Astronomy: Science Unit 1

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Vocabulary flashcards defining key stellar concepts, stages of stellar evolution, magnitude types, and elements of the Hertzsprung-Russell Diagram.

Last updated 11:46 PM on 9/7/26
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15 Terms

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Apparent Magnitude

The brightness of a star as seen from Earth. A lower or negative number represents a brighter star (e.g., the Sun is 26.8-26.8 and Sirius is 1.46-1.46) and a higher number represents a dim star.

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Absolute Magnitude

The actual brightness of stars measured as if all stars were located at the exact same distance from Earth.

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Nuclear Fusion

The core process that occurs throughout a star's life where gases fuse together, doing more than just sharing electrons, giving off light and heat at different wavelengths.

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Nebula

A giant cloud of dust and gas in space from which stars are created.

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Protostar

1st step in the life cycle of a star. formed from nebula, gravity, pulls gas/dust together nuclear fusion happens than light in heat are emitted

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Main-Sequence Star

2nd step in the life cycle of a star. Fusion continues longest cycle of a star‘s life light and heat continued to be admitted where our Sun is now.

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Red Giant

3rd step of a life cycle of a star, before the low mass and high mass stars split up. Hydrogen all used up, now helium atoms start fusing together core collapses, but atmosphere spreads out as a cooler red star


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Supergiant

3rd step of a life cycle of a star, before the low mass and high mass stars split up. A massive star that forms as hydrogen depletes and burns through its fuel so quickly that it dies off relatively faster than other stars.

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Supernova

Where high mass stars go after a supergiant. A giant explosion caused by the sudden collapse of a massive star because it’s hydrogen depletes

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Neutron Star

A very dense, tiny ball of neutrons that remains after a high-mass star explodes in a supernova.

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Pulsar

A rapidly spinning neutron star that sends out pulses of radiation.

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Black Hole

The most dense object in the universe, formed when the most massive stars contract so severely that radiation and light cannot escape its massive gravity.

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White Dwarf

Where low mass stars go after red giant. A hot, glowing star remnant formed after helium is completely used up and the star shrinks; white dwarfs have less mass than giants but are denser and hotter. Does not explode, instead it fades out.

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Black Dwarf

The final remnant stage of a low-mass star that occurs when the light of a white dwarf eventually fades out.

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Hertzsprung-Russell Diagram (HR diagram)

A scatter plot showing the relationship between a star's temperature (in Kelvin, decreasing to the right) and its luminosity or absolute magnitude.