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Planetary Systems Around White Dwarfs
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White dwarf planetary science is a rapidly growing field of research featuring a diverse set of observations and theoretical explorations. Giant planets, minor planets, and debris discs have all been detected orbiting white dwarfs. The innards of broken-up minor planets are measured on an element-by-element basis, providing a unique probe of exoplanetary chemistry. Numerical simulations and analytical investigations trace the violent physical and dynamical history of these systems from au-scale distances to the immediate vicinity of the white dwarf, where minor planets are broken down into dust and gas and are accreted onto the white dwarf photosphere. Current and upcoming ground-based and space-based instruments are likely to further accelerate the pace of discoveries.
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Cited by 1 Pith paper
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Thermal Emission and Confirmation of the Frigid White Dwarf Exoplanet WD 1856+534b
JWST MIRI photometry detects 15-18 micron thermal emission from WD 1856+534b, yielding a 186 K temperature and a mass below 5.9 Jupiter masses, confirming it as a planet in a white dwarf's forbidden zone.
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