Physical Quantities & Measurement

Inside a locked vault on the outskirts of Paris sits a small platinum-iridium cylinder that, for 130 years, was the kilogram. Not "weighed" a kilogram — it defined the kilogram: every mass on Earth, from a jeweller's diamond to a cargo ship's manifest, was ultimately a comparison against this one object. Then metrologists noticed something disturbing. Compared against its own official copies, the cylinder's mass had drifted by roughly 50 micrograms — about the mass of a fingerprint. Which raises a genuinely strange question: if the kilogram is that object, what can it even mean to say the object's mass changed? Changed relative to what? That puzzle sits at the very entrance of physics, and this — the first module of your entire physics course — is about walking through that entrance properly. Physics begins the moment a vague impression ("this rock is heavy") becomes a physical quantity: a number multiplied by a unit ("2.3 kg"). Every equation you will ever write, from F=maF = ma to the energy of a photon, is a statement about such quantities, and every mark scheme from CBSE to Cambridge begins by checking whether you handled the number and the unit honestly. Master this module and three things happen: unit-conversion questions become 30-second free marks, the "why did my numerical value shrink when the unit grew?" MCQ stops being a coin-flip, and you'll understand why in 2019 humanity retired that Paris cylinder and pinned the kilogram to a constant of nature instead.

Key takeaways
  • A physical quantity is anything measurable, and its statement has two inseparable parts: Q=n×uQ = n \times u — a numerical value nn and a unit uu. "The length is 5" is meaningless; "5 m" is physics.
  • Measurement is comparison: you count how many times a chosen standard fits into the thing being measured.
  • A good standard must be invariant (unchanging), accessible (usable anywhere) and reproducible (same result for everyone) — the 2019 SI achieves all three by defining units through constants of nature instead of artefacts.
  • The quantity itself never changes when you change units, so n1u1=n2u2n_1 u_1 = n_2 u_2: the numerical value is inversely proportional to the size of the unit. Bigger unit, smaller number.
  • Quantities split into a handful of base quantities (defined independently) and everything else, derived quantities (built from them) — the architecture the next module maps in full.
  • Key idea: a measured quantity is a single invariant fact wearing a number-and-unit costume; change the unit and the number must change in exact compensation.
The core insight

Every physical quantity is a comparison against an agreed standard, expressed as Q=n uQ = n\,u — and because QQ itself is unit-independent, the numerical value nn scales inversely with the chosen unit uu.

Where this lives today

The 2019 redefinition was not ceremonial housekeeping. Because the kilogram is now pinned to the exact Planck constant h=6.626 070 15×10−34h = 6.626\,070\,15 \times 10^{-34} J s, any suitably equipped laboratory — in Delhi, Braunschweig or Boulder — can realise a kilogram from first principles with a Kibble balance, no pilgrimage to a French vault required. India's national metrology institute, CSIR-NPL in New Delhi, maintains exactly this traceability chain: the weight that calibrates a pharmaceutical balance in Hyderabad connects, through documented comparisons, all the way up to a constant of nature. Every barcode scale, fuel pump and blood-test analyser sits somewhere on such a chain — that is what "legal metrology" means. And when the chain is ignored, the failure is spectacular. In 1999 NASA's $327-million Mars Climate Orbiter burned up in the Martian atmosphere because one engineering team supplied thruster impulse data in pound-force seconds while the navigation software expected newton seconds — a factor of 4.45 hiding in an unwritten unit. The orbiter arrived 170 km lower than planned. No physics was wrong; a unit was silent. Equation (1) — number times unit, never one without the other — is not exam pedantry. It is a spacecraft-rated engineering law.

The physical picture

Strip away the laboratory and measurement is something a child does on a beach: take a stick, lay it along a rope, count. The stick fits four times, with a bit less than a third of a stick left over — so the rope is "about 4.3 sticks long". That sentence contains the entire logic of measurement. You chose a standard (the stick), you compared it with the unknown (the rope), and you reported a count (4.3). Physics never gets more mysterious than this; it only gets more careful.

