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The total energy E of an electron in a hydrogen atom is the sum of its kinetic energy K and its potential energy U. According to the Bohr model of the hydrogen atom, the total energy of the electron is given by:
E = K + U
The kinetic energy K is equal in magnitude to the potential energy, but opposite in sign. Therefore, we have:
K = -U
The total energy of the electron is:
E = K + (-K) = -K
Thus, the ratio of the total energy E to the kinetic energy K is:
E / K = -K / K = -1
Correct Answer: (A) -1
Step 1: Consider the total energy and kinetic energy of an electron in a hydrogen atom using Bohr's model.
The electron experiences an electrostatic force due to the nucleus, which provides the centripetal force required for circular motion: \[ \frac{k e^2}{r^2} = \frac{mv^2}{r} \]
Step 2: Multiply both sides by \( r \): \[ \frac{k e^2}{r} = mv^2 \]
Kinetic energy of the electron is: \[ K = \frac{1}{2}mv^2 = \frac{1}{2} \cdot \frac{k e^2}{r} = \frac{k e^2}{2r} \]
Step 3: Potential energy of the electron in the electrostatic field is: \[ U = -\frac{k e^2}{r} \]
Total energy of the electron is: \[ E = K + U = \frac{k e^2}{2r} - \frac{k e^2}{r} = -\frac{k e^2}{2r} \]
Step 4: Now take the ratio of total energy to kinetic energy: \[ \frac{E}{K} = \frac{-\frac{k e^2}{2r}}{\frac{k e^2}{2r}} = -1 \]
Final Answer: -1
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
For the hydrogen spectrum,the wavelength in Balmer series is given by \(\frac{1}{λ}\)=R(\(\frac{1}{n_{1}^{2}}\)-\(\frac{1}{n_{2}^{2}}\)) where λ= wavelength and R is Rydberg constant. What are the values of n1 and n2,for the longest wavelength in the Balmer series?
Kepler's second law (law of areas) of planetary motion leads to law of conservation of