Planck’s HFI completes its survey of early Universe
Planck’s HFI completes its survey of early Universe
News from ESA
(Image:Located in the focal plane of the telescope, Planck’s Low Frequency Instrument (LFI), and the High Frequency Instrument (HFI), are equipped with a total of 74 detectors covering nine frequency channels. These detectors must be cooled to temperatures around or below 20 K so that their heat does not swamp the faint microwave signals they are designed to detect.
Planck’s active cooling system consists of a three-stage refrigeration chain which takes over after the passive cooling system cools the telescope to about 50 K. The first stage makes use of liquid hydrogen to reduce the temperatures to 20 K.
The second stage is a mechanical cooler (a pump) that uses liquid helium (4He) to bring the temperatures down to 4 K. The third stage makes use of a mixture of Helium 3 and Helium 4 (3He and 4He) to reach an amazingly low temperature of just 0.1 K.
This series of images shows the path that microwave light collected by telescope follows to reach the instrument detectors via the conical feed horns (for HFI on the top sequence, for LFI on the bottom sequence).
The bolometric detectors of the HFI, located behind the horns, absorb the light and heat up slightly. A thermometer reads the temperature rise and converts it to an electrical signal which travels down wires connecting the low- and high-temperature ends of the instruments.
For the LFI, the process is similar, but the conversion to an electrical signal takes place further down the line, beyond the waveguides that connect the focal plane unit to the LFI electronics placed in the service module.
Credits: ESA [images by AOES Medialab])
The High Frequency Instrument on ESA’s Planck mission has completed its survey of the remnant light from the Big Bang. The sensor ran out of coolant on Saturday as expected, ending its ability to detect this faint energy.
“Planck has been a wonderful mission; spacecraft and instruments have been performing outstandingly well, creating a treasure trove of scientific data for us to work with,” said Jan Tauber, ESA’s Planck Project Scientist.
Less than half a million years after the Universe was created in the Big Bang 13.7 billion years ago, the fireball cooled to temperatures of about 4000ºC, filling the sky with bright, visible light.
As the Universe has expanded, that light has faded and moved to microwave wavelengths.
By studying patterns imprinted in that light today, scientists hope to understand the Big Bang and the very early Universe, long before galaxies and stars first formed.
Planck has been measuring these patterns by surveying the whole sky with its High Frequency Instrument (HFI) and its Low Frequency Instrument (LFI).
Combined, they give Planck unparalleled wavelength coverage and the ability to resolve faint details.
Launched in May 2009, 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.
“This gives us even better data than we were expecting from the mission,” said Jean-Loup Puget, Université Paris Sud, Orsay, France, Principal Investigator of HFI.
Able to work at slightly higher temperatures than HFI, the LFI will continue surveying the sky for a large part of 2012, providing calibration data to improve the quality of the final results.
Planck sees not only the primordial microwaves from the Big Bang but also the emission from cold dust throughout the Universe.
(Image: ESA’s Planck spacecraft’s main goal is to study the Cosmic Microwave Background (CMB) – the relic radiation from the Big Bang. It will map the fluctuations in the CMB that became today’s clusters of galaxies.
Released just 380,000 years after the Big Bang, the CMB is the oldest ‘light’ that can be seen in the Universe. Planck will see both nearby and distant clusters of galaxies and be able to use its microwave ‘eyes’ to study cold gas in our Galaxy, the Milky Way. Credits: ESA – C. Carreau).
Initial results from Planck were announced last year. These include a catalogue of galaxy clusters in the distant Universe, many of which had not been seen before and included some gigantic ‘superclusters’ – probably merging clusters.
Another highlight from the initial results was the best measurement yet of an infrared background covering the sky, produced by stars forming in the early Universe.
This showed how some of the first galaxies were producing a thousand times more stars every year than our own Galaxy does today.
More results from Planck will be announced next month, but the first results on the Big Bang and very early Universe will not come for another year.
Extremely careful and painstaking analysis of the data is needed to remove all of the contaminating foreground emission and tease out the faintest, most subtle signals in the remnant emission.
The results are widely anticipated because, despite two previous space missions to map this emission, there are still many competing ideas about what happened during the Big Bang.
“Planck’s data will kill off whole families of models; we just don’t know which ones yet,” said Prof. Puget.
The Big Bang data will be released in two stages, the first 15.5 months’ worth in early 2013, and then the full data release from the entire mission a year after that.
“We’re very pleased with how Planck has performed, well beyond expectations,” said Prof. Alvaro Giménez, ESA’s Director of Science and Robotic Exploration.
“This is a great credit to the work done by the many scientists and engineers involved across Europe and elsewhere in the world.
“In reality though, we’re only halfway through the mission: there’s a lot still to be done to analyse the data and come up with the exciting scientific results that everyone’s anxiously expecting.”
©Typologos.com 2012 – The Article belongs to ESA. Credits of Images and belongs to ESA [images by AOES Medialab]) – C. Carreau.