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physics - astrophysics
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avantika aradhyula
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Cards (31)
difference between the orbits of planets and comets
orbits of
planets
are
roughly
circular
orbits of
comets
are
elliptical
force that causes one object to orbit around another
gravity
solar system
The
sun
and the
planets
,
dwarf planets
and
asteroids
that
orbit
the
Sun
planet
spherical body
that
orbits
a
star
in roughly
circular orbit
, and contains
majority
of
mass
in the
orbit
life cycle of a star
larger than the Sun
nebula
protostar
main sequence
red supergiant
supernova
black hole
or
neutron star
what happens to the pitch of sound when the source moves towards the observer
it is
higher
as the
waves
are
compressed
apparent magnitude of a star
how bright it appears to be
relationship between gravitational field strength and mass of the planet
greater
the
mass
,
greater
the
gfs
directly proportional
two factors that affect how bright a star appears to be
actual brightness
and
distance
big bang theory
all matter
in the
universe
started in
one hot dense place
before an
explosion
and expansion
equation linking orbital speed, time period, and orbital radius
orbital
speed
=
2pi
x
orbital
radius
/
time period
magnitude of dimmest stars
largest positive numbers
orbital period
time taken
for
one orbit
to be
completed
what happens to pitch of sound when source moves away from an observer
it
decreases
as
waves
are
stretched
star classes (hottest to coolest)
O
(oh)
B
(be)
A(a
)
F
(fine)
G(guy
)
K
(kiss)
M
(me)
moon
natural satellite
that
orbits
a
planet
2 sources of evidence for Big Bang Theory
Red Shift
,
Universe is expanding
Cosmic Microwave Background Radiation
(
leftover radiation from the Big Bang Theory
)
range of temperatures for star (approx)
3000K
to over
33000K
red shift
increased wavelength
observed from a
star
or
galaxy
moving
away
absolute magnitude
brightness
of a star
observed
at a
standard distance
of
10 parsecs
(
32.6 light years away
)
magnitude of brightest stars
largest negative numbers
colour of hottest stars
blue
source of CBMR
energy released
in the
Big Bang
(
red shifted
)
luminosity
actual brightness
of star, measure of
energy emitted every second
change in wavelength=
velocity of galaxy
/
speed of light
y axis of a Hertzsprung-Russel diagram
increasing luminosity
galaxy
group of billions of stars
doppler effect
apparent change
in
frequency
of a
wave
due to the
source
moving
relative
to the
observer
life cycle of a star the same size as the Sun
nebula
,
protostar
,
main sequence
,
red giant
,
white dwarf
x axis of Hertzsprung- Russel diagram
decreasing temperature
colour of coolest stars
red