectrograph. This is required, for example, to find earth-like planets. The optical fibre named MCF511 was manufactured at the University of Bath (UK).
Image: Dionne Haynes, Leibniz Institute for Astrophysics Potsdam
Figure 3: Photonic component for an astronomical interferometer. The light strips visible in the glass are light guides. Such components are used on large telescopes in the most modern observatories.
Photo: University of Cologne, University of Jena and Leibniz Institute for Astrophysics Potsdam
The key areas of research at the Leibniz Institute for Astrophysics Potsdam (AIP) are cosmic magnetic fields and extragalactic astrophysics. A considerable part of the institute's efforts aim at the development of research technology in the fields of spectroscopy, robotic telescopes, and e-science. The AIP is the successor of the Berlin Observatory founded in 1700 and of the Astrophysical Observatory of Potsdam founded in 1874. The latter was the world's first observatory to emphasize explicitly the research area of astrophysics. The AIP has been a member of the Leibniz Association since 1992.