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Stars and Star Clusters
Rating: 4.3 out of 5(7 ratings)
44 students

Stars and Star Clusters

Stars as the building blocks of the unvierse
Created byTony Ceraso
Last updated 1/2026
English

What you'll learn

  • Stars are the workhorses of the universe and account for most of its mass. They come in many shapes and sizes, some as small as just a few miles across and others that are as large as much of our solar system. Some are hundreds of times hotter than the Sun and others are just a few thousand degrees. When stars start running out of fuel they do some crazy things like explode into supernovae or implode into tightly packed white dwarfs or black holes.
  • How many stars are in the sky and how far are they?
  • Stars as the building blocks of the universe
  • Luminosity and Magnetude
  • Absolute magnitude
  • Aparent Magnitude
  • Magnitude Scale
  • The Steller Main Sequence
  • T Tauri Stars
  • Red Giant Stars
  • Blue Giant Stars
  • White Dwarfs
  • Neutron stars
  • Pulsars - Lighthouses of the Universe
  • Red and brown dwarfs, and other sub-stellar objects
  • Stars and nuclear fusion
  • What is a star?
  • The Sun: temperature, features, characteristics and atmospheres
  • Star Size, Mass and Density
  • Star clustering and gravity
  • Open and Closed Star Clusters
  • Galactic and Globular Star Clusters
  • Prisms and the Range of Light
  • Red and Blue Shifts in the Spectrum and what they mean
  • The Doppler Effect
  • Variable Stars: pulsating, intrinsic, extrinsic and cataclylsmic
  • Cepheid variable stars and the calculations of distances
  • Multiple star systems: binary and trinary stars
  • Types of Steller Orbits
  • Supernovae: causes and effects
  • Black Holes
  • Test Questions and Activities

Course content

10 sections10 lectures2h 15m total length
  • Introduction: Pacing, Warm-up, Objective1:52

Requirements

  • None

Description

Stars are the workhorses of the universe and account for most of its mass. They come in many shapes and sizes, some as small as just a few miles across and others that are as large as much of our solar system. Some are hundreds of times hotter than the Sun and others are just a few thousand degrees. When stars start running out of fuel they do some crazy things like explode into supernovae or implode into tightly packed white dwarfs or black holes.

This Course includes the following great BONUS LESSONS:

  • What on Earth is Astronomy?

  • Mini-Lesson: Eclipses

  • Mini-Lesson: Meteor Showers

  • Mini-Lesson: Aurora

  • Project Artemis: America Returns to the Moon

Stars and Star Clusters

1. Objective

2. Warm-up activity

3. Stars in our sky: number and distance

4. Stars as related to the entire Universe: scope and function

5. Luminosity and magnitude

6. Absolute magnitude and apparent magnitude

7. Magnitude scale

8. The main sequence of stars

9. T Tauri stars

10. Red giant stars

11. Blue giant stars

12. White dwarf stars

13. Neutron stars

14. Pulsars

15. Red and brown dwarfs, and sub-stellar objects

16. Nuclear fusion

17. Definition of a star

18. The Sun: temperature, features, characteristics and atmospheres

19. Star size, mass and density

20. Star clustering and gravity

21. Open and closed star clusters

22. Galactic and globular star clusters

23. Prisms and the range of light

24. Red and blue shifts in the spectrum

25. The Doppler effect

26. Variable stars: pulsating, intrinsic, extrinsic and cataclysmic

27. Cepheid variable stars and distance calculations

28. Multiple star systems: binary and trinary stars

29. Types of orbits

30. Supernovae: cause and effect

31. Black holes

32. Test questions

33. Cross-curricular activities

Who this course is for:

  • Anyone who want to know more about Astronomy