"With its unprecedented sensitivity, JWST is enabling the most detailed study of the atmospheres of these planets, giving us ...

Far beyond our solar system, in the distant Pegasus constellation, lies a star system that is reshaping our understanding of ...

In this Perspective, we examine the implications of modern cold-accretion and disk-mediated paradigms for two widely cited impact hypotheses: the Moon-forming giant impact and the Late Heavy ...

Detection of hydrogen sulfide in four HR 8799 gas giants provides evidence of solid accretion, clarifying how massive exoplanets form and distinguishing them from brown dwarfs ...

Abstract: This paper introduces a control strategy for servohydraulic systems, inspired by the complex mechanical processes of Planet Formation. The proposed controller is designed around four ...

One way gas giants form is through core accretion, where solid cores gradually grow in a disk by pulling in rocky and icy pebbles until they become massive enough to attract the gas that surrounds ...

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WASHINGTON — NASA is ending financial support for several planetary science groups as part of a broader drawdown of the agency’s advisory structure. In a Jan. 16 letter, Louise Prockter, director of ...

Astronomers tracked a decade of dramatic changes in P13, a neutron star undergoing supercritical accretion. Its X-ray luminosity rose and fell by factors of hundreds while its rotation rate ...

Astronomers have identified a white dwarf system, LSPM J0207+3331, that continues to accrete material from its former planetary system 3 billion years after the star’s death, as reported by Universe ...

Astronomers found an ancient planetary system being consumed by white dwarf LSPM J0207+3331, hosting the oldest, most metal-rich debris disk known. (Nanowerk News) Astronomers have identified a rare, ...

This artist’s illustration shows a 3-billion-year-old white dwarf star accreting material from the remnants of its former planetary system. Gravitational instabilities caused a surviving planet to ...