astrophysics dbl Flashcards

(52 cards)

1
Q

what is a universe

A

large collection of billions of galaxies

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2
Q

galaxy

A

a large collection of billions of stars

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3
Q

our solar system is in what galaxy

A

the milky way

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4
Q

what is at the centre of our solar system

A

the sun

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5
Q

gravitational field strength varies how

A

strength of gravity in different planets affects an objects weight on that planet

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6
Q

weight

A

force acting on an object due to gravitational attraction

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7
Q

fore of weight is responsible for (3)

A
  • objects staying firmly on the ground
  • objects always falling to the ground
  • satellites being kept in orbit
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8
Q

gravitational field strength depends on (2)

A

mass (greater the mass, greater the g)
distance from its centre (closer you are the stronger it is)

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9
Q

g on earth

A

10 N/Kg

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10
Q

higher gravitational field strength means

A

a larger force of attraction towards the centre of the planet or moon

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11
Q

does the mass of an object vary

A

no

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12
Q

does the weight of an object vary

A

yes depending on what planet its on, gravitational field strength

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13
Q

why does gravitational field strength vary (2)

A

as you move further away from a planet, gravity decreases

bigger mass= stronger gravity

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14
Q

smaller/larger bodies orbit smaller/larger bodies

A

smaller

larger

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15
Q

planets orbit the

A

sun

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16
Q

moons orbit the

A

planets

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17
Q

comets orbit the

A

sun

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18
Q

artificial satellites orbit the

A

earth

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18
Q

orbital motion is a result of

A

the gravitational force of attraction acting between 2 bodies.

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19
Q

asteroids orbit the

A

sun

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20
Q

gravitational force always acts in what direction

A

towards the centre of the larger body, causing smaller body to move in a circular motion

21
Q

similarities in the way different planets orbit the sun (3)

A
  • all orbit on the same plane
  • all travel in the same direction
  • orbits are all slightly eliptical
22
Q

differences in the way different planets orbit the sun (3)

A
  • orbit at different distances from the sun
  • orbit at different speeds
  • all take different amounts of time to orbit the sun
23
Q

planets closest to sun take how long and why

A

shortest amount of time as they are the fastest

24
planets furthest from the sun take how long to orbit sun and why
longest amount of time as they travel at slowest speeds
25
orbital motion of moons (3)
- orbit in circular path - some planets have more than one moon - the closer the moon to the planet, the shorter the time taken to complete and orbit and the greater the speed
26
orbital motion of comets (3)
highly eliptical as comet approaches sun, speed increases as it moves further away from the sun, its speed decreases
27
the comets orbital motion are highly eliptical, so?
speed changes significantly as their distance from the sun changes
28
do all comets orbit in the same plane
no, some don't even go in the same directions
29
what causes artificial satellites to orbit the earth
the gravity of the earth keeps them in orbit, and they're launched at high speeds and gravity bends their path into a continuous curved orbit around the sun
30
what is an orbital period
time taken for an object to perform one orbit
31
extremely hot objects emit what radiation what does this mean
visible light and infrared which means that the colour they emit depends on how hot they are
32
red star is
coolest
33
blue star is
hottest
34
colour of a star is related to its
surface temperature
35
as astronomical objects cool, they
expand
36
as astronomical objects heat, they
contract
37
when a star becomes a red giant, it does what
expands, cools and becomes redder
38
when a star becomes a white dwarf, it
contracts, heats up and gets whiter
39
life cycle of solar mass stars
stellar nebula → protostar → main sequence star - THEN EITHER STARS WITH MASS LOWER THAN SUN, OR STARS WITH MASS LARGER THAN SUN
40
nebula
a large interstellar cloud of dust and gas
41
how does a protostar form
The force of gravity within a nebula pulls the particles closer together until a hot ball of gas forms, known as a protostar As the particles are pulled closer together the density of the protostar will increase This results in more frequent collisions between the particles which causes the temperature to increase
42
how does a main sequence star form
Once the protostar becomes hot enough, nuclear fusion reactions occur within its core Once a star initiates fusion, it is known as a main-sequence star During the main sequence, the star is in equilibrium and said to be stable
43
low mass star cycle
red giant → planetary nebula → white dwarf
44
red giant forms how
After several billion years, the hydrogen causing the fusion reactions in the star will begin to run out Once this happens, the fusion reactions in the core will start to die down The star will begin to fuse helium which causes the outer part of the star to expand As the star expands, its surface cools and it becomes a red giant
45
white dwarf forms how
Once the helium fusion reactions have finished, the star collapses and becomes a white dwarf The white dwarf cools down over time and as a result, the amount of energy it emits decreases
46
larger mass cycle
red supergiant → supernova → neutron star / black hole
47
key differences between lower mass and larger mass stars
A higher mass star will stay on the main sequence for a shorter time before it becomes a red supergiant A lower mass star fuses helium into heavy elements, such as carbon, whereas a higher mass star fuses helium into even heavier elements, such as iron
48
red supergiant forms how
After several million years, the hydrogen causing the fusion reactions in the star will begin to run out Once this happens, the fusion reactions in the core will start to die down The star will begin to fuse helium which causes the outer part of the star to expand As the star expands, its surface cools and it becomes a red supergiant
49
supernova forms how
Once the fusion reactions inside the red supergiant cannot continue, the core of the star will collapse suddenly and cause a gigantic explosion called a supernova At the centre of this explosion, a dense body called a neutron star will form The outer remnants of the star are ejected into space forming new clouds of dust and gas (nebula) The heaviest elements are formed during a supernova, and these are ejected into space These nebulae may form new planetary systems
50
neutron star is formed how
forms when a massive star explodes in a supernova and its core collapses, compressing into an extremely dense ball of neutrons.
51
what happens to neutron stars
in the case of the most massive stars, the neutron star that forms at the centre will continue to collapse under the force of gravity until it forms a black hole A black hole is an extremely dense point in space that not even light can escape from