The Future of Exoplanet Direct Detection John D. Monnier , Gioia Rau , Ellyn K. Baines , J. Sánchez-Bermúdez , Martin Elvis , Sam Ragland , Rachel Akeson , Gerard van Belle , R. P. Norris , K. Gordon , Denis Defrère , S. Ridgway , Jean-Baptiste Le Bouquin , Narsireddy Anugu , Nicholas J. Scott , Stephen R. Kane , Noel D. Richardson , Zsolt Regaly , Zhaohuan Zhu , А. Чиавасса , Gautam Vasisht , Keivan G. Stassun , Chuanfei Dong , Olivier Absil , S. Lacour , G. Weigelt , Douglas R. Gies , Fred C. Adams , Nuria Calvet , Sascha P. Quanz , Catherine Espaillat , Tyler Gardner , Alexandra Z. Greenbaum , R. Millan‐Gabet , C. Packham , M. Gai , Quentin Kral , Jean–Philippe Berger , H. Linz , L. Klarmann , Jaehan Bae , Rebeca Lopez Garcia , A. Gallenne , Fabien Baron , Lee Hartmann , M. Kishimoto , Melissa McClure , Johan Olofsson , C. Haniff , Michael R. Line , Romain G. Petrov , Michael S. Smith , Christian A. Hummel , T. ten Brummelaar , Matthew De Furio , Stephen A. Rinehart , David Leisawitz , W. C. Danchi , Daniel Huber , Edward H. Wishnow , D. Mourard , Benjamin Pope , Michael Ireland , Stefan Kraus , Benjamin R. Setterholm , Russel White Bulletin of the American Astronomical Society（2019）
摘要
Diffraction fundamentally limits our ability to image and characterize exoplanets. Interferometry offers some advantages in exoplanet detection and characterization and we explore in this white paper some of the potential scientific breakthroughs possible.
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