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NCERT Solutions · Class 11 Chemistry Structure of Atom

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Exercises 2.41–2.50 (part 5 of 7)

  1. Exercise 2.41

    Symbols 35\displaystyle 35 79Br and 79Br can be written, whereas symbols 79\displaystyle 79 35Br and 35Br are not acceptable. Answer briefly.

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    NCERT’s answer
    For a given element the number of prontons is the same for the isotopes, whereas the mass number can be different for the given atomic number.
    The atomic number is fixed by which element the symbol names, so it can be dropped — the mass number cannot, because it changes from isotope to isotope, and swapping the two numbers' positions changes what the symbol is claiming.The full isotope symbol is written as \[{}^{A}_{Z}\text{X} \] where \(\displaystyle A\) is the mass number (protons + neutrons, written as a left superscript) and \(\displaystyle Z\) is the atomic number (protons alone, written as a left subscript). For bromine, \(\displaystyle Z = 35\) always — that is what makes an atom "bromine" — while the two naturally occurring isotopes have \(\displaystyle A = 79\) and \(\displaystyle A = 81\).Why \(\displaystyle {}^{79}_{35}\text{Br}\) and \(\displaystyle {}^{79}\text{Br}\) are fine. Writing the atomic number is optional, not required, because it carries no new information: the symbol "Br" already tells you \(\displaystyle Z=35\) — no other element has that atomic number, so stating it again is repetition, not identification. The mass number, on the other hand, is genuinely needed, because it is the one thing that changes between isotopes of the same element. So \(\displaystyle {}^{79}\text{Br}\) is a complete, unambiguous symbol: the "$\displaystyle 79$" sits in the correct upper-left slot reserved for the mass number, and \(\displaystyle Z=35\) is understood from "Br" itself.Why \(\displaystyle {}^{35}_{79}\text{Br}\) is not acceptable. Here the numbers have been swapped into the wrong slots: $\displaystyle 35$ now sits where the mass number belongs, and $\displaystyle 79$ sits where the atomic number belongs. That symbol is asserting \(\displaystyle Z = 79\) for bromine — but atomic number $\displaystyle 79$ belongs to gold, not bromine, so it directly contradicts the element named by the symbol "Br". It also fails on a physical count: the number of neutrons is \[N = A - Z \] Substituting the swapped values, \(\displaystyle N = 35 - 79 = -44\), a negative neutron count, which cannot exist. This is the mistake people make when they treat superscript and subscript as interchangeable labels instead of two specific quantities tied to specific positions.Why \(\displaystyle {}^{35}\text{Br}\) is not acceptable. With no subscript shown, the lone number "$\displaystyle 35$" is read as sitting in the mass-number position — so this symbol claims bromine has mass number \(\displaystyle A=35\). Combined with the correct \(\displaystyle Z=35\) that "Br" always implies, that would give \[N = A - Z = 35 - 35 = 0 \] a bromine atom with zero neutrons — which is not one of bromine's real isotopes (only \(\displaystyle A=79\) and \(\displaystyle A=81\) occur). Dropping the atomic-number subscript is allowed only because it duplicates information already fixed by the element symbol; it is never allowed to drop or misplace the mass number, since that is the one variable piece of information the symbol exists to convey.**Answer: \(\displaystyle {}^{79}_{35}\text{Br}\) and \(\displaystyle {}^{79}\text{Br}\) are valid because the atomic number ($\displaystyle 35$) is redundant once "Br" is written and can be omitted, while the mass number ($\displaystyle 79$) must always be shown in its correct upper-left position. \(\displaystyle {}^{35}_{79}\text{Br}\) is invalid because it misplaces the numbers and asserts \(\displaystyle Z=79\) (gold's atomic number, not bromine's), giving an impossible negative neutron count. \(\displaystyle {}^{35}\text{Br}\) is invalid because it misstates the mass number as $\displaystyle 35$, which is not a real isotope of bromine (only $\displaystyle 79$ and $\displaystyle 81$ are).
  2. Exercise 2.42

    An element with mass number 81\displaystyle 81 contains 31.7\displaystyle 31.7% more neutrons as compared to protons. Assign the atomic symbol.
