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Modern physics is defined mainly in terms of fields, which are physical entities that extend in space and time. These objects are the usual sources of non-contact forces and allow us to describe the dynamics of almost every system we know of.
British-born scientist Isaac Newton already figured that gravity is a field that exists because of the presence of mass. Furthermore, he realised that it was always an attractive force. Let’s take a look at the definition of gravitational field strength:
The gravitational field strength is the measure of the intensity of the gravitational field that has mass as a source and attracts other masses.
Gravitational field strength is generated by masses, and it gives rise to an attractive force that weakens with distance.
Historically, there has not been a unique description of gravity. Due to experimentation, we know that Newton’s expression works on planets, stars (etc.) and their surroundings.
When considering more complex phenomena, such as black holes, galaxies, deviation of light, we need more fundamental theories such as General Relativity, developed by Albert Einstein.
Recall Newton’s law of gravitation. Its formula is
where the vector Z is the field strength sourced by the mass M, G is the universal constant of gravitation, r is the radial distance measured from the centre of the mass of the source body, and the vector er is the radial unit vector going towards it. If we want to obtain the force a body with mass m experiences under the influence of the field Z, we can simply calculate it as
Concerning units and values, we find that the force of gravity is measured in Newtons [N = kg⋅m/s2]. As a result, the field strength is measured in m/s2, i.e. it is an acceleration. The mass is usually measured in kilograms and the distance in meters. This gives us the units of the universal gravitational constant G, which are Nm2/kg2 = m3/s2⋅kg. The value of G is 6.674 ⋅ 10-11m3/s2⋅kg.
Important to know! The value of the gravitational field strength on Earth is 9.81m/s2 or N/kg.
Newton’s law of gravitation, Wikimedia Commons
The main features of the gravitational field include
Understanding these characteristics is important, even for current scientists, to develop better models for gravity that reproduce the basic aspects of Newton’s gravity.
One of the most important consequences of Newton’s expression for the gravitational field strength is the reciprocity of the masses. This is consistent with Newton’s third law of motion, which states: if a body exerts a force on another body, the latter exerts the same force with opposite direction on the first.
The reciprocity is deeper than it seems since it states that a fundamental feature of the gravitational field strength is that it is equivalent to describing the gravity interactions from the perspective of one body or the other. This seems trivial but has deep implications concerning, for instance, general relativity.
One of the main features of Newton’s expression for the gravitational field strength is the radial quadratic dependence. It turns out that in three-dimensional space, this is the right dependence to achieve an infinite range of field strength reaching any part of the space. Any other dependence would not allow it to have an infinite range or cause physical inconsistencies.
Additionally, this spherical dependence is joined by a spherical radial symmetry in the direction of the field strength. This not only ensures an attractive character but is also consistent with isotropy: there is no special direction in three-dimensional space. The way to put all directions on equal footing is to impose spherical symmetry, which leads to the radial dependence and the radial vector.
The universal constant of gravitation or Cavendish constant measures the intensity of the gravitational field strength. Of course, the intensity of the field will depend on the characteristics for each case, but it is a measure in the following sense: if we set all variables to one (with appropriate units), what number do we get?
For instance, if we take two charges of 1 coulomb separated by 1 meter, we get a certain electrostatic force. If we do the same with two bodies of 1 kilogram each, we get another number for the gravitational force. The value is, essentially, the value of the constant in front of each of the formulae. It turns out that the constant for gravitation G is smaller than the constant for electromagnetism k (8.988 ⋅ 109N⋅m2/C2), so gravity is a weaker force.
In fact, out of the four fundamental forces (gravity, electromagnetism, strong force, and weak force), the gravitational field strength is the weakest one. It is also the only one acting relevantly at interplanetary scales.
The four fundamental forces are gravity, electromagnetism, strong force, and weak force.
Here are some examples of calculations of gravitational field strengths to get a better understanding of how it operates in various astronomical objects.
The gravitational field strength is the intensity of the gravitational field sourced by a mass. If multiplied by a mass subject to it, one obtains the gravitational force.
To calculate the gravitational field strength, we apply Newton’s formula with the universal constant of gravitation, the mass of the source, and the radial distance from the object to the point where we want to calculate the field.
The gravitational field strength is measured in m/s2 or N/kg.
The gravitational field strength on the Moon is approximately 1.62m/s2 or N/kg.
The gravitational field strength on Earth is 9.81m/s2 or N/kg.
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