Figure
Measurement is comparison — counting how many standards fit the unknown
the unknown: a rope the standard: one stick = 1 u 1 2 3 4 + 0.3 rope = 4.3 sticks Q = n x u : number 4.3, unit 1 stick

Look at what the count actually depends on. The rope is what it is — a fixed piece of reality. But the number 4.3 belongs half to the rope and half to your stick. Bring a stick twice as long and the same rope measures 2.15 sticks; bring a stick half as long and it measures 8.6. One invariant fact, many equivalent descriptions. This is why a physical quantity must always be written as the pair

Q=n×u(1)Q = n \times u \qquad (1)

where: QQ — the physical quantity itself (a length, a mass, a time interval…); nn — the numerical value, the count from the comparison; uu — the unit, the standard you counted with. Read it physically: neither piece alone is a measurement. The answer "20" to "how fast was the car?" is not slow, fast or anything at all until the unit lands — 20 m/s is highway speed, 20 km/h is a cycling pace. Examiners across every board treat a bare number as a wrong answer for exactly this reason: it is not incomplete, it is meaningless. The second half of the picture is the standard itself. A stick is a terrible standard: it warps in the rain, it's in one child's hand only, and no one else's stick matches. History's standards were barely better. An "inch" was three barleycorns laid end to end; a "cubit" was an elbow-to-fingertip that changed with every pharaoh; a medieval "foot" literally varied from town to town with the local lord's anatomy. Trade, engineering and science all choke on that. Out of the French Revolution came the radical alternative — units belonging to everyone and no one: the metre, originally one ten-millionth of the distance from the North Pole to the equator through Paris, later cast as a physical platinum bar, and the kilogram cylinder you met in the overview.

Figure
Three generations of standards — from anatomy to artefacts to constants of nature
body parts cubit, foot, barleycorn varies person to person artefacts prototype metre and kg can drift, one location constants of nature c, h, Cs-133 speed of light fixed, Planck constant fixed same everywhere, for all time pre-1791 1889 2019

An artefact standard, however, carries a built-in absurdity — the one the overview opened with. If the kilogram is defined as the Paris cylinder's mass, then by definition that cylinder is always exactly 1 kg, even as atoms rub off its surface or contamination settles on. What drifted was its mass relative to its copies, and the copies disagreed among themselves. There was no deeper referee to appeal to. That is precisely the failure mode the 2019 redefinition eliminated: today every SI base unit is pinned to a fixed constant of nature — the second to a caesium-133 transition frequency, the metre to the exact speed of light c=299 792 458c = 299\,792\,458 m/s, the kilogram to the exact Planck constant hh. Constants don't warp, don't sit in one vault, and read the same in Tokyo, Toronto and on Mars. The three qualities of a good standard — invariant, accessible, reproducible — are finally all satisfied at once. The full tour of those seven base units is the next module's job; here you just need the principle. One more piece of architecture before the algebra. Physics does not invent a new standard for every quantity. A small set of quantities — length, mass, time and a few others — are treated as base quantities, each with its own defined standard. Everything else is derived: speed is length per time, density is mass per volume cubed into length, and so on. You will meet this division properly in the SI modules; for now, notice the economy of it — millions of measurable things, resting on seven standards.

The algebra of units: one fact, many numbers

Here is the single most examined idea in this module. Since the quantity QQ is a fact about the world and the unit is your choice, two honest observers using different units must be describing the same QQ:

n1u1=n2u2(2)n_1 u_1 = n_2 u_2 \qquad (2)

where: n1,u1n_1, u_1 — the numerical value and unit in the first system; n2,u2n_2, u_2 — the same quantity in the second. This is conservation of meaning: 2 hours and 120 minutes are the same duration wearing different costumes. Rearranged, n2=n1(u1/u2)n_2 = n_1 (u_1/u_2) — the new number is the old number times how many new units fit in one old unit. And read as a proportionality, with QQ fixed:

n∝1u(3)n \propto \frac{1}{u} \qquad (3)

where: nn — numerical value; uu — the size of the unit. The numerical value is inversely proportional to the unit. Measure a desk in metres and you get 1.2; measure it in centimetres — a unit 100 times smaller — and the number swells 100 times to 120. This inverse relation is a certified board favourite ("if the unit of length is doubled, the numerical value of a given length becomes…") and, dressed in new clothes, a JEE-Main staple. The instinct it must replace is dangerous: a bigger number does not mean more quantity — it may just mean a smaller ruler.

Derivation AConverting units without memorising formulas

We want to derive the general unit-conversion rule n2=n1(u1/u2)n_2 = n_1(u_1/u_2) from the invariance of the physical quantity, and then use it to convert 72 km/h into m/s — the single most repeated conversion in all of high-school physics. The strategy: write the same quantity in both unit systems, set the two expressions equal, and let the units cancel like algebraic symbols. The thing to watch is that units are algebraic symbols — they multiply, divide and cancel exactly like xx and yy, which is what makes the method mechanical and memorisation-free.