    NCERT’s answer
    81Br $\displaystyle 35$
    The mass number tells you protons + neutrons; "$\displaystyle 31.7$% more neutrons than protons" tells you the ratio between them. Two equations, two unknowns — solve for the proton count, then read the symbol off the periodic table.Let the number of protons be \(\displaystyle p \). Since neutrons are $\displaystyle 31.7$% more than protons, the number of neutrons is\[n = p + 0.317\,p = 1.317\,p \]Step $\displaystyle 1$ — use the mass number.Mass number \(\displaystyle A \) is the total count of protons and neutrons in the nucleus, \(\displaystyle A = p + n \). Here \(\displaystyle A = 81 \):\[p + n = 81 \]Step $\displaystyle 2$ — substitute and solve for \(\displaystyle p\).Putting \(\displaystyle n = 1.317\,p \) into \(\displaystyle p + n = 81 \):\[p + 1.317\,p = 81 \] \[2.317\,p = 81 \] \[p = \frac{81}{2.317} = 34.96 \]The number of protons has to be a whole number (you cannot have a fraction of a proton) — this is the step people slip on, rounding a percentage-based equation and forgetting the answer must land on an integer. Rounding to the nearest whole number:\[p = 35 \]Step $\displaystyle 3$ — get the neutron count and check it.\[n = A - p = 81 - 35 = 46 \]Checking against the given condition, the percentage by which neutrons exceed protons is\[\frac{n - p}{p} \times 100 = \frac{46 - 35}{35} \times 100 = \frac{11}{35} \times 100 = 31.4\% \]This matches the stated $\displaystyle 31.7$% to the precision the problem's rounded percentage justifies, confirming \(\displaystyle p = 35 \) is correct.Step $\displaystyle 4$ — identify the element.The number of protons \(\displaystyle p \) is the atomic number \(\displaystyle Z \). \(\displaystyle Z = 35 \) is bromine (Br) on the periodic table. With mass number $\displaystyle 81$, the nuclide is written with mass number as a left superscript and atomic number as a left subscript:\[^{81}_{35}\text{Br} \]Answer: The element is bromine, \(\displaystyle ^{81}_{35}\text{Br} \), with $\displaystyle 35$ protons and $\displaystyle 46$ neutrons.
  3. Exercise 2.43

    An ion with mass number 37\displaystyle 37 possesses one unit of negative charge. If the ion conatins 11.1\displaystyle 11.1% more neutrons than the electrons, find the symbol of the ion.
    NCERT’s answer
    $\displaystyle 37$ Cl− $\displaystyle 1$ $\displaystyle 17$
    In an ion, the electron count shifts with the charge, but the neutron count depends only on the mass number and the (unchanged) proton count. Set up the three particle counts in terms of one unknown, the atomic number \(\displaystyle Z\), and use the two clues given — the ion's charge and the neutron-to-electron percentage — to pin \(\displaystyle Z\) down.Step $\displaystyle 1$: Write the neutron count from the mass number.Mass number \(\displaystyle A\) is protons plus neutrons: \(\displaystyle A = Z + n\), where \(\displaystyle Z\) is the number of protons and \(\displaystyle n\) is the number of neutrons. Here \(\displaystyle A = 37\), so\[n = 37 - Z \]Step $\displaystyle 2$: Write the electron count from the charge.The ion carries one unit of negative charge, meaning it has picked up one extra electron beyond the neutral atom's \(\displaystyle Z\) electrons. (This is the step people get backwards: a negative ion has more electrons than protons, a positive ion has fewer — the sign of the charge tells you which way to shift, not the mass number.) So the number of electrons in the ion is\[e = Z + 1 \]Step $\displaystyle 3$: Translate "$\displaystyle 11.1$% more neutrons than electrons" into an equation."$\displaystyle 11.1$% more than \(\displaystyle e\)" means \(\displaystyle n\) equals \(\displaystyle e\) plus $\displaystyle 11.1$% of \(\displaystyle e\), i.e. \(\displaystyle n = 1.111\,e\) (keeping the extra digit rather than rounding here, since this is mid-calculation, not the final answer):\[n = e + 0.111e = 1.111\,e \]Step $\displaystyle 4$: Combine and solve for \(\displaystyle Z\).Substitute the expressions for \(\displaystyle n\) and \(\displaystyle e\) from Steps $\displaystyle 1$ and $\displaystyle 2$:\[37 - Z = 1.111(Z + 1) \]\[37 - Z = 1.111Z + 1.111 \]\[37 - 1.111 = 1.111Z + Z \]\[35.889 = 2.111\,Z \]\[Z = \frac{35.889}{2.111} = 17.00 \]Since \(\displaystyle Z\) must be a whole number (it counts protons), this rounds — cleanly, with no ambiguity — to\[Z = 17 \]Step $\displaystyle 5$: Check the numbers against the original clue.With \(\displaystyle Z = 17\): neutrons \(\displaystyle n = 37 - 17 = 20\), and electrons \(\displaystyle e = 17 + 1 = 18\). The ratio is\[\frac{n}{e} = \frac{20}{18} = 1.1\overline{1} = 111.1\% \]so \(\displaystyle n\) is indeed $\displaystyle 11.1$% more than \(\displaystyle e\) — the numbers close exactly, confirming \(\displaystyle Z = 17\).Step $\displaystyle 6$: Identify the element and write the ion symbol.\(\displaystyle Z = 17\) is chlorine (Cl). With mass number $\displaystyle 37$ and a charge of \(\displaystyle -1\) ($\displaystyle 17$ protons, $\displaystyle 18$ electrons, $\displaystyle 20$ neutrons), the ion is written with the mass number as a left superscript, the atomic number as a left subscript, and the charge as a right superscript:\[{}^{37}_{17}\text{Cl}^- \]Answer: The ion is \(\displaystyle {}^{37}_{17}\text{Cl}^- \) — chlorine-$\displaystyle 37$ anion, with $\displaystyle 17$ protons, $\displaystyle 20$ neutrons, and $\displaystyle 18$ electrons.
