Lesson 5.6 • Summative AssessmentInteractive Simulation
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Unit 5 Summative Assessment: Gravitational Field

Comprehensive 16-question exam covering all competencies (5.1–5.4): Universal gravitation, field intensity, potential, orbital mechanics, geostationary satellites, and escape velocity with automated grading.

Marking a lesson complete represents finishing your study of the topic; it does not denote tested mastery.

Learning Objectives

  • Assess mastery across all 4 syllabus competencies for Gravitational Field under timed conditions.
  • Identify individual competency weaknesses and receive targeted lesson revision links.

Syllabus Topic Outline

Summative Assessment
  • 1Competency 5.1: Universal Gravitation and Field Intensity
  • 2Competency 5.2: Gravitational Potential and Energy
  • 3Competency 5.3: Orbital Mechanics and Satellites
  • 4Competency 5.4: Geostationary Satellites and Escape Velocity
Unit 5 Comprehensive Assessment: Gravitational Field

Summative evaluation covering syllabus competencies 5.1 and 5.2: Universal gravitation, field intensity, potential, orbital mechanics, geostationary satellites, and escape velocity.

Answered: 0 / 20
Question 1 (Competency 5.1)foundation

What are the SI base units of the Universal Gravitational Constant G?

Question 2 (Competency 5.1)foundation

If the distance between two point masses is reduced to one-third of its original value, by what factor does the gravitational force between them change?

Question 3 (Competency 5.1)intermediate

Two identical lead spheres, each of mass 50.0 kg, have their centers separated by 0.50 m. Calculate the magnitude of the gravitational attraction between them in nN (nanoNewtons). Take G = 6.674 × 10⁻¹¹ N m² kg⁻².

nN
Question 4 (Competency 5.1)foundation

How is the gravitational field strength (g) at a point in a gravitational field defined?

Question 5 (Competency 5.1)intermediate

The radius of planet Mars is 3.39 × 10⁶ m and its mass is 6.42 × 10²³ kg. Calculate the gravitational acceleration at the surface of Mars in m s⁻². Take G = 6.674 × 10⁻¹¹ N m² kg⁻².

m s⁻²
Question 6 (Competency 5.1)intermediate

At what altitude h above the Earth’s surface (radius R) is the gravitational field strength equal to g₀/4, where g₀ is the field strength at the surface?

Question 7 (Competency 5.1)intermediate

Assuming the Earth is a uniform solid sphere of radius R, how does the gravitational field strength g vary at depth d below the surface?

Question 8 (Competency 5.1)intermediate

Why is the measured value of gravitational acceleration g slightly greater at the poles than at the equator of the Earth?

Question 9 (Competency 5.1)advanced

The mass of the Earth is 81 times the mass of the Moon, and the distance between their centers is 3.84 × 10⁸ m. Find the distance from the center of the Earth to the neutral point between them (where the net gravitational field is zero) in units of 10⁸ m.

× 10⁸ m
Question 10 (Competency 5.1)intermediate

Two point masses M and 4M are separated by a distance d. Where should a third mass m be placed along the line connecting them so that the net gravitational force on m is zero?

Question 11 (Competency 5.2)foundation

Why is gravitational potential at any finite distance from an isolated mass defined to be negative (taking V = 0 at infinity)?

Question 12 (Competency 5.2)intermediate

Calculate the gravitational potential at the surface of the Earth in units of 10⁷ J kg⁻¹ (as a positive magnitude). Take Earth mass M = 5.972 × 10²⁴ kg, radius R = 6.371 × 10⁶ m, and G = 6.674 × 10⁻¹¹ N m² kg⁻².

× 10⁷ J kg⁻¹
Question 13 (Competency 5.2)intermediate

What is the relationship between gravitational field intensity g and gravitational potential V at a distance r from a point mass?

Question 14 (Competency 5.2)foundation

Which of the following statements about equipotential surfaces in a gravitational field is FALSE?

Question 15 (Competency 5.2)intermediate

A mass m is lifted from the surface of Earth (mass M, radius R) to an altitude h = R above the surface. What is the increase in its gravitational potential energy?

Question 16 (Competency 5.2)advanced

A 500 kg satellite is moved from an initial orbital radius of 7.0 × 10⁶ m to a higher orbit of radius 1.4 × 10⁷ m around the Earth (M = 5.972 × 10²⁴ kg). Calculate the change in gravitational potential energy in gigajoules (GJ). Take G = 6.674 × 10⁻¹¹ N m² kg⁻².

GJ
Question 17 (Competency 5.2)intermediate

Two masses m and 2m are held at distance 2a apart. What is the gravitational potential at the midpoint between them?

Question 18 (Competency 5.2)foundation

How much work is required to bring a 10 kg mass from infinity to a point where the gravitational potential is -40 MJ kg⁻¹?

Question 19 (Competency 5.2)advanced

A body is released from rest at a height h above Earth’s surface. Neglecting air resistance, what is its speed v upon reaching the surface (Earth radius R, surface gravity g)?

Question 20 (Competency 5.2)intermediate

A projectile is fired vertically upward from Earth’s surface with initial speed 4.0 km s⁻¹. To what maximum altitude in kilometers will it rise? Take Earth radius R = 6400 km and g = 9.80 m s⁻².

km