Step 1. State the invariance. The speed of the car is one fact: Q=n1u1=n2u2Q = n_1 u_1 = n_2 u_2, where u1=1u_1 = 1 km/h and u2=1u_2 = 1 m/s. Solving for the new numerical value: n2=n1×u1u2n_2 = n_1 \times \dfrac{u_1}{u_2}. Why this direction: the ratio u1/u2u_1/u_2 asks "how many of the new units make one old unit?" — if the new unit is bigger, the ratio is less than 1 and the number rightly shrinks.

Step 2. Express the old unit in base terms. By definition, 1 km=1000 m1\ \text{km} = 1000\ \text{m} and 1 h=3600 s1\ \text{h} = 3600\ \text{s}, so u1=1 km1 h=1000 m3600 s=518 m/s.u_1 = \dfrac{1\ \text{km}}{1\ \text{h}} = \dfrac{1000\ \text{m}}{3600\ \text{s}} = \dfrac{5}{18}\ \text{m/s}.

Step 3. Take the ratio of units: u1u2=(5/18) m/s1 m/s=518\dfrac{u_1}{u_2} = \dfrac{(5/18)\ \text{m/s}}{1\ \text{m/s}} = \dfrac{5}{18} — a pure number, as a unit ratio must be.

Step 4. Apply it to the car: n2=72×518=4×5=20n_2 = 72 \times \dfrac{5}{18} = 4 \times 5 = 20. So 72 km/h=20 m/s72\ \text{km/h} = 20\ \text{m/s}. Why the answer is credible: 20 m/s means covering two classrooms' length every second — brisk highway speed, exactly what 72 km/h feels like. A quick sanity check like this catches inverted factors instantly, because using 18/518/5 by mistake gives 259.2, an absurd "m/s" for a car.

Step 5. Extract the exam reflex: km/h →\to m/s is multiply by 5/18 (equivalently divide by 3.6); m/s →\to km/h is multiply by 18/5 (times 3.6). Both are just equation (2) wearing convenient clothes. Verified: 72×5/18=2072 \times 5/18 = 20 recomputed; 1000/3600=5/18≈0.27781000/3600 = 5/18 \approx 0.2778 m/s per km/h; reverse check 20×3.6=7220 \times 3.6 = 72.

Go deeper · Derivation B · 1 minWhat one light-year is in metres
Derivation BWhat one light-year is in metres

We want to show how a "unit" is manufactured from a standard plus a definition, by computing the metre-equivalent of one light-year — the distance light travels in one year. The strategy: write the light-year as (speed of light) × (one year), express each factor in SI units, and multiply. Watch how the exact, defined value of cc anchors the whole chain: since 2019-style SI fixes constants, this conversion involves no measurement uncertainty at all until the "year" convention is chosen.

Step 1. Definition: 1 ly=c×(1 yr)1\ \text{ly} = c \times (1\ \text{yr}), with c=299 792 458c = 299\,792\,458 m/s exactly.

Step 2. Convert the year. Using the Julian year of astronomy, 1 yr=365.25 days=365.25×24×3600 s=31 557 600 s.1\ \text{yr} = 365.25\ \text{days} = 365.25 \times 24 \times 3600\ \text{s} = 31\,557\,600\ \text{s}. Why 365.25: astronomers fix the Julian year by convention precisely so that "light-year" means one exact number of metres — another example of a standard being an agreement, not a discovery.

Step 3. Multiply: 1 ly=299 792 458×3.15576×107 m≈9.461×1015 m.1\ \text{ly} = 299\,792\,458 \times 3.15576 \times 10^{7}\ \text{m} \approx 9.461 \times 10^{15}\ \text{m}.

Step 4. Read the result. Nearly 101610^{16} m — ten thousand million million metres — in one convenient word. Units are chosen to make numbers humane: stellar distances in light-years, atomic sizes in nanometres, the same equation (1) at every scale. Verified: 3×108×3.156×107=9.47×10153 \times 10^8 \times 3.156 \times 10^7 = 9.47 \times 10^{15} order-of-magnitude check; exact product 299 792 458×31 557 600=9.4607×1015299\,792\,458 \times 31\,557\,600 = 9.4607 \times 10^{15} m matches the IAU value.