  4. Exercise 2.44

    An ion with mass number 56\displaystyle 56 contains 3\displaystyle 3 units of positive charge and 30.4\displaystyle 30.4% more neutrons than electrons. Assign the symbol to this ion.
    NCERT’s answer
    $\displaystyle 56$ Fe $\displaystyle 3$+ $\displaystyle 26$
    An ion's positive charge tells you how many more protons it has than electrons — start from that relationship, not from the mass number alone.Let the number of electrons in the ion be \(\displaystyle e \). Since the ion carries $\displaystyle 3$ units of positive charge, it has $\displaystyle 3$ more protons than electrons: \[p = e + 3 \]The mass number \(\displaystyle A\) counts protons plus neutrons, \(\displaystyle A = p + n\), and here \(\displaystyle A = 56\), so the number of neutrons is \[n = 56 - p = 56 - (e+3) = 53 - e \]"$\displaystyle 30.4$% more neutrons than electrons" is a statement about \(\displaystyle n\) in terms of \(\displaystyle e\), and it is the step where people plug in the wrong base number. It means \[n = e + 0.304\,e = 1.304\,e \] not \(\displaystyle 0.304\) times the mass number, and not \(\displaystyle 30.4\%\) of the protons.Now both expressions equal \(\displaystyle n\), so set them equal: \[53 - e = 1.304\,e \]Collect the \(\displaystyle e\) terms: \[53 = 1.304\,e + e = 2.304\,e \]\[e = \frac{53}{2.304} = 23.00 \]So \(\displaystyle e = 23 \) electrons.Now work back: \[p = e + 3 = 23 + 3 = 26 \] \[n = 53 - e = 53 - 23 = 30 \]Check the neutron condition directly, since it's easy to mis-substitute: \(\displaystyle 30.4\%\) more than $\displaystyle 23$ electrons is \[23 + 0.304 \times 23 = 23 + 6.99 = 29.99 \approx 30 \] which matches \(\displaystyle n = 30\). The mass number also checks out: \(\displaystyle p + n = 26 + 30 = 56\).The atomic number \(\displaystyle Z\) equals the number of protons, and \(\displaystyle Z = 26\) is the element iron (Fe). With $\displaystyle 23$ electrons against $\displaystyle 26$ protons, the ion carries a net charge of \(\displaystyle +3\), consistent with what was given.The ion is written with mass number as a left superscript, atomic number as a left subscript, and the ionic charge as a right superscript: \[{}^{56}_{26}\text{Fe}^{3+} \]Answer: \(\displaystyle {}^{56}_{26}\text{Fe}^{3+} \) — iron-$\displaystyle 56$ with $\displaystyle 26$ protons, $\displaystyle 30$ neutrons, and $\displaystyle 23$ electrons (a $\displaystyle 3$+ ion).
  5. Exercise 2.45

    Arrange the following type of radiations in increasing order of frequency:
    (a)
    radiation from microwave oven
    (b)
    amber light from traffic signal
    (c)
    radiation from FM radio
    (d)
    cosmic rays from outer space and
    (e)
    X-rays.

