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Abstract We validate the planetary nature of an ultra-short-period planet orbiting the M dwarf KOI-4777. We use a combination of space-based photometry from Kepler, high-precision, near-infrared Doppler spectroscopy from the Habitable-zone Planet Finder, and adaptive optics imaging to characterize this system. KOI-4777.01 is a Mars-sized exoplanet ( R p = 0.51 ± 0.03 R ⊕ ) orbiting the host star every 0.412 days (∼9.9 hr). This is the smallest validated ultra-short period planet known and we see no evidence for additional massive companions using our HPF RVs. We constrain the upper 3 σ mass to M p < 0.34 M ⊕ by assuming the planet is less dense than iron. Obtaining a mass measurement for KOI-4777.01 is beyond current instrumental capabilities.more » « less
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Haqq-Misra, Jacob ; Wolf, Eric. T. ; Joshi, Manoj ; Zhang, Xi ; Kopparapu, Ravi Kumar ( , The Astrophysical Journal)
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Gilbert, Emily A. ; Barclay, Thomas ; Schlieder, Joshua E. ; Quintana, Elisa V. ; Hord, Benjamin J. ; Kostov, Veselin B. ; Lopez, Eric D. ; Rowe, Jason F. ; Hoffman, Kelsey ; Walkowicz, Lucianne M. ; et al ( , The Astronomical Journal)null (Ed.)