Gravitational Field Examples in Physics

Start with the recap, study the fully worked examples, then use the practice problems to check your understanding of Gravitational Field.

This page combines explanation, solved examples, and follow-up practice so you can move from recognition to confident problem-solving in Physics.

Concept Recap

A gravitational field is the region around a mass where another mass experiences a gravitational force.

A planet creates an invisible pull around it. The closer you are, the stronger that pull is.

Read the full concept explanation →

How to Use These Examples

  • Read the first worked example with the solution open so the structure is clear.
  • Try the practice problems before revealing each solution.
  • Use the related concepts and background knowledge badges if you feel stuck.

What to Focus On

Core idea: Gravitational Field asks students to choose the object, list external interactions, and reason from the resulting force or torque pattern.

Common stuck point: Students often know a formula related to gravitational field but skip the recognition step: Have I isolated one system and listed the external forces or torques acting on it before applying a law? That leads to a correct-looking substitution attached to the wrong physical model.

Sense of Study hint: Ask: Have I isolated one system and listed the external forces or torques acting on it before applying a law?

Worked Examples

Example 1

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Find the height above Earth's surface where gg drops to 4.9N/kg4.9\,\text{N/kg}. Use R=6.4×106mR = 6.4\times 10^6\,\text{m}, gsurf=9.8N/kgg_{surf} = 9.8\,\text{N/kg}.

Answer

h2.65×106 mh \approx 2.65\times 10^6 \text{ m}

First step

1
g/gsurf=(R/r)2=0.5g/g_{surf} = (R/r)^2 = 0.5, so r/R=2r/R = \sqrt{2}.

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Example 2

hard
Inside a uniform-density planet (mass MM, radius RR), the field at radius r<Rr < R is g(r)=GMr/R3g(r) = GMr/R^3. Find the depth below the surface where gg equals half its surface value.

Example 3

hard
At Earth's surface a person weighs 700N700\,\text{N}. The same person stands on a tower at altitude h=2.0×106mh = 2.0\times 10^6\,\text{m}. Find their weight there. Use RE=6.4×106mR_E = 6.4\times 10^6\,\text{m}.

Example 4

challenge
Two stars of masses MM and 2M2M separated by distance LL orbit their common center of mass. At the center of mass, find the magnitude of the total gravitational field.

Practice Problems

Try these problems on your own first, then open the solution to compare your method.

Example 1

easy
A 2 kg2 \text{ kg} mass feels a gravitational force of 19.6 N19.6 \text{ N}. Find the gravitational field strength.

Example 2

easy
Find the gravitational field at distance r=2×107 mr=2 \times 10^7 \text{ m} from a planet of mass M=6×1024 kgM=6 \times 10^{24} \text{ kg}. (G=6.67×1011G=6.67\times10^{-11})

Example 3

easy
The gravitational field at a point is 5 N/kg5 \text{ N/kg}. Find the force on a 3 kg3 \text{ kg} mass there.

Example 4

easy
If you double your distance from a planet's centre, how does the gravitational field change?

Example 5

easy
Earth's surface field is 9.8 N/kg9.8 \text{ N/kg}. What is the weight of a 10 kg10 \text{ kg} object on Earth?

Example 6

easy
The Moon's surface field is about 1.6 N/kg1.6 \text{ N/kg}. Find the weight of a 60 kg60 \text{ kg} astronaut on the Moon.

Example 7

easy
Distinguish gg and GG in g=GM/r2g = GM/r^2. Which is the universal constant?

Example 8

easy
A planet has surface field 20 N/kg20 \text{ N/kg}. Find the acceleration of a freely falling object near its surface.

Example 9

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Planet X has twice Earth's mass and the same radius. Compare its surface field to Earth's 9.8 N/kg9.8 \text{ N/kg}.

Example 10

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Planet Y has the same mass as Earth but half the radius. Find its surface field relative to Earth's 9.8 N/kg9.8 \text{ N/kg}.

Example 11

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Find Earth's surface field given M=6×1024 kgM=6\times10^{24} \text{ kg}, R=6.4×106 mR=6.4\times10^6 \text{ m}, G=6.67×1011G=6.67\times10^{-11}.

Example 12

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At what height above Earth's surface (R=6.4×106 mR=6.4\times10^6 \text{ m}) is the field one quarter of the surface value?

Example 13

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Two planets have fields g1g_1 and g2g_2. Planet 1 has mass MM, radius RR; planet 2 has mass 4M4M, radius 2R2R. Find g2/g1g_2/g_1.

Example 14

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A satellite is at r=7×106 mr = 7\times10^6 \text{ m} from Earth's centre (M=6×1024M=6\times10^{24}, G=6.67×1011G=6.67\times10^{-11}). Find the field there.

Example 15

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An object weighs 50 N50 \text{ N} on Earth's surface. What does it weigh at a distance 2R2R from Earth's centre?

Example 16

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A 4extkg4 ext{ kg} mass weighs 24extN24 ext{ N} on a planet. Find that planet's surface gravitational field strength.