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    NCERT’s answer
    Cosmic rays > X–rays > amber colour > microwave > FM
    Frequency and wavelength run in opposite directions. The formula that connects them is\[\nu = \frac{c}{\lambda} \]where \(\displaystyle \nu\) is frequency, \(\displaystyle c\) is the speed of light \(\displaystyle \big(3.0\times10^{8}\ \text{m s}^{-1}\big)\), and \(\displaystyle \lambda\) is wavelength. Because \(\displaystyle c\) is fixed, a shorter wavelength always means a higher frequency. If you try to rank these radiations by imagining which one "feels bigger" or "more powerful" without going through this formula, it is easy to get the order backwards — always convert to frequency before comparing.Take each radiation's known wavelength (or frequency) range and put it through \(\displaystyle \nu = c/\lambda\):(c) FM radio. FM broadcast sits in the band $\displaystyle 88$–$\displaystyle 108$ MHz; take a representative value, \(\displaystyle \nu \approx 1\times10^{8}\ \text{Hz}\) (equivalently \(\displaystyle \lambda \approx 3\ \text{m}\), since \(\displaystyle \lambda = c/\nu = (3.0\times10^{8}\ \text{m s}^{-1})/(1\times10^{8}\ \text{Hz}) = 3\ \text{m}\)).(a) Microwave oven. Ovens are built to run at the fixed microwave frequency \(\displaystyle \nu = 2450\ \text{MHz} = 2.45\times10^{9}\ \text{Hz}\).(b) Amber light. Amber sits around \(\displaystyle \lambda \approx 600\ \text{nm} = 6.0\times10^{-7}\ \text{m}\). Then \[\nu = \frac{c}{\lambda} = \frac{3.0\times10^{8}\ \text{m s}^{-1}}{6.0\times10^{-7}\ \text{m}} = 5.0\times10^{14}\ \text{Hz} \](e) X-rays. X-rays span roughly \(\displaystyle \lambda \approx 10^{-8}\) to \(\displaystyle 10^{-11}\ \text{m}\); take a representative value \(\displaystyle \lambda = 1\ \text{nm} = 1\times10^{-9}\ \text{m}\): \[\nu = \frac{c}{\lambda} = \frac{3.0\times10^{8}\ \text{m s}^{-1}}{1\times10^{-9}\ \text{m}} = 3\times10^{17}\ \text{Hz} \](d) Cosmic rays. These are the most energetic radiations known to reach Earth, with wavelengths far shorter than X-rays (\(\displaystyle \lambda \ll 10^{-12}\ \text{m}\)), so \[\nu = \frac{c}{\lambda} \gg 3\times10^{20}\ \text{Hz} \]Lining the frequencies up from smallest to largest:\[\underbrace{1\times10^{8}}_{\text{(c) FM radio}} < \underbrace{2.45\times10^{9}}_{\text{(a) microwave}} < \underbrace{5.0\times10^{14}}_{\text{(b) amber light}} < \underbrace{3\times10^{17}}_{\text{(e) X-rays}} < \underbrace{\gg3\times10^{20}}_{\text{(d) cosmic rays}}\ \text{Hz} \]Answer: increasing order of frequency is (c) FM radio < (a) microwave oven < (b) amber light < (e) X-rays < (d) cosmic rays.
  6. Exercise 2.46

    Nitrogen laser produces a radiation at a wavelength of 337.1\displaystyle 337.1 nm. If the number of photons emitted is 5.6\displaystyle 5.6 × 1024\displaystyle 1024, calculate the power of this laser.
