unit 1 Flashcards

1
Q

what is necessary to keep an object in circular motion

A

centripetal force

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2
Q

what causes a change in the angular (rotational)
motion of an object.

A

an unbalanced torque

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3
Q

whats the moment of inertia of an object

A

a measure of its resistance to angular
acceleration about a given axis.

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4
Q

what does the moment of inertia depend on

A

mass and the distribution of mass about
a given axis of rotation.

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5
Q

whats conversation of momentum

A

the momentum before equals the momentum after a collision in the absence of external torques

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6
Q

whats gravitational field strength

A

as the gravitational force acting on a unit mass

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7
Q

whats gravitational potentail of a point in space

A

the work done in moving
unit mass from infinity to that point.

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8
Q

whats escape velocity

A

as the minimum velocity required to allow a mass to
escape a gravitational field to infinity, where the mass achieves zero kinetic energy and
maximum (zero) potential energy.

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9
Q

inertial?

A

non-accelerating

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10
Q

whats the equivalence principle

A

it is not possible to distinguish between the
effects on an observer of a uniform gravitational field and of a constant acceleration

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11
Q

whats spacetime

A

a unified representation of three dimensions of space
and one dimension of time.

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12
Q

general relativity leads to the interpretation that

A

mass curves
spacetime, and that gravity arises from the curvature of spacetime.

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13
Q

whats geodesic

A

the path with the
shortest distance between two points

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14
Q

escape velocity from the event horizon of a black hole is equal to

A

speed of light

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15
Q

from the perspective of a distant observer, time appears to be frozen
at

A

the event horizion of a black hole

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16
Q

whats schwarzchild radius

A

is the distance from its centre
(singularity) to its event horizon.

17
Q

how are stars formed

A

stars are formed in interstellar clouds when gravitational forces
overcome thermal pressure and cause a molecular cloud to contract until the core
becomes hot enough to sustain nuclear fusion, which then provides a thermal pressure
that balances the gravitational force

18
Q

give an exmaple of propton-protn chain

A
19
Q

what are the classifications of h-r diagrams

A

main sequence, giant, supergiant and white dwarf

20
Q

where does fusion of hydrogen occurs in the core of stars

A

main sequence

21
Q

what happens at the end of a stars life

A

. When the
hydrogen in the core becomes depleted, nuclear fusion in the core ceases. The gas
surrounding the core, however, will still contain hydrogen. Gravitational forces cause both
the core, and the surrounding shell of hydrogen to shrink. In a star like the Sun, the
hydrogen shell becomes hot enough for hydrogen fusion in the shell of the star. This leads
to an increase in pressure which pushes the surface of the star outwards, causing it to
cool. At this stage, the star will be in the giant or supergiant regions of a HertzspungRussell (H-R) diagram.

22
Q

what determines a stars lifetime

A

mass

23
Q

what will every star eventually become

A

a white dwarf, a neutron star or a black
hole.

24
Q

what will happen to the sun

A

the core shrinks and will become hot enough for the
helium in the core to begin fusion.