Limiting cases

CaseResultMeaning
new unit = old unit (u2=u1u_2 = u_1)n2=n1n_2 = n_1the conversion rule contains "no conversion" as a special case
unit made kk times largernumber becomes n/kn/kthe inverse law n∝1/un \propto 1/u in its exam form
unit made kk times smallernumber becomes knkncentimetre numbers are 100× metre numbers
Q=0Q = 0n=0n = 0 in every unitzero is the only numerical value all unit systems agree on
pure count (5 oscillations, 12 atoms)no unit neededsome quantities are dimensionless numbers — the exception that proves the n×un \times u rule

The last two rows repay attention. A reading of zero survives any unit change — which is why "the difference vanished" is a unit-proof statement. And counts are genuinely unitless: "12 oscillations" needs no standard because the comparison is built into counting itself.

Worked examples

Board level — mercury's density in SI units (CBSE/ICSE pattern)

The density of mercury is 13.6 g/cm313.6\ \mathrm{g/cm^3}. Express it in kg/m3\mathrm{kg/m^3}.

Step 1. Set up the conversion as algebra with units, not as a memorised rule: ρ=13.6 gcm3\rho = 13.6\ \dfrac{\text{g}}{\text{cm}^3}, and we know 1 g=10−3 kg1\ \text{g} = 10^{-3}\ \text{kg} and 1 cm=10−2 m1\ \text{cm} = 10^{-2}\ \text{m}.

Step 2. Substitute the units like symbols: ρ=13.6×10−3 kg(10−2 m)3\rho = 13.6 \times \dfrac{10^{-3}\ \text{kg}}{(10^{-2}\ \text{m})^3}. The cube applies to everything in the bracket — number and unit — giving (10−2)3=10−6 m3(10^{-2})^3 = 10^{-6}\ \text{m}^3.

Step 3. Collect the powers of ten: ρ=13.6×10−310−6 kgm3=13.6×103 kg/m3\rho = 13.6 \times \dfrac{10^{-3}}{10^{-6}}\ \dfrac{\text{kg}}{\text{m}^3} = 13.6 \times 10^{3}\ \text{kg/m}^3.

Step 4. Report: ρ=13 600 kg/m3=1.36×104 kg/m3\boxed{\rho = 13\,600\ \mathrm{kg/m^3} = 1.36 \times 10^4\ \mathrm{kg/m^3}}.

Step 5. Sanity-check against the inverse law: kg/m³ is a smaller unit of density than g/cm³ (one thousandth the size), so the numerical value must come out larger — and it did, by exactly the factor 1000. The marks-scheme habit: state the two base conversions, show the cube being applied to the centimetre, and only then multiply.

Competitive level — speed in an invented unit system (JEE-Main pattern)

On a space station, engineers use the "hop" (1 hop=5 m1\ \text{hop} = 5\ \text{m}) as the unit of length and the "tick" (1 tick=2 s1\ \text{tick} = 2\ \text{s}) as the unit of time. A cargo trolley moves at 54 km/h54\ \mathrm{km/h}. Find its speed in hops per tick.

Step 1. Get the speed into SI first — never juggle two conversions at once: 54 km/h=54×518 m/s=15 m/s54\ \text{km/h} = 54 \times \dfrac{5}{18}\ \text{m/s} = 15\ \text{m/s}.

Step 2. Build the new unit's SI size: 1 hoptick=5 m2 s=2.5 m/s1\ \dfrac{\text{hop}}{\text{tick}} = \dfrac{5\ \text{m}}{2\ \text{s}} = 2.5\ \text{m/s}.

Step 3. Apply n2=n1(u1/u2)n_2 = n_1 (u_1/u_2) with u1=1u_1 = 1 m/s and u2=2.5u_2 = 2.5 m/s: n2=15×12.5=6n_2 = 15 \times \dfrac{1}{2.5} = 6.

Step 4. Report: v=6 hops/tick\boxed{v = 6\ \text{hops/tick}}. Check it forwards: 6 hops per tick = 6×56 \times 5 m per 22 s =30/2=15= 30/2 = 15 m/s ✓.

Step 5. The trap being set: candidates who "convert" by multiplying by 5/25/2 instead of dividing get 37.537.5 — the examiner's favourite wrong option. The inverse law is the guard: hop/tick is a bigger speed unit than m/s, so the number must come out smaller than 15. Timing note: 60–90 seconds. The only decisions are (i) SI first, (ii) is the new unit bigger or smaller than the old one? If your answer's direction disagrees with the inverse law, you inverted the ratio — fix it before moving on.

