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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 5.

Dynamical separation distributions for the three combinations of interacting planets. We observe that all three combinations have Δ > 12 by a relatively wide margin. A priori, interactions between HD 190360 c and HD 190360 d would be expected to be the largest, and so their Δ distribution being the highest is a promising indicator that this configuration of planets would have been long-term stable.

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