If the earth had low density rings around it, but the mass of
these rings plus the mass of the earth with those rings equaled the
present mass of the earth without rings:
1>How would this affect the length of the year?
2>How would this affect the length of the month?
This sounds as though it's a trick question. Let E=mass of Earth
without rings, and R=mass of rings. Then we are given
"the mass of these rings plus the mass of the earth with those
rings equaled the present mass of the earth without rings"
R+(E+R)=E
subtracting E from both sides
2R=0
so R=0. So, with this in mind the answer to 1 would be: it
wouldn't. Can you guess the answer to number 2?
I'm not sure how hard the problem is supposed to be, and if this
problem was for a class doing gravitational physics or something,
I'm pretty sure I've not understood a point...
Brad
I think she was wondering if the different distribution of mass
would make a difference i.e. would it matter if the Earth's mass
was more spread out?
The answer is no. We can treat bodies (like the Earth) as if they
were point masses, with all their mass concentrated at their centre
of mass. Although they obviously aren't, the maths still works, so
if the rings were even (even thickness and material) then the
Earth's centre of mass would be the same as in the real situation,
and so the maths would give the same result. Obviously their is no
atmosphere in space, so the rings wouldn't cause any sort of 'air
resistance'.
Depending on how deep you want to take the problem, I'm not sure
how rings would have affected the Earth's route during the
formation of the solar system. I don't know much about
astrophysics, but I believe the system was a big cloud of gas at
that point, so a sort of 'air' resistance might have occured
(?)
Also, forgeting about be the system's formation, I don't actually
think an increase in mass would affect the path anyway. Circular
motion equations don't depend on mass, (you might understand this:
a = v2/r = GM/r2, where M is the mass of the
sun), so I doubt elliptical paths would.
If I have misunderstood what you are asking please post back.
Jim
By kepler's third law,
T2 proportional to r3
T = time period of earth
r = radius of orbit of earth with sun as center
In your problem,
since r remains unchanged,T will remain unchanged which i suppose
answers your question.
love arun
please do correct me if i missed anything...
What Arun and I have answered (assuming this question isn't a
trick one) is really question 1). For 2), assuming "month" means
lunar month (i.e. time for moon to orbit the earth) if the moon
orbits outside of the rings our answers still hold.
BUT: if the moon's orbit is lower than the rings or in between the
rings then the length of the month will change. I will explain why
if anyone wants.
Jim
No trick question, just the distribution of mass, as Jim
stated.
Is there a particular mass for the earth and moon that would make
the lunar month and solar year coincide in a simpler ratio?
Wouldn't increased tidal forces have a small (probably negligible) effect on the orbits?
In my last post when I said "...the length of the moon will
change" I was of course referring to the length of the moon's
orbit.
To answer Tobiah's most recent post, I believe the answer is...
yes. Ok, so you want a more detailed answer. Well, you would have
to start worrying about Netwon's Law of Gravitation (
F=Gm1m2/r2) and the equations of
bodies moving in an ellipse. I have studied circular motion but not
elliptical, so I get a bit stuck here (though I could always model
the motion as circular).
Tom, you're probably right. I don't know.
Jim