Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star

Direct imaging of gas giant exoplanets provides information on their atmospheres and the architectures of planetary systems. However, few planets have been detected in blind surveys with direct imaging. Using astrometry from the Gaia and Hipparcos spacecraft, we identified dynamical evidence for a gas giant planet around the nearby star HIP 99770. We confirmed the detection of this planet with direct imaging using the Subaru Coronagraphic Extreme Adaptive Optics instrument. The planet, HIP 99770 b, orbits 17 astronomical units from its host star, receiving an amount of light similar to that reaching Jupiter. Its dynamical mass is 13.9 to 16.1 Jupiter masses. The planet-to-star mass ratio [(7 to 8) x 10-3] is similar to that of other directly imaged planets. The planet's atmospheric spectrum indicates an older, less cloudy analog of the previously imaged exoplanets around HR 8799.

Automated summary

Using direct imaging, we have discovered a gas giant exoplanet, HIP 99770 b, located around 17 astronomical units away from its host star. The planet has a mass of 13.9 to 16.1 Jupiter masses and a similar atmospheric spectrum to previously imaged exoplanets around HR 8799.