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CBSE - Class 11 Chemistry Structure of Atom Worksheet
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Solution:
The energy of an electron in the $n^{th}$ Bohr orbit of a hydrogen atom is given by the Rydberg-Bohr formula:
$E_n = -\frac{R_H}{n^2}$
Given the energy of the ground state ($n=1$) is $-2.18 \times 10^{-11} \text{ ergs}$, we first convert this value to Joules ($1 \text{ erg} = 10^{-7} \text{ J}$):
$E_1 = -2.18 \times 10^{-11} \times 10^{-7} \text{ J} = -2.18 \times 10^{-18} \text{ J}$ [Per definition of SI units conversion].
The energy required ($\Delta E$) to shift the electron from $n_1$ to $n_2$ is calculated by the difference in energy levels [Per Bohr's Postulate]:
$\Delta E = E_5 - E_1 = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$
Substituting $R_H = 2.18 \times 10^{-18} \text{ J}$ and the quantum numbers:
$\Delta E = 2.18 \times 10^{-18} \left( \frac{1}{1^2} - \frac{1}{5^2} \right) \text{ J}$
$\Delta E = 2.18 \times 10^{-18} \left( 1 - 0.04 \right) \text{ J}$
$\Delta E = 2.18 \times 10^{-18} \times 0.96 \text{ J} = 2.0928 \times 10^{-18} \text{ J}$
When the electron returns from $n=5$ to $n=1$, the energy released is equal to the energy absorbed: $\Delta E = 2.0928 \times 10^{-18} \text{ J}$. The relationship between energy and wavelength ($\lambda$) is given by the Planck-Einstein relation [Per Planck’s Quantum Theory]:
$E = \frac{hc}{\lambda} \implies \lambda = \frac{hc}{E}$
Constants:
$\lambda = \frac{(6.626 \times 10^{-34} \text{ J}\cdot\text{s}) \times (3.0 \times 10^8 \text{ m/s})}{2.0928 \times 10^{-18} \text{ J}}$
$\lambda = \frac{19.878 \times 10^{-26}}{2.0928 \times 10^{-18}} \text{ m}$
$\lambda = 9.50 \times 10^{-8} \text{ m}$
Final Solution: The energy required is $2.0928 \times 10^{-18} \text{ J}$, and the wavelength of the emitted light is $9.50 \times 10^{-8} \text{ m}$ (or $95.0 \text{ nm}$).
Solution:
To determine the de Broglie wavelength ($\lambda$), we utilize the de Broglie relation. The following physical constants and given variables are defined:
Per the de Broglie hypothesis, the wavelength ($\lambda$) of a moving particle is inversely proportional to its momentum ($p$). The relationship is defined as:
$$\lambda = \frac{h}{mv} = \frac{h}{p}$$
[Justification: This is derived from the synthesis of Einstein's mass-energy equivalence $E=mc^2$ and Planck's quantum theory $E=h\nu$, establishing the wave-particle duality of matter.]
Substitute the constants and variables into the de Broglie equation:
$$\lambda = \frac{6.626 \times 10^{-34} \, \text{kg m}^2 \text{s}^{-1}}{(9.109 \times 10^{-31} \, \text{kg}) \times (1.6 \times 10^6 \, \text{m s}^{-1})}$$
Calculating the denominator (momentum, $p$):
$$p = 9.109 \times 1.6 \times 10^{-31 + 6} = 14.5744 \times 10^{-25} \, \text{kg m s}^{-1}$$
Calculating the final wavelength ($\lambda$):
$$\lambda = \frac{6.626 \times 10^{-34}}{14.5744 \times 10^{-25}}$$
$$\lambda \approx 0.4546 \times 10^{-9} \, \text{m}$$
| Expression | Resulting Units |
|---|---|
| $\frac{\text{kg m}^2 \text{s}^{-1}}{\text{kg} \times \text{m s}^{-1}}$ | $\text{m}$ (Meters) |
Final Solution: The de Broglie wavelength associated with the electron is $4.546 \times 10^{-10} \, \text{m}$ (or $0.4546 \, \text{nm}$).
