Revolving Around a Star: Calculating an Orbital Period

[danago]

A star has a mass approximately 100 times that of our sun. If a planet with the same mass as the Earth is oribiting at a radius similar to that of the Earth's radius around the sun, how long would it take the planet to revolve around the star once?

Ok, the period of the Earth's rotation is given by:
[tex]
T_e = \sqrt {\frac{{4\pi ^2 r^3 }}{{Gm_e}}}
[/tex]

If the radius remains the same, and the mass increases by a factor of 100, the period in comparison to the Earth's period is given by:

[tex]
T_p = \frac{1}{{10}}\sqrt {\frac{{4\pi ^2 r^3 }}{{Gm_e}}}
[/tex]

Comparing these two, we see that [tex]T_p = \frac{1}{{10}}T_e [/tex]

If the period of the Earth's revolution around the sun is 1 year i.e. 365 days, then the period of the other planet is one tenth of that i.e. 36.5 days.

It was an exam question and that was my working, and i got no marks for it. Where have i gone wrong?

Thanks,
Dan.

 

[learningphysics]

Looks right to me... only thing that maybe could be seen as a mistake is that you used "me"... with the subscript e... giving the impression that you might mean mass of the earth... instead of mass of the sun.

But your answer looks right... I'd talk to the prof and ask him...

 

[danago]

Ooops didnt mean to write m_e, i didnt even use any subscript in my exam, just used m. Well i thought that might be the case, because i was pretty confident with that question. Thanks for clearing it up

 

[pavadrin]

well i think that your physics teacher should be shot, that working is perfect, and ordered in a logical manner, find out where he lives and go right now to get the marks you deserve.