Q.(a) Account for the following:
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Start your 14-day free trial to unlock the full solution →Concept understanding — Magnetism and Color
Magnetism and Colour: An Intuitive First Look
You've probably noticed that some materials are magnetic (like iron) and others aren't (like wood). And you've seen that objects have different colours — a rose is red, the sky is blue. At first glance, these two properties seem completely unrelated. But at the deepest level, both magnetism and colour come from the same source: how electrons behave inside atoms.
Let's start with a simple picture.
The Intuition: Electrons as Tiny Magnets and Painters
Imagine an electron orbiting the nucleus of an atom. That moving charge is like a tiny loop of electric current — and any loop of current creates a magnetic field. So every electron is a microscopic magnet. In most materials, these tiny magnets point in random directions and cancel out. But in iron, they align, and the material becomes magnetic.
Now, colour. When light hits an atom, electrons can absorb some of its energy and jump to a higher orbit. The colour we see is the light that wasn't absorbed — the leftover wavelengths. Different atoms absorb different colours because their electrons have different "jump sizes" (energy levels).
So both magnetism and colour are about how electrons move and interact with their environment. One is about the direction of electron spin and orbit (magnetism), the other about the energy of electron jumps (colour).
The Precise Statement
Magnetism and colour are both consequences of the electronic structure of atoms, but they arise from different aspects of electron behaviour:
- Magnetism originates from the magnetic moments of electrons — their spin and orbital motion. A material is magnetic when these moments align cooperatively.
- Colour originates from the absorption of specific wavelengths of light by electrons, which occurs when the photon energy matches the energy difference between two electron states.
How They Connect (and How They Don't)
The two phenomena are linked because they both depend on the arrangement of electrons in orbitals — the so-called electronic configuration. But they are not the same thing, and one does not cause the other.
Here's a table to make the distinction clear:
| Property | Origin | What determines it? | Example |
|---|---|---|---|
| Magnetism | Electron spin and orbital motion | Unpaired electrons, crystal structure | Iron is magnetic because it has 4 unpaired electrons per atom |
| Colour | Electron transitions between energy levels | Energy gap between orbitals | Copper is reddish because its electrons absorb blue-green light |
A material can be magnetic and colourless (like pure iron — it's silvery, not colourful). A material can be brilliantly coloured and non-magnetic (like a ruby). The two properties are independent in most everyday cases.
The Deeper Link: Transition Metals
The most interesting connection appears in transition metals (elements like iron, cobalt, nickel, copper). These atoms have partially filled d orbitals. That partial filling does two things:
- It leaves unpaired electrons, which can align to produce magnetism. …
Why this formula?
Magnetism and Color: Why the Key Formulas Hold
This is a fascinating intersection of physics and perception. The core idea is that color is not a property of light itself, but of our brain's interpretation of different wavelengths. Magnetism, in turn, can influence how these wavelengths are produced or absorbed.
Let's break down the key formulas and their why.
1. The Fundamental Link: Energy, Frequency, and Color
The most important formula connecting magnetism and color is the Planck-Einstein relation:
Where:
- = energy of a photon (light particle)
- = Planck's constant ()
- = frequency of the light
Why does this hold?
- Quantum nature of light: Light is not a continuous wave, but comes in discrete packets called photons.
- Energy quantization: The energy of a photon is directly proportional to its frequency. Higher frequency means higher energy.
- Magnetism's role: When an electron in an atom jumps from a higher energy level to a lower one, it emits a photon. The energy difference () between these levels determines the photon's frequency:
- Color perception: Our eyes detect different frequencies as different colors. For example:
- Red light: (lower energy)
- Blue light: (higher energy)
Key insight: The color you see is determined by the energy gap between electron orbits. Magnetism can alter these energy gaps (via the Zeeman effect, see below).
2. The Zeeman Effect: How Magnetic Fields Split Colors
When a magnetic field is applied to an atom, a single spectral line (one color) splits into multiple lines. This is described by:
Where:
- = energy shift of the spectral line
- = Bohr magneton ()
- = magnetic field strength (in Tesla)
- = magnetic quantum number (integer: )
Why does this hold?
- Electron as a tiny magnet: An electron orbiting a nucleus behaves like a tiny current loop, creating a magnetic dipole moment.
- Energy in a magnetic field: This dipole moment interacts with an external magnetic field. The interaction energy depends on the orientation of the electron's orbit relative to the field.
- Quantized orientations: The magnetic quantum number tells us which orientation is allowed. Each orientation has a slightly different energy.
- Result: A single energy level splits into sub-levels. Transitions between these sub-levels produce photons with slightly different energies — hence different colors appear.
Example: A sodium lamp emits yellow light. In a strong magnetic field, that yellow line splits into three closely spaced lines (normal Zeeman effect).