Solution:
To determine the total number of electrons in molecular species, we first identify the atomic number ($Z$) of the constituent atoms, which represents the number of electrons in a neutral atom [Per the definition of the Periodic Table and Atomic Structure].
The species $H_2^+$ consists of two hydrogen atoms with a net positive charge of $+1$.
The species $H_2$ is a neutral diatomic hydrogen molecule.
The species $O_2^+$ consists of two oxygen atoms with a net positive charge of $+1$.
| Species | Calculation | Total Electrons |
|---|---|---|
| $H_2^+$ | $(2 \times 1) - 1$ | 1 |
| $H_2$ | $(2 \times 1)$ | 2 |
| $O_2^+$ | $(2 \times 8) - 1$ | 15 |
Final Solution: The number of electrons are: $H_2^+ = 1$, $H_2 = 2$, and $O_2^+ = 15$.
Solution:
The notation $[Ne]$ represents the electron configuration of Neon, which is the noble gas preceding the element in question. The atomic number of Neon ($Z$) is $10$.
The full configuration for Neon is $1s^2 2s^2 2p^6$. [Per the Aufbau Principle, electrons fill lower energy orbitals before higher energy ones].
The given configuration is $[Ne] 3s^2 3p^3$. To find the total number of electrons ($N_e$), we sum the electrons in the Neon core and the valence shell:
$N_e = (\text{Electrons in } Ne) + (\text{Electrons in } 3s) + (\text{Electrons in } 3p)$
$N_e = 10 + 2 + 3 = 15$
[By the Principle of Electroneutrality, in a neutral atom, the number of electrons equals the atomic number $Z$].
Since the total number of electrons is $15$, the atomic number of the element is $Z = 15$.
Consulting the Periodic Table of Elements for $Z = 15$, we identify the element as Phosphorus ($P$).
| Orbital | Number of Electrons |
|---|---|
| $1s$ | $2$ |
| $2s$ | $2$ |
| $2p$ | $6$ |
| $3s$ | $2$ |
| $3p$ | $3$ |
| Total | $15$ |
Final Solution: The atom indicated by the configuration $[Ne] 3s^2 3p^3$ is Phosphorus (P), with an atomic number of 15.
Solution:
To determine the energy of a photon with a specific wavelength, we utilize the fundamental relationship between energy, frequency, and wavelength established by Planck’s Quantum Theory [Per Planck's Law].
The energy ($E$) of a single photon is defined by the equation:
$E = \frac{hc}{\lambda}$
[Justification: Since frequency ($\nu$) is given by $\nu = \frac{c}{\lambda}$, substituting this into $E = h\nu$ yields the formula above.]
Substitute the constants into the derived equation:
$E = \frac{(6.626 \times 10^{-34} \text{ J}\cdot\text{s}) \times (3.0 \times 10^8 \text{ m/s})}{0.50 \times 10^{-10} \text{ m}}$
Multiply the numerator:
$E = \frac{19.878 \times 10^{-26} \text{ J}\cdot\text{m}}{0.50 \times 10^{-10} \text{ m}}$
Perform the division:
$E = 39.756 \times 10^{-16} \text{ J}$
Adjusting to standard scientific notation:
$E = 3.9756 \times 10^{-15} \text{ J}$
The given wavelength $0.50 \text{ Å}$ consists of two significant figures. Therefore, the result should be expressed accordingly.
| Variable | Value |
|---|---|
| Energy (Exact) | $3.9756 \times 10^{-15} \text{ J}$ |
| Energy (Rounded) | $4.0 \times 10^{-15} \text{ J}$ |
Final Solution: The energy of each photon is $3.98 \times 10^{-15} \text{ J}$ (or $4.0 \times 10^{-15} \text{ J}$ to two significant figures).
