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- W2200200051 endingPage "1321" @default.
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- W2200200051 abstract "Orbits don't forget their chaotic pasts Many exoplanets orbit in planes that don't correspond to their star's spin axis. This phenomenon may be the fossil record of a dynamical history. Storch et al. demonstrate in simulations that the evolution of a star's spin is key in determining how its planets' orbits are eventually oriented. A binary companion body can drive a hot Jupiter to migrate inward, which induces chaotic behavior in the stellar spin axis and feedback down the line. If we can accurately replicate the statistics observed in planetary surveys, we may understand better how planets form. Science , this issue p. 1317" @default.
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- W2200200051 date "2014-09-12" @default.
- W2200200051 modified "2023-09-30" @default.
- W2200200051 title "Chaotic dynamics of stellar spin in binaries and the production of misaligned hot Jupiters" @default.
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- W2200200051 doi "https://doi.org/10.1126/science.1254358" @default.
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