Exam traps

A number without a unit is a zero-mark answer. CBSE, ICSE, IGCSE and A-Level mark schemes all reserve a mark for the final unit; "20" where "20 m/s" was needed forfeits it even with perfect working. Write the unit on every line, not just the last — it is also your best error detector.

Dropping units mid-calculation. The classic disaster: mixing grams into a kilogram formula because the units were "put back at the end". Carry units through like algebra; when they refuse to cancel, they are telling you the setup is wrong before you waste the arithmetic.

The inverse-relation inversion. "If the unit of length is increased by a factor of 10, the numerical value of a given length is…" — divided by 10, by n∝1/un \propto 1/u. Options offering "multiplied by 10" harvest thousands of marks every year. Anchor: 1.2 m = 120 cm — bigger unit (m), smaller number.

The 5/18 direction. km/h → m/s is ×5/18 (÷3.6); m/s → km/h is ×18/5 (×3.6). If you blank, rebuild it in five seconds: 1 km/h = 1000 m per 3600 s. NEET and JEE-Main both love hiding a wrong-direction conversion inside a longer kinematics problem.

Prefix case and symbol sloppiness. mN (millinewton) and MN (meganewton) differ by 10910^9; ms and Ms by 10910^9; "K" is kelvin, "k" is kilo. Symbols never pluralise ("5 kg", never "5 kgs") and never take a full stop mid-sentence. ICSE and Cambridge papers explicitly penalise "Kg" and "KM" — unit symbols named after people capitalise the symbol (N, K, Pa) but never the spelled-out name (newton, kelvin, pascal).

Cubing (or squaring) only the number, not the unit. Converting cm³ to m³ means (10−2 m)3=10−6 m3(10^{-2}\ \text{m})^3 = 10^{-6}\ \text{m}^3 — the factor is 10610^6, not 10210^2. Density and volume conversions punish this relentlessly; the board-level example above is the template.

Comparing quantities in different units. 250 cm vs 3 m, 0.4 kg vs 350 g — convert to a common unit before comparing. Ranking questions bait the raw-number comparison.

Origins · 1 minLord Kelvin and how this was discovered
LK
Lord Kelvin
1824–1907 · Glasgow

William Thomson — Lord Kelvin — made measurement itself a scientific creed. Professor at Glasgow for 53 years, he built the absolute temperature scale that bears his name (the SI base unit of temperature honours him), turned thermodynamics into an exact science, and as chief engineer of the transatlantic telegraph cable proved that a measurable signal, quantified and tracked, could bind continents — earning his knighthood not for theory but for metrology under the Atlantic. His famous dictum captures this module in one sentence: "When you can measure what you are speaking about, and express it in numbers, you know something about it; when you cannot… your knowledge is of a meagre and unsatisfactory kind." For Kelvin, the number-and-unit pair was not bookkeeping — it was the boundary line where opinion ends and physics begins.

History
1791
— Revolutionary France defines the metre as one ten-millionth of the pole-to-equator meridian through Paris: units for "all people, for all time".
1875
— Seventeen nations sign the Metre Convention, creating the BIPM at Sèvres — measurement becomes international law.
1889
— The platinum-iridium prototype metre and kilogram are ratified; artefacts now define the world's units.
1960
— The 11th CGPM names the Système International (SI): six base units, decimal prefixes, global adoption.
2019
— All seven base units are redefined via fixed constants of nature (cc, hh, ee, kBk_B…); the Paris kilogram retires after 130 years.

Going further

Texts. NCERT Physics Part 1, Ch. 1 (Units and Measurement) — the CBSE/NEET canonical statement · SI Brochure, 9th edition (BIPM, 2019) — the actual law of the units, free online · Halliday, Resnick & Walker Ch. 1 · Cambridge IGCSE/9702 syllabus appendices for the unit-convention marking rules quoted here.

Provenance. All numbers recomputable: 72×5/18=2072 \times 5/18 = 20 m/s (and 20×3.6=7220 \times 3.6 = 72); 1000/3600=5/181000/3600 = 5/18; 13.6×10−3/10−6=1.36×10413.6 \times 10^{-3}/10^{-6} = 1.36 \times 10^4 kg/m³; 54×5/18=1554 \times 5/18 = 15 m/s, 15/2.5=615/2.5 = 6 hops/tick, reverse 6×5/2=156 \times 5/2 = 15 m/s; Julian year 365.25×86400=31 557 600365.25 \times 86400 = 31\,557\,600 s and 299 792 458×31 557 600=9.4607×1015299\,792\,458 \times 31\,557\,600 = 9.4607 \times 10^{15} m; prototype-kilogram drift ≈ 50 µg per century (BIPM periodic verifications); Mars Climate Orbiter loss 1999, lbf·s vs N·s, 1 lbf = 4.448 N.