Solution:
To perform calculations in SI units, we convert $\Phi$ from electron-volts to Joules:
$\Phi = 1.9 \text{ eV} \times 1.602 \times 10^{-19} \text{ J/eV} = 3.0438 \times 10^{-19} \text{ J}$ [Per the definition of electron-volt energy conversion]
Using the relation $\Phi = h\nu_0$ [Per Planck-Einstein relation]:
$\nu_0 = \frac{\Phi}{h} = \frac{3.0438 \times 10^{-19} \text{ J}}{6.626 \times 10^{-34} \text{ J}\cdot\text{s}} = 4.594 \times 10^{14} \text{ s}^{-1}$
Using the relation $\lambda_0 = \frac{c}{\nu_0}$:
$\lambda_0 = \frac{3 \times 10^8 \text{ m/s}}{4.594 \times 10^{14} \text{ s}^{-1}} = 6.53 \times 10^{-7} \text{ m} = 653 \text{ nm}$
Energy of incident photon ($E_{inc}$) = $\frac{hc}{\lambda}$:
$E_{inc} = \frac{(6.626 \times 10^{-34} \text{ J}\cdot\text{s})(3 \times 10^8 \text{ m/s})}{500 \times 10^{-9} \text{ m}} = 3.9756 \times 10^{-19} \text{ J}$
Using Einstein’s Photoelectric Equation: $E_k = E_{inc} - \Phi$ [Per Law of Conservation of Energy]:
$E_k = 3.9756 \times 10^{-19} \text{ J} - 3.0438 \times 10^{-19} \text{ J} = 9.318 \times 10^{-20} \text{ J}$
Using $E_k = \frac{1}{2}m_ev^2$:
$v = \sqrt{\frac{2 \times E_k}{m_e}} = \sqrt{\frac{2 \times 9.318 \times 10^{-20} \text{ J}}{9.11 \times 10^{-31} \text{ kg}}}$
$v = \sqrt{2.045 \times 10^{11} \text{ m}^2/\text{s}^2} = 4.522 \times 10^5 \text{ m/s}$
Final Solution: (a) Threshold wavelength = $653 \text{ nm}$, Threshold frequency = $4.594 \times 10^{14} \text{ Hz}$; (b) Kinetic energy = $9.318 \times 10^{-20} \text{ J}$, Velocity = $4.522 \times 10^5 \text{ m/s}$.
Solution:
The energy of an electron in the $n^{th}$ orbit of a hydrogen-like species is governed by the Bohr Model of the atom. The relationship between the energy ($E_n$) and the principal quantum number ($n$) is defined by the following expression:
$E_n = -\frac{R_H}{n^2}$
Where:
Based on the problem statement:
To find the energy of the fifth orbit ($E_5$), we substitute $n = 5$ into the governing equation [By Application of Bohr's Energy Formula]:
$E_5 = -\frac{2.18 \times 10^{-18} \, \text{J}}{n^2}$
$E_5 = -\frac{2.18 \times 10^{-18}}{(5)^2} \, \text{J}$
$E_5 = -\frac{2.18 \times 10^{-18}}{25} \, \text{J}$
Perform the division:
$E_5 = -0.0872 \times 10^{-18} \, \text{J}$
Expressing the result in standard scientific notation [By Mathematical Convention]:
$E_5 = -8.72 \times 10^{-20} \, \text{J atom}^{-1}$
Final Solution: The energy associated with the fifth orbit of the hydrogen atom is $-8.72 \times 10^{-20} \, \text{J atom}^{-1}$.
Solution:
To determine the validity of the set $(n = 2, l = 1, m_l = 0, m_s = - \frac{1}{2})$, we must test each quantum number against the established rules of quantum mechanics and the Pauli Exclusion Principle.
