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are very likely to observe more lines than what you expect from a pure hydrogen gas emission spectrum. Additionally, hydrogen

Part 4 (Hydrogen) *19 20 22 24 26 28 30 32 34 700 600 500 400

Part 4 (Helium) 17 18 19 20 La 30 32 34 III 700 600 500 400

Part 4 (Neon) גי. 19. זי 2. 22. 24. ,20. ,2 ,30 ,32 34. ייייייייייייייייייייייייייייייייייייייייי יייויויויויויויויויויויוין

Part 4 (Argon) 20 28 30 32 34 700 600 500

Part 4 (Mercury) 17 18 19 20 21 22., 24., 2,6 30 32 3 700 600 500 400

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