Astrophysics Flashcards

(11 cards)

1
Q

Define the universe

A

a large collection of billions of galaxies

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2
Q

Define a galaxy

A

a large collection of billions of stars

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3
Q

what is a solar system

A

a collection of planets orbiting a common star

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4
Q

where is our solar system

A

in the milky way galaxy

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5
Q

Why does gravitational field strength vary

A

• it varies with the mass and size of the body
• it is different on other planets and the moon compared to earth

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6
Q

What does gravitational force cause

A

• causes moons to orbit planets
• causes planets to orbit sun
• causes artificial satellites to orbit earth
• causes comets to orbit sun (highly elliptical)

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7
Q

Describe the differences in the orbits of comets, moons and planets

A

• comets = highly elliptical
• moons = slightly elliptical, near constant orbital speed
• planets = slightly elliptical, near constant orbital speed

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8
Q

what is a stars colour related to

A

• The colour of star = surface temperature
• hotter stars = blue
• cooler stars = red

blue hottest
white ^
yellow l
Orange l
red coolest

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9
Q

how can stars be classified

A

• by their colours
• colour depends on how much light they emit

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10
Q

describe evolution of a star of similar mass to the sun

A

nebula - stars form form from a cloud of dust and gas

protostar - force of gravity pulls dust and gas closer together to form protostar. The density increases. More frequent collisions. Temperature increases.

Main sequence star - once protostar is not enough, nuclear fusion reactions happen in core. The star is in equilibrium and stable

Red giant - eventually hydrogen in core begins to run out. Star begins to fuse with helium, causes outer part of star to expand. As star expands, surface cools and becomes red giant

White dwarf - a small to medium sized star like the sun becomes unstable and ejects it’s outer layers of dust and gas. This leaves a hot dense solid core, a white dwarf

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11
Q

Describe evolution of star with a mass larger than sun

A

nebula - stars form form from a cloud of dust and gas

protostar - force of gravity pulls dust and gas closer together to form protostar. The density increases. More frequent collisions. Temperature increases.

Main sequence star - once protostar is not enough, nuclear fusion reactions happen in core. The star is in equilibrium and stable

red supergiant - eventually hydrogen in core begins to run out. This causes outer part to expand and become a red supergiant

Supernova - once fusion reactions finally stop, the core of star collapses suddenly and causes gigantic explosion called supernova

neutron star - at the centre of this explosion, a dense body called a neutrons star will form

Black hole - neutron star will collapse continuously under force of gravity until it forms a black hole

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