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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.

Start at chapter 1

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.

a = g × sin(angle)
Effective acceleration down a frictionless slope.
10°: a = 9.8 × sin(10°) ≈ 1.70 m/s²
A gentle slope, easy to time by hand.
d = ½ a t²
The same square-law rule, just with a smaller a.

Predict first

A ball is released from rest on a 10° ramp, with a = 1.70 m/s². It has rolled 0.213 m after 0.5 s. If the square law still holds, how far will it have rolled after 1.0 s — twice the time?

TableTesting the square law on a 10° ramp (a = 1.70 m/s², computed from a = g sin(10°))
Time rollingDistance rolledRatio to the first value
0.5 s0.213 m
1.0 s0.851 m4.0×
1.5 s1.914 m9.0×
TableChoosing a ramp angle: steeper means less slowing-down, and less measuring time to play with
AngleEffective a = g sin(angle)Compared with a free fall (9.8)
0.854 m/s²about 1/11 — very gentle, easy to time, but a long ramp needed
10°1.702 m/s²about 1/6 — Galileo’s rough range, a good balance
20°3.352 m/s²about 1/3 — faster, needs a shorter reaction-time budget
30°4.900 m/s²exactly 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.

Where are we?

Earth: gravity pulls at 9.81 m/s². Home. Everything you have ever weighed was weighed here.

22110metresgroundMarble (rolled, not dropped)0.02 kgSteel ball, dropped straight down0.2 kg0.00 s
Marble (rolled, not dropped)2.0 m up

0.0 m/s · lands at 0.64 s

Steel ball, dropped straight down2.0 m up

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.

Need a different angle?

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

A ₹1 coin (about 3.09 g) and a ₹10 coin (about 7.74 g) are dropped together from the same height, indoors, over a short distance. What will you most likely see?

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.

TableWhy direct stopwatch timing struggles with short, single events
What you are timingTrue durationTypical reaction-time errorError 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

You want to measure how long it takes a small steel ball to fall exactly 20 cm, as precisely as you can with an ordinary phone. Which method will give the smallest percentage error?

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

A 0.25 m pendulum has a period of 1.00 s. If you make the string four times longer (1.00 m), what happens to the period?

TablePredicted periods for four string lengths (T = 2π √(L ÷ 9.8)) — measure these yourself before checking
LengthPredicted periodTime for 20 swings
0.25 m1.00 s20.1 s
0.50 m1.42 s28.4 s
1.00 m2.01 s40.1 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 shown

Measuring 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.

Need a different angle?

Try it

N/kg

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

Two identical paper cupcake cases are nested together (doubling the mass, keeping the shape and area almost the same) and dropped against a single case from the same height. What do you expect?

Lab

Compare two fair tests side by side: same shape with different mass, and same mass with different shape.

Where are we?

Earth: gravity pulls at 9.81 m/s². Home. Everything you have ever weighed was weighed here.

32210metresgroundOne paper case0.003 kg · fluffyOne paper case0.003 kg · fluffy0.00 s
One paper case3.0 m up

0.0 m/s · lands at 2.58 s

One paper case3.0 m up

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.

Need a different angle?

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.

TableNewton’s Moon test, redone with today’s numbers
MethodWhat it usesResult
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
Agreementwithin about 1.2 %

Predict first

Suppose the 1 % gap between the predicted and observed Moon accelerations had instead come out as a factor of 2 (100 % off), no matter how carefully the calculation was checked. What would that mean?

Related to

Phases of the Moon

The 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.

EarthFalls back to the ground Earth 221 px across · mountain drawn far too tall

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.

Need a different angle?

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

A spacecraft is in an elliptical orbit. Each time it passes its closest point to Earth, its engine fires briefly, speeding it up a little more in the direction it is already travelling. What happens to the orbit over several such burns?

Mangalyaan: raising an orbit until it reaches Mars

  1. 5 Nov 2013
    Launch A PSLV rocket — not powerful enough to send the spacecraft straight to Mars — puts it into a stretched Earth orbit instead.
  2. Nov 2013
    Six 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.
  3. 1 Dec 2013
    Trans-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.
  4. 24 Sep 2014
    Mars 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

days

Related to

Body systems and how they connect

The 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

You let go of the leaking cup and it falls freely (with the hole open) for the half-second or so before it lands. What happens to the jet of water coming out of the hole during the fall?

Explore

Real laboratories that manufacture free fall

Pick a method scientists actually use to get a few seconds of weightlessness for testing.

  1. Air pumped out of a tall shaft
  2. Sealed capsule released
  3. Capsule falls freely
  4. A few seconds of microgravity
  5. 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.

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.
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.

  1. Q1Why did Galileo use a ramp instead of dropping objects straight down?
  2. Q2Why is racing two coins of different value a fairer test of "does mass affect falling speed" than racing a coin against a flat sheet of paper?
  3. Q3A class doubles the mass of the bob on their pendulum, keeping the length the same. What happens to the period?
  4. Q4A pendulum of length 0.50 m completes 20 swings in 28.4 s. What period does that give for one swing?
  5. Q5What makes Newton’s Moon test convincing?
  6. Q6In a binary search for orbital speed between a "lands" result at 6 km/s and an "escapes" result at 10 km/s, what should you try next?
  7. Q7Firing an engine briefly at the perigee (closest point) of an elliptical orbit, in the direction of travel, mainly changes...
  8. Q8Why does the jet from a leaking, falling cup almost stop during the fall?

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

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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.

The web

Explore a connection

  • Helps you understandanother area

    Phases of the Moon

    Gravity is what keeps the Moon in the orbit that produces the monthly cycle of phases.

  • Helps you understandanother area

    Tides

    Tides are gravity made visible: the Moon pulls the near ocean harder than the far ocean.

  • Helps you understandanother area

    Eclipses

    Eclipses 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