Braik-Ross common-energy (1,1)a Earth-Moon cycler (CR3BP, C=3.1294)
braik-ross-c11a-cycler-2026 · source: literature ·
validation: V1
Signature
- Bodies
- E-Moon
- Primary
- Earth
- Sequence (canonical)
E-Moon- Sense
- n/a
- Orbit class
- Cycler strict cycler (infinite returns)
- Cycler class
- non-keplerian (CR3BP)
- Trajectory regime
- ballistic
- Maintenance ΔV band
- unclassified
- Model assumption
- cr3bp CR3BP — Jacobi-constant-conserved; signature not patched-conic comparable.
- Period
- — yr (1 × E-Moon synodic)
Period T_PO = 42.140 d (Braik & Ross 2026 Table 2 "(1,1)a-cycler" row, reported in days at the common C_J=3.1294); reproduced in-repo at 42.1405 d (+0.0011%). Encounter cadence: k1=1 perigee + k2=1 perilune pass per period (Ross-RT 2025 Def. 1, family-anchor row ross-rt-em-cycler-11-2025). years: null (CR3BP, rotating-frame periodic orbit; the heliocentric-synodic-multiple convention does not apply).
- Priority date
- 2026-05-29
V∞ at encounters
- E (encounter 1)
- — (not published) CR3BP periodic orbit: conserved quantity is the Jacobi constant, not V_inf.
- Moon (encounter 2)
- — (not published) Same — Jacobi-constant model.
CR3BP orbit identity
- Family
- (1,1) prograde Earth-Moon cycler — short-period branch (C11a)
- Mass ratio (μ)
- 0.012150584270572
- Jacobi constant
- 3.1294
- Period (non-dim)
- 9.6911
- Stability index
- 12902.660
Planar CR3BP rotating-frame periodic orbit; Keplerian elements inapplicable. CR3BP identity tuple below.
Orbit view 2.5D ecliptic projection
Not renderable from current data. This is a rotating-frame (CR3BP) periodic orbit. A faithful render requires numerical propagation of the synodic-frame state, which the catalogue does not yet publish as a sampled path — so no stand-in ellipse is drawn (drawing a heliocentric ellipse here would misrepresent the dynamics). The CR3BP identity (Jacobi constant, period, stability) is tabulated above.
model: CR3BP (rotating frame)
3D view not available for rotating-frame (CR3BP) orbits.
Definition status
incomplete — core fields missing or known-unknowns tracked below
Known-unknowns (1)
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
Braik, A. & Ross, S. D. (2026). Orbital Networks in the Three-Body Problem. arXiv preprint arXiv:2605.31543 (29 May 2026).
URL: https://arxiv.org/abs/2605.31543
arXiv submission dated 29 May 2026; PDF dated June 1, 2026 (title page). Table 2 lists thirteen common-energy representative periodic orbits at C_J=3.1294. The (1,1)a-cycler row carries T_PO=42.140 d and instability rate sigma=1.0482 TU^-1 (sigma_d=0.2410 d^-1). The paper does NOT print the initial state.
Corroborating sources
- Ross, S. D. & Roberts-Tsoukkas, M. (2025). Stable, Low-Energy Prograde Earth-Moon Cycler Orbits. AAS/AIAA Astrodynamics Specialist Conference, 2025, paper AAS 25-621. · link Family anchor: Ross-RT 2025 defines the (k1,k2)-cycler family numbering (Def. 1) and proves the (1,1) family's stable subfamily at C^stable=3.151; ross-rt-em-cycler-11-2025 is its nu=0 midpoint. C11a is a DIFFERENT member of the same continuous (1,1) family at the lower Jacobi C=3.1294, on the short-period branch of a saddle-center fold inside the family (mining note). Same family identity (k1=1, k2=1, prograde); different orbit (UNSTABLE, T=42.140 d vs the anchor's STABLE T=44.754 d).
Notes
Common-energy (1,1)a-cycler from Braik & Ross 2026 Table 2, the SHORT-PERIOD branch of the (1,1) family at C_J=3.1294. Distinct from the family-anchor row ross-rt-em-cycler-11-2025 (Ross-RT 2025), which is the (1,1) family's per- family STABLE midpoint at C^stable=3.151175879508174 (T=44.754 d, |nu|<1). C11a sits at a different Jacobi (3.1294, below C^stable) and a different branch (short-period side of a saddle-center fold inside the family — the fold geometry is documented in the mining note). At C=3.1294 the (1,1) family is UNSTABLE; Braik-Ross publishes instability rate sigma=1.0482 TU^-1 (sigma_d=0.2410 d^-1, Floquet exponent of the largest-magnitude nontrivial monodromy eigenvalue per Eq. 20), reproduced in-repo as Barden nu=1.29e4 (|lambda|=2.58e4 ~ exp(sigma*T_PO)). REPRODUCTION (2026-06-14): symmetric perpendicular-x-axis-crossing corrector at C=3.1294 from seed x0=-0.81164067 with ydot0_sign=-1 and the 3rd x-axis crossing pinned as half-period -> T=42.140462 d (sourced 42.140, error +0.0011%); Jacobi 3.1294 enforced to machine eps; topology (1,1) prograde confirmed by winding-number diagnostic. Independent Radau integrator at rtol/atol 1e-11 closes the Jacobi (dJ=1.9e-13 over one period); the rotating-frame state closes to ~2.8e-9 (well-conditioned for the moderate instability). Reproduction harness: src/cyclerfinder/search/reachable_representatives.py + docs/notes/2026-06-14-249-unstable-member-recovery-plan.md (final disposition section; commits a19eb24, 4a20243, f608c6b, 325c8a2). MODEL: pure planar CR3BP (PCR3BP). No bicircular / solar-gravity / lunar- eccentricity / ephemeris refinement. Every number here is PCR3BP-only at the Braik-Ross common Jacobi.
Source quotes (per-field provenance)
Every numerical value in this entry traces to a verbatim or paraphrased quote from a cited source.
orbit_elements.cr3bp.period_ndBraik & Ross 2026 Table 2 (p. 12): (1,1)a-cycler T_PO=42.140 d at C_J=3.1294.
orbit_elements.cr3bp.braik_ross_sigma_per_tuBraik & Ross 2026 Table 2 (p. 12): (1,1)a-cycler instability rate sigma=1.0482 TU^-1.
orbit_elements.cr3bp.braik_ross_sigma_per_dayBraik & Ross 2026 Table 2 (p. 12): (1,1)a-cycler instability rate sigma_d=0.2410 day^-1.
orbit_elements.cr3bp.jacobi_constantBraik & Ross 2026 Sec. 2.4 / Table 2 header: common Jacobi level C_J=3.1294 used throughout the accessibility study.
orbit_elements.cr3bp.mass_ratioBraik & Ross 2026 Table 1 (p. 8): Earth-Moon mass parameter mu = 0.012150584270572 (== Ross-RT 2025 p. 3).