Year 13
Side B1: Gravitational Fields
Start Side B with field strength, gravitation, potentials, and orbital motion.
Part of Year 13 CIE Physics 9702.
What students will cover
This topic develops gravitational field models from definitions through orbital applications. Keep the build-up from field strength to potentials and orbits clear as you work through the topic.
You begin by defining gravitational field strength and representing fields with field lines. The next lessons use Newton’s law of gravitation to model forces and field strength around point masses, then develop gravitational potential and potential energy. The topic closes by applying the same ideas to circular and geostationary orbits before you consolidate the topic through revision and review.
Topic revision route
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Recall vocabulary
Gravitational field
a region where a mass experiences a force; gravitational field strength is force per unit mass.
field strength
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field lines
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point mass
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inverse square law
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centripetal acceleration
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geostationary orbit
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Gravitational potential
the work done per unit mass in bringing a small test mass from infinity to the point.
gravitational potential energy
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force per unit mass
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Newton's law of gravitation
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gravitational constant
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potential energy
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work done
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infinity
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circular orbit
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orbital period
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satellite
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Resource bank
- Lesson resources
- 5
- Topic resources
- 0
Open the relevant lesson first, then use its linked slides, worksheets, simulations, or practice tasks.
Syllabus CIE 9702 coverage in this topic
12 points across 7 lessons
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CIE 9702 coverage in this topic
12 points across 7 lessons
understand that a gravitational field is an example of a field of force and define gravitational field as force per unit mass
represent a gravitational field by means of field lines
understand that, for a point outside a uniform sphere, the mass of the sphere may be considered to be a point mass at its centre
recall and use Newton’s law of gravitation F = Gm1m2 / r2 for the force between two point masses
analyse circular orbits in gravitational fields by relating the gravitational force to the centripetal acceleration it causes
understand that a satellite in a geostationary orbit remains at the same point above the Earth’s surface, with an orbital period of 24 hours, orbiting from west to east, directly above the Equator
derive, from Newton’s law of gravitation and the definition of gravitational field, the equation g = GM / r 2 for the gravitational field strength due to a point mass
recall and use g = GM / r 2
understand why g is approximately constant for small changes in height near the Earth’s surface
define gravitational potential at a point as the work done per unit mass in bringing a small test mass from infinity to the point
use ϕ = –GM / r for the gravitational potential in the field due to a point mass
understand how the concept of gravitational potential leads to the gravitational potential energy of two point masses and use EP = –GMm / r
Lesson sequence
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Lesson
01Fields and Field Strength
Introduce the concept of gravitational fields and field strength.
Lesson
02Newton's Law of Gravitation
Use Newton's law of gravitation to model interactions between masses.
Lesson
03Potential Energy and Potentials
Develop gravitational potential energy and gravitational potential.
Lesson
04Orbits
Apply gravitational field ideas to orbital motion.
Lesson
05Revision
Consolidate gravitational fields before assessment.
Lesson
06Test
Assess understanding of gravitational fields.
Lesson
07Review
Review the gravitational fields test and strengthen weak areas.