When our Sun dies, it will turn into a white dwarf. They are a common aspect of stellar evolution and a team of researchers have now turned their attention onto them. They have just completed a survey of 26,000 white dwarfs and confirmed a long-predicted theory that the hotter the star, the puffier it is! This new study will help us to understand white dwarfs and the processes that drive them. All stars age. Our Sun is a giant ball of electrically charged gas and, during the majority of its life will be fusing hydrogen to helium in its core. During this process, the fusion will generate an outward pushing force known as thermonuclear pressure which will for the most part, balance the inward pull of gravity. Eventually, the thermonuclear force will overcome the force of gravity and the star will shed its outer layers, leaving behind a dense, hot core. The core is known as a white dwarf and it is this which, despite its small size and incredibly high density, has captivated astron...
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