{"action":"created","issue":{"url":"https://api.github.com/repos/geodynamics/burnman/issues/110","labels_url":"https://api.github.com/repos/geodynamics/burnman/issues/110/labels{/name}","comments_url":"https://api.github.com/repos/geodynamics/burnman/issues/110/comments","events_url":"https://api.github.com/repos/geodynamics/burnman/issues/110/events","html_url":"https://github.com/geodynamics/burnman/pull/110","id":53716935,"number":110,"title":"Add new example for building a planet","user":{"login":"ian-r-rose","id":5728311,"avatar_url":"https://avatars.githubusercontent.com/u/5728311?v=3","gravatar_id":"","url":"https://api.github.com/users/ian-r-rose","html_url":"https://github.com/ian-r-rose","followers_url":"https://api.github.com/users/ian-r-rose/followers","following_url":"https://api.github.com/users/ian-r-rose/following{/other_user}","gists_url":"https://api.github.com/users/ian-r-rose/gists{/gist_id}","starred_url":"https://api.github.com/users/ian-r-rose/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/ian-r-rose/subscriptions","organizations_url":"https://api.github.com/users/ian-r-rose/orgs","repos_url":"https://api.github.com/users/ian-r-rose/repos","events_url":"https://api.github.com/users/ian-r-rose/events{/privacy}","received_events_url":"https://api.github.com/users/ian-r-rose/received_events","type":"User","site_admin":false},"labels":[],"state":"open","locked":false,"assignee":null,"milestone":null,"comments":8,"created_at":"2015-01-08T05:47:00Z","updated_at":"2015-01-08T19:26:00Z","closed_at":null,"pull_request":{"url":"https://api.github.com/repos/geodynamics/burnman/pulls/110","html_url":"https://github.com/geodynamics/burnman/pull/110","diff_url":"https://github.com/geodynamics/burnman/pull/110.diff","patch_url":"https://github.com/geodynamics/burnman/pull/110.patch"},"body":"I promised this one a while back.  This is an example which self-consistently calculates pressure, gravity, and density for a planet (using Mercury as an example).  It then calculates the planet's mass and moment-of-inertia, which can be compared to geodetic constraints.  Kind of a neat example of the kind of things we can do..."},"comment":{"url":"https://api.github.com/repos/geodynamics/burnman/issues/comments/69233812","html_url":"https://github.com/geodynamics/burnman/pull/110#issuecomment-69233812","issue_url":"https://api.github.com/repos/geodynamics/burnman/issues/110","id":69233812,"user":{"login":"ian-r-rose","id":5728311,"avatar_url":"https://avatars.githubusercontent.com/u/5728311?v=3","gravatar_id":"","url":"https://api.github.com/users/ian-r-rose","html_url":"https://github.com/ian-r-rose","followers_url":"https://api.github.com/users/ian-r-rose/followers","following_url":"https://api.github.com/users/ian-r-rose/following{/other_user}","gists_url":"https://api.github.com/users/ian-r-rose/gists{/gist_id}","starred_url":"https://api.github.com/users/ian-r-rose/starred{/owner}{/repo}","subscriptions_url":"https://api.github.com/users/ian-r-rose/subscriptions","organizations_url":"https://api.github.com/users/ian-r-rose/orgs","repos_url":"https://api.github.com/users/ian-r-rose/repos","events_url":"https://api.github.com/users/ian-r-rose/events{/privacy}","received_events_url":"https://api.github.com/users/ian-r-rose/received_events","type":"User","site_admin":false},"created_at":"2015-01-08T19:26:00Z","updated_at":"2015-01-08T19:26:00Z","body":"I am not actually trying to fit the planet in this example, as it would involve a much more complicated model for the interior.  This is a simple two-layer model with a solid iron core.  Yes, the resulting mass is too large by about 35%.\r\n\r\n"}}