Gravitational field and potential
The gravitational field describes the force per unit mass at a point in space due to one or more masses, while gravitational potential is the work done per unit mass to bring a mass from infinity to that point.
Why this shows up in the exam
You need to calculate field intensity, potential, and understand their relationship for NEET problems.
How NEET tests this
Learn the idea
Gravitational field intensity is the force that a unit mass would feel at a point, while gravitational potential is the work needed per unit mass to bring it from infinity. The key insight: field = force / mass and potential = work / mass, so once you know one you can get the other by differentiation or integration.
🧠 Memory hook: Think of g as ‘weight per kilogram’ – just how heavy you feel per each kilogram of your own mass.
Get this one clearly and it pays off every single time it shows up in the paper. 🎯
Formulas & facts to keep ready
- g = F / m (unit N kg⁻¹)
- Gravitational potential V = –GM / r (unit J kg⁻¹)
- Relation: g = –dV/dr (magnitude g = |dV/dr|)
- Superposition holds for both field and potential
- SI units: mass in kg, distance in m, force in N
- Potential is scalar, field is vector
How to approach it
- 1Read the question and list what is given – force, mass, distance, etc.
- 2Convert every quantity to SI units (g → kg, cm → m).
- 3Apply the definition that matches the asked quantity – use g = F/m for field, V = –GM/r for potential.
- 4If both field and potential appear, use g = –dV/dr or integrate accordingly.
Worked example — watch it click
A body of mass 60 g experiences a gravitational force of 3.0 N, when placed at a particular point. The magnitude of the gravitational field intensity at that point is:
- A)0.05 N/kg
- ✅50 N/kg
- C)20 N/kg
- D)180 N/kg
The concept behind this problem
The example checks whether you can translate the definition of gravitational field intensity into a numerical answer by correctly handling the force‑per‑unit‑mass relation.
Step by step
- 1The gravitational field intensity (often denoted g) at a point is defined as the force per unit mass placed at that point: g = (F)/(m).
- 2The mass of the body is 60 g, which is 60/1000 = 0.06 kg.
- 3The gravitational force acting on it is 3.0 N.
- 4Now compute the field intensity: g = 3.0 N0.06 kg = 50 N kg⁻¹.
- 5Thus the field intensity is 50 N per kilogram.
- 6The option “0.05 N/kg” would correspond to using the mass in grams directly, which is incorrect because the SI unit of mass is kilogram.
- 7So the correct answer is 50 N/kg.
Watch out
Students often forget to change 60 g to 0.06 kg, leading to the wrong 0.05 N kg⁻¹ option.
Common slip-ups that cost marks
- •Using gram directly instead of kilogram gives a factor 1000 error
- •Ignoring the negative sign of potential – it is always negative for attractive gravity
- •Treating potential as a vector; it is a scalar quantity
🌟 That's the whole idea — you've got this. Try the practice set below; every question you attempt makes it stick a little harder.
Practise it
These are real questions from past NEET papers that test this exact idea.
A body of mass 60 g experiences a gravitational force of 3.0 N, when placed at a particular point. The magnitude of the gravitational field intensity at that point is:
Push further
More challenging2 harder questions built from the past papers above — a step up in difficulty, with distractors designed so you can't get there by elimination. Written and checked by our reviewers, not from a real paper.
A spherical planet has a mass of 5.0 x 10²³ kg and a radius of 2.0 x 10⁶ m. What is the gravitational field intensity on its surface? (Given G = 6.67 x 10⁻¹¹ N m²/kg²)
More from Gravitation
Acceleration due to gravity and its variation
Acceleration due to gravity (g) is the acceleration experienced by a body due to Earth's gravity, and it varies with height, depth, and planetary properties.
Kepler's laws of planetary motion
Kepler's laws describe the motion of planets and satellites: orbits are ellipses (first law), equal areas are swept in equal times (second law), and the square of the period is proportional to the cube of the semi-major axis (third law).
Gravitational potential energy and work
Gravitational potential energy is the energy an object possesses due to its position in a gravitational field, and work is required to move it against gravity.
Satellite motion and orbital parameters
Satellite motion involves understanding orbital velocity, time period, escape velocity, and the specific conditions for geostationary orbits.
Newton's law of universal gravitation
Newton's law of universal gravitation states that every two masses attract each other with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
Conservative nature of gravitational force
Gravitational force is a conservative force, meaning the work done in moving an object between two points is independent of the path taken.