Schwaniger 1963 retrograde (counter-rotation) cislunar symmetric periodic free return, Earth-Moon CR3BP (perigee 6555 km = 177 km altitude, periselene about 2200 km, T = 26.06 d)
schwaniger-1963-em-cislunar-retrograde-periodic-free-return · source: literature ·
validation: V0 · reproduction
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)
T = 6.001502749598107 TU at the registry mu (625.47 h = 26.061 d, t_s = 375190.26 s). One perigee and one perilune per period. Schwaniger prints "about 650 hours" (p.6, read off Fig. 11); the 3.8% difference is within the graph-reading precision of the source. Not a lunar-synodic multiple (the sidereal month is 27.32 d = 6.2832 TU).
- Maintenance ΔV
- 0 km/s — strict ballistic
- Priority date
- 1963-06-01
V∞ at encounters
- E (encounter 1)
- — (not published) CR3BP periodic orbit: the conserved quantity is the Jacobi constant. Perigee speed 10,959.95 m/s Earth-relative inertial (10,977.42 m/s rotating frame) at r = 6555 km.
- Moon (encounter 2)
- — (not published) CR3BP periodic orbit; Jacobi-constant model. Periselene 2202.64 km from the Moon's centre at the start state.
CR3BP orbit identity
- Family
- Schwaniger 1963 counter-rotation cislunar symmetric free return of the first kind (Miele image theorem), periodic member (perigee on the Earth-Moon line, sec. III.E)
- Mass ratio (μ)
- 0.01215058439469525
- Jacobi constant
- 1.0854
- Period (non-dim)
- 6.0015
- Stability index
- 262.652
Planar CR3BP rotating-frame periodic orbit, symmetric about the Earth-Moon line (two perpendicular x-axis crossings: periselene at t = 0, perigee at T/2).
Orbit view 2.5D ecliptic projection
Not renderable from current data. This is a rotating-frame (CR3BP-family — CR3BP, CCR4BP, or CRNBP) periodic or quasi-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). Whatever identity fields the model supports (Jacobi constant, period, stability — not all apply to every model in this family; see "Model assumption" above) are tabulated above.
model: CR3BP (rotating frame)
3D view not available for rotating-frame (CR3BP-family) orbits.
Definition status
incomplete — core fields missing or known-unknowns tracked below
Known-unknowns (3)
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
Schwaniger, A. J. (1963). Trajectories in the Earth-Moon Space with Symmetrical Free Return Properties. NASA TN D-1833 (Lunar Flight Study Series Vol. 5), NASA Marshall Space Flight Center, June 1963.
URL: https://ntrs.nasa.gov/citations/19630007117
Sec. III.E (p.6-7): cross-plotting Fig. 15 gives "one cislunar case... counter-rotational injection at 180 degrees longitude and periselenum radius of about 2150 km", period "about 650 hours or about one month" (Fig. 11). Summary (p.7): "a periodic trajectory which approaches the moon at about 2150 km radius approximately once each month." No initial conditions printed.
Notes
Reproduced with the project corrector (cyclerfinder.search.cr3bp_periodic. correct_symmetric_fixed_jacobi, plain DOP853 rtol = atol = 1e-12 in physical time, no regularisation) plus a secant on C for the perigee condition r1(T/2) = 6555 km. Full-period closure 8.5e-7 km / 3.7e-7 m/s (plain); the Moon-centred KS propagator (core.cr3bp_ks) and the Sundman r1*r2 propagator (core.cr3bp_regularized) re-close it to 1.1e-5 km and 8.7e-6 km. The KS transition matrix gives b_h within 3e-8 of the plain one. det M = 1 - 2.3e-8; the trivial eigenvalue pair is recovered at 0.99914 / 1.00086. Positive control for CR3BP correctors and for any corrector regularised at both primaries (R4): tests/core/test_970_schwaniger_control.py. It is a WEAK regularisation control: the plain integrator already handles the 177 km perigee and 465 km perilune. The C = 1.09727 quoted in the digest-era summaries (with the mu(1-mu) term) belongs to the 6-digit rounded initial state, a neighbouring member with perigee 6560 km; the 6555 km member reproduced here has C = 1.0854167 (1.0974197 with mu(1-mu)). Not a duplicate: no catalogue Earth-Moon row has C near 1.085 with T near 6.0 (digest grep inventory). NOT the arenstorf-em-figure8-1963 orbit and must not fill that row's nulls. Literature novelty check deferred to (not needed for a literature row).
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.periselene_kmSchwaniger 1963 sec. III.E (p.6-7): 'one cislunar case is a periodic orbit which has counter-rotational injection at 180 degrees longitude and periselenum radius of about 2150 km.'
periodSchwaniger 1963 sec. III.E: 'From the curve in Figure 11, the period is ascertained to be about 650 hours or about one month.'
orbit_elements.cr3bp.perigee_kmSchwaniger 1963 sec. II.C: 'injection (and, therefore, reentry) is assumed to occur at 100 nautical mile altitude or 6555 km radius from the earth's center with horizontal path angle.'