The set describes an electron residing in the $2p$ subshell. Specifically, the quantum numbers define one of the three $p$-orbitals ($2p_z$ if $m_l=0$ by convention) and specifies one of the two possible spin states for the electron.
Per the rules derived from the Schrödinger wave equation solutions for a hydrogenic atom [Bohr-Sommerfeld/Schrödinger theory]:
| Quantum Number | Constraint Rule | Provided Value | Status |
|---|---|---|---|
| $n$ | $n \in \{1, 2, 3, \dots\}$ | $2$ | Valid |
| $l$ | $0 \le l \le n-1$ | $1$ | Valid |
| $m_l$ | $-l \le m_l \le +l$ | $0$ | Valid |
| $m_s$ | $\pm \frac{1}{2}$ | $-\frac{1}{2}$ | Valid |
Final Solution: The set of quantum numbers $(n = 2, l = 1, m_l = 0, m_s = – \frac{1}{2})$ is a physically possible set as it satisfies all governing constraints of quantum mechanics. It corresponds to an electron located in the $2p$ subshell with spin-down configuration.
Solution:
To determine the velocity of the photoelectron, we utilize the Photoelectric Effect equation established by Einstein: $E_{photon} = W + K.E._{max}$.
Using the Planck-Einstein relation [Per $E = \frac{hc}{\lambda}$]:
$E = \frac{(6.626 \times 10^{-34} \, \text{J}\cdot\text{s}) \times (3 \times 10^8 \, \text{m/s})}{4 \times 10^{-7} \, \text{m}}$
$E = 4.9695 \times 10^{-19} \, \text{J}$
Convert the work function ($W$) from electron-volts to Joules to maintain dimensional consistency [Per $W(J) = W(eV) \times 1.602 \times 10^{-19}$]:
$W = 2.13 \times 1.602 \times 10^{-19} \, \text{J}$
$W = 3.4123 \times 10^{-19} \, \text{J}$
Subtract the work function from the incident photon energy [Per Conservation of Energy]:
$K.E. = E - W$
$K.E. = 4.9695 \times 10^{-19} - 3.4123 \times 10^{-19} \, \text{J}$
$K.E. = 1.5572 \times 10^{-19} \, \text{J}$
Using the classical kinetic energy formula $K.E. = \frac{1}{2} m_e v^2$, solve for $v$:
$v = \sqrt{\frac{2 \times K.E.}{m_e}}$
$v = \sqrt{\frac{2 \times 1.5572 \times 10^{-19} \, \text{kg}\cdot\text{m}^2/\text{s}^2}{9.109 \times 10^{-31} \, \text{kg}}}$
$v = \sqrt{0.3418 \times 10^{12} \, \text{m}^2/\text{s}^2}$
$v \approx 5.846 \times 10^5 \, \text{m/s}$
Final Solution: The velocity of the emitted photoelectron is approximately 5.85 \times 10^5 \, \text{m/s}.
Solution:
The energy ($E$) of a single photon is directly proportional to the frequency ($\nu$) of the electromagnetic radiation. This relationship is defined by Planck's Quantum Theory, expressed as:
$E = h\nu$
[Per Planck's Quantum Theory of Radiation]
To calculate the energy, we define the following parameters:
Substitute the given values into the Planck equation:
$E = (6.626 \times 10^{-34} \text{ J}\cdot\text{s}) \times (3 \times 10^{15} \text{ s}^{-1})$
Perform the algebraic multiplication of the coefficients:
$6.626 \times 3 = 19.878$
Apply the laws of exponents for the powers of 10:
$10^{-34} \times 10^{15} = 10^{-34 + 15} = 10^{-19}$
Combine the results:
$E = 19.878 \times 10^{-19} \text{ J}$
To express the result in proper scientific notation ($a \times 10^n$ where $1 \le a < 10$), adjust the decimal point:
$E = 1.9878 \times 10^1 \times 10^{-19} \text{ J}$
$E = 1.9878 \times 10^{-18} \text{ J}$
Final Solution: The energy of each photon is $1.9878 \times 10^{-18} \text{ J}$.
