Stars Flashcards

1
Q

What is a meteroits

A

Bits of asteroid or bits of rock which make it through the journey of the earths atmosphere and the to the surface

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2
Q

Define a planet

A

An object with sufficient mass for their own gravity force to make them a spherical shape where no nuclear fusions occur and the object has cleared its orbit of other objects

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3
Q

What is a dwarf planet

A

Planets where the orbit has not been cleared of other objects

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4
Q

what are asteroids

A

objects which are too small or too uneven in shape to be planets with a near circular orbit around the sun

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5
Q

what are comets

A

small irregularly sized balls of rock,dust and ice

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6
Q

give the timeline for the evolution of a low mass star and give the size

A

Nebula, protostar, Main sequence star, Red giant, white dwarf, black dwarf
from 0.5- 10 solar masses

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7
Q

give the timeline for the evolution of high mass stars

A

Nebula, protostar, Main sequence, Red super Giant, supernova, Neutron star, black hole

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8
Q

what is nebula

A

gigantic clouds of dust and gas, over millions of years the gravitational attraction between the particles pulls them together to form clouds. As they come closer together the gravitational collapse accelerates and some regions become denser and pull in even more dust and gas. this energy is then converted to thermal energy

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9
Q

what happens after the gravitational energy converts into thermal energy in the nebula

A

a protostar is formed,

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10
Q

what is required in the protostar for a star to e formed

A

the temp and pressure must be high enough for the hydrogen nuclei in the protostar to overcome the electrostatic forces of repulsion and undergo nuclear fusion, producing helium producing a star

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11
Q

what happens in the main sequence star phase how is this stage different in larger stars

A

the star is in a stable equillibrium where the gravitational forces of the particles act to compress the star but are counteracted by the radiation pressure from the photons emitted in fusion and gas pressure from the nuclei
in larger stars they are hotter therfore this stage is shorter as they undergo faster fusion

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12
Q

what is the solar mass equal to

A

= 1.99 x 10^30 kg

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13
Q

explain what happens after the main stage of a low mass star

A

once the hydrogen supply is low the gravitational forces inwards overcome the radiation and gas pressures so the star collapses inwards and evolve into a red giant (cooler ) the core of the red giant is too cool for fusion to occur, but the pressure in the outer layers is great enough for fusion to occur.

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14
Q

what happens after the red giant phase for a low mass star

A

fusion occurs in the outer layers but not in the core, so the giant evolve into a hotter white dwarf as the outer shells drift off as planetary nebula , the core remains dense which has a very high temp

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15
Q

what happens in the white dwarf in low mass stars

A

the photons which were produced leak out dissipating heat and the core starts collapsing however electron degeneracy prevents the core from collapsing completely. and as long as the mass of the core is less than 1.44 solar masses the white dwarf is stable

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16
Q

what is electron degeneracy

A

where 2 electrons can not exist in the same state

17
Q

what happens after the amin stage for a high mass star

A

stars which are larger than 10 solar masses, after the main phase will have a high enough temp for helium fusion into heavier elements producing elements upto iron

18
Q

why does fusion only happen upto iron in high mass stars after main stage

A

iron does not release energy therfore can not fuse further

19
Q

what happens after iron is prod high mass star

A

the star becomes unstable and a type2 supernova occurs where there is a shockwave which ejects materials into outer space and the core collapses however elements hevier than iron can be formed in supernovas

20
Q

what happens after the supernova
high mass stars

A

if the remaining core mass is larger than 1.44 solar masses protons and electrons combine to become neutrons producing an extremely small neutron star and if the remaining mass is more than 3 solar masses it will become a black hole where light can not escape

21
Q
A