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Polarisation of the Cosmic Microwave Background, detail (20 arcminutes scale features)

Polarisation of the Cosmic Microwave Background, detail (20 arcminutes scale features)


Date: 04 February 2015
Satellite: Planck
Copyright: ESA and the Planck Collaboration

A visualisation of the polarisation of the Cosmic Microwave Background, or CMB, as detected by ESA's Planck satellite on a small patch of the sky measuring 20° across.

The CMB is a snapshot of the oldest light in our Universe, imprinted on the sky when the Universe was just 380 000 years old. It shows tiny temperature fluctuations that correspond to regions of slightly different densities, representing the seeds of all future structure: the stars and galaxies of today.

A small fraction of the CMB is polarised – it vibrates in a preferred direction. This is a result of the last encounter of this light with electrons, just before starting its cosmic journey. For this reason, the polarisation of the CMB retains information about the distribution of matter in the early Universe, and its pattern on the sky follows that of the tiny fluctuations observed in the temperature of the CMB.

In this image, the colour scale represents temperature differences in the CMB, while the texture indicates the direction of the polarised light. The curly textures are characteristic of 'E-mode' polarisation, which is the dominant type for the CMB.

In this image, both data sets have been filtered to show mostly the signal detected on scales around 20 arcminutes on the sky. This shows the fine structure of the measurement obtained by Planck, revealing fluctuations in both the CMB temperature and polarisation on very small angular scales.

Another image of the same sky region and data sets, but filtered to show mostly the signal detected on scales around 5° on the sky, is available here.

Last Update: 1 September 2019
1-Jun-2020 13:56 UT

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https://sci.esa.int/s/wK5YdP8

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