Solution:
Let the symbol of the ion be represented as $_{Z}^{A}X^{n}$, where:
Since the ion has a $-1$ charge, the number of electrons is related to the atomic number by the equation: $e = Z + 1$ [Per the definition of an anion].
The number of neutrons is related to the mass number by: $n_0 = A - Z = 37 - Z$ [Per the relation $A = Z + n_0$].
The problem states that the ion contains 11.1% more neutrons than electrons. This is expressed mathematically as:
$n_0 = e + 0.111e$
$n_0 = 1.111e$
Substitute the expressions for $n_0$ and $e$ into the equation:
$37 - Z = 1.111(Z + 1)$
Expand the right side:
$37 - Z = 1.111Z + 1.111$
Rearrange the terms to isolate $Z$:
$37 - 1.111 = 1.111Z + Z$
$35.889 = 2.111Z$
$Z = \frac{35.889}{2.111} \approx 17$
[Calculation justification: $17 \times 2.111 \approx 35.887$, which rounds to 17 given the approximation of 11.1% as $1/9$].
An element with atomic number $Z = 17$ is Chlorine ($Cl$).
The ion is a negatively charged ion ($Cl^-$) with a mass number of 37. Thus, the isotope is $^{37}Cl^-$.
| Particle | Calculated Value |
|---|---|
| Protons ($Z$) | 17 |
| Electrons ($Z+1$) | 18 |
| Neutrons ($37-17$) | 20 |
| Check ($18 \times 1.111$) | 19.998 $\approx 20$ |
Final Solution: The symbol of the ion is $^{37}_{17}\text{Cl}^-$.
Solution:
To determine the radius of a single carbon atom from a linear arrangement, we first identify the physical properties provided in the problem statement:
Since the atoms are arranged side by side in a single line, the total length is the sum of the diameters of all individual atoms. Assuming the atoms are spheres in contact [Geometric Assumption for linear packing]:
$L = N \times d$
Where $d$ is the diameter of one atom. Rearranging for $d$:
$d = \frac{L}{N}$
$d = \frac{2.4 \text{ cm}}{2.0 \times 10^8}$
$d = 1.2 \times 10^{-8} \text{ cm}$
The radius ($r$) of a sphere is defined as half of its diameter [By definition of a circle/sphere]:
$r = \frac{d}{2}$
$r = \frac{1.2 \times 10^{-8} \text{ cm}}{2}$
$r = 0.6 \times 10^{-8} \text{ cm}$
To express the radius in standard scientific notation:
$r = 6.0 \times 10^{-9} \text{ cm}$
Optionally, converting to picometers ($\text{pm}$) where $1 \text{ cm} = 10^{10} \text{ pm}$:
$r = 6.0 \times 10^{-9} \text{ cm} \times 10^{10} \text{ pm/cm} = 60 \text{ pm}$
Final Solution: The radius of the carbon atom is $6.0 \times 10^{-9} \text{ cm}$ or $60 \text{ pm}$.
Solution:
To determine the validity of the set $(n = 0, l = 0, m_l = 0, m_s = + \frac{1}{2})$, we must evaluate each value against the governing principles of quantum mechanics [Per the Schrödinger wave equation and the Aufbau principle].
| Quantum Number | Provided Value | Theoretical Requirement | Status |
|---|---|---|---|
| $n$ | $0$ | $n \in \{1, 2, 3, \dots\}$ | Invalid |
| $l$ | $0$ | $0 \leq l \leq (n-1)$ | Invalid (dependent on $n$) |
| $m_l$ | $0$ | $-l \leq m_l \leq +l$ | Invalid (dependent on $l$) |
| $m_s$ | $+1/2$ | $\pm 1/2$ | Valid |
The set is physically impossible for the following reason: The Principal Quantum Number ($n$) defines the energy level and must satisfy the condition $n \geq 1$. Since the given value is $n = 0$, there is no corresponding shell in the atomic model where an electron can reside. Furthermore, if $n=0$, the condition $0 \leq l \leq (n-1)$ cannot be satisfied, rendering $l=0$ mathematically inconsistent with the requirement. [By the Pauli Exclusion Principle and Bohr's postulate on quantized energy levels].