Example 17

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Planet Q has 99 times Earth's mass and 33 times its radius. Find its surface field relative to Earth's 9.8extN/kg9.8 ext{ N/kg}.

Example 18

challenge
A planet has surface field gsg_s. A deep mine sits at half the radius. Treating the planet as uniform density (field r\propto r inside), find the field there.

Example 19

challenge
Two stars of mass MM each are a distance dd apart. Find the gravitational field at the midpoint between them.

Example 20

challenge
On planet Z, a pendulum's period is 2\sqrt{2} times its period on Earth (same length). Find planet Z's surface field given Earth's is 9.8 N/kg9.8 \text{ N/kg}.

Example 21

easy
A 0.5kg0.5\,\text{kg} stone feels a 4.9N4.9\,\text{N} gravitational pull. Find the local field strength.

Example 22

easy
A planet has M=3×1023kgM = 3\times 10^{23}\,\text{kg} and radius r=2×106mr = 2\times 10^6\,\text{m}. Find its surface field. (G=6.67×1011G = 6.67\times 10^{-11})

Example 23

easy
In a field of g=3.7N/kgg = 3.7\,\text{N/kg}, what force acts on a 25kg25\,\text{kg} rover?

Example 24

easy
At distance rr from a planet, g=8N/kgg = 8\,\text{N/kg}. Find gg at distance 2r2r.

Example 25

easy
A satellite weighs 1500N1500\,\text{N} on Earth's surface (g=9.8N/kgg = 9.8\,\text{N/kg}). Find its mass.

Example 26

easy
A satellite orbits at altitude h=Rh = R above a planet of radius RR. By what factor is the field weaker than at the surface?

Example 27

medium
Find the gravitational field at Mars's surface: M=6.4×1023kgM = 6.4\times 10^{23}\,\text{kg}, r=3.4×106mr = 3.4\times 10^6\,\text{m}.

Example 28

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At what distance from Earth's center is the field g=2.45N/kgg = 2.45\,\text{N/kg}? Use gsurf=9.8N/kgg_{surf} = 9.8\,\text{N/kg} at R=6.4×106mR = 6.4\times 10^6\,\text{m}.

Example 29

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A planet has the same density as Earth but twice the radius. Find its surface field relative to Earth.

Example 30

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Find Jupiter's surface field: M=1.9×1027kgM = 1.9\times 10^{27}\,\text{kg}, r=7.0×107mr = 7.0\times 10^7\,\text{m}.

Example 31

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Two point masses MM sit at the ends of a 2L2L segment. Find the field at the midpoint.

Example 32

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A point lies r1=3×108mr_1 = 3\times 10^8\,\text{m} from Earth (ME=6×1024kgM_E = 6\times 10^{24}\,\text{kg}) and r2=1×108mr_2 = 1\times 10^8\,\text{m} from the Moon (MM=7.3×1022kgM_M = 7.3\times 10^{22}\,\text{kg}) on the line between them. Find the Earth-produced field at that point. (G=6.67×1011G = 6.67\times 10^{-11})

Example 33

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A free-fall accelerometer reads a=1.6m/s2a = 1.6\,\text{m/s}^2 on a planet. What is the local gravitational field strength?

Example 34

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A spring scale shows W1=600NW_1 = 600\,\text{N} on Earth and W2=100NW_2 = 100\,\text{N} on planet P. Find gPg_P.

Example 35

hard
At what fraction of Earth's radius above the surface is gg reduced to 1%1\,\% of its surface value?

Example 36

hard
Two stars of masses MM and 4M4M are separated by distance dd. On the line between them, where is the field zero?

Example 37

hard
On the line from Earth (MEM_E) to the Moon (MM=ME/81M_M = M_E/81), separation dd, find the distance from Earth to the null point.

Example 38

hard
A geostationary satellite orbits at r=4.22×107mr = 4.22\times 10^7\,\text{m} from Earth's center. Find gg there. (GME=4.0×1014GM_E = 4.0\times 10^{14})

Example 39

hard
Two equal point masses MM sit at (±a,0)(\pm a, 0). Find the field magnitude at (0,a)(0, a).

Example 40

hard
A spherical asteroid has mass M=1.0×1015kgM = 1.0\times 10^{15}\,\text{kg} and radius r=5kmr = 5\,\text{km}. Find the surface field.

Example 41

hard
Estimate the gravitational field on the surface of a neutron star: M=1.4M=2.8×1030kgM = 1.4 M_\odot = 2.8\times 10^{30}\,\text{kg}, r=1.0×104mr = 1.0\times 10^4\,\text{m}.

Example 42

challenge
A thin uniform ring of mass MM and radius RR has field g(x)=GMx/(x2+R2)3/2g(x) = GMx/(x^2+R^2)^{3/2} on its axis at distance xx. Find the xx at which the field is maximum.

Background Knowledge

These ideas may be useful before you work through the harder examples.

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