Q.If the speed of light is 3.0×108 m s−1, calculate the distance covered by light in 2.00 ns.
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Speed Distance Time
Speed, Distance, Time — The First Meeting
Imagine you're walking to school. You know the distance is 2 km. Some days you walk slowly, taking 40 minutes. Other days you're in a hurry and cover the same 2 km in just 30 minutes. What changed? Your speed changed.
Speed is simply how fast you cover a distance. It answers the question: "How much distance do I cover in one unit of time?"
The Core Idea
If you walk 2 km in 30 minutes, then in one minute you cover 302=0.067 km. That's your speed: 0.067 km per minute.
But we usually measure speed in km per hour (km/h) or metres per second (m/s). So let's convert: 30 minutes is 0.5 hours. Speed = 0.5 h2 km=4 km/h. That means in one hour, at that same pace, you'd cover 4 km.
Speed is not a separate thing — it's the ratio of distance to time. If you know any two of the three, you can find the third.
The Precise Statement
Speed=TimeDistance
This single equation is the whole story. From it, you get:
Distance=Speed×Time
Time=SpeedDistance
Units must match. If speed is in km/h, distance must be in km and time in hours. If speed is in m/s, distance in metres and time in seconds. Mixing units is the most common mistake.
A Simple Example
A train travels 300 km at a speed of 60 km/h. How long does it take?
Time = SpeedDistance=60300=5 hours.
That's it. The train covers 60 km every hour, so after 5 hours it has covered 5×60=300 km.
What Speed Actually Tells You
Speed is not about how far you go — it's about how quickly you cover ground. A car at 80 km/h covers 80 km in one hour. A bicycle at 20 km/h covers only 20 km in the same hour. The car is faster because it covers more distance per unit time.
To compare speeds, always use the same time unit. 10 m/s is faster than 30 km/h? Let's check: 30 km/h = 360030×1000=8.33 m/s. So 10 m/s is indeed faster.
The Triangle Trick (For Quick Recall)
Draw a triangle. Write D at the top, S at bottom-left, T at bottom-right. Cover the quantity you want to find:
- Cover D: you see S×T → Distance = Speed × Time …
Why this formula?
Speed, Distance, and Time — The Why Behind the Formula
Let’s start with the core idea: Speed is a measure of how fast something is moving. It tells us the distance covered per unit of time.
The Fundamental Relationship
Imagine you are walking. In 1 hour, you cover 5 kilometres.
That means your speed is 5 kilometres per hour.
Now, if you walk for 2 hours at the same speed, you will cover:
Distance=5×2=10 km
This is the intuitive origin of the formula:
Distance=Speed×Time
Why This Formula Holds — The Derivation
1. Speed is a rate
- Speed is defined as distance per unit time.
- Mathematically:
Speed=TimeDistance
This is not a "magic formula" — it is the definition of speed.
If you travel 100 km in 2 hours, your speed is:
Speed=2100=50 km/h
2. Rearranging the definition
From the definition:
Speed=TimeDistance
Multiply both sides by Time:
Speed×Time=Distance
This gives us the distance formula.
3. The other two forms
From the same definition, we can also solve for Time:
Time=SpeedDistance
And for Speed (already the definition):
Speed=TimeDistance
The Key Insight — Why It’s Not Just Memorisation
Think of it as a proportionality:
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Distance is directly proportional to Speed (if time is fixed).
→ Double the speed → double the distance in the same time.
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Distance is directly proportional to Time (if speed is fixed).
→ Double the time → double the distance at the same speed.
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Speed is inversely proportional to Time (if distance is fixed).
→ Double the speed → half the time to cover the same distance.
The Three Formulas at a Glance …
The key idea is the speed-distance-time relation: distance = speed × time. The only catch is that time is given in nanoseconds, so you must convert to seconds first.
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Convert 2.00 ns to seconds:
1 ns=10−9 s, so 2.00 ns=2.00×10−9 s.
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Apply the formula:
distance=(3.0×108 m/s)×(2.00×10−9 s).
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Multiply: …
The key idea is to use the speed-distance-time relation d=v×t, converting the time from nanoseconds to seconds first. The distance covered by light in 2.00 ns is 0.600 m.