    NCERT’s answer
    3.$\displaystyle 3$ × $\displaystyle 106$ J
    Power is energy delivered per second — so the first job is to find the total energy carried by all the photons, then treat "photons emitted" as "photons emitted per second."Each photon of the laser radiation carries a fixed quantum of energy given by Planck's relation\[E = \frac{hc}{\lambda} \]where \(\displaystyle h = 6.626 \times 10^{-34}\ \text{J s}\) is Planck's constant, \(\displaystyle c = 3 \times 10^{8}\ \text{m s}^{-1}\) is the speed of light, and \(\displaystyle \lambda\) is the wavelength of the radiation.Step $\displaystyle 1$: Convert the wavelength to metres.The formula needs \(\displaystyle \lambda\) in metres, not nanometres — mixing units here is the step people slip on.\[\lambda = 337.1\ \text{nm} = 337.1 \times 10^{-9}\ \text{m} = 3.371 \times 10^{-7}\ \text{m} \]Step $\displaystyle 2$: Find the energy of one photon.\[E = \frac{(6.626 \times 10^{-34}\ \text{J s})(3 \times 10^{8}\ \text{m s}^{-1})}{3.371 \times 10^{-7}\ \text{m}} \]\[E = \frac{1.9878 \times 10^{-25}\ \text{J m}}{3.371 \times 10^{-7}\ \text{m}} = 5.897 \times 10^{-19}\ \text{J} \]So every photon this laser emits carries \(\displaystyle 5.897 \times 10^{-19}\ \text{J}\).Step $\displaystyle 3$: Find the total energy carried by all the photons.Total energy is just (energy per photon) × (number of photons), \(\displaystyle N\):\[E_{\text{total}} = N \times E = (5.6 \times 10^{24}) \times (5.897 \times 10^{-19}\ \text{J}) \]\[E_{\text{total}} = 3.302 \times 10^{6}\ \text{J} \]Step $\displaystyle 4$: Turn this energy into power.Power is energy per unit time,\[P = \frac{E_{\text{total}}}{t} \]Here the \(\displaystyle 5.6 \times 10^{24}\) photons are the number the laser emits in one second of operation, so \(\displaystyle t = 1\ \text{s}\) and the total energy computed above is delivered in that one second — this is the step that is easy to miss, because the problem never states "per second" outright, it is built into what "number of photons emitted" means for a running laser.\[P = \frac{3.302 \times 10^{6}\ \text{J}}{1\ \text{s}} = 3.302 \times 10^{6}\ \text{W} \]Rounding to three significant figures (matching the precision of the given wavelength and photon count):\[P \approx 3.30 \times 10^{6}\ \text{W} \]Answer: The power of the laser is \(\displaystyle 3.30 \times 10^{6}\ \text{W}\) (about $\displaystyle 3.3$ megawatts).
  7. Exercise 2.47

    Neon gas is generally used in the sign boards. If it emits strongly at 616\displaystyle 616 nm, calculate
    (a)
    the frequency of emission,
    (b)
    distance traveled by this radiation in 30\displaystyle 30 s
    (c)
    energy of quantum and
    (d)
    number of quanta present if it produces 2\displaystyle 2 J of energy.
    NCERT’s answer
    (a)
    4.$\displaystyle 87$ × $\displaystyle 1014$ s–$\displaystyle 1$ (b) $\displaystyle 9.0$ × $\displaystyle 109$ m (c) $\displaystyle 32.27$ × $\displaystyle 10$–$\displaystyle 20$ J (d) $\displaystyle 6.2$ × $\displaystyle 1018$ quanta
    Frequency, wavelength and energy of a photon are all linked through the same two constants, \(\displaystyle c\) and \(\displaystyle h\) — convert the wavelength to metres first, or every part after it goes wrong.Given: \(\displaystyle \lambda = 616\ \text{nm} = 616 \times 10^{-9}\ \text{m} = 6.16 \times 10^{-7}\ \text{m}\)A stray factor of \(\displaystyle 10^{3}\) or \(\displaystyle 10^{6}\) at this step is the single most common mistake in this problem, since nm, µm and m are three different scales — always write the conversion out before substituting.(a) Frequency from \(\displaystyle \nu = \dfrac{c}{\lambda}\)Here \(\displaystyle c\) is the speed of light in vacuum \(\displaystyle \left(3 \times 10^{8}\ \text{m s}^{-1}\right)\), \(\displaystyle \lambda\) is the wavelength, and \(\displaystyle \nu\) is the frequency.\[\nu = \frac{c}{\lambda} = \frac{3 \times 10^{8}\ \text{m s}^{-1}}{6.16 \times 10^{-7}\ \text{m}} = \frac{3}{6.16} \times 10^{8-(-7)}\ \text{s}^{-1} \]\[\nu = 0.48701 \times 10^{15}\ \text{s}^{-1} = 4.8701 \times 10^{14}\ \text{s}^{-1} \]Rounded to three significant figures (matching the three figures in $\displaystyle 616$ nm):\[\nu \approx 4.87 \times 10^{14}\ \text{s}^{-1} \;(= 4.87 \times 10^{14}\ \text{Hz}) \](b) Distance travelled uses the ordinary speed–time relation, not anything specific to light's wave nature.Distance = speed × time, with \(\displaystyle c = 3 \times 10^{8}\ \text{m s}^{-1}\) and \(\displaystyle t = 30\ \text{s}\):\[d = c \times t = \left(3 \times 10^{8}\ \text{m s}^{-1}\right) \times \left(30\ \text{s}\right) = 90 \times 10^{8}\ \text{m} \]\[d = 9 \times 10^{9}\ \text{m} \](c) Energy of one quantum comes from Planck's relation \(\displaystyle E = h\nu\).Here \(\displaystyle h\) is Planck's constant \(\displaystyle \left(6.626 \times 10^{-34}\ \text{J s}\right)\) and \(\displaystyle \nu\) is the frequency found in part (a) (using the unrounded value keeps the rounding error out of this step).