I forgot to mention on this blog some important news about the Planck mission which many people here in the School of Physics & Astronomy at Cardiff University are heavily involved in.
Here is the official announcement from The Planck Science Team home page:
The High Frequency Instrument (HFI) on ESA’s Planck mission has completed its survey of the remnant light from the Big Bang. The sensor ran out of coolant on January 14 2012 as expected, ending its ability to detect this faint energy. Planck was launched in May 2009, and the minimum requirement for success was for the spacecraft to complete two whole surveys of the sky. In the end, Planck worked perfectly for 30 months, about twice the span originally required, and completed five full-sky surveys with both instruments. Able to work at slightly higher temperatures than HFI, the Low Frequency Instrument (LFI) will continue surveying the sky for a large part of 2012, providing even more data to improve the Planck final results.
For more details, see here. Basically, the HFI instrument consists of bolometers contained in a cryogenic system to keep them cool and thus suppress thermal noise in order to enable them to detect the very weak signals coming from the cosmic microwave background radiation. The helium required to maintain the low temperature is gradually lost as Planck operates, and has now run out. The HFI bolometers consequently warmed up, which makes them useless for cosmological work, so the instrument has been switched off. I’m sure you all understand how uncomfortable it is when your bolometers get too hot…
You can find a host of public information about Planck here but the scientific work is under strict embargo until early next year. However, as a Telescoper exclusive I am able to offer you a sneak preview of the top secret Planck data well in advance of official release. If you want to see what Planck scientists have been looking at for the last couple of years, just click here.
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