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(News source: European Space Agency. An Italian version, with an interview to Reno mandolesi, Principal Investigator of Planck LFI, is available on www.media.inaf.it) New images from ESA’s Planck mission reveal details of the structure of the coldest regions in our Galaxy. Filamentary clouds predominate, connecting the largest to the smallest scales in the Milky Way. […]
New images from ESA’s Planck mission reveal details of the structure of the coldest regions in our Galaxy. Filamentary clouds predominate, connecting the largest to the smallest scales in the Milky Way. These images are a scientific by-product of a mission which will ultimately provide the sharpest picture ever of the early Universe.
ESA’s Planck microwave observatory – the first European mission designed to study the Cosmic Microwave Background (CMB) – has begun the second of four sky surveys, which will ultimately provide the most detailed information yet about the size, mass, age, geometry, composition and fate of the Universe. Although the primary goal of Planck is to map the CMB, by surveying the entire sky with an unprecedented combination of frequency coverage, angular resolution, and sensitivity, Planck will also provide valuable data for a broad range of studies in astrophysics. This is clearly demonstrated by new Planck images, published today, which trace cold dust in our Galaxy and reveal the large-scale structure of the interstellar medium filling the Milky Way.
The images are a scientific ‘by-product’ of the data analysis that is currently underway, which aims to produce the highest-sensitivity (a few parts per million), highest-angular resolution (5 arcminutes) maps of the CMB. Part of the analysis process involves peeling away the foreground emission arising from a number of ‘contaminants’ – namely: the cosmic dipole (a signal due to our motion relative to the microwave background), and the radiation from gas and dust in the Milky Way and in distant galaxies – to reveal the underlying map of the CMB. In the process, a series of scientifically valuable maps of this foreground emission is obtained. The maps will be constructed from images like these first Planck snapshots.
One of the key characteristics of Planck is its ability to measure the temperature of the coldest dust particles. Temperature is an important physical indicator as it reflects the balance of energies in the interstellar medium, and changes significantly from place to place, tracing the evolution of the star formation process.
Among the astrophysics-related investigations to be undertaken with Planck is a programme which aims to locate the coldest dusty clumps in the Galaxy, areas where star formation is about to occur. This image demonstrates how Planck traces this cold dust: reddish tones correspond to temperatures as cold as 12 degrees above absolute zero, and whitish tones to much warmer ones (of order a few tens of degrees) in regions where massive stars are currently forming. Planck excels at detecting these dusty clumps across the whole sky and contributes the crucial information required to measure accurately the temperature of dust at these large scales. By combining data from Planck with data from other satellites, such as Herschel or NASA’s Spitzer Space Telescope (both of which probe the very small scales where star formation occurs), and IRAS (which has mapped the whole sky at shorter wavelengths) astronomers will be able to study the formation of stars across the entire Milky Way.
The richness of structure that is observed, and the way in which small and large scales are interconnected, provide important clues to the physical mechanisms underpinning the formation of stars and of galaxies. This example illustrates the synergy between Herschel and Planck; together these missions are imaging both the large-scale and the small-scale structure of our Galaxy.