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Francesco Pepe, an astronomer who works on HARPS data at the Geneva Observatory, said at the IAU meeting this week that his team could not confirm the existence of Gliese 581g.
This is no surprise at all. First of all the 100% claim was obviously bogus.
Originally posted by fieryjaguarpaw
These so called scientists get everyone excited over a planet that is the first to be found in this made up hypothetical "goldie locks zone" say it has a 100% chance of having life on it and the truth is they aren't even sure if it even exists at all.
"Since Mayor's announcement in 2009 of the lowest-mass planet Gliese 581e, 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 four 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.
Not exactly. The Radial Velocity technique tells us something about the mass, like the minimum mass.
Originally posted by fieryjaguarpaw
I don't think I was being harsh at all.
The way I understand it is that we can detect a planet because of the gravitational effect it has on it's star. So we can detect it's effects but not actually see it. This greater the effect on the star, the greater the size of the planet. But mass and size don't always corralate and gravity isn't well understood, so even things like the size isn't really known.
Radial-velocity: A planet orbiting a star exerts a small gravitational pull which causes the star to wobble very slightly about the system's centre of mass (barycentre). If the planet is aligned edge-on to the Earth we can observe this wobble as a 'Doppler' shift in the emitted light. As the star is pulled away from us its spectrum is shifted towards the red end and as it is pulled towards us it is shifted to the blue end. The gravitational pull from the planet is minute and so very accurate spectroscopic measurements are required. This is the most common type of detection technique and is responsible for the most planets to date. By measuring the radial velocity of a star it is possible to determine the exoplanet's orbital period but only a minimum mass (as the system's inclination is not known). It is also not possible to determine the size of these planets.
Photometry: This is the 'Transit' technique as used by SuperWASP. When a planet passes in front of its parent star edge-on, a decrease in the star's brightness can be detected. Periodic decreases in brightness can indicate the presence of a planet and measurements of the light-curve and spectral type of the star can indicate the size and orbital period of the planet.
It is thought the most likely location for life to exist is on small 'Earth-like' rocky planets within a region of the stellar system known as the 'Habitable zone' where temperatures are suitable for liquid water to form.
Unfortunately these planets are extremely difficult to detect.