\[E = h\nu = \left(6.626 \times 10^{-34}\ \text{J s}\right) \times \left(4.87013 \times 10^{14}\ \text{s}^{-1}\right) \]\[E = 6.626 \times 4.87013 \times 10^{-34+14}\ \text{J} = 32.2695 \times 10^{-20}\ \text{J} \]\[E = 3.22695 \times 10^{-19}\ \text{J} \approx 3.23 \times 10^{-19}\ \text{J} \]This \(\displaystyle E\) is the energy carried by a single photon (quantum) of this light — it is not the total energy of the beam, which is the quantity part (d) asks about.(d) Number of quanta in a given total energy is total energy divided by energy per quantum.If \(\displaystyle n\) quanta together carry energy \(\displaystyle E_{\text{total}}\), then \(\displaystyle E_{\text{total}} = n \times E\), so:\[n = \frac{E_{\text{total}}}{E} = \frac{2\ \text{J}}{3.22695 \times 10^{-19}\ \text{J}} \]\[n = 0.61978 \times 10^{19} = 6.1978 \times 10^{18} \]\[n \approx 6.20 \times 10^{18}\ \text{quanta} \]The unit check here is what protects the answer: J divided by J leaves a pure number, which is exactly what "number of quanta" must be — if units survive the division, a wrong formula was used.Answer: (a) \(\displaystyle \nu \approx 4.87 \times 10^{14}\ \text{s}^{-1}\); (b) \(\displaystyle d = 9 \times 10^{9}\ \text{m}\); (c) \(\displaystyle E \approx 3.23 \times 10^{-19}\ \text{J}\) per quantum; (d) \(\displaystyle n \approx 6.20 \times 10^{18}\) quanta.
  8. Exercise 2.48

    In astronomical observations, signals observed from the distant stars are generally weak. If the photon detector receives a total of 3.15\displaystyle 3.15 × 10\displaystyle 1018\displaystyle 18 J from the radiations of 600\displaystyle 600 nm, calculate the number of photons received by the detector.
    NCERT’s answer
    $\displaystyle 10$
    The energy carried by one photon is fixed by its wavelength; divide the total energy landing on the detector by the energy of a single photon to get how many photons that must be.Step $\displaystyle 1$ — energy of one photonPlanck's relation \(\displaystyle E = h\nu = \dfrac{hc}{\lambda} \) gives the energy of a single photon, where
    \(\displaystyle h = 6.626 \times 10^{-34}\ \text{J s} \) (Planck's constant),
    \(\displaystyle c = 3.0 \times 10^{8}\ \text{m s}^{-1} \) (speed of light),
    \(\displaystyle \lambda \) is the wavelength of the radiation.
    The wavelength is given in nanometres, and the formula needs metres — mixing nm with SI \(\displaystyle h\) and \(\displaystyle c\) is the step that quietly wrecks this calculation. Convert first: \[\lambda = 600\ \text{nm} = 600 \times 10^{-9}\ \text{m} = 6.00 \times 10^{-7}\ \text{m} \]Now substitute: \[E = \frac{(6.626 \times 10^{-34}\ \text{J s})(3.0 \times 10^{8}\ \text{m s}^{-1})}{6.00 \times 10^{-7}\ \text{m}} \]Multiply the numerator first: \[6.626 \times 3.0 = 19.878 \quad\Rightarrow\quad hc = 19.878 \times 10^{-34+8}\ \text{J m} = 1.9878 \times 10^{-25}\ \text{J m} \]Divide by \(\displaystyle \lambda\): \[E = \frac{1.9878 \times 10^{-25}\ \text{J m}}{6.00 \times 10^{-7}\ \text{m}} = 0.3313 \times 10^{-18}\ \text{J} = 3.313 \times 10^{-19}\ \text{J} \]So each photon of $\displaystyle 600$ nm light carries \(\displaystyle 3.313 \times 10^{-19}\ \text{J}\).Step $\displaystyle 2$ — how many such photons make up the total energy receivedThe detector's total energy is the sum of the energies of all the photons it absorbed, so \[N = \frac{\text{total energy received}}{\text{energy of one photon}} = \frac{E_{\text{total}}}{E} \]This is the step where it's tempting to divide the wrong way (energy-per-photon ÷ total) — keep total energy on top, since more total energy for the same wavelength must mean more photons, not fewer.\[N = \frac{3.15 \times 10^{-18}\ \text{J}}{3.313 \times 10^{-19}\ \text{J}} = \frac{3.15}{3.313} \times 10^{-18+19} = 0.9508 \times 10^{1} = 9.508 \]Step $\displaystyle 3$ — round to what the data supportsThe given data (\(\displaystyle 3.15\), \(\displaystyle 600\)) carry three significant figures, so the count rounds to \(\displaystyle 9.51\). But a "number of photons" is a count of discrete particles — it cannot be a fraction of a photon — so the physically meaningful reading is the nearest whole number, about $\displaystyle 10$ photons.\[N \approx 9.51 \approx 10 \text{ photons} \]Answer: N ≈ $\displaystyle 9.51$ (≈ $\displaystyle 10$ photons, since the detector must receive a whole number of photons).
