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ESA’s Planck Proves Potential

September 18, 2009

The Planck mission has captured its first rough images of the sky, demonstrating the observatory is working and ready to measure light from the dawn of time. Planck — a European Space Agency (ESA) mission with significant NASA participation — will survey the entire sky to learn more about the history and evolution of our universe.

Planck's first image (ESA JPL)

The space telescope started surveying the sky regularly August 13th from its vantage point far from Earth. Planck is in orbit around the second Lagrange point of our Earth-sun system, a relatively stable spot located 930,000 miles (1.5 million kilometers) away from Earth. Following launch May 14th, the satellite’s subsystems were checked out in parallel with the cool-down of its instruments’ detectors. The detectors are looking for temperature variations in the cosmic microwave background, which consists of microwaves from the early universe. The temperature variations are a million times smaller than 1 degree. To achieve this precision, Planck’s detectors have been cooled to extremely low temperatures, some of them very close to the lowest temperature theoretically attainable. Instrument commissioning, optimization, and initial calibration were completed by the second week of August.

During the “first-light” survey, which took place August 13 to 27, Planck surveyed the sky continuously. It was carried out to verify the stability of the instruments and the ability to calibrate them over long periods to the exquisite accuracy needed. The survey yielded maps of a strip of the sky, one for each of Planck’s nine frequencies. Preliminary analysis indicates that the quality of the data is excellent. Routine operations will now continue for at least 15 months without a break. In this time, Planck will be able to gather data for two full independent all-sky maps. To fully exploit the high sensitivity of Planck, the data will require a great deal of delicate calibrations and careful analysis. The mission promises to contain a treasure trove of data that will keep cosmologists and astrophysicists busy for decades to come.

Filed Under: Exploration & Science Missions

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