Published March 29, 2019
| Version Submitted
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Worlds in Migration
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Abstract
In this paper we discuss an alternative track for migration that can explain the existence of Hot Jupiters observed in close orbits around their stars based on a novel interpretation of established work. We also discuss the population of sub-Earth rogue planets that would be created via this migration method, which would be on the order of 2 to 40 billion, many of which would still be present in the Galaxy and potentially detectable.
Additional Information
The author thanks Savannah R. Jacklin for her valuable feedback on this manuscript. This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al., 2013; Price-Whelan et al., 2018).Attached Files
Submitted - 1903.12437.pdf
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1903.12437.pdf
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Identifiers
- Eprint ID
- 95589
- Resolver ID
- CaltechAUTHORS:20190520-090948164
Related works
- Describes
- https://arxiv.org/abs/1903.12437 (URL)
Dates
- Created
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2019-05-20Created from EPrint's datestamp field
- Updated
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2023-06-02Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)