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Paper: The Role of Stellar Multiplicity in the Prevalence of Small, Cool Planets
Monograph: 10, HWO25 Proceedings Part I: Community Science Case Development Documents
Page: 457
Authors: Elisabeth Newton; Malena Rice; Kendall Sullivan; Jessie Christiansen; Sarah Blunt; Sabina Sagynbayeva
DOI: 10.26624/CQQQ8023
Abstract: Stellar companions separated by < 100 au can reduce the number of observed planets, but what are the effects on temperate, Earth-like worlds? We outline scenarios in which stellar companions could either suppress or enhance the occurrence of small, cool planets. We find that binary star samples sizes > 50 are needed to meaningfully test suppression and enhancement scenarios. To obtain a sample of this size requires pushing HWO’s technical limits for sensitivity and starlight suppression.

This article is an adaptation of a science case document developed as part of HWO’s Demographics and Architectures Steering Committee.

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