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First direct detection of an exoplanet by optical interferometry Astrometry and K-band spectroscopy of HR 8799 e

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  • First direct detection of an exoplanet by optical interferometry Astrometry and K-band spectroscopy of HR 8799 e
Astronomy

To date, infrared interferometry at best achieved contrast ratios of a few times 10−4 on bright targets. GRAVITY, with its dual-field mode, is now capable of high contrast observations, enabling the direct observation of exoplanets. We demonstrate the technique on HR 8799, a young planetary system composed of four known giant exoplanets.

https://doi.org/10.1051/0004-6361/201935253

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