Need help with transfer orbit time period

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Homework Help Overview

The discussion revolves around calculating the time period of a transfer orbit from Earth to Mars, specifically using Kepler's third law. The original poster expresses uncertainty about the formulas and approach needed to solve the problem.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the application of Kepler's third law and its implications for determining the orbital period. There is a question regarding the correct formulation of the law and how to apply it to the given semi-major axis.

Discussion Status

Some participants are exploring the relationship defined by Kepler's third law, while others are attempting calculations based on the semi-major axis provided. There is no explicit consensus on the correct approach yet, but guidance on the proportionality aspect of Kepler's law has been offered.

Contextual Notes

The original poster has provided a specific semi-major axis value but has not indicated familiarity with the necessary constants or units for applying Kepler's third law effectively. There may be assumptions about the alignment of celestial bodies that are not fully articulated.

HoboMoo
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I just don't even know where to begin. I'm not sure what formulas to use and just can't do anyhting with it. any help would be great. Thanks!

Recall that your trip to Mars is accomplished by using an elliptic transfer orbit going from Earth to Mars as shown in Fig. 1. This trajectory assumes that Earth at departure, the Sun, and Mars at arrival, are aligned. You calculated that the semi-major axis for this transfer orbit was a= 190100208000 m.

How long, in days, would the interplanetary trip last? Hint: first, determine the period of the transfer orbit.


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How about Kepler's third law?
 
So if a=190100208000m, its P^2=19010020800^3?

If that's the case, i get P^2= 6.8699 E 33 and square root that to get P?

P=8.2885 E 16?
 
Kepler's third law (in its original form) is a law of proportionality, not equality. To make it an equality you would have to use either a suitable (i.e. special) choice of units, a constant of proportionality, or form a ratio with another known pair of semi-major axis and period. So:

$$P^2 \propto T^3 $$
$$P^2 = k\;T^3$$
$$\frac{P2^2}{P1^2} = \frac{T2^3}{T1^3}$$
The last version is probably the easier to use if you happen to know of another suitable body orbiting the Sun for which you know the semi-major axis and the orbital period :wink:
 

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