TOI-201 Exoplanet System

New Planet Recently Confirmed in a chaotic young system// TOI-201 also known as HD 39474, is an F6V type star located in the southern constellation of Pictor about 366 light years away. Being only a little under 700 million years old, the system it gave birth to is chaotic with a brown dwarf companion (TOI-201c), a hot jupiter (TOI-201b), and most recently confirmed: an innermost rocky planet (TOI-201d). Such system as one may expect, is subject to immense change and will not be observable via the transit method that is used right now in about 200 or so years due to such strong gravitational interactions between the objects. However it is expected to make a reappearance in 10000 years. I presume much of the data particuraly in composition and appearance as well as temperature which I had to set myself due to this game's horrendous thermodynamics engine. SPECIAL THANKS to: "definitely not a tau" and "Kapteyn" for the gas giant templates used for TOI-201b and TOI-201c respectively. Greatly appreciate your work in making them since I do not have that kind of patience. Works Cited Jones, Matías I., et al. “A Very Eccentric Brown Dwarf Coplanar to a Warm Jupiter and a Hot Super Earth.” ArXiv.org, Cornell University, 27 Apr. 2026, arxiv.org/abs/2604. 23926. Accessed 13 May 2026. Maciejewski, Gracjan, and Weronika Łoboda. “A Transiting Giant on a 7. 7 Yr Orbit Revealed by Transit Timing Variations in the TOI-201 System.” The Astrophysical Journal Letters, vol. 988, no. 2, July 2025, p. L63, https://doi.org/10. 3847/2041-8213/adefe5. IOPscience. Accessed 13 May 2026. Mireles, Ismael, et al. “Uncovering the Rapidly Evolving Orbits of the Dynamic TOI-201 System.” Science Advances, vol. 12, no. 16, American Association for the Advancement of Science, Apr. 2026, pp. eaef2618–18, https://doi.org/10. 1126/sciadv.aef2618. Science.org. Accessed 13 May 2026.