Is High-Eccentric Tidal Migrations a Plausible Pathway to Explain Hot Jupiter’s Short Orbital Periods?

Chick, Dave (2022). Is High-Eccentric Tidal Migrations a Plausible Pathway to Explain Hot Jupiter’s Short Orbital Periods? Student research project for the Open University module SXP390 Radiation and Matter Project Module

This dissertation was produced by a student studying the Open University module SXP390 Radiation and Matter Project Module. The research showcased here achieved a grade in either the Pass 1 band (equivalent to a 1st) or the Pass 2 band (equivalent to a 2.i).
Please note that this student dissertation is made available in the format that it was submitted for examination, thus the author has not been able to correct errors and/or departures from academic standards in areas such as referencing.
Copyright resides with the author.

DOI: https://doi.org/10.21954/ou.ro.00015197

Viewing alternatives

Download history

Metrics

Public Attention

Altmetrics from Altmetric

Number of Citations

Citations from Dimensions

Item Actions

Export

About