Calculates observed bulk density #59
Merged
Conversation
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
lsoucasse
approved these changes
Sep 12, 2024
|
Thanks! |
lsoucasse
pushed a commit
that referenced
this pull request
Sep 24, 2024
Calculates observed bulk density
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment
Add this suggestion to a batch that can be applied as a single commit.
This suggestion is invalid because no changes were made to the code.
Suggestions cannot be applied while the pull request is closed.
Suggestions cannot be applied while viewing a subset of changes.
Only one suggestion per line can be applied in a batch.
Add this suggestion to a batch that can be applied as a single commit.
Applying suggestions on deleted lines is not supported.
You must change the existing code in this line in order to create a valid suggestion.
Outdated suggestions cannot be applied.
This suggestion has been applied or marked resolved.
Suggestions cannot be applied from pending reviews.
Suggestions cannot be applied on multi-line comments.
Suggestions cannot be applied while the pull request is queued to merge.
Suggestion cannot be applied right now. Please check back later.
A new function to calculate the observed bulk density of the planet.
This is done by taking the total mass (= atm + int) and comparing it to the observed radius. Since we don't have optical depth stored, this is taken to be observed at the 1 mbar level and is a grey quantity.
This function is called by PROTEUS at runtime, so we can track how this quantity changes as the planet cools.