Habitable Zones of Host Stars During the Post-MS Phase
Jianpo Guo, Fenghui Zhang, Zhanwen Han

TL;DR
This paper investigates how the habitable zones of stars evolve during post-main sequence phases, identifying potential habitable planets and moons, including Mars, Jupiter, Saturn, and Titan, as stars become brighter and expand their habitable zones.
Contribution
It provides a detailed calculation of the shifting habitable zones during stellar evolution phases using Eggleton's code, highlighting potential habitability of planets and moons outside the main sequence.
Findings
Mars and Jupiter enter habitable zones during stellar evolution
Saturn's orbit becomes habitable for 137 million years during He-burning phase
Titan may become suitable for life during Saturn's habitable phase
Abstract
A star will become brighter and brighter with stellar evolution, and the distance of its habitable zone will become farther and farther. Some planets outside the habitable zone of a host star during the main sequence phase may enter the habitable zone of the host star during other evolutionary phases. A terrestrial planet within the habitable zone of its host star is generally thought to be suited to life existence. Furthermore, a rocky moon around a giant planet may be also suited to life survive, provided that the planet-moon system is within the habitable zone of its host star. Using Eggleton's code and the boundary flux of habitable zone, we calculate the habitable zone of our Solar after the main sequence phase. It is found that Mars' orbit and Jupiter's orbit will enter the habitable zone of Solar during the subgiant branch phase and the red giant branch phase, respectively. And…
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