GravityInvestigateabout 45 min
Test it: predictions, ramps, pendulums and Newton’s own proof
Predict, try, compare and ask "is it always true?" — with a ramp, a pendulum, a leaking cup and a spacecraft
Turn gravity into hands-on science: rebuild Galileo’s ramp, design fair tests for mass and shape, weigh the Earth with a pendulum, check whether Newton’s law survives the trip to the Moon, hunt for orbital speed by binary search, and see how ISRO climbs to the Moon and Mars one burn at a time.
In this part you’ll
- Design a fair test that changes one variable at a time, and explain why the coin-vs-paper race is not one.
- Explain why repeating an event (like 20 pendulum swings) shrinks a fixed timing error into a much smaller percentage.
- Use T = 2π√(L/g) to predict a pendulum’s period and to calculate g from measured swings.
- Describe Newton’s Moon test and explain why two independent methods agreeing is strong evidence.
- Explain how repeated perigee burns raise a spacecraft’s orbit, using Mangalyaan and Chandrayaan-3 as real examples.
Discover told the story. Understand gave you the rules. This layer asks you to be the scientist: predict what should happen, try it (for real, or in a lab), compare your prediction with what actually happens, and ask is it always true?
Every experiment below is one that a real scientist could do — some are hundreds of years old, one used a spacecraft. You will time falls, swing a pendulum to weigh the Earth, test whether Newton's law survives a 384,400 km stretch to the Moon, and pull apart how ISRO actually gets to Mars.
Chapter 01
Rebuilding Galileo’s ramp
Galileo could not time a one-second fall accurately — nobody could, before accurate clocks existed. His trick was to slow gravity down by rolling a ball down a gentle slope instead of dropping it.
A ball on a slope tilted at an angle still accelerates because of gravity, but only the part of gravity that points along the slope gets to act. Tilt the slope only 10° and the effective acceleration is far gentler than a straight drop: about 1.70 m/s² instead of 9.8 m/s² — roughly a sixth as strong, easily slow enough to time with a heartbeat, or today, a phone.
Predict first
| Time rolling | Distance rolled | Ratio to the first value |
|---|---|---|
| 0.5 s | 0.213 m | 1× |
| 1.0 s | 0.851 m | 4.0× |
| 1.5 s | 1.914 m | 9.0× |
| Angle | Effective a = g sin(angle) | Compared with a free fall (9.8) |
|---|---|---|
| 5° | 0.854 m/s² | about 1/11 — very gentle, easy to time, but a long ramp needed |
| 10° | 1.702 m/s² | about 1/6 — Galileo’s rough range, a good balance |
| 20° | 3.352 m/s² | about 1/3 — faster, needs a shorter reaction-time budget |
| 30° | 4.900 m/s² | exactly half of g — still much gentler than a vertical drop |
Lab
Compare a short, gentle fall with what the full drop from the same height would look like.
0.0 m/s · lands at 0.64 s
0.0 m/s · lands at 0.64 s
Dead heat: 0.64 s each. Neither of these is fluffy enough for the air to matter.
The sum
t = √(2h / g) = √(2 × 2 / 9.81) = 0.64 s
v = √(2gh) = 6.3 m/s on landing (23 km/h)
That is the no-air answer, and it is the same for every object, however heavy.
Text version of this activity
A short 2 m drop, timed on Earth and the Moon, to build intuition for how much gentler a ramp-style experiment feels compared with a full vertical fall — the timings are short enough to compare against your own reaction time, which sets up the next chapter.
Chapter 02
Testing "heavy falls faster" for yourself
Chapter 4 of Discover told you the answer. Here is how to check it is not just something a book says.
Round 1. Drop a coin and a flat sheet of paper together, from the same height, over a hard floor. Predict, then try it, five times.
Round 2. Crumple the same sheet of paper into a ball and race it against the coin again, five times.
Round 3 (the real test of the idea). Take two coins of different value — say a ₹1 coin and a ₹10 coin, which have different masses but similar shapes — and drop them together. Predict, then try it.
Predict first
Reflect
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Chapter 03
Why a stopwatch is not good enough
Try timing a coin's one-metre fall with a phone stopwatch, starting and stopping it by hand. The fall itself takes about 0.45 seconds. Your own reaction time — the delay between deciding to tap and your finger actually moving — is typically about 0.2 seconds, for each tap.
