The story begins almost 14 billion years ago but we are going to take it up in 1948, when Ralph Alpherin, while doing research on Big Bang together with Robert Herman and George Gamow, predicted the Cosmic Microwave Background (CMB).
The Big Bang theory postulates that 12 to 14 billion years ago, our universe was only a few millimeters across. From this hot dense state it expanded into the vast and much cooler cosmos we currently inhabit. The theory predicts that when the gases cooled, the universe was filled with radiation that is “literally the remnant heat left over from the Big Bang”, called the Cosmic Microwave Background or CMB.
Move forward to 1964 and Arno Penzias and Robert Wilson at the Bell Telephone Laboratories in Murray Hill, New Jersey, were building a radio receiver that they intended to use for radio astronomy and satellite communication experiments. However, something was acting as a source of excess noise in the receiver. At first they put down the disturbance to droppings of a pair of pigeons that were roosting on the antenna and had it extensively cleaned. This still did not get rid of the noise.
Meanwhile, Robert Dicke and other researchers at nearby Princeton University were devising an experiment to find the CMB. Having rejected all possible sources for the noise, Penzias contacted Robert Dicke, who suggested that it might be the predicted background radiation. Both teams published papers in 1965 and Penzias and Wilson shared the 1978 Nobel prize in physics for their discovery.
The CMB is invisible to humans because it is so cold, just 2.725 degrees above absolute zero (minus 459.67 degrees Fahrenheit, or minus 273.15 degrees Celsius). As such,its radiation is most visible in the microwave part of the electromagnetic spectrum. However, it fills the whole universe and can be found everywhere we look. Because it was emitted 13.7 billion years ago, only a few hundred thousand years after the Big Bang, long before stars or galaxies ever existed, studying its properties in detail are helping us understand the conditions in the early Universe.
Which brings us to the iconic image, created out of nine years of data collected by the Wilkinson Microwave Anisotropy Probe (WMAP), which operated from 2001 to 2010.
WMAP’s measurements played a key role in establishing the current Standard Model of Cosmology. The image reveals 13.77 billion year old temperature fluctuations (shown as color differences) that correspond to the seeds that grew to become the galaxies, all of which is helping cosmologists learn about the origin and structures of galaxies, and measure the basic parameters of the Big Bang theory.
And what we have learned is that the young Universe – before there were stars, planets or galaxies – was denser and much hotter. It was filled with a plasma of ionized hydrogen. Expansion resulted in the plasma and radiation cooling down, so that the protons and electrons combined to form hydrogen atoms. While earlier it was opaque, it now became transparent and photons began to travel freely through space instead of being scattered by the earlier electrons and photons.
The WMAP image takes us back to 380,000 years after the Big Bang. And then in 2013, ESA’s Planck space telescope, which replaced WMAP, perfected that picture and gave us the most detailed map ever created of the cosmic microwave background, using over 15 months of data. The new image told us that the Universe is not the same in all directions and so much more.
Look at the image. It us our Universe during its baby years. We are the result of that expansion.
Featured image: ESA/ Planck telescope