New Issue: Science’s Impossible Questions. Read Now

Cosmic Microwave Background Radiation's Polarization Detected at Last

Join Our Community of Science Lovers!


On supporting science journalism

If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today.


Although it was discovered less than 40 years ago, the cosmic microwave background (CMB) radiation has been around a lot longer than that. A relic from the early days of the Universe more than 14 billion years ago, the CMB is the oldest radiation on record. Current cosmological models posit that the CMB should be slightly polarized but this property has never been observed--until now. Researchers have successfully detected the CMB's polarization and found that it agrees with the theoretical estimates.

Erik Leitch and John Kovac of the University of Chicago and their colleagues used the Degree Angular Scale Interferometer (DASI), which is located at the Amundsen-Scott South Pole Station, to study the CMB radiation. Over a two-year period, this array of radio telescopes collected radiation signals coming from deep space in two patches of blank sky. The resulting 271 days worth of useable data revealed the light's polarization (the direction in which the light's field oscillates as it travels toward an observer on the ground). Writing in the journal Nature, the scientists report that the CMB radiation's level and spatial distribution are in excellent agreement with the predictions of the standard theory. "If the light hadn't been polarized, that would mean that we would have to throw out our whole model of how we understand the physics of the early universe," Leitch notes. In an accompanying commentary, Matias Zaldarriaga of New York University calls the findings "both a remarkable technical achievement and a wonderful consistency check for the theory."

Subscribe to Support Independent Journalism

Great science journalism requires human expertise, time, effort and creativity. And it costs money. That’s why I and the journalists here at Scientific American hope you’ll join our community.

When you subscribe, you are supporting staff and freelance journalists who are passionate about telling science stories that are true, important and compelling. Our editors and reporters are often experts in their fields, which means they understand the nuances of big discoveries and can untangle the breakthroughs from the hype. With a subscription, you are also supporting rigorous fact-checking to ensure the words we publish are precise and accurate. And you’re supporting original illustrations, graphics and photos that bring you closer to an advanced laboratory, an ice sheet in Antarctica or a space mission in orbit. You’re helping us craft other types of high-quality journalism as well: Our newsletters are carefully written, edited and curated by staffers you have or will come to know and love. Our Science Quickly podcast is based on original reporting, collaboration with editors and scientists and exacting production.

Subscriptions keep this engine running so we can continue to deliver thoughtful, rigorous and independent science journalism to you. In an era of viral misinformation, this work is crucial. If you value what we do, I hope you’ll consider joining us as a subscriber

Thank you,

Jeanna Bryner, Editor in Chief, Scientific American

Subscribe