That error is not a rounding problem. It is roughly 44 % of the entire fall time. You could easily "measure" a fall as anywhere from 0.25 s to 0.65 s and never notice anything was wrong, because there is nothing to compare it with.
| What you are timing | True duration | Typical reaction-time error | Error as a share of the reading |
|---|---|---|---|
| A coin falling 1 m | ≈ 0.45 s | ≈ 0.2 s | ≈ 44 % |
| A coin falling from a first-floor balcony (5 m) | ≈ 1.01 s | ≈ 0.2 s | ≈ 20 % |
| 20 swings of a 1 m pendulum | ≈ 40.1 s | ≈ 0.2 s (once, not per swing) | ≈ 0.5 % |
Predict first
Chapter 04
Weighing the Earth with a piece of string
A pendulum is the oldest precision instrument in this whole topic, and you can build one from a metre of string and a small weight (a washer, a key, a small stone) tied at the end.
Swing it through a small angle — no more than about 15° from vertical — and something remarkable happens: the time for one full swing, called the period, does not depend on how heavy the bob is, and barely depends on how wide you swing it. It depends on only two things: the length of the string and g.
T = 2π × √(length ÷ g)
Notice mass is not in the formula at all. This is the same "mass cancels" idea from Understand, showing up again in a completely different experiment.
Predict first
| Length | Predicted period | Time for 20 swings |
|---|---|---|
| 0.25 m | 1.00 s | 20.1 s |
| 0.50 m | 1.42 s | 28.4 s |
| 1.00 m | 2.01 s | 40.1 s |
Lab
Sort six changes to a pendulum experiment by what they do to the period.
Does changing this make the pendulum swing faster, slower, or does it make no difference?
6 cards, 3 bins. Tap a card, then tap its bin. You can also drag, or press a bin’s number key.
Text version of this activity
Six changes to sort into faster, slower or no difference.
No difference: a heavier bob; a wider swing (while still under about 15°) — both surprising the first time you meet them, because "heavier things should swing differently" feels intuitive and is wrong here.
Faster (shorter period): a shorter string; stronger gravity (Jupiter's cloud tops).
Slower (longer period): a longer string; weaker gravity (the Moon, where the same pendulum takes about 2.46 times as long per swing).
Worked example
0 / 5 steps shownMeasuring g with a pendulum: a real class result
A class ties a small weight to a 0.80 m string and times 20 complete swings, getting a total of 35.9 seconds. Use this to calculate their measured value of g, and compare it with the accepted 9.8 N/kg.
Try it
Chapter 05
Testing terminal velocity
Understand claimed that shape sets terminal velocity, and that a heavier object of the same shape falls faster in air. Both claims are testable.
Test A — same mass, different shape. Take two identical sheets of paper. Leave one flat; fold the other into a tight paper aeroplane or a ball. Drop from the same height. Predict, then try it.
Test B — same shape, different mass. Nest two paper coffee filters or cupcake cases inside each other so they keep the same shape and area, doubling the mass. Drop one filter, then the doubled pair, from the same height. Predict, then try it.
Predict first
Lab
Compare two fair tests side by side: same shape with different mass, and same mass with different shape.
0.0 m/s · lands at 2.58 s
0.0 m/s · lands at 2.58 s
Dead heat: 2.58 s each. Neither of these is fluffy enough for the air to matter.
The sum
t = √(2h / g) = √(2 × 3 / 9.81) = 0.78 s
v = √(2gh) = 7.7 m/s on landing (28 km/h)
That is the no-air answer, and it is the same for every object, however heavy.
Text version of this activity
Four light objects dropped from 3 m on Earth.
The two nested paper cases have almost the same shape but the doubled case has twice the mass, and it noticeably wins the race — confirming that, with shape held fixed, more mass means a higher terminal velocity.
The flat sheet and the crumpled version of the same sheet have identical mass but very different shape, and the crumpled one wins by a wide margin — confirming that, with mass held fixed, a smaller, more compact shape means less drag and a higher terminal velocity.
Together the two results show that both mass and shape affect terminal velocity, through the single idea of a balance between weight and drag.
