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Case 1 ballistic two-synodic-period Earth-Mars cycler (S2L1 family)

mcconaghy-2005-em-case1 · source: literature · validation: V0

Signature

Bodies
E-M
Sequence (canonical)
E-E-M-M
Sense
outbound
Period
4.270 yr (2 × E-M synodic)
Two Earth-Mars synodic periods = 2 x 2.135 yr = 4.27 yr; consistent with the four-vehicle count in Rogers 2012 Table 1 (one vehicle per outbound/inbound branch x 2 synodic phases).
Priority date
2002-08-05

V∞ at encounters

E (#1)
— (not published)
Steady-state cycling V_inf at Earth not in Rogers 2012 Table 1 (Table 1 gives orbital elements only). Rogers 2012 Table 3 reports the 4:3(2)- establishment-cycler V_inf,flyby = 3.378 km/s (the post-Earth flyby V_inf for the establishment trajectory matching Case 1's orbital elements). McConaghy/Longuski/Byrnes 2002 AIAA 2002-4420 (paywalled at AIAA) is the originating source for the steady-state cycler V_inf; Russell 2004 Table 3.4 does not pair "Case 1" to a Russell-numbered row (only Case 2 = 2.1.1.+2 and Case 3 = 2.3.1.+1 are footnoted).
M (#2)
— (not published)
Same — steady-state V_inf at Mars not transcribed by Rogers 2012; awaiting direct access to McConaghy 2005 dissertation or AIAA 2002-4420.

Orbit elements (heliocentric)

Semi-major axis a
1.220 AU
Eccentricity e
0.238
Perihelion
0.930 AU
Aphelion
1.510 AU
Inclination
0.00°

Rogers et al. 2012 Table 1: 'Case 1 ... Semi-Major Axis 1.22 AU, Eccentricity 0.238, Aphelion Radius 1.51 AU, Perihelion Radius 0.93 AU' (circular-coplanar model). 0.0 inclination follows from the modelling assumption.

Legs

Primary citation

McConaghy, T. T. et al. (2002). Analysis of a Broad Class of Earth-Mars Cycler Trajectories. AIAA/AAS Astrodynamics Specialist Conference, Monterey CA, AIAA 2002-4420.

DOI: 10.2514/6.2002-4420

First publication of the broad-class enumeration that includes Case 1. The journal version is McConaghy/Longuski 2004 JSR 'Analysis of a Class of Earth-Mars Cycler Trajectories' (DOI 10.2514/1.11939, paywalled). The comprehensive dissertation treatment is McConaghy 2005 Purdue PhD.

Corroborating sources

Notes

"Case 1" is the third (alongside Case 2 and Case 3) of the two-synodic- period ballistic cyclers tabulated in McConaghy/Longuski/Byrnes 2002 AIAA 2002-4420 and the Byrnes/McConaghy/Longuski 2002 AIAA 2002-4423 follow-on ("Analysis of Various Two Synodic Period Earth-Mars Cycler Trajectories"). The SnLm classification is S2L1: 2 synodic periods, 1 intermediate Earth-Earth loop between Mars encounters. Russell 2004 Table 3.4 footnotes only Cases 2 (= Russell 2.1.1.+2) and 3 (= Russell 2.3.1.+1) to Byrnes 2002; Case 1 is not footnoted to a specific Russell row in the dissertation excerpt visible from the UT Austin abstract page, but it shares the same generic family. Among the four McConaghy-Byrnes-Longuski 2002 two-synodic-period cyclers, Rogers 2012 §III.A flags Case 2 as having the lowest launch V_inf and shortest 171-day Earth-Mars flight time in the analytic ephemeris (Table 4). Case 1 has the longest first-leg ToF (365 d, Rogers Table 4) — implying the spacecraft completes roughly one full heliocentric orbit before reaching Mars on its first leg, distinguishing it geometrically from Cases 2/3. DATA COMPLETENESS: orbital elements (a, e, peri, apo) populated from Rogers 2012 Table 1. Steady-state cycling V_inf values left null pending direct access to McConaghy 2005 dissertation or the AIAA 2002-4420 / JSR 2004 papers. M7 matching against finder hits can use the orbital-element signature without the V_inf multiset. The 4:3(2)- prefix in Rogers 2012 Tables 3-5 refers to the V_inf-leveraging K:L(M)+/- notation introduced in their Nomenclature table: K = number of Earth orbit revolutions, L = number of spacecraft orbit revolutions, M = spacecraft orbit revolution on which the deep-space maneuver is performed, with +/- denoting flyby before (-) or after (+) perihelion. This is a separate nomenclature from McConaghy's SnLm cycler classification.

Source quotes (per-field provenance)

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

a_au
Rogers et al. 2012 Table 1: 'Case 1 ... Semi-Major Axis, AU: 1.22'.
e
Rogers et al. 2012 Table 1: 'Case 1 ... Eccentricity: 0.238'.
perihelion_au
Rogers et al. 2012 Table 1: 'Case 1 ... Perihelion Radius, AU: 0.93'.
aphelion_au
Rogers et al. 2012 Table 1: 'Case 1 ... Aphelion Radius, AU: 1.51'.
legs[0].tof_days
Rogers et al. 2012 Table 4 (STOUR analytic-ephemeris results): row 'Case 1, 4:3(2)-, LD 12/14/2024, TOF 365 days, Periapse 0.946 AU, Apoapse 1.503 AU' — the 365-day TOF for the first leg of the establishment-cycler trajectory that matches the Case 1 cycler orbital elements.
period.years
Period = k * synodic = 2 * 2.135 yr = 4.27 yr; derived from the two-synodic-period family membership confirmed by Rogers 2012 §III.A "various two synodic period cyclers".