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Spectra of the atmosphere of the planet GJ436b in the constellation Loe show evidence for carbon monoxide. Theoretical studies using numerical models however predicted that this planet's carbon inventory should be stored in the form of methane rather than CO as its temperature is estimated to be 800K. Where this inaccuracy of atmospheric models comes from is not known and has to be investigated further.

To determine the mass of an exoplanet using transmission spectroscopy, de Wit relied on the effect that a planet's mass has on its atmosphere, as transmission spectra give information on a planet's atmospheric properties. To do that, he worked from a standard equation describing the effect of a planet's temperature, gravitational force, and atmospheric density on its atmospheric pressure profile-the extent to which pressure changes throughout its atmosphere.

antihydrogen propulsion...?

didn't roger write an assessment of antimatter propulsion when he was in the ACT?

yeah the problem is the amount of antimatter you can get and more specifically how to trap it. I found that you would need around one gram to go to the outer Solar System. So we are far from that, but finding an efficient way to trap it, with an electromagnetic trap rather than solid walls is a first step !