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Gravity and force

Earth gravitational pull on the Moon

Earth’s gravitational pull on the Moon is the force that keeps the Moon in orbit around the Earth.

Also known as: Earth Moon gravitational force

How big is it?

1.98 × 10¹⁴ MN · mean-separation gravitational force

Mean-separation gravitational force · derived
Typical recorded range: 1.93 × 10¹⁴ MN to 2.03 × 10¹⁴ MN.

Scale illustration of Earth’s gravitational pull on the Moon, showing the recorded mean-separation gravitational force.
Recorded mean-separation gravitational force: 1.98 × 10¹⁴ MN.

A little perspective

Earth gravitational pull on the Moon vs Moon tidal force across Earth: weight comparison

Earth’s gravitational pull on the Moon is about 30 times the Moon’s tidal force across Earth.

Scale

FORCE

Earth gravitational pull on the Moon

Earth’s gravitational pull on the Moon is the force that keeps the Moon in orbit around the Earth.

1.98 × 10¹⁴ MNMean-separation gravitational force
0
Moon tidal force across Earth

The Moon tidal force across Earth is the difference in lunar gravitational pull between the near and far sides of the planet, which drives ocean tides.

6.6 × 10¹² MNDefined differential-force scale
0
Bar length measures force in newtons. Mass and local gravity determine weight.
Measurements, assumptions & sources +

Earth gravitational pull on the Moon

Mean-separation gravitational force: 1.98 × 10¹⁴ MN; derived; range 1.93 × 10¹⁴ MN–2.03 × 10¹⁴ MN.

Approximately 1.98 × 10²⁰ N, calculated with F = GMm/r² using JPL Earth and Moon masses and the 384,400 km mean centre-to-centre separation. The elliptical orbit changes the instantaneous force.

NASA — Moon facts

The marked mean-separation gravitational force is calibrated. Unmeasured illustration details are representative.

Moon tidal force across Earth

Defined differential-force scale: 6.6 × 10¹² MN; derived calculation; range 6 × 10¹² MN–7.2 × 10¹² MN.

Approximately 6.6 × 10¹⁸ N, a teaching scale formed by multiplying Earth’s mass by the near-to-centre lunar tidal-acceleration difference 2GMₘRₑ/r³. It is not the Moon’s total attraction on Earth and ignores solar tides and Earth deformation.

Defined examples — our methodology

The marked defined differential-force scale is calibrated. Unmeasured illustration details are representative.

Use the visual comparison to explore its scale, then check the measurements and sources.

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Why this measurement?

Why we use 1.98 × 10¹⁴ MN

We compare Earth’s gravitational pull on the Moon. The measurement is labelled derived. Check the source notes for its basis. The recorded range is 1.93 × 10¹⁴ MN to 2.03 × 10¹⁴ MN.

Approximately 1.98 × 10²⁰ N, calculated with F = GMm/r² using JPL Earth and Moon masses and the 384,400 km mean centre-to-centre separation. The elliptical orbit changes the instantaneous force.

The picture identifies the subject; the diagram compares the recorded values. How calibrated comparisons work →

Explore gravity and force →

Recorded properties

Dimensions and measurements

PropertySelected valueRecorded rangeBasis
1.98 × 10¹⁴ MN1.93 × 10¹⁴ MN to 2.03 × 10¹⁴ MNderived

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Sources and method

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