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Physics Paper 3
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Red Shift
Shift of an objects wavelength towards the red end of the
spectrum
due to the object moving away from
earth.
What is red-shift evidence for?
Expansion
of the
universe
blue shift
Shift of the objects wavelength
towards
the blue end of the spectrum due to object
moving
towards the
earth.
absolute magnitude
Magnitude
of a star as it appears if placed
10
parsecs from earth
astronomical
unit
the
average distance
between the centre of the earth and the centre of the
sun
Apparent
magnitude
the
magnitude
of a
star
as it appears to an observer on the earth.
Big Bang Theory
Theory that the earth originated as a small, dense and
hot
region that expanded and cooled forming the
universe
Black body radiation
Perfect
absorber
and
emitter
of all possible
wavelengths
of light
Binary star system
Two
stars orbiting their common center of
gravity.
Black hole
Region with an
escape velocity
>
speed of light
How
are black holes formed?
1.
Mass
is so dense
neutrons
form into other neutrons. Mass tends to a singular point.
Size of star that forms a black hole
>
3
Msol
Mass of core that will form a neutron star
>
1.4
Msol
Chandrasekhar limit
the upper
limit
to the mass of a
white dwarf
(<1.4 Msol)
How
can black holes be observed?
1. Material falling into the
black
hole
2.
Stars
orbiting an
invisible
centre of mass
Charged
-Coupled device (
CCD
)
Use the photoelectric effect to
convert
light into
digital
information.
What are CCD's made of
-
Silicone chips divided
into
pixels.
-
Potential Wells (CCDs)
Electrons get trapped in potential wells causing a potential difference
identical
to the image produced.
Chromatic Aberration
Different
focal
lengths of different wavelengths of light lead to
colours
being focused at different points
Collecting
power
Measure of ability of lens/
mirror
to collect
em
radiation
Collecting power
equation
Collecting power =
Area
of
lens/mirrors
Concave/ diverging lens
Light spreads out
Convex
/
converging
lens
Light focuses
in
Doppler
Effect
Apparent change in
frequency
of a wave caused by the
relative motion
between the source of a wave and an observer
Event
horizon
Boundary of black hole where
escape velocity
=
speed of light
Exoplanet
Planets not part our
solar system
and
orbit
other starts
Eyepiece
Magnifies
the image produced by the
objective
lens
Objective
Collects light to form a
real
image
Focal
length
Distance between
centre
of lens and
principal
focus
Hipparcos
scale
Classification of objects by their apparent
magnitude
Hipparcos scale- Brightest star
1
Hipparcos scale- dullest star
6
How many times greater is a magnitude 1 star compare to a magnitude 6 star?
100
Hubbles Law
Speed of
galaxy
moving
away
from ours is proportional to distance away from us
Intensity
Power
received from a star per
unit
area
Light
year (
ly
)
Distance than an
EM
wave travels in a
year
(In a vacuum)
Long
-lived Gamma ray bursts
Bursts of gamma lasting between 10 and
100
seconds. In a type 2 supernova
Magnifying
power/ Angular Magnification
Angle made by the image from
eyepiece
: angle made by object with the unaided
eye
Normal adjestment
Distance between the object and eyepiece in a refracting telescope us = sum of
focal length
Parallax
Apparent change of
position
of a
nearer star
in comparison to distant stars in the background as a result of the earths orbit
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