Astronomers recently announced the discovery of the first potentially habitable extrasolar planet, Gliese 581 g which is thought to have three times the mass of Earth, and to orbit in the middle of its star's habitable zone, meaning liquid water could exist on the planet's surface.
But this week at an International Astronomical Union meeting, doubts were raised about the existence of this exciting new planet said to be orbiting the star Gliese 581.
Called ‘Gliese 581 g,’ the planet was determined to a rocky world, not a gas giant like Jupiter. Rocky extrasolar planets have been found before, but the unique trait about this planet was that it orbited within the red dwarf star’s habitable zone, that region of space where temperatures are sufficient for water to remain as a liquid on a planetary surface.
Astrobiologists were thrilled at the news, since liquid water is considered necessary for the origin and evolution of life. In fact, NASA has made it a primary aim to ‘follow the water’ in the search for life elsewhere in the galaxy.
Enter Francesco Pepe, an astronomer who works on HARPS data at the Geneva Observatory, who said at the IAU meeting this week that his team could not confirm the existence of Gliese 581 g. In email correspondence with Astrobiology Magazine, Pepe said that they could not confirm the existence of planet ‘f’ either.
The Geneva team, led by Michel Mayor, announced in 2009 the discovery of planet ‘e’ in the Gliese 581 solar system. At approximately 1.9 Earth masses, this ‘e’ planet is the lowest mass extrasolar planet yet found, and has a 3.15-day orbital period around the star.
“Since Mayor's announcement in 2009 of the lowest-mass planet Gliese 581 e, we have gathered about 60 additional data points with the HARPS instrument for a total of 180 data points spanning 6.5 years of observations,” said Pepe. “From these data, we easily recover the 4 previously announced planets b, c, d, and e.”
However, he said they do not see any evidence for planet ‘g’, the fifth planet in the system as announced by Vogt and his team.
“The reason for that is that, despite the extreme accuracy of the instrument and the many data points, the signal amplitude of this potential fifth planet is very low and basically at the level of the measurement noise,” said Pepe.
The planets in the Gliese 581 system were discovered using spectroscopic radial velocity measurements. Planets ‘tug’ on the star they orbit, causing it to shift in position (stars and planets actually orbit a common center of mass). By measuring the star’s movement in the sky, astronomers can figure out what sort of planets are orbiting it.
Multi-planet systems create a complicated signal, and astronomers must tease out the spectral lines to figure out what represents a planet, and what is just “noise” – shifts in the star light not caused by an orbiting planet. Astronomers have developed various ways to reduce such noise in their telescopic observations, but it still creates a level of uncertainty in detecting extrasolar planets.
The Geneva team plugged the HARPS data on Gliese 581 into computer models to check on the odds the signal was the result of noise, rather than evidence of the habitable planet ‘g’ as claimed by the Lick-Carnegie team.
“Simulations on the real data have shown that the probability that such a signal is just produced 'by chance' out of the noise is not negligible, of the order of several percents,” Pepe said. “Under these conditions we cannot confirm the presence of the announced planet Gliese 581 g.”
Pepe noted that while he did not speak at the IAU meeting about Gliese 581 f, the other potential planet in this system announced by the Lick-Carnegie team, the HARPS data calls that planet into question as well.
“We haven't made a detailed analysis yet, but at first glance no statistically significant signal [for planet f] is emerging from our data set,” he said.
Gliese 581 is already one of the most intriguing solar systems known, with four planets confirmed orbiting the star. The addition of the potentially habitable planet ‘g’ would make the system the go-to place in the search for alien life, but more work needs to be done to either confirm or refute the planet’s existence.
Jason McManus via Astrobio.net