3. Faraday Rotation: Magnetic Field Twists Light's Color
When polarized light passes through a material in a magnetic field, its plane of polarization rotates. The rotation angle is:
Where:
- = rotation angle (in radians)
- = Verdet constant (material-specific, depends on wavelength)
- = magnetic field strength
- = path length through the material
Why does this hold?
- Circular birefringence: In a magnetic field, the material has different refractive indices for left- and right-circularly polarized light.
- Phase difference: These two components travel at different speeds, creating a phase difference.
- Recombination: When they recombine, the resulting linear polarization is rotated. …
(a) () white vs () coloured; chromate↔dichromate with pH; Zn/Cd/Hg so not transition; (, 3 unpaired) → BM.
(b) Ln vs An differ in oxidation states, radioactivity and complex formation; () diamagnetic; Cr > Cu in m.p./b.p.
(i) Cu(I) white, Cu(II) coloured
Colour needs a d–d transition, hence a partly filled d-subshell. is (completely filled) → no transition → white/colourless. is (one vacancy) → an electron can be promoted within the split d-orbitals, absorbing visible light → coloured (e.g. blue ).
(ii) Chromates in acid
Chromate–dichromate is a pH-dependent equilibrium:
Adding acid shifts it right (Le Chatelier) → yellow turns orange. Cr stays +6, so this is not a redox change.
(iii) Zn, Cd, Hg not transition elements
Their configurations are , , ; in the common +2 ion the d-subshell is completely filled (). A transition element must have a partly filled d-subshell in its atom or a common ion, which these never do — so they are d-block but non-transition.
Concept understanding — Actinoids
Actinoids: The Heavy, Radioactive Inner Transition Metals
Imagine you are walking through the periodic table, row by row. You know the lanthanoids — the 14 elements from cerium to lutetium that sit below the main table, where the 4f subshell is being filled. Now go one row lower. The elements that follow actinium (atomic number 89) are the actinoids: thorium (90) through lawrencium (103). Here, the 5f subshell is being filled.
The name comes from actinium, the first element of the series. But the real story begins with uranium and plutonium — the elements that made nuclear energy and atomic bombs possible. These are not just academic curiosities; they are the workhorses of nuclear physics.
The Precise Statement
Actinoids are the 14 elements from thorium () to lawrencium () in which the 5f orbitals are progressively filled. They are all radioactive, exhibit a wide range of oxidation states, and show a steady decrease in ionic radii across the series — the actinoid contraction.
Why They Are Special
1. Radioactivity is the rule, not the exception. Every actinoid is radioactive. Some, like uranium-238, have half-lives comparable to the age of the Earth. Others, like lawrencium, exist for only seconds. This radioactivity is not a side effect — it is the defining property. It means their chemistry is often studied with trace amounts, using radiation detectors rather than test tubes.
2. Multiple oxidation states — more than you expect. Unlike the lanthanoids, which mostly stick to +3, the actinoids show a rich variety. Uranium, for example, exists as U, U, UO (U), and UO (U). The early actinoids (Th, Pa, U, Np, Pu) are especially versatile because the 5f, 6d, and 7s orbitals are close in energy. As you move right, the +3 state becomes more stable — curium and beyond behave more like lanthanoids.
3. The actinoid contraction. As you go from Th to Lr, the nuclear charge increases by 14 protons. The 5f electrons are poor at shielding each other, so the effective nuclear charge felt by the outer electrons rises steadily. The result: ionic radii shrink smoothly across the series. This is exactly analogous to the lanthanoid contraction, and it has the same consequence — the chemistry of later actinoids becomes very similar to their lanthanoid counterparts, making separation difficult.
The actinoid contraction is why americium and curium are so hard to separate from the lanthanoids in nuclear waste. Their ionic radii are nearly identical.
A Quick Comparison with Lanthanoids
| Property | Lanthanoids (4f) | Actinoids (5f) |
|---|---|---|
| Radioactivity | Mostly stable (except Pm) | All radioactive |
| Common oxidation state | +3 (strongly dominant) | +3, +4, +5, +6 (early ones) |
| 5f vs 4f character | 4f deeply buried, little bonding | 5f more exposed, can participate in bonding |
(a) () white vs () coloured; chromate↔dichromate with pH; Zn/Cd/Hg so not transition; (, 3 unpaired) → BM.
(b) Ln vs An differ in oxidation states, radioactivity and complex formation; () diamagnetic; Cr > Cu in m.p./b.p.
spin-only moment
Co (Z=27): . Removing the two 4s electrons gives : , which has 3 unpaired electrons.
(Alternative) Part (a): Lanthanoids vs Actinoids — three differences
| Property | Lanthanoids | Actinoids |
|---|---|---|
| Oxidation states | mainly +3 (few +2/+4) | wide range +3 to +7 |
| Radioactivity | only Pm radioactive | all are radioactive |
| Complex formation | limited (4f buried, poorly shielded) | greater (5f more available) |
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