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Webb Turns A Dead-Star Planet Into The Solar System's Future

NASA's Webb telescope has turned a planet around a dead star into a preview of our own solar system's far future. WD 1856 b is a Jupiter-size exoplanet orbiting a white dwarf every 34 hours at less than 2 million miles from the remnant star. [1]

The paper's July 1 account of Rubin Observatory opening its sky survey argued that space science matters when it changes who can observe and verify the sky. Webb's new result is the opposite scale but the same discipline: one planet, one dead star, and a chain of inference that makes a cosmic future measurable. [1]

The basic puzzle is survival. A Sun-like star swelled into a red giant before shedding its outer layers and becoming a white dwarf. A planet now orbits the remnant 50 times closer than Earth orbits the Sun. If it had been there during the red-giant phase, NASA says, it should have been destroyed. [1]

Webb watched the planet transit the star, measured its temperature at about 260 degrees Fahrenheit, and detected atmospheric signatures including methane. The warmth matters because the white dwarf cannot explain it by current heating alone. Researchers concluded the planet most likely migrated inward later, warmed by gravitational interactions, and has been cooling ever since. [1]

This is where the X/MSM gap appears. X will share the art: a giant orange world beside a tiny white spark. MSM will headline the wonder of a planet that survived a star's death. The useful story is quieter. A measurement of heat becomes a history of motion. Methane becomes evidence that an atmosphere can be read around a dead star. A strange world 80 light-years away becomes a laboratory for Jupiter, Saturn, Uranus and Neptune after the Sun runs out of hydrogen. [1]

NASA says the Sun will swell into a red giant in about five billion years, destroying Mercury, Venus and possibly Earth, then ending as a white dwarf. The outer planets' fate is less certain. WD 1856 b is not a prophecy. It is a test case for how planets can survive, migrate, and remain readable after their stars die. [1]

-- KENJI NAKAMURA, Tokyo

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[1] https://science.nasa.gov/missions/webb/nasas-webb-studies-how-planet-survived-death-of-its-star/

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