Is There Anybody Out There?
RAS NAM 2010
SETI have been hard at it, looking for evidence of intelligent life since the mid 1980s. Despite so far finding not very much, they perhaps have cause for cheer as an international team of astronomers have discovered compelling evidence that rocky planets are commonplace in our galaxy. Leicester University scientist and lead researcher Dr Jay Farihi surveyed white dwarfs, the compact remnants of stars that were once like our Sun, and found that many show signs of contamination by heavier elements, possibly even water, improving the prospects for extraterrestrial life.
White dwarf stars are the endpoint of stellar evolution for the vast majority (>90%) of all stars in the Milky Way, including our sun. Since they should have essentially pure hydrogen or pure helium atmospheres, if heavier elements (in astronomy described as ‘metals’, examples including calcium, magnesium and iron) are found then these must be external pollutants. For decades, it was believed that the interstellar medium, the tenuous gas between the stars, was the source of metals in these polluted white dwarfs.
Farihi and his team used data from the Sloan Digital Sky Survey (SDSS), a project that aims to survey the sky in infrared light, imaging more than 100 million objects, and following up 1 million of these by obtaining their spectrum (dispersing the light by colour).
By examining the positions, motions and spectra of the white dwarfs identified in the SDSS, Farihi and his team show that this is no longer a viable theory. Instead, rocky planetary debris is almost certainly the culprit in most or all cases.
The new work indicates that at least 3%, and perhaps as much as 20%, of all white dwarfs are contaminated in this way, with the debris most likely in the form of rocky minor planets, with a total mass of about that of a 140 km diameter asteroid.
This implies that a similar proportion of stars like our sun, as well as stars that are a little more massive such as Vega and Fomalhaut, build terrestrial planetary systems. Astronomers are thus playing the role of celestial archaeologists by studying the ‘ruins’ of rocky planets and their building blocks.
The scientists also measured the composition of the contaminating planetary debris through its chemical signature, which stands out in the otherwise pure atmosphere of the white dwarfs.
Excitingly, it appears that a significant fraction of these stars are polluted with material that contained water, with important implications for the frequency of habitable planets around other stars. If internal water is present in a substantial fraction of asteroids around other stars, like those that contaminated the white dwarfs, it is conceivable that at least simple life may be common throughout the galaxy.
Dr Farihi comments:
“In our own Solar System with at least one watery, habitable planet, the asteroid belt – the leftover building blocks of the terrestrial planets – is several percent water by mass. From our study of white dwarfs, it appears there are basic similarities found among asteroid-like objects around other stars; hence it is likely a fraction of these white dwarfs once harbored watery planets, and possibly life.”
Research like this allows us to make more informed guesses as to the inputs to Drake’s equations. For SETI and others looking to the sky in search of intelligent life, the news that planets capable of supporting life may be, or have been, commonplace will be very welcome indeed.