Lund, Michael B. (2019) Worlds in Migration. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20190520-090948164
![[img]](https://authors.library.caltech.edu/style/images/fileicons/application_pdf.png) |
PDF
- Submitted Version
See Usage Policy. 218kB |
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190520-090948164
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.
| Item Type: | Report or Paper (Discussion Paper) | ||||||
|---|---|---|---|---|---|---|---|
| Related URLs: |
| ||||||
| ORCID: |
| ||||||
| 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). | ||||||
| Group: | Infrared Processing and Analysis Center (IPAC) | ||||||
| Record Number: | CaltechAUTHORS:20190520-090948164 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190520-090948164 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 95589 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Tony Diaz | ||||||
| Deposited On: | 20 May 2019 17:24 | ||||||
| Last Modified: | 03 Oct 2019 21:14 |
Repository Staff Only: item control page
