Stars Flashcards

0
Q

Nebula

A

Stars form from large clouds of gas and dust in space fake nebula. This gas and dust are usually located in the spiral arms of the galaxy.

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1
Q

Life cycle

A

Nebula –> protostar –> main sequence star
High mass –> supergiant –> supernova –> neutron star or black hole (depending on mass)
Low/medium mass –> red giant –> planetary nebula –> white dwarf

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2
Q

Compressional waves

A

Occur in nebulas. These waves move across and squeeze together the gas and dust and trigger star birth. The “clouds” begin to shrink and increase in density.

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3
Q

Protostar

A

Formed when the temperature reached about 1 million degrees. The cloud begins warming due to the release of gravitational potential energy.

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4
Q

Main sequence star

A

Once temperatures reach about 10 million degrees, nuclear fusion occurs (H -> He + energy). A main sequence star has reached stellar equilibrium where there is a balance between the outward pressure due to the energy released in fusion as well as the inward pressure due to gravity

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5
Q

High mass stars

A

Highest temperatures (35000°C)
Shine blue/white
Live 10-100 million years

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6
Q

Middle mass stars

A

Mid temp (6000°C)
Shine yellow/white
Live around 10 billion years
Our sun is classified as a middle mass main sequence star

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7
Q

Low mass stars

A
Lowest temp (3500°C)
Shine red
Live longest : 100 billion - trillions of years long
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8
Q

Red giant

A

This is when the hydrogen in a star is gone and the core collapses. This heats up the core and helium begins fusing into heavier elements like carbon and oxygen.

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9
Q

Supergiants

A

Similar to red giants. These stars develop several shells of fusion which leads to heavier elements such as iron being formed in the core.

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10
Q

Planetary nebula

A

Once the helium in the core runs out the star begins to fall apart. The outer layers lift off to form a planetary nebula. A tiny white hot stellar core is left behind as a white dwarf.

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11
Q

Supernova

A

The core collapses violently when the accumulation of iron in the core eventually reaches a point where equilibrium is disturbed. The outer portion of the star explodes and produces a supernova.

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12
Q

Neutron star

A

The enormous explosion of a supernova causes protons and electrons to get packed together and form neutrons. This is known as a neutron star. Incredibly dense.

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13
Q

Black holes

A

Result of very massive stars. They have so much mass that during a supernova, gravity crushes the core to a pint of infinite density.

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