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| // Complete periodic table data with cosmic origins and spectral lines | |
| // This will be integrated into index.html | |
| const ALL_ELEMENTS = [ | |
| // Period 1 | |
| { symbol: "H", name: "Hydrogen", atomicNumber: 1, category: "nonmetal", row: 1, col: 1, | |
| cosmicOrigin: "Big Bang", originColor: "#FFD700", | |
| astronomyInfo: "The most abundant element in the universe, created during the Big Bang 13.8 billion years ago. Hydrogen makes up about 75% of all normal matter and is the fuel that powers stars through nuclear fusion.", | |
| spectralLines: [{ wavelength: 656.3, intensity: 1.0 }, { wavelength: 486.1, intensity: 0.5 }, { wavelength: 434.0, intensity: 0.3 }, { wavelength: 410.2, intensity: 0.2 }]}, | |
| { symbol: "He", name: "Helium", atomicNumber: 2, category: "noble-gas", row: 1, col: 18, | |
| cosmicOrigin: "Big Bang", originColor: "#FFD700", | |
| astronomyInfo: "The second most abundant element in the universe, primarily created during the Big Bang. Also produced by nuclear fusion in stars.", | |
| spectralLines: [{ wavelength: 587.6, intensity: 1.0 }, { wavelength: 667.8, intensity: 0.3 }, { wavelength: 501.6, intensity: 0.4 }]}, | |
| // Period 2 | |
| { symbol: "Li", name: "Lithium", atomicNumber: 3, category: "alkali-metal", row: 2, col: 1, | |
| cosmicOrigin: "Cosmic Ray & Dying Stars", originColor: "#9370DB", | |
| astronomyInfo: "Created through multiple processes: some from the Big Bang, most from dying low-mass stars, and some isotopes from cosmic ray collisions.", | |
| spectralLines: [{ wavelength: 670.8, intensity: 1.0 }, { wavelength: 610.4, intensity: 0.3 }]}, | |
| { symbol: "Be", name: "Beryllium", atomicNumber: 4, category: "alkaline-earth", row: 2, col: 2, | |
| cosmicOrigin: "Cosmic Ray Fission", originColor: "#9370DB", | |
| astronomyInfo: "Created by cosmic ray spallation - when high-energy cosmic rays collide with heavier elements in space, breaking them apart.", | |
| spectralLines: [{ wavelength: 234.9, intensity: 1.0 }, { wavelength: 313.0, intensity: 0.4 }]}, | |