Astronomers released the latest and most exquisite baby picture yet of the universe on Thursday, one that showed it to be 80 million to 100 million years older and a little fatter, with more light and dark matter than previously thought, and perhaps ever so slightly lopsided. Recorded by the European Space Agency's Planck satellite, the image is a heat map of the cosmos as it appeared only 380,000 years after the Big Bang, showing space speckled with faint spots from which galaxies would grow over billions of years. It shows the seeds from which the current universe grew. Marc Kamionkowski, Johns Hopkins University The map, the Planck team said is in stunning agreement with the general view of the universe that has emerged during the past 20 years, of a cosmos dominated by dark energy that is pushing it apart, and dark matter that is pulling galaxies together. It also shows a universe that seems to have endured an explosive burp known as inflation, which was the dynamite in the Big Bang. A view of the cosmic microwave background collected by the European Space Agency?s Planck satellite. The heat map of the cosmos was imprinted on the sky when the universe was just 380,000 years old. Photo: ESA In a statement issued by the European Space Agency, Jean-Jacques Dordain, its director-general, said, "The extraordinary quality of Planck's portrait of the infant universe allows us to peel back its layers to the very foundations, revealing that our blueprint of the cosmos is far from complete." Marc Kamionkowski, an astrophysicist at Johns Hopkins University who commented on the work at a news teleconference sponsored by NASA, called Planck "cosmology's human genome project." "It shows the seeds from which the current universe grew," he said. A map of relic radiation (microwave sky) from the Big Bang. David N. Spergel, a Princeton University cosmologist, described the new results as "beautiful," adding that "the standard cosmological model looks even stronger today than yesterday. The universe remains simple and strange. Within the standard cosmological framework, however, the new satellite data underscored the existence of puzzling anomalies that may yet lead theorists back to the drawing board. The universe appears to be slightly lumpier, with bigger and more heat spots on one side than on the other, for example, and there is an unexplained cool spot in the middle of the map. Those anomalies had shown up on previous maps by NASA's Wilkinson Microwave Anisotropy Probe, or WMAP, satellite, but some had argued that they were because of a bad analysis or contamination from the Milky Way. The evolution of satellites designed to measure ancient light left over from the Big Bang: From left: NASA's Cosmic Background Explorer, or COBE, 1989; the Wilkinson Microwave Anisotropy Probe, or WMAP, 2001; Planck, 2009. Now cosmologists will have to take them more seriously, said Max Tegmark, an expert on the early universe at the Massachusetts Institute of Technology, who was not part of the Planck team and who called the new results "very exciting." It could be, he said, that "the universe is trying to tell us something." George Efstathiou of Cambridge University, one of the leaders of the Planck project, said in the European Space Agency news release: "Our ultimate goal would be to construct a new model that predicts the anomalies and links them together. But these are early days; so far, we don't know whether this is possible and what type of new physics might be needed. And that's exciting. The Planck satellite was launched in 2009 and has been scanning the sky ever since, recording the faint variations in a haze of radio microwaves that fill the sky. Those microwaves are believed to be the cooled-off remains of the fires of the Big Bang, shown 380,000 years later, when the first hydrogen atoms formed. The microwaves were discovered by accident in 1965 by a pair of Bell Labs radio astronomers, Arno Penzias and Robert W. Wilson, who later won the Nobel Prize in Physics. Using balloons, a U-2 spy plane and a series of satellites like the WMAP, astronomers have been teasing out the detailed features of this radiation. Analysing the relative sizes and frequencies of spots and ripples has allowed astronomers to describe the birth of the universe so precisely that it would make the philosophers weep. The new data have allowed astronomers to tweak their model a bit. It now seems the universe is 13.8 billion years old, instead of 13.7 billion, and consists by mass of 4.9 per cent atoms, 27 per cent dark matter and 71 per cent dark energy. The biggest surprise here, astronomers said, is that the universe is expanding slightly more slowly than previous measurements had indicated. The Hubble constant, which characterises the expansion rate, is 67 kilometres per second per megaparsec - the units astronomers use - according to Planck. Recent ground-based measurements combined with the WMAP data gave a value of 69, offering enough of a discrepancy to make cosmologists re-run their computer simulations of cosmic history. The fact that astronomers once would go to war with one another over a factor of two in measurements of this parameter shows how cosmology has progressed over the past 20 years. Pressed for a possible explanation for the discrepancy, Martin White, a Planck team member from the University of California, Berkeley, said it represents a mismatch between measurements made at the beginning of time and those made more recently. He said it could mean that dark energy, which is speeding up the expansion of the universe, is more complicated than cosmologists thought. He termed the possibility "pretty radical," adding, "That would be pretty exciting." The data also offered striking support for the notion of inflation, which has been the backbone of Big Bang theorising for 30 years. Under the influence of a mysterious force-field during the first fraction of a second, what would become the observable universe ballooned by 100 trillion trillion times in size from a subatomic pinprick to a grapefruit in less than a violent eye-blink, according to the story first enunciated by Alan Guth of MIT. Submicroscopic quantum fluctuations in this force-field are what would produce the hot spots in the cosmic microwaves, which in turn would grow into galaxies. According to Planck's measurements, those fluctuations so far fit the predictions of the simplest model of inflation, invented by Andrei Linde of Stanford, to a tee. Dr Tegmark of MIT said, "We're homing in on the simplest model." Cosmologists still don't know what might have caused inflation, but the recent discovery of the Higgs boson has provided evidence that the kinds of fields that can provoke such behaviour really exist. Dr Tegmark and others said that another clue to the nature of inflation could come from the anomalies in the microwave data, which tend to happen on the largest scales in the universe. By the logic of quantum cosmology, they were the first patterns to be laid down on the emerging cosmos - that is to say, when inflation was just starting. He compared it to walking in someplace and encountering a fight. If the fight had been going on for a while, he said, it is impossible to tell who started it or who was hurt first. But if you come in only a few seconds after it started, you have a better chance of figuring out who did what to whom. "It may be," he said, "we're coming in early to the cosmic brawl."