  9. Exercise 2.49

    Lifetimes of the molecules in the excited states are often measured by using pulsed radiation source of duration nearly in the nano second range. If the radiation source has the duration of 2\displaystyle 2 ns and the number of photons emitted during the pulse source is 2.5\displaystyle 2.5 × 1015\displaystyle 1015, calculate the energy of the source.
    NCERT’s answer
    8.$\displaystyle 28$ × $\displaystyle 10$–$\displaystyle 10$ J
    The trick here is finding the frequency: the pulse duration itself is treated as one full cycle of the wave, so frequency is $\displaystyle 1$ divided by that duration — not something you're given directly.You're told how long the pulse lasts and how many photons come out of it, but not the frequency or wavelength of the radiation directly. The bridge is this: if a pulse lasts a time \(\displaystyle t \), that time is taken as the period of one oscillation of the wave, so the frequency is\[\nu = \frac{1}{t} \]where \(\displaystyle \nu \) is frequency (in \(\displaystyle \text{s}^{-1} \), i.e. Hz) and \(\displaystyle t \) is the pulse duration in seconds.Step $\displaystyle 1$ — Frequency of the radiation\[t = 2\ \text{ns} = 2 \times 10^{-9}\ \text{s} \]\[\nu = \frac{1}{2 \times 10^{-9}\ \text{s}} = 5 \times 10^{8}\ \text{s}^{-1} \]Step $\displaystyle 2$ — Energy of one photonPlanck's relation gives the energy of a single photon:\[E = h\nu \]where \(\displaystyle h = 6.626 \times 10^{-34}\ \text{J s} \) is Planck's constant and \(\displaystyle \nu \) is the frequency just found. Using \(\displaystyle \nu \) here (not the wavelength, and not the pulse duration itself) is exactly the point where it's easy to plug in the wrong number.\[E = (6.626 \times 10^{-34}\ \text{J s})(5 \times 10^{8}\ \text{s}^{-1}) = 3.313 \times 10^{-25}\ \text{J} \]This is the energy carried by a single photon of this radiation.Step $\displaystyle 3$ — Total energy of the sourceThe source doesn't emit one photon, it emits \(\displaystyle N = 2.5 \times 10^{15} \) photons during the pulse. The total energy is the energy per photon multiplied by the number of photons — a step that's easy to skip if you stop at Step $\displaystyle 2$ and mistake "energy of one photon" for "energy of the source":\[E_{\text{total}} = N \times E \]\[E_{\text{total}} = (2.5 \times 10^{15})(3.313 \times 10^{-25}\ \text{J}) = 8.2825 \times 10^{-10}\ \text{J} \]The input data ($\displaystyle 2$ ns, \(\displaystyle 2.5 \times 10^{15} \) photons) carries at most three significant figures, so the result is rounded once, at the end, to three significant figures:\[E_{\text{total}} \approx 8.28 \times 10^{-10}\ \text{J} \]Answer: \(\displaystyle 8.28 \times 10^{-10}\ \text{J} \)
  10. Exercise 2.50

    The longest wavelength doublet absorption transition is observed at 589\displaystyle 589 and 589.6\displaystyle 589.6 nm. Calcualte the frequency of each transition and energy difference between two excited states.