Chapter 06
Does the law reach the Moon? Newton’s own test
Here is the test that convinced Newton his law was truly universal — that the same rule pulling an apple off a tree also steers the Moon. It can be run with only two facts you already have: Earth's surface gravity, and the Moon's distance.
The prediction. If gravity really fades as one over the distance squared, then at the Moon's distance — about 60.3 Earth radii from the centre — the pull should be 60.3² ≈ 3,640 times weaker than at the surface. Predicted acceleration: 9.8 ÷ 3,640 ≈ 0.00269 m/s².
The independent check. The Moon's acceleration can also be worked out without assuming anything about gravity at all — purely from how fast it moves and how tightly it curves. A body moving at speed v on a circle of radius r has a centripetal acceleration of v² ÷ r. The Moon's observed orbital speed is about 1.02 km/s, and its distance is 384,400 km, which gives an acceleration of about 0.00272 m/s².
Two completely different routes — one from extrapolating a law measured on the ground, one from watching the sky — land within about 1 % of each other.
| Method | What it uses | Result |
|---|---|---|
| Predicted (inverse-square law) | Surface g (9.8) and distance ratio (60.3 Earth radii) | ≈ 0.00269 m/s² |
| Observed (pure orbital geometry) | Moon’s speed (1.02 km/s) and distance (384,400 km), via v² ÷ r | ≈ 0.00272 m/s² |
| Agreement | — | within about 1.2 % |
Predict first
Related to
Phases of the MoonThe same orbit whose acceleration is tested here is what carries the Moon through its monthly cycle of phases.
Chapter 07
Hunting for the orbit speed
Understand told you the orbital speed at the surface is about 7.91 km/s and escape velocity is about 11.19 km/s. Rather than take those numbers on trust, use the cannon lab as a proper investigation: a binary search.
Fire at a speed you are confident is too slow (it lands). Fire at a speed you are confident is too fast (it escapes or makes a huge ellipse). Then narrow the gap by trying the middle each time, exactly like guessing a number between 1 and 100.
Lab
Use a binary search — too slow, too fast, then the middle — to home in on the exact orbital and escape speeds.
Falls back to the ground
Too slow. The ball curves down and lands. Newton’s point: this path is already part of an ellipse — the rest of the ellipse is just buried inside the Earth.
It lands 5° round the Earth from the cannon — about 561 km away.
The two magic numbers
7.9 km/s — fast enough that the ground curves away underneath you as fast as you fall. That is an orbit: falling for ever and always missing.
11.2 km/s — fast enough to leave for good.
The cannon sits 35 km up, above the thick air, and we pretend there is no air at all. A real cannonball would burn up.
Text version of this activity
Start with 4 km/s (lands quickly) and 12 km/s (clearly escapes). Try the midpoint, 8 km/s: it makes a wide ellipse but still comes back, so it is just above orbital speed. Try 7 km/s: it lands, so it is just below. Narrow again between 7 and 8, and you converge on the true value of about 7.91 km/s within a few tries.
Repeat the same hunt between 10 km/s (a huge ellipse, still returns) and 12 km/s (escapes) to close in on escape velocity, about 11.19 km/s.
This is exactly how you would search for any unknown threshold: bracket it, then halve the gap, again and again.
Try it
Chapter 08
How ISRO actually gets to the Moon and Mars
India's Moon and Mars missions did not fire straight there in one giant push. Both used a strategy you can test the logic of yourself, in the orbit lab: raise the orbit gradually, one careful burn at a time.
Here is the idea in miniature. Put a spacecraft in a stretched, oval (elliptical) orbit around the Earth. Every time it swings back to its closest point (perigee), fire the engine briefly, forward, in the direction it is already moving. Predict what happens to the far point of the orbit (the apogee).
Predict first
Mangalyaan: raising an orbit until it reaches Mars
- 5 Nov 2013Launch A PSLV rocket — not powerful enough to send the spacecraft straight to Mars — puts it into a stretched Earth orbit instead.
- Nov 2013Six orbit-raising burns The spacecraft fires its own engine at perigee, six separate times, each one stretching the far point of its orbit further out.
