15
Hohmann Transfers and Plane Changes Daniel Rowe 1

Hohmann Transfers and Plane Changes

  • Upload
    borna

  • View
    92

  • Download
    0

Embed Size (px)

DESCRIPTION

Hohmann Transfers and Plane Changes. Daniel Rowe. Hohmann Transfer. In its simplest form, a Hohmann transfer is an elliptical orbit used to transfer between two circular orbits. Most energy efficient transfer technique for the majority of transfer orbit cases. Elliptical Starting Orbits. - PowerPoint PPT Presentation

Citation preview

Page 1: Hohmann Transfers and Plane Changes

Hohmann Transfers and Plane Changes

Daniel Rowe

1

Page 2: Hohmann Transfers and Plane Changes

Hohmann Transfer

• In its simplest form, a Hohmann transfer is an elliptical orbit used to transfer between two circular orbits.– Most energy efficient

transfer technique for the majority of transfer orbit cases

2

Page 3: Hohmann Transfers and Plane Changes

Elliptical Starting Orbits

• The most efficient transfer is from perigee A of orbit 1, regardless of whether B or B’ is apogee of orbit 2.

• If orbit 1 is a circle, the target point should be the apogee of orbit 2.

3

Page 4: Hohmann Transfers and Plane Changes

Bi-Elliptic Transfers

• More efficient than Hohmann transfers when transferring from a very low orbit to a very high orbit– More efficient than

Hohmann if rC/rA > 15.58– If 11.94 < rC/rA < 15.58,

the relative efficiency depends on how far out point B is.

4

Page 5: Hohmann Transfers and Plane Changes

Example: Efficiency Determination

• 300 km altitude LEO to 35,786 km GEO– rC= 300 + 6,371 = 6,673 km– rA= 35,793 + 6,371 = 42,164 km– rC/rA= 42,164/6,673 = 6.32<11.94• Hohmann transfer is more efficient

• To reach a ratio of 15.58 from a 300 km LEO altitude, one must travel to a radius of 103,965 km

5

Page 6: Hohmann Transfers and Plane Changes

Important Orbital Parameters

• For the purposes of this tutorial, the most important orbital parameter for every orbit, is Velocity

• For a circular orbit • For an elliptic orbit– Where h is the angular momentum specific to

your orbit can be solved from the formula

6

Page 7: Hohmann Transfers and Plane Changes

Important Orbital Parameters Cont

• Using the above equations, it is a simple matter to find the ΔV requirement for your entire mission– Simply find the differences between the circular

orbits’ velocities (1 and 3) and the velocity at periapsis and velocity at apoapsis of your elliptic orbit (2)

– Total ΔV is found by adding these two differences

7

Page 8: Hohmann Transfers and Plane Changes

Simple Plane Changes

• It can be shown that for a plane change accompanied by a speed change

• Without any change in speed, this reduces to

8

Page 9: Hohmann Transfers and Plane Changes

9

Page 10: Hohmann Transfers and Plane Changes

10

Page 11: Hohmann Transfers and Plane Changes

11

Page 12: Hohmann Transfers and Plane Changes

Simple Plane Changes

• It can be shown that for a plane change accompanied by a speed change

• Without any change in speed, this reduces to

12

Page 13: Hohmann Transfers and Plane Changes

13

Page 14: Hohmann Transfers and Plane Changes

14

Page 15: Hohmann Transfers and Plane Changes

References

• Curtis, Howard D. Orbital Mechanics for Engineering Students. 1st ed. Amsterdam [u.a.: Elsevier/Butterworth-Heinemann, 2006. Print.

• Tran, Peter. STK for Dummies. Jan.-Feb. 2011. Raw data. Pomona, CA.

• The Astrogator’s Guild. Web. 23 Jan. 2011. <http://www.astrogatorsguild.com/>.

• Analytical Graphics, Inc. Web. 4 Feb. 2011. <http://www.agi.com/default.aspx>.

15