From 4117ee7523e3e1b17d3b23fce8f0cc8b0eb6ad73 Mon Sep 17 00:00:00 2001 From: "M. Kanamaru" Date: Fri, 10 Nov 2023 01:48:29 +0900 Subject: [PATCH] Update README.md (#98) Removed outdated sample code. --- README.md | 17 ----------------- 1 file changed, 17 deletions(-) diff --git a/README.md b/README.md index 61361453..3f9d2777 100644 --- a/README.md +++ b/README.md @@ -41,20 +41,3 @@ Based on orbit, spin, and 3-D shape, you can calculate the distribution of the s Distribution of surface temperature on asteroid Ryugu. The color map ranges from 200 to 400 K. ![Thermophysics_Ryugu](https://user-images.githubusercontent.com/21192162/149468024-f403011f-b3d3-47ce-a69c-7daf78a40658.png) - -## Start to play -Let's visualize a shape model of asteroid Ryugu. -Please download a Ryugu model from AsteroidThermoPhysicalModels/test/ryugu_test.obj. - -```julia -using AsteroidThermoPhysicalModels - -shapepath = "ryugu_test.obj" # Path to the shape model -shape = load_shape_obj(shapepath; scale=1000, find_visible_facets=true) - -draw(shape) -# draw(shape, data=:radius) # Radius of each surface facet -# draw(shape; data=:illumination, r̂☉=[1,0,0.]) # Illumination when the Sun is in the direction of r̂☉ -``` - -start_to_play