|Back to Press Kit|
|11 January 2011|
Planck is Europe’s first space mission to study the relic radiation from the Big Bang. Ever since the detection of small fluctuations in the temperature of this radiation, announced in late 1992, astronomers have used the fluctuations to understand both the origin of the Universe and the formation of galaxies.
The mission is named after the German physicist Max Planck, whose work on the behaviour of radiation won the Nobel Prize in 1918.
The Planck satellite is observing the cosmic microwave background radiation (CMB). This is the radiation released into the Universe by the Big Bang itself, about 14 thousand million years ago. Since that time, what was once a searing fireball has cooled to become a background sea of microwaves.
Planck is measuring the temperature variations across this microwave background with much better sensitivity, angular resolution and frequency range than any previous satellite. The combination of these factors gives astronomers an unprecedented view of our Universe when it was extremely young: just 380 000 years old.
Planck was launched in tandem with ESA’s Herschel space telescope. Together, they are studying different aspects of the cold cosmos.
Planck’s maps allow a number of specific investigations to take place:
The total cost of the Planck mission is about €700 million. This includes the spacecraft and its scientific payload, the launch and the operations.
Planck was launched on an Ariane 5 from Europe’s Spaceport in Kourou, French Guiana, on 14 May 2009. It was launched together with ESA’s Herschel spacecraft, in a dual launch configuration
Planned mission lifetime
Planck was designed to carry out at least two full sky surveys over a period of 15 months. Instead, Planck's two instruments observed the sky for more than 30 months, allowing it to gather a total of 5 complete surveys of the sky. In January of 2012, the High Frequency Instrument exhausted its supply of Helium and stopped producing scientifically useful data. However, the Low Frequency Instrument continues to operate and is foreseen to continue acquiring observations for a large part of 2012.
The Planck telescope and instruments are mounted on top of an octagonal service module. A baffle surrounds the telescope and instruments to prevent straylight from the Sun and Moon from spoiling the detection of microwave radiation. The baffle is also used to radiate to cold space the heat generated by the focal plane units of the scientific payload, and to provide to the instrument coolers a cold and stable background environment of about –233ºC (or 40K).
Inside the service module are the computers and subsystems that allow the spacecraft to function and to process the raw data signals from the instrument detectors. At the base of the service module is a flat, circular solar panel to generate electricity from sunlight to power the spacecraft, and to protect the whole spacecraft from direct solar radiation.
In order to achieve its scientific objectives, Planck’s detectors have to operate at very low and stable temperatures. The spacecraft is therefore equipped with the means of cooling the detectors to levels close to absolute zero (–273.15ºC), ranging from about –253ºC to only a few tenths of a degree above absolute zero.
Approximately 1950 kg at launch.
Planck is 4.2 m high and has a maximum diameter of 4.2 m.
The prime contractor was Thales Alenia Space (Cannes, France). It led a consortium of industrial partners with Thales Alenia Space (Turin, Italy), who were responsible for the Service Module. A host of subcontractors were spread throughout Europe, with a few more in the USA. ESA and the Danish National Space Centre (Copenhagen, Denmark, funded by the Danish Natural Science Research Council) were responsible for the provision of Planck’s telescope mirrors, which were manufactured by EADS Astrium (Friedrichshafen, Germany).
Low Frequency Instrument (LFI)
Principal Investigator (PI): Nazzareno Mandolesi of the Istituto di Astrofisica Spaziale e Fisica Cosmica in Bologna (Italy).
Deputy Principal Investigator (PI): Marco Bersanelli of the University of Milan (Italy).
LFI was designed and built by a consortium (led by the PI) of scientists and institutes from Italy, Finland, the United Kingdom, Spain, the United States, Germany, the Netherlands, Switzerland, Norway, Sweden and Denmark.
High Frequency Instrument (HFI)
Principal Investigators: Jean-Loup Puget (PI) of the Institut d’Astrophysique Spatiale in Orsay (France) François Bouchet (co-PI) of the Institut d’Astrophysique de Paris.
HFI was designed and built by a consortium (led by the PIs) of scientists and institutes from France, the United States, the United Kingdom, Canada, Italy, Spain, Ireland, Germany, the Netherlands, Denmark and Switzerland.
Many funding agencies contributed to the LFI and HFI instrument hardware; the major ones are: CNES (France), ASI (Italy), NASA (USA), STFC (UK), Tekes (Finland), the Ministry of Education and Science (Spain) and ESA.
Primary Ground Station: ESA’s deep space antenna in New Norcia (Australia).
Planck Mission Manager: Damien Texier
General information about this and other ESA Science missions can be found at: http://www.esa.int/science
Copyright 2000 - 2012 © European Space Agency. All rights reserved.