In astrodynamics, orbit phasing is the adjustment of the time-position of spacecraft along its orbit, usually described as adjusting the orbiting spacecraft's true anomaly.[1] Orbital phasing is primarily used in scenarios where a spacecraft in a given orbit must be moved to a different location within the same orbit. The change in position within the orbit is usually defined as the phase angle, ϕ, and is the change in true anomaly required between the spacecraft's current position to the final position.

The phase angle can be converted in terms of time using Kepler's Equation:[2]

\( t=\frac{T_1}{2 \pi} (E-e_1 \sin E) \)

\( E=2 \arctan (\sqrt{\frac{1-e_1}{1+e_1}} \tan{\frac{\phi}{2}}) \)

where

*t*is defined as time elapsed to cover phase angle in original orbit*T*is defined as period of original orbit_{1}*E*is defined as change of Eccentric anomaly between spacecraft and final position*e*is defined as Orbital eccentricity of original orbit_{1}*Φ*is defined as change in true anomaly between spacecraft and final position

Phase Orbit

If spacecraft is behind the final position on the same orbit, the spacecraft must slow down to enter a smaller, faster phasing orbit to catch up to final position.

This time derived from the phase angle is the required time the spacecraft must gain or lose to be located at the final position within the orbit. To gain or lose this time, the spacecraft must be subjected to a simple two-impulse Hohmann transfer which takes the spacecraft away from, and then back to, its original orbit. The first impulse to change the spacecraft's orbit is performed at a specific point in the original orbit (point of impulse, POI), usually performed in the original orbit's periapsis or apoapsis. The impulse creates a new orbit called the “phasing orbit” and is larger or smaller than the original orbit resulting in a different period time than the original orbit. The difference in period time between the original and phasing orbits will be equal to the time converted from the phase angle. Once one period of the phasing orbit is complete, the spacecraft will return to the POI and the spacecraft will once again be subjected to a second impulse, equal and opposite to the first impulse, to return it to the original orbit. When complete, the spacecraft will be in the targeted final position within the original obit.

To find some of the phasing orbital parameters, first one must find the required period time of the phasing orbit using the following equation.

\( T_2=T_1-t \)

where

*T*is defined as period of original orbit_{1}*T*is defined as period of phasing orbit_{2}*t*is defined as time elapsed to cover phase angle in original orbit

Once phasing orbit period is determined, the phasing orbit semimajor axis can be derived from the period formula:[3]

\( a_2= (\frac{\sqrt{\mu} T_2}{2 \pi})^{\frac{2}{3}} \)

where

*a*is defined as semimajor axis of phasing orbit_{2}*T*is defined as period of phasing orbit_{2}*μ*is defined as Standard gravitational parameter

From the semimajor axis, the phase orbit apogee and perigee can be calculated:

\( 2a_2=r_a+r_p

where

*a*is defined as semimajor axis of phasing orbit_{2}*r*is defined as apogee of phasing orbit_{a}*r*is defined as perigee of phasing orbit_{p}

Finally, the phasing orbit's angular momentum can be found from the equation:

\( {\displaystyle h_{2}={\sqrt {2\mu }}{\sqrt {\frac {r_{a}r_{p}}{r_{a}+r_{p}}}}} \)

where

*h*is defined as angular momentum of phasing orbit_{2}*r*is defined as apogee of phasing orbit_{a}*r*is defined as perigee of phasing orbit_{p}*μ*is defined as Standard gravitational parameter

To find the impulse required to change the spacecraft from its original orbit to the phasing orbit, the change of spacecraft velocity,∆V, at POI must be calculated from the angular momentum formula:

\( \Delta V = v_2-v_1 = \frac{h_2}{r} - \frac{h_1}{r} \)

where

*∆V*is change in velocity between phasing and original orbits at POI*v*is defined as the spacecraft velocity at POI in original orbit_{1}*v*is defined as the spacecraft velocity at POI in phasing orbit_{2}*r*is defined as radius of spacecraft from the orbit’s focal point to POI*h*is defined as angular momentum of original orbit_{1}*h*is defined as angular momentum of phasing orbit_{2}

Co-orbital Rendezvous

If the target (satellite) is behind the spacecraft (shuttle) in the same orbit, the spacecraft must speed up to enter a larger, slower phasing orbit to allow the target to catch up.

