Stars and Planets Flashcards

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1
Q

What kind of planets are the planets in our solar system?

A

The closest 4 to the sun are rocky, and the furthest 4 from the sun are gaseous

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2
Q

What units of distance are used in space?

A
  • astronomical unit: the mean distance from the centre of the Earth to the centre of the sun is 1 AU
  • light year: the distance that light travels in a year is 1 light year
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3
Q

What is an asteroid?

A

A lump of rock which orbits the sun. The asteroid belt is between Mars and Jupiter

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4
Q

What is a comet?

A

Lumps of ice and dust that are in a highly elliptical orbit around the sun

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5
Q

What is the life cycle of a low mass star?

A

Gravitational collapse of a nebula forms a protostar. If it’s mass is below 8SM, it becomes a yellow, average mass main sequence star. As the star begins running out of hydrogen, it becomes a red giant. It then becomes a planetary nebula and it’s outer layers expand towards space. Finally, it becomes a white dwarf.

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6
Q

What is the life cycle of a high mass star?

A

Gravitational collapse of a nebula forms a protostar. If it’s mass is above 8SM, it becomes a blue, massive main sequence star. As the star begins running out of hydrogen, it becomes a red supergiant. It then explodes into a supernova, and elements heavier than lead are formed. Stars greater than 25SM will become blackholes, and stars above 8SM but below 25SM will become neutron stars.

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7
Q

What is a brown dwarf?

A

A failed star that never had enough mass to get hot enough to achieve nuclear fusion

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8
Q

What is a red dwarf?

A

Low mass stars that do achieve nuclear fusion. They are main sequence stars

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9
Q

What forces act inside a star?

A

Gravity acts inwards, and gas and radiation pressure act outwards

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10
Q

What happens when an imbalance of pressure occurs within a star?

A

If pressure in the middle falls, it will shrink, and if pressure in the middle increases, it’s size will increase

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11
Q

What does a Hertzsprung-Russel diagram depict?

A

Stars according to their temperature and brightness

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