Polarization of the Cosmic Microwave Background: Detail (20 Arcminutes) (image) International School of Advanced Studies (SISSA) Share Print E-Mail Caption This is a visualization of the polarization of the Cosmic Microwave Background, or CMB, as detected by ESA's Planck satellite on a small patch of the sky measuring 20º 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 polarized -- 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 polarization 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 color scale represents temperature differences in the CMB, while the texture indicates the direction of the polarized light. The curly textures are characteristic of "E-mode" polarization, 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 polarization on very small angular scales. Credit Credits: ESA and the Planck Collaboration Usage Restrictions None Share Print E-Mail Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.