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Big Bang
The origin of the universe.
Black Hole
An object that has gravity so strong that light can not even escape it. Black holes form when massive stars collapse at the end of their lives
Galaxy
A group of millions or billions of stars held together by gravity.
Large Star
A star with more than 8 times the mass of the sun.
Light - Year
the distance light travels in a year
Main Sequence Star
A main sequence star is a star in the most stable and longest phase of its life. It is currently fusing hydrogen into helium in its core.
Neubla
a vast cloud of dust and gas in space
Neutron Star
The remains of the core of a large star. It has many neutrons densley packed in.
Nucelar Fusion
a nuclear reaction in which two atomic nuclei join together
Nuclear Reaction
A reaction in which an atom’s nucleus changes.
Planetary Nebula
a nebula formed from a red giant star
Prostar
a dense ball of gas that has not formed into a star yet.
Red Giant
a small star that fuses helium causing its outer layer to expand
Red Supergiant
a large star that fuses helium causing its outer layer to expand
redshift
the stretching of light waves emitted by objects moving away from us.
Star
hot ball of gas held together by gravity
supernova
an explosion of a red supergiant star
white dawrf
the remains of the core of a white star
Doppler Effect
The change in the way you hear a noise as it moves toward or away from you
How does the Doppler Effect cause red and blue shift
If a star is moving away from us, its light appears redshifted (shifted towards the red end of the spectrum, with longer wavelengths), and if it's moving towards us, its light appears blueshifted (shifted towards the blue end, with shorter wavelengths)
Life cycle of a normal star
Nebula
ProStar
Main Sequence Star
Red Giant
Planetary Nebula
White Dwarf
Life cycle for massive stars
Nebula
ProStar
Main Sequence Star
Red Supergiant
Supernova
Neutron Star or Black Hole
Using Light Colour and Brightness to Identify Star Properties
Blue/White Stars: Hottest stars
Yellow Stars: Intermediate stars like the sun
Orange/Red Stars: Cooler stars
What do Hertzsprung-Russel diagrams show
It plots stars based on their brightness and temperature