Can use the change of light frequencies to determine the speed of a star or the
rotation of a star.
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Doppler Effect with Light
6378 km
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Radius of Earth
,The velocity required to resist the gravitational pull of a body and leave it (11.2 km/s on
Earth).
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Escape Velocity
Northern hemisphere is tipped most directly away from the Sun.
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December Solstice
The process by which massive stars implode on themselves at the end of their life,
which releases all the elements the star has fused into space.
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Supernova
p^2 = a^3, where p = orbital period in years and a = average distance from Sun in AU.
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Kepler's Third Law
, Moon blocks the sunlight from the Earth; Moon's shadow falls on the Earth.
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Solar Eclipse
Amplitude of wave is orthogonal to the direction the wave travels.
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Transverse Wave
A dense, opaque object that emits thermal radiation.
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Blackbody
Fg = G(Mm)/(r^2)
f = ma
ma = G(Mm)/(r^2)
a = GM/(r^2)
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rotation of a star.
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Doppler Effect with Light
6378 km
Give this one a try later!
Radius of Earth
,The velocity required to resist the gravitational pull of a body and leave it (11.2 km/s on
Earth).
Give this one a try later!
Escape Velocity
Northern hemisphere is tipped most directly away from the Sun.
Give this one a try later!
December Solstice
The process by which massive stars implode on themselves at the end of their life,
which releases all the elements the star has fused into space.
Give this one a try later!
Supernova
p^2 = a^3, where p = orbital period in years and a = average distance from Sun in AU.
Give this one a try later!
Kepler's Third Law
, Moon blocks the sunlight from the Earth; Moon's shadow falls on the Earth.
Give this one a try later!
Solar Eclipse
Amplitude of wave is orthogonal to the direction the wave travels.
Give this one a try later!
Transverse Wave
A dense, opaque object that emits thermal radiation.
Give this one a try later!
Blackbody
Fg = G(Mm)/(r^2)
f = ma
ma = G(Mm)/(r^2)
a = GM/(r^2)
Give this one a try later!
