Studying the birth of the Universe
Planck will help scientists answer some of the most fundamental questions about the birth and evolution of the Universe.
Planck is, in effect, a kind of time machine. The mission will attempt to predict the future of the Universe by studying its past. Scientists hope it will help them answer key questions such as: - How old is the Universe and how quickly is it expanding? - Will it continue to grow forever or ultimately collapse? - What is the nature of dark matter and dark energy?
Using Planck to examine the ancient radiation released shortly after the Universe was formed, known as the cosmic microwave background radiation, scientists will be able to study all the way back to the time of the Big Bang itself 13.7 billion years ago years ago.
The mission will provide information about how our Galaxy and others first formed and will give us clues about when they may end.
Mission facts
Technology
More than 40 European scientific institutes, and a small number of US ones, are helping to build the instruments Planck will use.
The telescope will work with two instruments, one to detect high frequency cosmic microwave background signals, the other low frequency signals. A complex system of refrigerators will help to achieve the necessary temperature for the experiments.
UK involvement
The UK is playing a major role in the Planck mission. A number of UK institutes and companies form part of the consortium that built the two focal plane instruments, HFI and LFI. The Jodrell Bank Observatory at The University of Manchester produced critical elements of the LFI receiver modules. Cardiff University, STFC RAL and SEA were involved with hardware development for HFI, while various UK research groups including Imperial College London and University of Cambridge form the London Planck Analysis Centre and Cambridge Planck Analysis Centre. These groups are involved with data analysis and simulation for the HFI data analysis and simulation software.