The problem is a straightforward application of the Speed, Distance, Time relationship — one of the most fundamental ideas in physics. The trick here is not the formula itself, but handling the units carefully. Light travels at an enormous speed, and the time given is in nanoseconds (ns), a very small unit. If you plug in the numbers without converting, you'll get a wildly wrong answer.
Let’s break it down.
- Recall the basic relation. The distance d travelled by an object moving at constant speed v in time t is:
d=v×t
Here, v=3.0×108 m/s (the speed of light) and t=2.00 ns.
- Convert nanoseconds to seconds. The prefix "nano" means 10−9. So:
1 ns=10−9 s
Therefore:
t=2.00 ns=2.00×10−9 s
A common mistake is to forget this conversion and treat ns as seconds, which would give a distance of 6.0×108 m — that’s over half a million kilometres, clearly absurd for 2 billionths of a second!
- Plug into the formula.
d=(3.0×108 m/s)×(2.00×10−9 s)
- Multiply the numbers and the powers of ten separately. First, the coefficients: 3.0×2.00=6.0 …
Here are the common mistakes students make on this Speed-Distance-Time problem, and how to avoid each.
1. Forgetting to convert nanoseconds to seconds
The Mistake:
Plugging in t=2.00 directly into d=v×t, treating nanoseconds as seconds.
This gives a tiny, wrong answer:
d=3.0×108×2.00=6.0×108 m — which is incorrect because the time unit is wrong.
Why it happens:
Students see a number and forget that nano (n) means 10−9. The unit is ns, not s.
How to avoid:
Always write the unit conversion explicitly before substituting.
1 ns=10−9 s
So 2.00 ns=2.00×10−9 s
Then use:
d=v×t=(3.0×108)×(2.00×10−9)
2. Mishandling powers of ten (exponent arithmetic)
The Mistake:
Adding exponents incorrectly — e.g., writing 108×10−9=10−1 (correct) but then misplacing the decimal in the final answer.
Why it happens:
Rushing through the multiplication of coefficients and exponents separately.
How to avoid:
Separate the work into two clear steps:
- Multiply the coefficients: 3.0×2.00=6.0
- Multiply the powers of ten: 108×10−9=108+(−9)=10−1
Then combine:
d=6.0×10−1 m
3. Reporting the answer in wrong units
The Mistake:
Giving the answer in kilometres, centimetres, or leaving it without units — e.g., writing 0.6 instead of 0.6 m.
Why it happens:
Not checking what the question asks for. The speed is in m/s, so distance naturally comes out in metres.
How to avoid:
Always write the unit after every numerical answer. If the question doesn’t specify a unit, use the one that follows from the given data — here, metres.
4. Confusing nanoseconds with microseconds or milliseconds
The Mistake:
Using 10−6 (micro) or 10−3 (milli) instead of 10−9.
Why it happens:
Mixing up metric prefixes — nano, micro, milli are easy to confuse under time pressure.
How to avoid:
Memorise the common prefixes with a mnemonic or a quick reference:
| Prefix | Symbol | Power | …
- TG EAPCET 2026Set eng-2026-05-11-FN1 markMCQQ.If v0 and v represent the threshold frequency and frequency of incident light respectively, then the correct equation for the velocity of photoelectrons emitted from the metal surface will be (A) v=m2h(v−v0) (B) v=m2h(v0−v) (C) v=2hm(v−v0) (D) v=2hcm(v0−v)
›Reveal solutionSolution
The photoelectric effect gives kinetic energy K=h(v−v0), and since K=21mv2, solving for v yields v=m2h(v−v0), which matches option (A).
The core idea here is the photoelectric effect equation from Einstein: the energy of an incident photon (hν) is used first to overcome the work function (hν0) and the remainder becomes the kinetic energy of the emitted electron. That kinetic energy is 21mv2, so equating and solving for v gives the velocity.
- Write the photoelectric equation The maximum kinetic energy of an emitted photoelectron is
Kmax=hν−hν0=h(ν−ν0).
Here ν is the frequency of incident light and ν0 is the threshold frequency (the minimum frequency needed to eject an electron).
- Relate kinetic energy to velocity For a non‑relativistic electron (which is the case here),
Kmax=21mv2,
where m is the electron’s mass and v is its speed.
- Equate and solve for v Set the two expressions equal:
21mv2=h(ν−ν0).
