Need help with transfer orbit time period

In summary, the conversation is discussing the use of an elliptic transfer orbit for a trip to Mars and how to calculate the interplanetary trip duration using Kepler's third law. The conversation also mentions the need for a constant of proportionality or another known body's semi-major axis and period to accurately calculate the trip duration.
  • #1
HoboMoo
2
0
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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  • #2
How about Kepler's third law?
 
  • #3
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?
 
  • #4
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:
 
  • #5


To calculate the period of the transfer orbit, we can use Kepler's third law, which states that the square of the period (T) is proportional to the cube of the semi-major axis (a) of the orbit. This can be expressed as T^2 = (4π^2/GM)*a^3, where G is the gravitational constant and M is the combined mass of the Earth and Sun.

Plugging in the values for a and G (6.67x10^-11 m^3/kg/s^2), we can solve for T:

T^2 = (4π^2/6.67x10^-11 m^3/kg/s^2)*(190100208000 m)^3

T^2 = 5.182x10^19 s^2

T = 2.277x10^10 s

Converting this to days, we get approximately 662 days for the interplanetary trip to Mars. Of course, this is assuming a perfect alignment of the planets and a constant velocity throughout the trip. In reality, the trip may vary in duration depending on the launch window and the velocity of the spacecraft. I recommend consulting with a specialist or using more advanced simulations to get a more accurate estimate. Best of luck with your calculations!
 

1. What is a transfer orbit time period?

A transfer orbit time period is the time it takes for a spacecraft or satellite to travel from one orbit to another, typically between two different celestial bodies.

2. How is the transfer orbit time period calculated?

The transfer orbit time period is calculated using Kepler's third law, which states that the square of the orbital period is proportional to the cube of the semi-major axis of the orbit.

3. What factors affect the transfer orbit time period?

The transfer orbit time period is affected by the mass of the spacecraft, the distance between the two orbits, and the gravitational forces of the celestial bodies involved.

4. Can the transfer orbit time period be shortened?

Yes, the transfer orbit time period can be shortened by using a more powerful rocket or by taking advantage of gravitational assists from other celestial bodies.

5. How can the transfer orbit time period be optimized?

The transfer orbit time period can be optimized by carefully planning the trajectory of the spacecraft and taking into account the gravitational forces of all celestial bodies involved.

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