Do Now warm-up prompt

Do Now: The Moon is 384,000 km away, with nothing in between. How can Earth pull on it without touching it?

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Through its gravitational field. Every mass creates a field in the space around it. Any other mass in that field feels a force.

A. What Is a Field?

Gravitational field lines around Earth

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

B. Field Strength

g = Fgm

Gravitational field strength (N/kg)

g = force per kilogram on a test mass. It does not depend on the test mass.

At Earth’s surface, g = 9.81 N/kg. Since 1 N/kg = 1 m/s², that’s also the acceleration of free fall.

Review: Weight (Fg = mg)

C. Where Does g Come From?

Start with Newton’s law of gravitation and divide by the test mass:

Fg = Gm1m2r2   →   g = Fgm2 = Gm1r2

g = Gmr2

m = mass making the field, r = distance from its center, G = 6.67 × 10−11 N•m²/kg²

Example 1

Earth’s mass is 5.97 × 1024 kg and its radius is 6.37 × 106 m. Find g at the surface.

g = (6.67 × 10−11)(5.97 × 1024)(6.37 × 106)2

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g = 9.81 N/kg ✓

Example 2

Mars has a mass of 6.42 × 1023 kg and a radius of 3.39 × 106 m. Find g on Mars, and the weight of a 60.-kg student there.

g = (6.67 × 10−11)(6.42 × 1023)(3.39 × 106)2

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g = 3.73 N/kg

Fg = mg = (60. kg)(3.73 N/kg) = 224 N — about 38% of the student’s weight on Earth

D. The Inverse Square Law

Field strength at 1, 2, 3, and 4 Earth radii
Example 3

The Space Station orbits about 400 km above Earth, at about 6,770 km from Earth’s center. Compare g there to the surface value.

Earth’s radius is 6,370 km.

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g = 9.81 × (6,3706,770)2 = 8.7 N/kg — about 89% of surface gravity!

The astronauts float because they are in free fall, not because gravity is gone.

Explore: Field Explorer

Drag the test mass around the planet. Change the planet and the mass.

Try This

1. Change the test mass. Does g change? Does Fg change?
2. Drag the mass from 1R to 2R. What happens to g?
3. Compare g at the surface of each planet.

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1. g stays the same; Fg changes in proportion to the mass. g belongs to the field, not the test mass. 2. g drops to one-fourth. 3. Moon 1.62, Mars 3.73, Earth 9.81, Jupiter about 24.8 N/kg.

E. Practice

Problem 1

A 50.-kg astronaut stands on the Moon, where g = 1.62 N/kg. Find her weight.

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Fg = (50. kg)(1.62 N/kg) = 81 N

Problem 2

What is g at 3 Earth radii from Earth’s center?

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9.81 ÷ 32 = 1.09 N/kg

Problem 3

A 2.0-kg mass feels a 7.4-N gravitational force on a planet. Find g.

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g = 7.4 / 2.0 = 3.7 N/kg (about the same as Mars)

Problem 4

A planet has twice Earth’s mass and twice Earth’s radius. Compare its surface g to Earth’s.

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×2 for mass, ÷22 = ÷4 for radius → half of Earth’s: about 4.9 N/kg

Check Your Understanding

5 quick questions — pick an answer to see if you’re right.

1. Gravitational field strength is measured in

2. Doubling a test mass at the same location makes g

3. If you move to 2 Earth radii from Earth’s center, g becomes

4. Field lines around a planet point

5. Astronauts on the Space Station feel weightless because