Multiply both sides by 2:
mv2=2h(ν−ν0).
Divide by m:
v2=m2h(ν−ν0).
Take the square root (velocity is positive):
v=m2h(ν−ν0).
- Match with the options …
- TG EAPCET 2024Set eng-2024-05-09-AN1 markMCQQ.The kinetic energy of electrons emitted, when radiation of frequency 1.0×1015 Hz hits a metal, is 2×10−19 J. What is the threshold frequency of the metal (in Hz)? (h = 6.6×10−34 Js) (A) 3.5×1015 (B) 3.3×1014 (C) 6.97×1015 (D) 6.97×1014
›Reveal solutionSolution
The photoelectric effect equation Kmax=hf−hf0 gives the threshold frequency f0=f−hKmax. Substituting the given values yields f0≈6.97×1014 Hz, which corresponds to option (D).
The key concept here is the photoelectric effect, where light of frequency f ejects electrons from a metal surface. The maximum kinetic energy Kmax of the emitted electrons is given by Einstein’s equation:
Kmax=hf−hf0
where h is Planck’s constant, f is the incident frequency, and f0 is the threshold frequency (the minimum frequency needed to eject electrons). The term hf0 is the work function of the metal.
Why this works: The incident photon gives energy hf to an electron. Some of that energy is used to overcome the binding energy (work function hf0), and the rest appears as kinetic energy. So, if we know Kmax and f, we can solve for f0 by rearranging.
Let’s go step by step.
- Write the photoelectric equation
Kmax=hf−hf0
We want f0, so isolate it:
hf0=hf−Kmax⇒f0=f−hKmax
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Insert the given values
- f=1.0×1015 Hz
- Kmax=2×10−19 J
- h=6.6×10−34 Js
Compute hKmax:
6.6×10−342×10−19=6.62×1015≈0.30303×1015=3.0303×1014 Hz
- Subtract to find f0
- TG EAPCET 2022Set eng-2022-07-19-FN1 markMCQQ.A metal has 9×1028 conduction electrons per m3 and its resistivity is 1×10−8 Ω⋅m. If the drift speed of an electron in the metal is 1.6×106 m/s then its mean free path is (mass of electron =9×10−31 kg and charge of electron =1.6×10−19C) (A) 55.5 nm (B) 78.0 nm (C) 40.0 nm (D) 62.5 nm
›Reveal solutionSolution
The mean free path is found by combining the drift-speed relation with the resistivity formula. Using vd=meEτ and ρ=ne2τm, the relaxation time cancels to give λ=ne2ρmvd, yielding 62.5 nm.
The question gives you drift speed vd, resistivity ρ, electron density n, and asks for the mean free path λ. The link between these quantities runs through the relaxation time τ — the average time between collisions of an electron. Once you have τ, the mean free path is simply λ=vdτ (since drift speed is the average speed between collisions in the direction of the field).
But you don't have τ directly. You have two separate equations that each involve τ: one from the definition of drift speed, and one from the definition of resistivity. Equating them lets you eliminate τ and solve for λ in one clean step.
- Drift speed relation. In an electric field E, an electron accelerates for a time τ between collisions, gaining a drift speed
vd=meEτ.
This is just v=aτ with a=eE/m.
- Resistivity relation. Resistivity is related to the relaxation time by
ρ=ne2τm.
This comes from the Drude model: conductivity σ=mne2τ, and ρ=1/σ.
- Eliminate E and τ. From the drift equation, τ=eEmvd. From the resistivity equation, τ=ne2ρm. Equate them:
eEmvd=ne2ρm.
Cancel m and one e:
Evd=neρ1.
So E=neρvd. You don't actually need E — but notice that the two τ expressions are equal, so you can directly write
eEmvd=ne2ρm⇒vd=neρE.
That's a consistency check. The real shortcut: since λ=vdτ, substitute τ from the resistivity formula:
λ=vd⋅ne2ρm.
- Plug in the numbers.
m=9×10−31 kg,vd=1.6×106 m/s,
n=9×1028 m−3,e=1.6×10−19 C,ρ=1×10−8 Ω⋅m.
