Quote:
Originally Posted by Baldrick
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Actually, it is the planet's proximity to the AB Doradus Moving Group (ABDMG), a nearby star cluster, that allows astronomers to guess its age, metallicity, and density. They also gave it a spectral type of T7/T7.5 which makes it a T Dwarf or Brown Dwarf, but well under the 13 Jupiter masses required to burn deuterium.
They still do not have a parallax for CFBDSIR2149 yet. They used a combination of redshift and the distance to the ABDMG as an estimate of its distance. Spectral analysis shows it to be a low density Brown Dwarf, with a gravity estimated to be between 3.75 and 4.0 G. The spectrum also indicates its age to be between 20 and 200 million years old, however, because there is an 87% probability that it is a member of the ABDMG which is known to be younger than 150 million years, they are claiming the rogue planet is between 20 and 150 million years old, with a 95% probability that the Brown Dwarf is younger than 150 million years.
Source:
http://arxiv.org/pdf/1210.0305v1.pdf