Stellar Evolution Stellar Birth Stages of a Star Death of a Star The Hertzsprung-Russell Diagram
100
What is Stellar Evolution?
The process by which a star changed over the course of time.
100
What is a supernova?
The main trigger of star formation is a shock wave from a catastrophic explosion of a nearby star known as this
100
What is the protostar stage?
During this stage, gravitational contraction continues and this collapse causes the core of the developing star to heat much faster than its outer envelope
100
What is 1/2?
Low mass stars less than this fraction of the mass of the sun consume their fuel at relatively low rates
100
Who are Ejnar Hertzsprung and Henry Russell?
These two astronomers created the diagram
200
What are first generation stars?
Early stars that are massive; they often had short lifetimes
200
What is thermal energy?
Once the cloud collapses, potential energy turns into this type of energy
200
What is the Main-Sequence Stage?
During this stage, stars experience minimal changes in size or energy output
200
What are Massive Stars?
This type of star exceeds 8 solar masses and have relatively short life spans and terminate in brilliant explosions called supernovas

200
What is the temperature of a star?
The diagram can be used to learn about the relationships among sizes, colors, and this
300
What is the Hertzsprung-Russell Diagram?
The diagram that displays stellar evolution
300
What are interstellar clouds?
The birthplace of stars are in this type of cloud
300
What is a Main-Sequence Star?
The average star spends 90 percent of its life at this star stage
300
What is a planetary nebula?
Medium-mass stars collapse from red giants to white dwarfs then to this
300
What is its luminosity?
Each star is plotted based on its temperature and this
400
What is the Big Bang?
The first star is estimated to have formed 300 million years after this theory
400
What are protostars?
Red objects that are no hot enough to engage in nuclear fusion, they are not yet stars.
400
What is the Red Giant Stage?
the evolution of this stage begins when the usable hydrogen in the star’s interior is consumed, the core then collapses on itself and the internal temperature rises, which causes the star to expand
400
What are Medium-mass stars?
These stars are sun-like
400
What are main-sequence stars?
These stars appear in decreasing order, from hotter, more massive blue stars to cooler, less massive red stars
500
What are Hydrogen and Helium?
First generation stars are made up of these two elements
500
What is long-wavelength red light?
When the temperature of these gaseous bodies increases sufficiently they begin to radiate energy in the form of this
500
What are supergiants?
The most massive stars become this
500
What are white dwarfs?
Low-mass stars remain stable main-sequence stars until they consume their usable hydrogen energy fuel and collapse into hot, dense these
500
What is the 20th century?
The diagram was created in this century






Classification of Stars

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