First compute ne2ρ:
ne2ρ=(9×1028)×(1.6×10−19)2×(1×10−8). …
- TG EAPCET 2022Set eng-2022-07-20-FN1 markMCQQ.KBr has rock salt type structural arrangements and has a density of 3.70 g/cm3. The edge length of the unit cell is approximately [molecular weight of KBr =120 g/mol] (A) 3×10−8 cm (B) 12×10−8 cm (C) 9×10−8 cm (D) 6×10−8 cm
›Reveal solutionSolution
For a rock salt (FCC) structure, there are 4 formula units per unit cell. Using the density formula for a unit cell, the edge length is calculated to be approximately 6×10−8 cm.
The problem asks us to find the edge length of a KBr unit cell, given its density and molecular weight, and knowing it has a rock salt type structure. This is a classic application of the density formula for crystalline solids.
The core idea is that the density of a unit cell is determined by the total mass of the atoms (or ions) within that unit cell divided by the volume of the unit cell.
Concept and Intuition
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Rock Salt Structure: KBr crystallizes in a rock salt structure, which is a face-centered cubic (FCC) lattice. In this arrangement, one type of ion (say, Br⁻) forms an FCC lattice, and the other type of ion (K⁺) occupies all the octahedral voids.
- For an FCC lattice, there are 4 atoms (or ions) effectively present per unit cell.
- For a rock salt structure like KBr, this means there are 4 K⁺ ions and 4 Br⁻ ions per unit cell. Therefore, the number of formula units of KBr per unit cell, denoted by Z, is 4.
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Density Formula: The density (ρ) of a unit cell is given by the formula:
ρ=a3⋅NAZ⋅M
Where:
- ρ is the density of the crystal.
- Z is the number of formula units per unit cell.
- M is the molecular weight (or molar mass) of the compound.
- a is the edge length of the unit cell.
- NA is Avogadro's number (6.022×1023 mol−1).
We are given ρ, M, and we've determined Z. We need to find a. We can rearrange the formula to solve for a3 and then take the cube root.
Step-by-Step Solution
-
Identify the given values and constants:
- Density, ρ=3.70 g/cm3
- Molecular weight of KBr, M=120 g/mol
- Avogadro's number, NA=6.022×1023 mol−1
-
Determine the number of formula units per unit cell (Z):
As KBr has a rock salt type structure, it is an FCC arrangement of ions. In an FCC unit cell, there are 4 formula units.
Therefore, Z=4.
-
Rearrange the density formula to solve for a3:
From the formula ρ=a3⋅NAZ⋅M, we can isolate a3:
a3=ρ⋅NAZ⋅M
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Substitute the values into the rearranged formula:
a3=3.70 g/cm3⋅6.022×1023 mol−14⋅120 g/mol …
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- TG EAPCET 2021Set ap-2021-08-09-FN1 markMCQQ.For what distance the ray optics will be a good approximation when the aperture is 5 mm wide and the wavelength is 450 nm? (A) 45.55 m (B) 55.55 m (C) 35.55 m (D) 40.55 m
›Reveal solutionSolution
The key idea is the Fresnel distance ZF=a2/λ, which marks the boundary where ray optics becomes a good approximation. For a=5 mm and λ=450 nm, we get ZF≈55.55 m, so option (B) is correct.
Ray optics (geometrical optics) treats light as straight rays, ignoring diffraction. But light is a wave, so diffraction always spreads a beam. The question asks: for a given aperture width a and wavelength λ, at what distance does the spreading due to diffraction become negligible compared to the aperture size? That distance is called the Fresnel distance (or Rayleigh distance) ZF=a2/λ. Beyond this, the beam’s angular spread θ≈λ/a causes the beam width to increase by roughly the original aperture size, so ray optics is a good approximation. Inside this distance, diffraction effects (like Fresnel fringes) are significant.
Let’s compute it step by step.
-
Identify the given quantities
Aperture width: a=5 mm = 5×10−3 m
Wavelength: λ=450 nm = 450×10−9 m = 4.5×10−7 m
-
Recall the Fresnel distance formula
The condition for ray optics to be valid is that the distance L satisfies L≫a2/λ. The threshold distance is
ZF=λa2
This comes from comparing the path difference at the edge of the aperture to λ/2 — when the Fresnel number N=a2/(λL)≈1, diffraction is significant; for N≪1, ray optics works.
- Plug in the numbers
ZF=4.5×10−7(5×10−3)2=4.5×10−725×10−6
Simplify:
-
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