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The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30 Day Orbit and a More Massive Outer World

  • Authors: Victoria DiTomasso, David Charbonneau, Andrew Vanderburg, Mercedes López- Morales, Shreyas Vissapragada, Annelies Mortier, Thomas G. Wilson, Elyse Incha, Andrew Collier Cameron, Luca Malavolta, Lars A. Buchhave, David W. Latham, Matteo Pinamonti, Stephanie Striegel, Michael Fausnaugh, Luke Bouma, Ben Falk, Robert Aloisi, Xavier Dumusque, A. Anna John, Ben S. Lakeland, A. F. Martínez Fiorenzano, Luca Naponiello, Belinda Nicholson, Emily K. Pass, Francesco Alfonso Pepe, Federica Rescigno, Alessandro Sozzetti, Daisy A. Turner, Saul A. Rappaport, Mark Omohundro, Brian P. Powell, Robert Gagliano, Thomas L. Jacobs, Veselin B. Kostov, Martti H. Kristiansen, Daryll M. LaCourse, Allan R. Schmitt, Hans Martin Schwengeler, Ivan A. Terentev

Victoria DiTomasso et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 10.

Host star G magnitudes and orbital periods of their sub-Neptunes (2R⊕ < Rp < 4R⊕) with measured masses and radii. We have labeled the only other planets on orbits longer than 25 days around stars brighter than G = 7.5, along with HD 60779 b.

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