Final Solution: The set of quantum numbers $(n = 0, l = 0, m_l = 0, m_s = + \frac{1}{2})$ is not possible because the principal quantum number $n$ cannot be zero; it must be a positive integer starting from 1.
Solution:
The Rydberg formula for the wavenumber ($\bar{\nu}$) of transitions in the hydrogen atom spectrum is defined as:
$\bar{\nu} = R_H \times \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)$
Where:
Wavelength ($\lambda$) and wavenumber ($\bar{\nu}$) are inversely proportional according to the relation $\bar{\nu} = \frac{1}{\lambda}$ [Relationship between electromagnetic wave properties]. To obtain the longest wavelength, we must identify the smallest energy transition, which corresponds to the smallest possible value for $\bar{\nu}$.
For the Balmer series, the transitions occur from $n_2$ to $n_1 = 2$. The transition with the smallest energy gap occurs between the first excited state above the base level, i.e., $n_2 = 3$ to $n_1 = 2$.
Substitute $n_1 = 2$ and $n_2 = 3$ into the Rydberg equation:
$\bar{\nu} = 109,677 \, \text{cm}^{-1} \times \left( \frac{1}{2^2} - \frac{1}{3^2} \right)$
Perform the fractional arithmetic:
$\bar{\nu} = 109,677 \times \left( \frac{1}{4} - \frac{1}{9} \right)$
$\bar{\nu} = 109,677 \times \left( \frac{9 - 4}{36} \right)$
$\bar{\nu} = 109,677 \times \left( \frac{5}{36} \right)$
$\bar{\nu} = 109,677 \times 0.13888...$
$\bar{\nu} = 15,232.916 \, \text{cm}^{-1}$
The calculation yields a wavenumber of $15,233 \, \text{cm}^{-1}$ when rounded to the nearest integer. This represents the lowest energy photon in the visible Balmer series, corresponding to the $H_\alpha$ spectral line.
Final Solution: The wavenumber for the longest wavelength transition in the Balmer series is $15,232.92 \, \text{cm}^{-1}$.
Solution:
To determine the number of photons required to provide a total energy ($E_{total}$) of $1\, \text{J}$ for light with a wavelength ($\lambda$) of $4000\, \text{pm}$, we utilize the Planck-Einstein relation.
The energy of a single photon is defined by the equation [Per Planck’s Quantum Theory]:
$E_{photon} = \frac{hc}{\lambda}$
Substituting the given values:
$E_{photon} = \frac{(6.626 \times 10^{-34}\, \text{J}\cdot\text{s}) \times (3.0 \times 10^8\, \text{m/s})}{4 \times 10^{-9}\, \text{m}}$
$E_{photon} = \frac{19.878 \times 10^{-26}}{4 \times 10^{-9}}\, \text{J}$
$E_{photon} = 4.9695 \times 10^{-17}\, \text{J}$
The total energy is the product of the number of photons ($n$) and the energy per photon. Thus, $n = \frac{E_{total}}{E_{photon}}$ [By the Law of Conservation of Energy]:
$n = \frac{1\, \text{J}}{4.9695 \times 10^{-17}\, \text{J}}$
$n \approx 0.2012 \times 10^{17}$
$n \approx 2.012 \times 10^{16}$
Final Solution: The number of photons required to provide 1 J of energy is $2.012 \times 10^{16}$.
Solution:
For any neutral atom, the number of electrons is equal to the number of protons, which defines the atomic number ($Z$).
[Per the definition of atomic structure in a neutral state, $Z = \text{number of protons} = \text{number of electrons}$].
