Dynamical Packing in the Habitable Zone by Kane

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Table of Contents

Introduction
Summary
Reflection
Conclusion
Work Cited

Introduction

Earth is the only known to scientists planet that has life. However, researchers have been trying to estimate the number of planets in other solar systems that have the potential of containing life. In the article Dynamical Packing in the Habitable Zone: The Case of Beta CVn, Kane et al. focus on exploring other inhabitable planets. This paper will summarize the article by Kane et al. and present a reflection on the matter.

Summary

The study in question was published in The Astronomical Journal and Science Direct. The topic of the research article relates to many scientific fields and issues, including physics and biology. The study was conducted by Kane et al., and the researchers focused on examining Earth-like planets. Past research on this topic focused on the exploration of the so-called habitable zone, which is an area near a star where orbiting planets can have a liquid (Surprising number of exoplanets could host life). Trappist-1 is a solar system located not far from the Solar System, and previously three planets within this system that can have water were identified by scientists. Therefore, the objective of the examined research was to determine whether Trappist-1 can have other inhabitable planets.

The researchers used computer modeling and the input of data about Trappist-1 to determine the gravity and other forces. As a result, Kane et al. found that within this solar system, some stars could support up to seven inhabitable planets (Surprising number of exoplanets could host life). Moreover, a star similar to the Sun supports six planets with liquid water. The researchers note that if a system has more than seven planets in the inhabitable zone, they begin to destabilize the orbits of one another.

Reflection

In my opinion, studies similar to the one by Kane et al. are critical because they help advance astrophysics and other scientific fields. Moreover, biologists and chemists can also benefit from this research since it contains some explanations for the atmospheric chemistry of these planets. This study relates to the content in this course because it shows the connection between different scientific fields and the potential of applying the acquired knowledge. Hence, although the focus of this research is on trying to find life outside the Earth, it also contributes to the development of multiple scientific fields.

By using models, similar to the ones developed by these researchers, others, for example, NASA can use their resources, such as telescopes to study the potentially inhabitable planets more precisely. Otherwise, the number of potential planets that should be considered in the first place would be too large, and the scientists would dedicate most of the time to trying to find these habitable zones (Surprising number of exoplanets could host life). Moreover, I think that similar studies are a valuable contributor to understanding how the conditions that allowed life to develop on Earth emerged. This process is complicated and time-consuming, and this study can help understand the specific requirements necessary to support the properties that make this planet inhabitable.

Conclusion

Overall, this article provides an outline of the research on the potential of other planets being inhabitable. Kane et al. successfully created a computer model that simulates the environment of the Trappist-1 solar system. They determined that the maximum number of inhabitable planets in it is seven. In the reflection part, the critical role of similar studies and their contribution to multiple scientific disciplines is discussed.

Work Cited

Surprising Number of Exoplanets Could Host Life: New Insights to Inform Future NASA Missions. ScienceDaily, 2020, Web.

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Dynamical Packing in the Habitable Zone by Kane

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