- 1 Dec 2013Trans-Mars injection A final burn, now that the orbit is stretched far enough, sends the spacecraft out of Earth orbit entirely, on a curving path towards Mars.
- 24 Sep 2014Mars orbit insertion The engine fires again, this time to slow down and be captured by Mars’s gravity — 323 days after launch.
Landing is the same idea in reverse — and far more urgent, because there is no atmosphere on the Moon to help slow a spacecraft down the way Earth's atmosphere helps a returning capsule.
Chandrayaan-3's lander, Vikram, arrived at the Moon travelling at roughly 1.68 km/s sideways. To land safely it had to shed nearly all of that speed using only its own engines, arriving at the surface at under 2 metres per second — its speed cut by roughly a factor of 840, entirely under its own control, with no second attempt possible once the descent began. It launched on 14 July 2023 and landed on 23 August 2023, 40 days later.
Try it
Related to
Body systems and how they connectThe precise, no-second-attempt engine burns of a landing are a reminder of how unforgiving a world without air can be — the same reason astronauts must exercise hard to counter the effects of long, weightless journeys.
Chapter 09
A kitchen-table test of weightlessness
Here is a genuinely surprising experiment you can do with a paper or plastic cup, some water and a bit of care over a sink.
Punch a small hole near the bottom of the cup. Fill it with water and hold it up: water squirts out of the hole, pulled by gravity and pushed by the weight of water above it.
Now predict what happens to that squirting jet at the exact instant you let the whole cup fall — drop it a short, safe distance into a bucket or over a sink.
Predict first
Explore
Real laboratories that manufacture free fall
Pick a method scientists actually use to get a few seconds of weightlessness for testing.
- Air pumped out of a tall shaft
- Sealed capsule released
- Capsule falls freely
- A few seconds of microgravity
- Caught by a cushion below
Free fall on the ground
Some laboratories have built very tall, evacuated shafts so that a sealed capsule can fall for several seconds with almost no air resistance to interfere, giving researchers a short but genuine and repeatable window of microgravity without leaving the ground — far cheaper than a rocket, though far shorter than a space station.
Chapter 10
Bringing the investigations together
Lab
Match eight investigations in this lesson to the question each one actually answered.
Match each investigation to what it actually tested.
8 pairs are hiding in two mixed-up columns. Pick one from each side to join them.
Text version of this activity
Eight matches: the ramp tested whether the square law survives slower gravity; two coins of the same shape tested whether mass alone changes falling speed; nested paper cases tested whether mass affects terminal velocity when shape is fixed; the 20-swing pendulum tested how to shrink a timing error into a tiny percentage; Newton's Moon test checked whether the inverse-square law reaches the Moon; the binary search on the cannon narrowed in on the exact orbital and escape speeds; six perigee burns showed how a small engine gradually raises an orbit; and the leaking, falling cup showed weightlessness is about falling together, not an absence of gravity.
Words to know
All maths vocabulary →New words from this investigation
- Perigee
- The point in an orbit around Earth that is closest to the planet.
- Example: Mangalyaan fired its engine at perigee, six times.
- Apogee
- The point in an orbit around Earth that is farthest from the planet.
- Example: Each perigee burn raised Mangalyaan’s apogee.
- Binary search
- Narrowing in on an unknown value by repeatedly testing the midpoint of a bracket known to contain it.
- Example: Used to home in on the exact orbital speed in the cannon lab.
- Fair test
- An experiment that changes only one variable at a time, so the result can be trusted.
- Example: Nested paper cases changed mass while keeping shape fixed.
- Period (of a pendulum)
- The time for one complete swing, out and back.
- Example: A 1 m pendulum on Earth: about 2.01 s.
Quick check
Investigate: check your reasoning
8 questions · answer what you can, then check. Getting one wrong is useful.
Keep this
Cheat sheet: how these investigations were run
- Ramps slow gravity down without changing the rule: a = g sin(angle), and distance still grows with time squared.
- A fair test changes one variable at a time. Two coins of different mass, same shape, isolate mass; flat versus crumpled paper (same mass) isolates shape.
- Repeating an event beats timing it once. A 0.2 s reaction-time error is about 44 % of a single 1 s fall, but only about 0.5 % of a 20-swing pendulum timing.
