THE subtle signal of ancient helium has shown up for the first time in light left over from the big bang. The discovery will help astronomers work out how much of the stuff was made during the big bang and how much was made later by stars.
Helium is the second-most abundant element in the universe after hydrogen. The light emitted by old stars and clumps of hot pristine gas from the early universe suggest helium made up some 25 per cent of the ordinary matter created during the big bang.
The new data provides another measure. A trio of telescopes has found helium’s signature in the cosmic microwave background (CMB, pictured), radiation emitted some 380,000 years after the big bang. The patterns in this radiation are an important indicator of the processes at work at that time. Helium affects the pattern because it is heavier than hydrogen and so alters the way pressure waves must have travelled through the young cosmos. But helium’s effect on the CMB was on a scale too small to resolve until now.
By combining seven years of data from NASA’s Wilkinson Microwave Anisotropy Probe with observations by two telescopes at the South Pole, astronomers have confirmed its presence. “This is the first detection of pre-stellar helium,” says WMAP’s chief scientist, Charles Bennett.
These observations are in line with earlier measurements, although less accurate. “I think CMB measurements will surpass them eventually,” says team member David Spergel.
More accurate numbers could reveal how quickly the early universe expanded. Helium forms from the interaction between protons and neutrons. This is constrained by the number of available neutrons, which would have dropped during the time the brand new universe was expanding as they decayed into protons. So the amount of helium that formed places important limits on how quickly this expansion took place. That could help test theories that postulate extra dimensions or as-yet-unseen particles.
Better data should be available in the next few years. The European Space Agency’s Planck satellite, which launched last year, is poised to measure the amount of helium even more precisely.
This glowing stellar nursery is home to the most massive star yet found in the Milky Way galaxy.
Captured by the European Southern Observatory’s 27-foot-diameter Very Large Telescope at Cerro Paranal, Chile, the image above combines data taken with violet, red and infrared filters.
The nebula, NGC 3603, is surrounded by a cloud of glowing gas and dust in the Carina spiral arm of the Milky Way galaxy, about 20,000 light-years from Earth in the Carina constellation. This active star-forming region is one of the brightest and most compact star clusters in our galaxy. The cosmic nursery is teeming with thousands of young, massive suns, including several blue supergiants and three massive Wolf-Rayet stars. These brilliant stars eject huge amounts of mass before blazing out in spectacular supernova explosions. The most massive star in the cluster is 116 times as massive as the sun.
The photo below shows the broader area around the NGC 3603 nebula.
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