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.
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.
FORCE
Earth’s gravitational pull on the Moon is the force that keeps the Moon in orbit around the 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.
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.
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 →
Recorded properties
Dimensions and measurements
| Property | Selected value | Recorded range | Basis |
|---|---|---|---|
| 1.98 × 10¹⁴ MN | 1.93 × 10¹⁴ MN to 2.03 × 10¹⁴ MN | derived |
Around this scale
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Compare examples with lower, similar and higher values. Each card names the measurement being compared.
Sources and method
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The source records and measurement method remain available for inspection.
- NASA — Moon factsMean lunar orbital speed and synodic phase-cycle context.
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