Asked by Annoyingmous
The average energy flux in the sunlight on the Earth is ⟨S⟩=1.4×103 W/m2. You might need to use some of the following constants:
Distance from earth to the sun=AU=150×109m
REarth=6.4×106m
RSun=7.0×108m
G=6.67×10−11m3/(kgs2)
MEarth=5.97219×1024kg
MSun=1.9891×1030kg
(a) What force (in N) does the pressure of light exert on the Earth? Assume that all the light striking the Earth is absorbed.
(b) What is the gravitational force (in N) that the Sun exerts on the Earth? (Think about how that compares to the force due to the pressure of light. Does your answer make sense?)
Distance from earth to the sun=AU=150×109m
REarth=6.4×106m
RSun=7.0×108m
G=6.67×10−11m3/(kgs2)
MEarth=5.97219×1024kg
MSun=1.9891×1030kg
(a) What force (in N) does the pressure of light exert on the Earth? Assume that all the light striking the Earth is absorbed.
(b) What is the gravitational force (in N) that the Sun exerts on the Earth? (Think about how that compares to the force due to the pressure of light. Does your answer make sense?)
Answers
Answered by
bobpursley
Check units: W/m^2 = Js^(-1) m^(-2)
J= N m =>W/m^2= Js^(-1)m^(-2)=Nm^(-1)s^(-1)
so W/m^2/(m/s) = Nm^(-1)s^(-1)/ms^(-1) = Nm^(-2) = pressure
so we have verified that the units of intensity/speed of light = units of radiation pressure
therefore, the force of radiation acting on the earth is:
force = radiation pressure x area = (intensity/c)xpi R^2
force = 1400W/m^2 x pi x( 6.37x10^6m)^2/3x10^8m/s
force = you do it.
I am presuming that the sun's gravitational attraction means the magnitude of the solar gravitational force on earth: If that's the case, the answer is approx 10^22 N:
F=GMm/r^2
G=6.67x10^(-11)=6.67e-11
M=mass sun = 2x10^30kg=2e30
m=mass earth = 6x10^24kg
r=earth sun distance = 1.5x10^11m
F=(6.6e-11)(2e30)(6e24)/(1.5e11)^2 = 3.56e22N
J= N m =>W/m^2= Js^(-1)m^(-2)=Nm^(-1)s^(-1)
so W/m^2/(m/s) = Nm^(-1)s^(-1)/ms^(-1) = Nm^(-2) = pressure
so we have verified that the units of intensity/speed of light = units of radiation pressure
therefore, the force of radiation acting on the earth is:
force = radiation pressure x area = (intensity/c)xpi R^2
force = 1400W/m^2 x pi x( 6.37x10^6m)^2/3x10^8m/s
force = you do it.
I am presuming that the sun's gravitational attraction means the magnitude of the solar gravitational force on earth: If that's the case, the answer is approx 10^22 N:
F=GMm/r^2
G=6.67x10^(-11)=6.67e-11
M=mass sun = 2x10^30kg=2e30
m=mass earth = 6x10^24kg
r=earth sun distance = 1.5x10^11m
F=(6.6e-11)(2e30)(6e24)/(1.5e11)^2 = 3.56e22N
Answered by
FLu
Thanks bobpursley!
The first problem does not give right answer, could you tell, if this is the right calculation as 10^22 and the formula was not right.
1400/6x10^24*pi*(6.37*10^6)^2/3*10^8
Is this formula above right?
The first problem does not give right answer, could you tell, if this is the right calculation as 10^22 and the formula was not right.
1400/6x10^24*pi*(6.37*10^6)^2/3*10^8
Is this formula above right?
Answered by
hmmmm
ist part ans is 5.823e8
Answered by
FLu
Thanks hmmmmm for help!
Answered by
Anonymous
Pls other questions, 1, 2, 4?
Answered by
hmmmm
B=(meu not*N*I)/((2*pi*R/km) +d)
Answered by
hmmmm
this was for question 4
Answered by
ggggg
what is meu not?
Answered by
Anonymous
the correct ans is:
B=(mu_0*N*I)/((2*pi*R/km) +d)
B=(mu_0*N*I)/((2*pi*R/km) +d)
Answered by
Anonymous
¿Problems 1, 2 & 5?
Answered by
ggggg
how to count 3b (Bo) and 3c (Poynting vector)?
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