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    Fact Sheet

    Fact Sheet: Planck is the first European mission to study the birth of the Universe
      Planck is the first European mission to study the birth of the Universe
    Planck will help provide answers to some of the most important questions in modern science: how did the Universe begin, how did it evolve to the state we observe today, and how will it continue to evolve in the future? Planck's objective is to analyse, with the highest accuracy ever achieved, the remnants of the radiation that filled the Universe immediately after the Big Bang - this we observe today as the Cosmic Microwave Background.

    Mission Objectives

    The primary science goals of Planck include:

    • Mapping the Cosmic Microwave Background anisotropies with improved sensitivity and angular resolution
    • Testing inflationary models of the early Universe
    • Measuring the amplitude of structures in the Cosmic Microwave Background
    • Determination of Hubble constant
    • Perform measurements of Sunyaev-Zel'dovich effect

    Mission Name

    Planck, originally named COBRAS/SAMBA, was renamed on approval of the mission in 1996 in honour of the German scientist Max Planck (1858-1947) who won the Nobel Prize for Physics in 1918. J.C. Mather and G.F. Smoot have received the Nobel Prize for Physics in 2006 for their discovery of the blackbody nature of the Cosmic Microwave Background radiation and the small-scale deviations from the blackbody curve.

    Spacecraft

    Mass - about 1900 kg at launch

    Dimensions - 4.2 m high, 4.2 m maximum diameter 

    Launcher - Ariane 5 ECA from Guiana Space Centre

    Mission Lifetime - 15 months nominal from end of Calibration and Performance Verification Phase

    Wavelength - Microwave: 27 GHz to 1 Thz

    Telescope - 1.9×1.5m primary mirror (1.5m projected aperture)

    Instruments


    HFI
    High
    Frequency Instrument
    Description 83 GHz - 1 THz
    Array of 52 bolometric detectors, operated at 0.1K
    Principal Investigator Jean-Loup Puget,
    Institut d'Astrophysique Spatiale (Orsay, France)
    Deputy Principal Investigator François Bouchet,
    Institut d'Astrophysique de Paris (Paris, France)
     
    LFI
    Low
    Frequency Instrument
    Description 27 - 77 GHz
    Array of 22 tuned radio receivers, operated at 20K
    Principal Investigator Nazzareno Mandolesi,
    Istituto di Tecnologie e Studio delle Radiazioni Extraterrestri (Bologna, Italy)
    Deputy Principal Investigator Marco Bersanelli,
    Universita' degli Studi di Milano (Milan, Italy)

    Orbit

    Planck was launched on an Ariane 5 ECA rocket together with ESA's Herschel spacecraft on 14 May 2009, at 13:12 UTC.The two spacecraft separated after launch and were directly injected towards the second Lagrange point of the Sun-Earth system. On 3 July, following a few orbit correction manoeuvres, Planck reached its final operational orbit: a Lissajous orbit with an average amplitude of about 400 000 km around the L2 point at a distance of around 1.5 million km from Earth.

    Operations Centre

    The ground segment of Planck is composed of the Operations Ground Segment, comprising all the elements under the responsibility of the European Space Operations Centre (ESOC), which includes the Mission Operations Centre, the ground stations and the communications network, and the Scientific Ground Segment.

    The Mission Operations Centre (MOC) is located at ESA's European Space Operations Centre (ESOC) in Darmstadt, Germany. For communication with the spacecraft ESA's 35-m deep-space antenna at New Norcia (close to Perth, Australia) is the prime ground station, and Cebreros (close to Avila, Spain) is the back-up.

    The Scientific Ground Segment is distributed between the following centres: the Planck Science Office, taking care of the scheduling of the survey strategy, and the two instrument teams' Data Processing Centres and Instrument Operations Teams, responsible for each instrument to process the telemetry and monitor the instrument operations respectively.


    Last Update: 14 Dec 2012

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