earth weight
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How much does the Earth weigh?

Earth is the third planet from the Sun and the only known celestial body to harbor life. Earth’s mass, measured in tons, determines its gravitational pull and influences various planetary processes. The weight of Earth, though a misnomer in space, is used to describe its mass in relation to gravity. Earth’s density plays a role in its composition and structure. Estimates of Earth’s mass have been refined over time through scientific observations and calculations. Learn about Earth’s measurements and how they impact our understanding of planetary formation and dynamics.

Earth’s mass is large to be measured on a scale, so gravitational calculations are used to determine its value. Approximations exist, with some scientists rounding Earth’s mass to 6 × 10^24 kg (13.2 × 10^24 lbs) for simplicity in calculations.

Earth’s density is 5.513 g/cm³ (0.199 lb/in³) or 8850 kg/m³ (0.321 lb/ft³). Scientists calculate Earth’s density by dividing its mass by its volume. Earth’s density varies by depth and location, with the core being the densest part. The inner core has a density of around 13 g/cm³ (0.47 lb/in³), while the outer core has a density of 12 g/cm³ (0.43 lb/in³). Earth is the densest planet in our solar system due to its composition of metals and silicate rocks.

Earth gains 40,000 tonnes of mass from space debris annually.  Earth’s atmosphere has a mass of 5.5 quadrillion tons. The maximum sustainable human population adds between 25-50 trillion kg of mass to Earth.

Earth’s mass is 81 times the Moon’s mass. Earth weighs 5.98 × 10^24 kg (1.32 × 10^25 lbs), while the Moon weighs 7.35 × 10^22 kg (1.62 × 10^23 lbs). Earth’s surface has a gravitational acceleration of 9.8 m/s^2 (32.2 ft/s^2), compared to the Moon’s 1.625 m/s^2 (5.34 ft/s^2).

Scientists use Newton’s Law of Gravitation and the Moon’s orbit to calculate Earth’s mass. The formula F = GMm/r^2 is used, where G is the gravitational constant (6.674 × 10^-11 m^3 kg^-1 s^-2). Earth’s radius of 6,371 km (3,959 miles) is crucial for mass determination. Satellite orbital characteristics and the density and volume approach provide methods to calculate Earth’s mass.

What is the weight of Earth in kg?

The weight of Earth in kg is not measured. Earth’s mass, which is 5.9722 × 10^24 kg (1.316 × 10^25 lbs), is used to calculate its weight. Weight varies depending on location due to gravity, while mass remains constant.

The current best estimate for Earth’s mass is 5.9722 × 10^24 kg (1.316 × 10^25 lbs). Scientists have established this value through measurements and calculations. Earth’s mass is large to be measured on a scale. Gravitational calculations have been used to determine this large mass value.

A value cites Earth’s mass as 5.974 × 10^24 kg (1.320 × 10^25 lbs). An estimate puts Earth’s mass at 5.9736 × 10^24 kg (1.316 × 10^25 lbs). Scientists have rounded Earth’s mass to 6 × 10^24 kg (13.2 × 10^24 lbs) for simplicity in some calculations. An approximation states Earth’s mass as 5.97 × 10^24 kg (1.32 × 10^25 lbs). These variations in estimates all fall within a range of the current best estimate.



What is the density of Earth?

The density of Earth is 5.513 g/cm³ (0.199 lb/in³). Scientists calculate this density by dividing Earth’s mass of 5.972 × 10^24 kg (1.316 × 10^24 lbs) by its volume of 1.08 × 10^12 km³ (2.59 × 10^11 mi³). Earth’s density varies by depth and location.

Earth’s density has been measured and calculated with varying degrees of precision. The overall average density of Earth is 5.513 g/cm³ (0.199 lb/in³). Earth’s average density is reported as 5.514 g/cm³ (0.199 lb/in³) in literature. The mean density of Earth is calculated to be 5.515 g/cm³ (0.199 lb/in³). Earth’s approximate average density is 5.52 g/cm³ (0.199 lb/in³). The mean density of Earth in SI units is 5520 kg/m³ (344.1 lb/ft³). Scientists round Earth’s density to 5.5 g/cm³ (0.199 lb/in³) for simplicity in calculations. Earth’s density makes it the densest planet in our solar system. Earth’s composition of metals and silicate rocks containing iron, oxygen, silicon, and magnesium contributes to its density. Earth’s density varies within its different layers. Earth’s core is the densest part, with the inner core having a density around 13 g/cm³ (0.47 lb/in³) and the outer core around 12 g/cm³ (0.43 lb/in³). Earth’s mantle has a density ranging from 4,500 kg/m³ (281.5 lb/ft³) to 5,600 kg/m³ (349.5 lb/ft³). Earth’s crust is the least dense layer. Earth’s high overall density indicates the presence of dense materials like iron and nickel in its interior.



How much weight can the Earth hold?

