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Created by
Holly Attwell
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Cards (18)
Luminosity - the
rate
of
light
energy
released
or
power
output
of a
star
Intensity - the
power
received
from a
star
per
unit
area
Parallax - the apparent
change
of
position
of a
nearer
star
in
comparison
to
distant
stars
Parsec - the
distance
when the
parallax
angle
is
1
arcsecond
Parallax method only works when the distance is
less
than
100
light
years.
Standard candle - an object with a
known
luminosity.
Astronomical distances can be determined by measuring the
intensity.
Life cycle of a star
Nebula
Protostar
Main
sequence
Small
Red
giant
White
dwarf
Big
Red
supergiant
Supernova
Neutron
star
or black
hole
/
singularity
Protostar -
dust
and
gas
collect
due
to
gravity
Main sequence star
gravity
and
fusion
are in
equilibrium
hydrogen
nuclei
are
fused
into
helium
Red giant
hydrogen
runs
out
helium
is
fused
into
heavier
elements
White dwarf
fusion
stops
when the star
runs
out
of
fuel
gravity
is
greater
than
outwards
force
, so the
star
collapses
Red supergiant
hydrogen
runs
out
helium
is
fused
into
heavier
elements
Supernova
fusion
stops
when the star
runs
out
of
fuel
core
collapses
inwards
suddelny
elements
heavier
than
iron
are
fused
Neutron star
gravity
forces
protons
and
electrons
into
neutrons
Main sequence star on HR diagram
begins as a
protostar
heats
up
, moving
left
becomes
main
sequence
star
runs out of
hydrogen
, moves
up
and
right
becomes
red
giant
runs out of
helium
, moves
down
and
left
becomes
white
dwarf
z =
red
shift
lambda =
original
wavelength
f =
original
frequency
v =
receding
velocity
Hubbles constant - rate of
expansion
of the
universe
Controversy over the age and fate of the universe
difficulty
making
accurate
measurements
of
distances
to
galaxies
hubble’s
constant
has a
large
uncertainty
existence
of
dark
matter
dark
energy
may
mean
we don’t
understand
gravity
as we think