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The NEID Earth Twin Survey. IV. Confirming an 89 days, ﹩m\,\sin \,i=10\,{M}_{\oplus }﹩ Planet Orbiting a Nearby Sun-like Star

  • Authors: Mark R. Giovinazzi, Evan Fitzmaurice, Arvind F. Gupta, Paul Robertson, Suvrath Mahadevan, Eric B. Ford, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, Jiayin Dong, Rachel B. Fernandes, Samuel Halverson, Te Han, Shubham Kanodia, Daniel M. Krolikowski, Sarah E. Logsdon, Joe P. Ninan, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Ryan C. Terrien, Jason T. Wright

Mark R. Giovinazzi et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Orbital architectures of known three-planet systems in the NASA Exoplanet Archive. Host stars are shown along the y-axis, with planet orbital periods on the x-axis. Marker size scales with planet mass, and marker shape distinguishes ﹩m\sin i﹩ measurements (triangles) from true masses (circles). The HD 190360 system is highlighted in green.

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