A team of astronomers headed by Dr Nikku Madhusudhan of the Cambridge University’s Institute of Astronomy has found that the abundance of water vapor in the atmospheres of the three newly discovered hot Jupiters – HD 189733b, HD 209458b, and WASP-12b – is between ten and a thousand times less than what standard planet formation theories predict. This is an illustration of a hot Jupiter orbiting a Sun-like star. According to the core...