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Convert Galileo to Standard Gravity

Use this free converter to change galileos (Gal) into standard gravity (g). Galileo and standard gravity both measure acceleration. As a quick reference, 1 Gal equals 0.0010197162 g, and 1 g equals 980.665 Gal.

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Standard Gravity (g)
0.0010197162

1 Gal = 0.0010197162 g

Acceleration conversion table

GalileoStandard Gravity
0.010.000010197162
0.10.00010197162
0.50.00050985811
10.0010197162
20.0020394324
30.0030591486
50.0050985811
100.010197162
200.020394324
250.025492905
500.050985811
1000.10197162
1,0001.0197162

How to convert Galileo to Standard Gravity

Multiply the galileo value by 0.0010197162 to get standard gravity.

  1. Enter the number of galileos you want to convert.
  2. The converter instantly shows the equivalent value in standard gravity.
  3. Worked example: 15 Gal × 0.0010197162 = 0.015295743 g.
  4. Use the swap button to reverse the conversion (standard gravity to galileo).

About these units

Galileo (Gal)

Definition
A galileo (Gal) is a CGS acceleration unit equal to one centimeter per second squared.
History
Named after Galileo Galilei, it is used in geodesy and gravimetry.
Current use
Galileos (and milligals) measure tiny variations in Earth’s gravity.

Standard Gravity (g)

Definition
Standard gravity (g) is the nominal acceleration of free fall at Earth’s surface, defined as 9.80665 m/s².
History
It was standardised so weights and forces could be defined consistently.
Current use
It expresses g-forces in aviation, vehicle dynamics, and spaceflight.

Frequently asked questions

How many standard gravity are in a galileo?

There are 0.0010197162 g in 1 Gal. To convert, multiply the number of galileos by 0.0010197162.

How do I convert galileos to standard gravity?

Multiply the galileo value by 0.0010197162 to get standard gravity. For example, 10 Gal = 0.010197162 g.

Is this galileo-to-standard gravity converter free?

Yes. This converter is completely free, runs entirely in your browser, and requires no sign-up. Your inputs never leave your device.

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