# Interaction of Stars Hosting Planets with Sgr A* Black hole

**Authors:** Nazanin Davari, Roberto Capuzzo-Dolcetta, Rainer Spurzem

arXiv: 1908.06298 · 2020-03-18

## TL;DR

This paper investigates the potential survival and evolution of planetary systems around stars near the Galactic Center's supermassive black hole, focusing on their interactions and fate after close encounters.

## Contribution

It presents preliminary results on the dynamics and survivability of planetary systems around S-stars influenced by the Sgr A* black hole.

## Key findings

- Planetary systems may survive close interactions with Sgr A*
- Migration history affects planetary system stability
- Preliminary models suggest possible retention of planets

## Abstract

We present some preliminary results of our ongoing project about planetary systems around S-stars in the vicinity of Sgr A* black hole. Since S-stars might have migrated in the Galactic Centre (GC) from elsewhere, they probably still keep their planetary systems throughout their voyage. In this work, we study the destiny of their putative planetary systems after close interaction with the central black hole of our galaxy.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1908.06298/full.md

## References

15 references — full list in the complete paper: https://tomesphere.com/paper/1908.06298/full.md

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Source: https://tomesphere.com/paper/1908.06298