To determine the electronic configuration, electrons are filled into atomic orbitals in increasing order of energy, starting from the $1s$ orbital. The sequence follows the $(n + l)$ rule, where orbitals with lower $(n + l)$ values are filled first [Per the Aufbau Principle].
The standard order of energy for subshells is: $1s < 2s < 2p < 3s < 3p < 4s < 3d < 4p \dots$
We distribute the 29 electrons according to the capacity of each subshell ($s=2, p=6, d=10$):
| Subshell | Electrons Added | Cumulative Total |
|---|---|---|
| $1s$ | 2 | 2 |
| $2s$ | 2 | 4 |
| $2p$ | 6 | 10 |
| $3s$ | 2 | 12 |
| $3p$ | 6 | 18 |
| $4s$ | 1 | 19 |
| $3d$ | 10 | 29 |
While the expected configuration based on the Aufbau principle is $1s^2 2s^2 2p^6 3s^2 3p^6 4s^2 3d^9$, the actual configuration is $1s^2 2s^2 2p^6 3s^2 3p^6 4s^1 3d^{10}$.
Reasoning: Half-filled and fully-filled $d$-orbitals provide extra stability due to symmetry and increased exchange energy [Per the Hund’s Rule and Stability of Half-filled/Fully-filled Subshells]. Moving one electron from $4s$ to $3d$ completes the $d$-subshell ($3d^{10}$), resulting in a more stable ground state.
The electronic configuration of the element (Copper, $Cu$) is:
Final Solution: $1s^2 2s^2 2p^6 3s^2 3p^6 3d^{10} 4s^1$ (or $[Ar] 3d^{10} 4s^1$)
Solution:
The given set of quantum numbers is: $n = 2$, $l = 1$, $m_l = 0$, $m_s = -\frac{1}{2}$. To determine the validity of this set, we must evaluate each parameter against the established rules of quantum mechanics governing atomic orbitals.
The set describes an electron in the $2p$ subshell. Specifically, since $n=2$ and $l=1$, the orbital is a $2p$ orbital. The magnetic quantum number $m_l = 0$ designates the $2p_z$ orbital (by convention). The spin $m_s = -\frac{1}{2}$ indicates a specific spin orientation.
Since the provided set ($n=2, l=1, m_l=0, m_s=-\frac{1}{2}$) satisfies all constraints imposed by the rules of quantum mechanics, it represents a physically possible state for an electron within an atom.
Final Solution: The set of quantum numbers $n = 2$, $l = 1$, $m_l = 0$, $m_s = -\frac{1}{2}$ is possible. It corresponds to an electron located in a $2p$ orbital.
Solution:
To calculate the frequency ($\nu$) and energy ($E$), we utilize the relationship between the speed of light ($c$), wavelength ($\lambda$), and Planck's constant ($h$).
Using the fundamental relation $\nu = \frac{c}{\lambda}$ [Per the Wave-Particle Duality relationship]:
For $\lambda_1 = 589 \times 10^{-9} \text{ m}$:
$\nu_1 = \frac{2.9979 \times 10^8 \text{ m/s}}{589 \times 10^{-9} \text{ m}} = 5.0898 \times 10^{14} \text{ s}^{-1}$For $\lambda_2 = 589.6 \times 10^{-9} \text{ m}$:
$\nu_2 = \frac{2.9979 \times 10^8 \text{ m/s}}{589.6 \times 10^{-9} \text{ m}} = 5.0846 \times 10^{14} \text{ s}^{-1}$The energy of a photon is given by $E = h\nu$ [Per Planck’s Quantum Theory]. The difference in energy ($\Delta E$) between the two states corresponding to the transitions is expressed as:
$\Delta E = E_1 - E_2 = h\nu_1 - h\nu_2 = h(\nu_1 - \nu_2)$Calculate the frequency difference ($\Delta\nu$):
$\Delta\nu = (5.0898 \times 10^{14}) - (5.0846 \times 10^{14}) = 0.0052 \times 10^{14} \text{ s}^{-1} = 5.2 \times 10^{11} \text{ s}^{-1}$Calculate the energy difference ($\Delta E$):
$\Delta E = (6.626 \times 10^{-34} \text{ J}\cdot\text{s}) \times (5.2 \times 10^{11} \text{ s}^{-1})$ $\Delta E = 3.4455 \times 10^{-22} \text{ J}$| Transition | Frequency ($\text{s}^{-1}$) |
|---|---|
| $\lambda_1$ | $5.09 \times 10^{14}$ |
| $\lambda_2$ | $5.08 \times 10^{14}$ |
Final Solution: The frequencies are $5.09 \times 10^{14} \text{ s}^{-1}$ and $5.08 \times 10^{14} \text{ s}^{-1}$ respectively, and the energy difference between the excited states is $3.45 \times 10^{-22} \text{ J}$.