The Earth can hold more weight than its current mass, as it is capable of incorporating unlimited additional mass without impact. Earth’s mass is 5,974,000,000,000,000,000,000 kg (13,167,000,000,000,000,000,000 lbs). Earth gains 40,000 tonnes of mass from space debris. Earth loses 90,000 tonnes of mass from escaping gases and nuclear reactions.  Scientists estimate the maximum sustainable human population ranges from 500 million to 1 trillion people, adding between 25-50 trillion kg of mass to Earth.

How does the mass of the Earth compare to that of the Moon?

The mass of the Earth compared to the Moon is larger. Earth’s mass is 5.98 × 10^24 kg (13.2 × 10^24 lbs), while the Moon’s mass is 7.35 × 10^22 kg (16.2 × 10^22 lbs). Earth weighs 81 times more than the Moon.

The comparison of the mass of the Earth to the Moon is detailed in the table below.

FeatureEarthMoon
Mass in kg5.9724 × 10^24 kg0.07346 × 10^24 kg
Mass Ratio81.3 times more1/81.3 of Earth’s mass
Gravitational Acceleration (m/s^2)9.80 m/s^21.62 m/s^2
Gravitational Acceleration (ft/s^2)32.2 ft/s^25.31 ft/s^2
Weight of a 100 kg object in kg100 kg16.5 kg
Weight of a 100 kg object in lbs220.5 lbs36.4 lbs
Gravitational Force Percentage100%16.5%
Volume (10^10 km^3)1.08321 × 10^12 km^32.1968 × 10^10 km^3
Equatorial Radius (km)6378.1 km1738.1 km
Polar Radius (km)6356.8 km1736.0 km
Volumetric Mean Radius (km)6371.0 km1737.4 km
Mean Density (kg/m^3)5514 kg/m^33344 kg/m^3
Escape Velocity (km/s)11.2 km/s2.38 km/s

The Earth exerts a stronger gravitational force due to its mass. Earth’s surface has a gravitational acceleration of 9.8 m/s^2 (32.2 ft/s^2), while the Moon’s surface has a gravitational acceleration of 1.625 m/s^2 (5.34 ft/s^2). The Moon’s gravitational force equals 16.6% of Earth’s gravitational force. An object’s mass remains constant on both bodies. A 100 kg (220.5 lbs) object on Earth weighs 16.5 kg (36.4 lbs) on the lunar surface due to the Moon’s weaker gravity.

Scientists use kilograms as the unit for measuring celestial body masses. The Earth has a mass of 5.9724 x 10^24 kg (1.316 x 10^25 lbs), while the Moon has a mass of 0.07346 x 10^24 kg (1.620 x 10^23 lbs). Exponential notation is crucial for expressing such large masses. Researchers calculate the Earth-to-Moon mass ratio as 81.3, meaning the Earth is 81.3 times more massive than the Moon. The Moon’s mass equals 1.2% of Earth’s mass in percentage terms.



How to calculate the mass of Earth?

To calculate the mass of Earth, scientists use Newton’s Law of Gravitation and the Moon’s orbit. Earth’s mass can be determined by equating gravitational force to centripetal force, considering the Moon’s orbital period and distance. Another method uses surface gravity and Earth’s radius.

To calculate the mass of Earth, follow the steps outlined below.

  • Use Newton’s Law of Gravitation formula, F = GMm/r^2.
  • Employ the value of gravitational constant G as 6.674 × 10^-11 m^3 kg^-1 s^-2.
  • Measure Earth’s average radius, approximately 6,371 km (6.371 × 10^6 m).
  • Calculate the orbital period and distance from Earth for celestial bodies like the Moon or satellites.
  • Apply centripetal force equations for orbital motions to estimate Earth’s mass.
  • Utilize the density and volume approach, using Earth’s density and volume formulas.
  • Incorporate Earth’s surface gravity value of 9.8 m/s^2 for mass calculations.
  • Combine astronomical observations and modern data to refine mass approximations.
  • Conclude that Earth’s mass is approximately 5.972 × 10^24 kg based on calculations.



Satellite orbital characteristics offer another method to calculate Earth’s mass. Orbital period measurement of satellites, combined with Earth radius and satellite distance, allows scientists to determine the mass using centripetal force equations. The accepted value for the mass of Earth is 5.972 x 10^24 kg (1.316 x 10^25 lbs), derived from these precise astronomical observations.

Density and volume approach provides a method to estimate Earth’s mass. Volume calculation involves using the Earth radius measurement in the formula V = (4/3)πr^3. The density formula ρ = m/V relates mass to volume and density. Earth has an average density of 5.51 g/cm^3 (0.199 lb/in^3).

Surface gravity method relates the gravitational force exerted on objects to Earth’s mass. The acceleration due to gravity on Earth’s surface is 9.8 m/s^2 (32.2 ft/s^2). Scientists use this value in conjunction with Newton’s second law of motion to calculate Earth’s mass.

Approximation techniques refine Earth’s mass calculations with improved measurements. Scientists combine data of acceleration due to gravity or orbital motions with Newton’s laws of motion and gravitation. These methods allow researchers to find Earth’s mass with precision without directly measuring its volume or using density formulas.