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一分钟完成验证Show a star's color and spectral density given a temperature in Kelvin using Planck's law
翻译准备中
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查看完整 README ↗An interactive blackbody-radiation explorer. Pick a temperature to see the Planck spectrum, the color and brightness a human eye would actually see, where that color sits on the CIE 1931 color map, and the math behind it.
/): a dependency-free rewrite. It has three color models: the original simple one, CIE 1931 colorimetry, and colors of real stars from model spectra (Harre & Heller 2021, with the sRGB gamma correction applied). Brightness follows human vision, so cold objects go black instead of red. Each page ships as a single ~25 KB file./v1/): the original 2023 Create React App version, kept as it was.npm install
npm run build:v2 # v2 only -> build/
npm run build # v1 into build/v1, then v2
python3 -m http.server 4173 --directory build
npm run test:v2 # physics and slider-scale tests
v1's dev server is npm start.
v2/: pages, partials, source, data and tests for the current site. See CLAUDE.md for a map.src/, public/: v1.docs/v2/PLAN.md: the v2 plan, including the v1 math audit, data sources, verified reference values and open questions.docs/WHY.md: why things are the way they are.