1. | \(\frac{\lambda_1\lambda_2}{\lambda_1-\lambda_2}\) | 2. | \(\frac{\lambda_1+\lambda_2}{2}\) |
3. | \(\sqrt{\lambda^2_1+\lambda^2_2}\) | 4. | \(\frac{\lambda_1\lambda_2}{\lambda_1+\lambda_2}\) |
1. | the first line of the Lyman series. |
2. | the second line of the Balmer series. |
3. | the first line of the Paschen series. |
4. | the second line of the Paschen series. |
1. | \(\dfrac{25}{9}\) | 2. | \(\dfrac{17}{6}\) |
3. | \(\dfrac{9}{5}\) | 4. | \(\dfrac{4}{3}\) |
1. | \(\dfrac{3}{23}\) | 2. | \(\dfrac{7}{29}\) |
3. | \(\dfrac{9}{31}\) | 4. | \(\dfrac{5}{27}\) |
The wavelength of the first line of the Lyman series for a hydrogen atom is equal to that of the second line of the Balmer series for a hydrogen-like ion. What is the atomic number \(Z\) of hydrogen-like ions?
1. \(4\)
2. \(1\)
3. \(2\)
4. \(3\)
1. | visible region |
2. | far infrared region |
3. | ultraviolet region |
4. | infrared region |