    NCERT’s answer
    3.$\displaystyle 45$ × $\displaystyle 10$–$\displaystyle 22$ J
    A doublet means two very close spectral lines — here two slightly different wavelengths from transitions ending on two closely-spaced excited states. Frequency comes from \(\displaystyle \nu = c/\lambda \), and the energy gap between those two states is \(\displaystyle \Delta E = h\,\Delta\nu \), not \(\displaystyle h\nu \) of either line alone.Step $\displaystyle 1$ — convert wavelengths to metres.The two lines are given in nanometres; the frequency formula needs SI units (metres), so first convert:\[\lambda_1 = 589\ \text{nm} = 589\times10^{-9}\ \text{m} = 5.89\times10^{-7}\ \text{m} \] \[\lambda_2 = 589.6\ \text{nm} = 589.6\times10^{-9}\ \text{m} = 5.896\times10^{-7}\ \text{m} \]A common slip here is plugging the nanometre number straight into \(\displaystyle \nu = c/\lambda \) with \(\displaystyle c \) in m/s — the powers of ten don't cancel, and the frequency comes out a billion times too large.Step $\displaystyle 2$ — frequency of each line, using \(\displaystyle \nu = c/\lambda \) (here \(\displaystyle \nu \) = frequency, \(\displaystyle c \) = speed of light \(\displaystyle = 3.0\times10^{8}\ \text{m s}^{-1} \), \(\displaystyle \lambda \) = wavelength).\[\nu_1 = \frac{c}{\lambda_1} = \frac{3.0\times10^{8}\ \text{m s}^{-1}}{5.89\times10^{-7}\ \text{m}} = 5.093\times10^{14}\ \text{s}^{-1} \]\[\nu_2 = \frac{c}{\lambda_2} = \frac{3.0\times10^{8}\ \text{m s}^{-1}}{5.896\times10^{-7}\ \text{m}} = 5.088\times10^{14}\ \text{s}^{-1} \]Step $\displaystyle 3$ — energy difference between the two excited states.Each line's photon energy is \(\displaystyle E = h\nu \) (\(\displaystyle h \) = Planck's constant \(\displaystyle = 6.626\times10^{-34}\ \text{J s} \)), so the energy gap between the two excited states the photons come from is\[\Delta E = h\nu_1 - h\nu_2 = h(\nu_1-\nu_2) = h\,\Delta\nu \]Subtracting \(\displaystyle \nu_1 - \nu_2 \) directly from the two rounded frequencies above would throw away most of the significant figures — two nearly equal $\displaystyle 15$-digit numbers minus each other loses precision fast. It is safer to get \(\displaystyle \Delta\nu \) straight from the wavelengths, without rounding \(\displaystyle \nu_1 \) and \(\displaystyle \nu_2 \) first:\[\Delta\nu = \frac{c}{\lambda_1}-\frac{c}{\lambda_2} = c\left(\frac{\lambda_2-\lambda_1}{\lambda_1\lambda_2}\right) \]With \(\displaystyle \lambda_2-\lambda_1 = 589.6\ \text{nm} - 589\ \text{nm} = 0.6\ \text{nm} = 6\times10^{-10}\ \text{m} \) and \(\displaystyle \lambda_1\lambda_2 = (5.89\times10^{-7}\ \text{m})(5.896\times10^{-7}\ \text{m}) = 3.4727\times10^{-13}\ \text{m}^2 \):\[\Delta\nu = \left(3.0\times10^{8}\ \text{m s}^{-1}\right)\times\frac{6\times10^{-10}\ \text{m}}{3.4727\times10^{-13}\ \text{m}^2} = 5.184\times10^{11}\ \text{s}^{-1} \]Now bring in Planck's constant:\[\Delta E = h\,\Delta\nu = \left(6.626\times10^{-34}\ \text{J s}\right)\times\left(5.184\times10^{11}\ \text{s}^{-1}\right) = 3.435\times10^{-22}\ \text{J} \]Rounding to three significant figures, matching the precision the given wavelengths justify ($\displaystyle 589$ nm has three sig figs):\[\nu_1 = 5.093\times10^{14}\ \text{s}^{-1}, \qquad \nu_2 = 5.088\times10^{14}\ \text{s}^{-1}, \qquad \Delta E = 3.43\times10^{-22}\ \text{J} \]Answer: \(\displaystyle \nu_1 = 5.093\times10^{14}\ \text{s}^{-1} \) (for $\displaystyle 589$ nm), \(\displaystyle \nu_2 = 5.088\times10^{14}\ \text{s}^{-1} \) (for $\displaystyle 589.6$ nm), and the energy difference between the two excited states is \(\displaystyle \Delta E \approx 3.43\times10^{-22}\ \text{J} \).