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  By observing the transit of the planet using X-rays, the astronomers were able to learn even more about the composition for the planet. First, they discovered that its atmosphere is most likely much larger than originally estimated. They could tell that because the atmosphere of a planet blocks X-rays, but not normal light. In this case, the planet blocked about 2-3 times as big an area of X-rays as it did optical light, meaning the atmosphere extends out quite further. They also ascertained that as a result, the planet is losing its atmosphere at a very fast rate over time.