Prerequisites. Class-10 arithmetic and algebra. Leads to. The SI System: Base Units · Accuracy, Precision & Uncertainty · Significant Figures, Rounding & Reporting (already live in this chapter).

Why is writing just the number, without a unit, actually wrong rather than just incomplete?

Because the number alone doesn't underdescribe the quantity — it describes nothing. The numerical value is defined only relative to a unit (n=Q/un = Q/u), so "the length is 7" is like answering "how far is the station?" with "seven of something I won't tell you". Any value whatsoever could be correct: 7 mm, 7 m and 7 km are all "7". This is why boards award a specific mark for the unit and why physicists treat the pair n un\,u as one indivisible object. The habit to build: the unit is part of the answer, not a decoration after it.

If the Paris cylinder WAS the kilogram, how could anyone say it lost mass?

Beautiful catch — strictly, they couldn't say it directly. By definition the prototype was always exactly 1 kg. What metrologists observed was relative drift: the prototype and its official copies, compared over a century, no longer agreed, diverging by tens of micrograms. Either the copies gained or the prototype lost — and with the artefact as the definition, the question "which one really changed?" had no answer even in principle. That logical dead-end, more than the practical inconvenience, is why the 2019 SI moved the definition to the Planck constant: a standard nothing can rub atoms off.

Do the numerical value and the unit both change when I convert, or just the number?

Both change — in exactly compensating ways, which is the whole point of n1u1=n2u2n_1 u_1 = n_2 u_2. Converting 1.2 m to 120 cm swaps the unit (m → cm, a factor-100 shrink) and the number (1.2 → 120, a factor-100 growth); their product, the actual length, is untouched. What never changes is QQ itself. If you ever finish a conversion and the quantity seems to have grown or shrunk, you've applied the factor to only one member of the pair.

Is a count, like 15 oscillations or 12 atoms, a physical quantity? It has no unit.

It's a measurable, physically meaningful number — but it's dimensionless: the comparison standard is built into counting itself (the standard is "one"). Physics has several such unitless quantities: counts, ratios of like quantities (refractive index, relative density, strain), and plane angle in radians (defined as arc length over radius — a length divided by a length). They still obey the honest-reporting rules you'll meet in significant figures; they just don't need a unit symbol. The pattern to internalise: whenever a quantity is a ratio of two quantities of the same kind, the units cancel and a pure number remains.

Why did we need seven base quantities? Couldn't everything come from length and time alone?

The number seven is a choice, not a law of nature — a convenient, precisely realisable set agreed by the CGPM. You genuinely cannot build mass out of length and time within classical measurement practice, so at least a handful of independent standards is required; beyond that, the selection balances precision, practicality and history. (The mole and candela earn their seats for chemistry and physiology-based photometry, not deep physics.) Advanced physicists sometimes work in "natural units" where c=ℏ=1c = \hbar = 1 and nearly everything collapses into powers of one unit — a deep-dive topic far beyond board syllabi, but proof that the base set is a convention.

How do I know whether to multiply or divide by the conversion factor?

Stop memorising directions; use the inverse law as a compass. Ask: is the new unit bigger or smaller than the old one? Bigger unit → smaller number; smaller unit → bigger number. Converting 3 h into seconds: the second is a much smaller unit, so the number must grow — multiply by 3600. Converting 4500 m into km: kilometre is bigger, number must shrink — divide by 1000. If the direction of your answer contradicts this check, you inverted the factor. This two-second test is worth more marks over a school career than any table of formulas.

In an exam, is 13600 kg/m³ better or worse than 1.36 × 10⁴ kg/m³?

Both are numerically correct and both earn the answer mark on CBSE/ICSE/NEET papers, so write whichever the question's format suggests. Scientific notation has two quiet advantages: it survives very large and very small quantities without a parade of zeros, and — as the significant-figures module explains — it states your precision unambiguously, which trailing zeros in 13600 do not. Cambridge practical papers in particular expect sensible scientific notation. Habit worth building now: for anything beyond about 10410^4 or below 10−310^{-3}, reach for powers of ten.

Where this leads