Remember that this change in velocity, ∆V, is only the amount required to change the spacecraft from its original orbit to the phasing orbit. A second change in velocity equal to the magnitude but opposite in direction of the first must be done after the spacecraft travels one phase orbit period to return the spacecraft from the phasing orbit to the original orbit. Total change of velocity required for the phasing maneuver is equal to two times ∆V.

Orbit phasing can also be referenced as co-orbital rendezvous [4] like a successful approach to a space station in a docking maneuver. Here, two spacecraft on the same orbit but at different true anomalies rendezvous by either one or both of the spacecraft entering phasing orbits which cause them to return to their original orbit at the same true anomaly at the same time.

Phasing maneuvers are also commonly employed by geosynchronous satellites, either to conduct station-keeping maneuvers to maintain their orbit above a specific longitude, or to change longitude altogether.

See also

Spaceflight portal

Orbital maneuver

Hohmann transfer orbit

Clohessy-Wiltshire equations for co-orbit analysis

Space rendezvous

References

"Archived copy". Archived from the original on 2013-12-16. Retrieved 2013-12-13.

Curtis, Howard D (2014). Orbital Mechanics for Engineering Students (Third Edition). Butterworth-Heinemann. p. 312-316. ISBN 978-0-08-097747-8.

Francis, Hale J (1994). Introduction To Space Flight. Prentice-Hall, Inc.. p. 33. ISBN 0-13-481912-8.

Sellers, Jerry Jon (2005). Understanding Space An Introduction to Astronautics (Third Edition). McGraw-Hill. p. 213-214. ISBN 978-0-07-340775-3.

General

Curtis, Howard D (2014). Orbital Mechanics for Engineering Students (Third ed.). Butterworth-Heinemann. ISBN 978-0-08-097747-8.

Francis, Hale J (1994). Introduction To Space Flight. Prentice-Hall, Inc. ISBN 0-13-481912-8.

Sellers, Jerry Jon; Marion, Jerry B. (2005). Understanding Space An Introduction to Astronautics (Third ed.). McGraw-Hill. ISBN 978-0-07-340775-3.

http://arc.aiaa.org/doi/pdf/10.2514/2.6921[permanent dead link] Minimum-Time Orbital Phasing Maneuvers - AIAA, CD Hall - 2003

Phasing Maneuver

Gravitational orbits

Types

General

Box Capture Circular Elliptical / Highly elliptical Escape Horseshoe Hyperbolic trajectory Inclined / Non-inclined Lagrange point Osculating Parabolic trajectory Parking Prograde / Retrograde Synchronous

semi sub Transfer orbit

Geocentric

Geosynchronous

Geostationary Geostationary transfer Graveyard High Earth Low Earth Medium Earth Molniya Near-equatorial Orbit of the Moon Polar Sun-synchronous Tundra

About

other points

Mars

Areocentric Areosynchronous Areostationary Lagrange points

Distant retrograde Halo Lissajous Lunar Sun

Heliocentric

Earth's orbit Heliosynchronous

Parameters

ShapeSize

e Eccentricity a Semi-major axis b Semi-minor axis Q, q Apsides

Orientation

i Inclination Ω Longitude of the ascending node ω Argument of periapsis ϖ Longitude of the periapsis

Position

M Mean anomaly ν, θ, f True anomaly E Eccentric anomaly L Mean longitude l True longitude

Variation

T Orbital period n Mean motion v Orbital speed t0 Epoch

Maneuvers

Bi-elliptic transfer Collision avoidance (spacecraft) Delta-v Delta-v budget Gravity assist Gravity turn Hohmann transfer Inclination change Low energy transfer Oberth effect Phasing Rocket equation Rendezvous Transposition, docking, and extraction

Orbital

mechanics

Celestial coordinate system Characteristic energy Escape velocity Ephemeris Equatorial coordinate system Ground track Hill sphere Interplanetary Transport Network Kepler's laws of planetary motion Lagrangian point n-body problem Orbit equation Orbital state vectors Perturbation Retrograde motion Specific orbital energy Specific relative angular momentum Two-line elements

List of orbits

Hellenica World - Scientific Library

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