Optimizing Orbital Trajectories for Efficient Mars Encounter

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The discussion revolves around optimizing orbital trajectories for a space probe to efficiently encounter Mars from a 1 AU circular orbit around the sun. Participants explore the implications of changing the probe's velocity in a radial direction and its effect on reaching Mars.

Discussion Character

  • Exploratory, Assumption checking, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the nature of the velocity change intended for a Hohmann transfer orbit and question whether a radial change would allow the probe to reach Mars. There are inquiries about calculating the semi-major axis based on the new velocity and radius.

Discussion Status

Some participants have provided insights into the mechanics of orbital transfers and the calculations involved in determining the semi-major axis. There is an ongoing exploration of the implications of the velocity change on the probe's trajectory.

Contextual Notes

Participants are working under the assumption that the velocity change was made in a radial direction, which raises questions about the energy expenditure and trajectory feasibility. The discussion includes references to specific velocities and mechanical energy calculations.

olyviab
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A space probe initially moving in a 1 AU circular orbit around the sun (i.e. moving with the earth). The aim is to put this space probe in an orbit that will encounter Mars, using the least possible expenditure of rocket fuel (energy). This orbit, it turns out, is one in which perihelion (closest approach to the sun) is at the Earth's orbit (r=1AU), and aphelion (furthest approach from the sun) is at Mars' orbit.Suppose that the rockets had fired so that the change in velocity was in the radial direction (outwards). Calculate a (semi major axis) Will this orbit ever reach Mars?
 
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olyviab said:
A space probe initially moving in a 1 AU circular orbit around the sun (i.e. moving with the earth). The aim is to put this space probe in an orbit that will encounter Mars, using the least possible expenditure of rocket fuel (energy). This orbit, it turns out, is one in which perihelion (closest approach to the sun) is at the Earth's orbit (r=1AU), and aphelion (furthest approach from the sun) is at Mars' orbit.


Suppose that the rockets had fired so that the change in velocity was in the radial direction (outwards). Calculate a (semi major axis) Will this orbit ever reach Mars?

Do you mean that the original velocity change intended for the Hohmann orbit injection was mistakenly made in a radial direction? If so, then no, the orbit would not reach Mars. The Hohmann transfer is the least energy direct transfer orbit. If it's not the Hohmann orbit, then it can't reach Mars with the same energy expenditure.
 
gneill said:
Do you mean that the original velocity change intended for the Hohmann orbit injection was mistakenly made in a radial direction? If so, then no, the orbit would not reach Mars. The Hohmann transfer is the least energy direct transfer orbit. If it's not the Hohmann orbit, then it can't reach Mars with the same energy expenditure.

Yeah i assume it was the least energy in the Hohmann orbit directed outwards. I understand if its the 3 km/s (i calculated that number as being the least v) being directed outward that it won't reach the Mars orbit. How am i able to calculate the semi-major axis?
 
olyviab said:
Yeah i assume it was the least energy in the Hohmann orbit directed outwards. I understand if its the 3 km/s (i calculated that number as being the least v) being directed outward that it won't reach the Mars orbit. How am i able to calculate the semi-major axis?

If you have the new velocity (after the ∆V) and the radius, then you can calculate the total mechanical energy, ξ. Then 2a = -µ/ξ.
 
gneill said:
If you have the new velocity (after the ∆V) and the radius, then you can calculate the total mechanical energy, ξ. Then 2a = -µ/ξ.

Great! Thanks for all the help :)
 

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