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Russell-Ocampo cycler 4.1.1.-4 (4-synodic)

russell-ocampo-4.1.1-4 · source: literature · validation: V1

Signature

Bodies
E-M
Primary
Sun (default — heliocentric)
Sequence (canonical)
E-E-M-M
Sense
outbound
Orbit class
Cycler
strict cycler (infinite returns)
Cycler class
multi-arc
Trajectory regime
ballistic
Maintenance ΔV band
unclassified
Model assumption
circular-coplanar
Idealised: planets on circles, coplanar ecliptic.
Period
8.540 yr (4 × E-M synodic)
4 x Earth-Mars synodic period (2.135 yr) per Russell 2004 §3.8 row 4.1.1.-4; n_flybys = 2.
Priority date
2003-02-09

V∞ at encounters

E (encounter 1)
5.50 km/s
Russell 2004 Table 3.4 row 4.1.1.-4: Earth v_inf = 5.5 km/s.
M (encounter 2)
9.30 km/s
Russell 2004 Table 3.4 row 4.1.1.-4: Mars v_inf = 9.3 km/s.

Cycle-level identity (multi-arc invariants)

Aphelion ratio (AR)
1.44
Turn ratio (TR)
0.89
Transit times (days)
137 d

Aphelion derived from Russell 2004 Table 3.4 Aphelion Ratio AR = 1.44 x 1.52 AU (Mars sma) = 2.189 AU. Other elements (a, e, perihelion) not tabulated in Table 3.4.

Orbit view 2.5D ecliptic projection

Top-down ecliptic view: the Sun at centre with planet reference circles and the cycler's sourced max-aphelion ring (2.189 AU). 0 of 3 trajectory segments carry published (a,e) and are drawn; 3 are shown as "elements not published" gaps, never interpolated. E M Sun Cycler max aphelion 2.189 AU (sourced)
spacecraft: idealized coplanar ellipse planets: J2000 osculating ellipse (Standish & Williams Table 1) orientation: coplanar-idealized (no Ω/ω published — in-plane ellipse)

3D view not available for multi-arc trajectories yet. The 3D system can now render a numerically-sampled polyline (n-body or multi-arc), but no sampled trajectory is published for this row — each leg is a separate ellipse with honest gaps where elements are unpublished (the 2D view above shows them). The button will appear here once a sampled path is exported for this trajectory; we never interpolate one from the catalogue's per-leg (a, e).

— — planet orbit (true J2000 ellipse) ◌ max aphelion ring (sourced)
Not-published gaps (never interpolated):
  • E → M — segment elements (a, e) not published; no curve drawn.
  • M → E — segment elements (a, e) not published; no curve drawn.
  • E → E — segment elements (a, e) not published; no curve drawn.
Real DE440 encounter dates (5)
  • 2026-12-10 V∞ 5.84 / 9.54 km/s
  • 2029-01-18 V∞ 5.52 / 8.91 km/s
  • 2031-02-07 V∞ 4.22 / 9.86 km/s
  • 2033-03-08 V∞ 5.08 / 9.71 km/s
  • 2035-04-27 V∞ 7.00 / 8.72 km/s

Real, verifiable JPL DE440 geometric-match dates (see Launch windows). Positions on the map are idealized; these are the true dates.

Legs (trajectory segments)

Definition status

incomplete — core fields missing or known-unknowns tracked below

Family: Russell 4-synodic Earth-Mars ballistic · Russell-Ocampo cycler code

Known-unknowns (4)

Values we expect to exist but have not yet filled (distinct from "not applicable"). Tracked per upstream docs/spec.md §16.6.4.

Primary citation

Russell, R. P. & Ocampo, C. A. (2005). Geometric Analysis of Free-Return Trajectories Following a Gravity-Assisted Flyby. Journal of Spacecraft and Rockets, Vol. 42, No. 1, pp. 138-152.

DOI: 10.2514/1.5571

URL: https://arc.aiaa.org/doi/abs/10.2514/1.5571

Peer-reviewed venue for the ballistic cycler catalogue (geometric analysis branch). Conference precursor Russell/Ocampo AAS 03-145 (Feb 2003) establishes priority.

orbit source Russell 2004, Table 3.4 orbit fidelity circular-coplanar V∞ source Russell 2004, Table 3.4 V∞ fidelity circular-coplanar

Corroborating sources

Notes

Near-ballistic per Russell's Table 3.4 (passes the AR_MIN=0.9 / TR_MIN=0.85 documentation gate but not strictly ballistic: AR=1.44, TR=0.89). 4-synodic period. 2 required Earth flybys (turning angles [95, 95] deg per Table 3.4 last column). Where AR<1 the cycler does not quite reach Mars / where TR<1 a small powered turn is required; Russell does not tabulate the per-cycle DV (left null). Russell nomenclature p.h.s.i: the trailing index (-4) is the lower-energy multiple-revolution Lambert branch of the generic-return solution (sign: + fast, - slow). Circular-coplanar simple-model values (Russell 2004 Ch.3); modern ephemeris families (App.C / DE405) refine the dynamics. Ingested 2026-06-07 from docs/notes/2026-06-07-russell-2004-member-tables-transcription.md (Table 3.4, p.83).

Source quotes (per-field provenance)

Every numerical value in this entry traces to a verbatim or paraphrased quote from a cited source.

vinf_kms_at_encounters[0].vinf_kms
Russell 2004 Table 3.4 row 4.1.1.-4: Earth v_inf (km/s) = 5.5.
vinf_kms_at_encounters[1].vinf_kms
Russell 2004 Table 3.4 row 4.1.1.-4: Mars v_inf (km/s) = 9.3.
legs[0].tof_days
Russell 2004 Table 3.4 row 4.1.1.-4: Earth->Mars (or aphelion) Time (days) = 137.
aphelion_au
Russell 2004 Table 3.4 row 4.1.1.-4: Aphelion Ratio = 1.44; aphelion = 1.44 x 1.52 AU = 2.189 AU.