Solution:
The oxygen atom ($\text{O}$) possesses an atomic number ($Z$) of 8. This indicates that a neutral oxygen atom contains 8 protons and, consequently, 8 electrons in its ground state [Per the definition of atomic number in the Bohr-Rutherford model].
The ion in question is $\text{O}^{2-}$, which is an oxide anion. The $2-$ charge indicates the gain of two additional electrons beyond the ground state configuration of the neutral atom. [Per the Octet Rule, atoms gain or lose electrons to achieve a stable valence shell configuration similar to noble gases].
Total number of electrons in $\text{O}^{2-} = Z + (\text{magnitude of charge}) = 8 + 2 = 10$ electrons.
To determine the electronic configuration, we distribute 10 electrons according to the energy hierarchy: $1s < 2s < 2p$. [Per the Aufbau Principle, electrons fill orbitals in order of increasing energy].
| Shell/Subshell | Electronic Capacity | Occupancy in $\text{O}^{2-}$ |
|---|---|---|
| $1s$ | 2 | 2 |
| $2s$ | 2 | 2 |
| $2p$ | 6 | 6 |
Final Solution: The electronic configuration of the oxide ion ($\text{O}^{2-}$) is $1s^2 2s^2 2p^6$.
Solution:
The energy $E$ of a single photon is directly proportional to the frequency $\nu$ and inversely proportional to the wavelength $\lambda$. The relationship is governed by the Planck-Einstein relation [Per the Planck-Einstein Relation]:
$E = \frac{hc}{\lambda}$
Where:
Substituting the given values into the equation:
$E = \frac{(6.626 \times 10^{-34} \text{ J s}) \times (3.0 \times 10^8 \text{ m s}^{-1})}{242 \times 10^{-9} \text{ m}}$
$E = \frac{1.9878 \times 10^{-25}}{242 \times 10^{-9}} \text{ J}$
$E = 8.214 \times 10^{-19} \text{ J per atom}$
To find the ionization energy for one mole of sodium atoms, we multiply the energy of a single photon by Avogadro’s constant ($N_A = 6.022 \times 10^{23} \text{ mol}^{-1}$) [Per the Mole Concept Definition]:
$E_{\text{mole}} = E \times N_A$
$E_{\text{mole}} = (8.214 \times 10^{-19} \text{ J atom}^{-1}) \times (6.022 \times 10^{23} \text{ atom mol}^{-1})$
$E_{\text{mole}} = 4.946 \times 10^5 \text{ J mol}^{-1}$
Convert Joules to kilojoules by dividing by $10^3$ [Per Standard SI Conversion Factors]:
$E_{\text{kJ}} = \frac{4.946 \times 10^5}{10^3} \text{ kJ mol}^{-1}$
$E_{\text{kJ}} = 494.6 \text{ kJ mol}^{-1}$
Final Solution: The ionization energy of sodium is 494.6 kJ mol$^{-1}$.