Mass of Planet Using Radius and Doppler Effect

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Homework Help Overview

The problem involves calculating the mass of a distant planet based on the observed Doppler shift of a spacecraft's radio signal while it orbits the planet at a specified radius. The context includes the use of gravitational equations and the Doppler effect in a physics setting.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to calculate the mass of the planet using the change in wavelength of the radio signal and gravitational equations. Participants raise questions about unit conversions and the values of constants used in the calculations.

Discussion Status

The discussion is ongoing, with participants providing guidance on unit conversions and the importance of using consistent measurement units. There is acknowledgment of an error in the original poster's approach regarding the units of the gravitational constant.

Contextual Notes

Participants note the need to convert kilometers to meters for accurate calculations, highlighting the importance of unit consistency in physics problems.

Linuxkid
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Homework Statement


Imagine you are observing a spacecraft moving in a circular orbit of radius 128,000 km around a distant planet. You happen to be located in the plane of the spacecraft 's orbit. You find that the spacecraft 's radio signal varies periodically in wavelength between 2.99964 m and 3.00036 m. Assuming that the radio is broadcasting normally, at a constant wavelength, what is the mass of the planet?


Homework Equations


M= \displaystyle{\frac{rv^2}{G}}; \space<br /> <br /> where \space G= 6.67\times10^{-11} \space m^3 kg^{-1} s^{-2},<br /> <br /> \space r \space is \space km, \space and \space v \ is \space<br /> km/s <br />



The Attempt at a Solution



Well, as we have a change in wavelength 2.99964 m and 3.00036 m respectively, the original signal should equal 3.00000m. With the formula from my textbook ( "Astronomy" 6th edition by Chaisson and McMillan, page 63), \frac{apparent\space \lambda}{true \space \lambda} -1 = speed \space in \space c Then I multiply it by c and convert meters to kilometers and get\approx 36 km/s.

I input r and G as G= 6.67\times10^{-11} \space m^3 kg^{-1} s^{-2}, \space r= 128, 000 km.


So: M= \displaystyle{\frac{(128000km)*(36 km/s)^2}{6.67\times 10^{-11}\space m^3 kg^{-1} s^{-2}}} = 2.48\times10^{18} kg.


When I input this answer into the website in which we do our homework by, it gives me a lousy red X. I'm sure I messed up, because I was expecting a planet approximately in the 10^20-28 kg range.


Regardless, I've been stuck on this for a bit. Help is much appreciated.





Nikos
 
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Check your units, I think you are not converting km to m.
 
possibly you are using different values for your constants, or you have rounded off differently?
[edit]ah - your value for G has length in meters.
 
Hey there,


Aha! I missed that my constant was in meters.



Honest mistake. Thanks a lot.
 

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