- A pendulum measures g: T = 2π√(L/g), so g = 4π²L ÷ T². Mass and (small) amplitude do not affect the period.
- Same shape, more mass → higher terminal velocity. Same mass, smaller/denser shape → also higher terminal velocity. Both were tested by isolating one variable at a time.
- Newton’s Moon test: predicted acceleration from the inverse-square law (≈0.00269 m/s²) matches the acceleration implied by the Moon’s actual orbit (≈0.00272 m/s²) to about 1 %.
- A binary search (try the midpoint, then halve the bracket) is an efficient way to hunt for an unknown threshold, such as orbital or escape speed.
- ISRO raises orbits gradually: repeated perigee burns lift the apogee lap by lap, letting a smaller rocket do a bigger job — used for both Mangalyaan and Chandrayaan-3.
- Weightlessness is testable at home: a leaking cup’s jet nearly stops in free fall, because the water and the cup fall together.
Reflect
This stays on this page only. It isn’t saved or sent anywhere.
Where this comes from
Sources
Gravity and Newton’s law of universal gravitation (opens another website) — HyperPhysics, Georgia State Universityawaiting check
Supports F = G m₁ m₂ ÷ r², the value of G, the inverse-square fall-off with distance, g = G M ÷ r² at a surface, and circular-orbit and escape-speed relations.
Free Fall and Air Resistance (opens another website) — The Physics Classroomawaiting check
Supports free fall at a constant 9.8 m/s² regardless of mass, distance = ½ g t², why heavier objects reach a higher terminal speed, and how terminal velocity and parachutes work.
Newton’s Law of Universal Gravitation (opens another website) — The Physics Classroomawaiting check
Supports the apple-and-Moon reasoning, the inverse-square test against the Moon’s acceleration of about 0.0027 m/s², and the statement that gravity acts between every pair of masses.
Planetary Fact Sheet (opens another website) — NASA Space Science Data Coordinated Archiveawaiting check
Supports the masses, radii and surface gravity figures used throughout: Earth 9.8, Moon 1.62, Mars 3.72, Jupiter 24.79, Sun 274 and Pluto 0.62 m/s², plus the Moon’s orbital distance of 384,400 km and speed of about 1.02 km/s.
Chandrayaan-3 mission (opens another website) — Indian Space Research Organisation (ISRO)awaiting check
Supports the Chandrayaan-3 launch on 14 July 2023, the Vikram lander’s soft landing near the lunar south pole on 23 August 2023, and the powered-descent problem of shedding about 1.68 km/s with no atmosphere to help.
Mars Orbiter Mission (Mangalyaan) (opens another website) — Wikipediaawaiting check
Supports the six Earth-orbit-raising burns after the 5 November 2013 launch, trans-Mars injection on 1 December 2013 and Mars orbit insertion on 24 September 2014, and why a small rocket could still reach Mars.
End of Investigate
What you just read
- Design a fair test that changes one variable at a time, and explain why the coin-vs-paper race is not one.
- Explain why repeating an event (like 20 pendulum swings) shrinks a fixed timing error into a much smaller percentage.
- Use T = 2π√(L/g) to predict a pendulum’s period and to calculate g from measured swings.
- Describe Newton’s Moon test and explain why two independent methods agreeing is strong evidence.
- Explain how repeated perigee burns raise a spacecraft’s orbit, using Mangalyaan and Chandrayaan-3 as real examples.
- Next depthGo deeper: Go deeperMechanisms, reasoning, calculations and nuance.
- Practise70 questionsHints and a worked solution for every question — or play a 10-question round.
- Step backUnderstandGo back over the ground before this one — you can move up and down as often as you like.
- TopicAll of gravityThe whole ladder, the connections and the words to know, on one page.
The web
Explore a connection
Helps you understandanother area
Phases of the MoonGravity is what keeps the Moon in the orbit that produces the monthly cycle of phases.
Helps you understandanother area
TidesTides are gravity made visible: the Moon pulls the near ocean harder than the far ocean.
Helps you understandanother area
EclipsesEclipses happen only because the Sun, Earth and Moon move on fixed gravitational paths we can predict.
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Revision 1 · release preview-7e1cbbcc4f · accepted 20/09/2026