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akatsuki operational_plan, Schemi e mappe concettuali di Gestione Delle Operations

Operational plan for akastuki mission

Tipologia: Schemi e mappe concettuali

2024/2025

Caricato il 15/05/2026

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Akatsuki Operational Plan Draft
Executive summary. Akatsuki must be treated as two different trajectory designs: the
original nominal mission and the recovered mission after the 2010 VOI failure. The
recovery campaign worked because heliocentric perihelion maneuvers lowered the later
Venus arrival energy enough to allow RCS-only capture in 2015.
1. Mission phases and trajectory logic
Akatsuki’s trajectory has to be read in two different ways: the nominal mission design and
the recovered mission design after the 2010 failure. This distinction is essential, because
the original target was a 30 h quasi-equatorial retrograde Venus orbit optimized for
tracking atmospheric super-rotation, while the recovered mission ended up in a much
higher and more weakly bound Venus orbit, chosen because only the RCS was available for
the second insertion attempt.
From the mission timeline, the operational phases can be divided into:
• Cruise phase from launch on 20 May 2010 to the first Venus encounter.
• Sun-orbiting phase after the failed VOI on 7 December 2010.
• Primary science phase starting with the successful VOI-R1 on 7 December 2015.
• Then extended science phases.
Functionally, the trajectory logic is:
Nominal design
• Direct Earth-to-Venus transfer.
• One critical VOI burn with the OME.
• Injection into a 30 h retrograde, near-equatorial science orbit.
After failure
• The spacecraft missed capture because only about 18–20% of the planned deceleration
was achieved.
• It escaped Venus and entered a heliocentric orbit with period about 203 days, perihelion
about 0.61 AU, and aphelion about 0.74 AU.
• The next natural return would have been only in early 2017, too late and with a high
reinsertion cost.
• JAXA therefore redesigned the transfer using perihelion maneuvers and a non-tangent V-
Infinity Leveraging Transfer, so as to anticipate the Venus re-encounter to late 2015 and
reduce the required capture energy.
This is also why the recovery design is operationally more robust than the original VOI
architecture: the perihelion correction can be split into several burns over days, whereas
VOI must be completed within minutes during a single critical event.
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Akatsuki Operational Plan Draft

Executive summary. Akatsuki must be treated as two different trajectory designs: the original nominal mission and the recovered mission after the 2010 VOI failure. The recovery campaign worked because heliocentric perihelion maneuvers lowered the later Venus arrival energy enough to allow RCS-only capture in 2015.

1. Mission phases and trajectory logic

Akatsuki’s trajectory has to be read in two different ways: the nominal mission design and the recovered mission design after the 2010 failure. This distinction is essential, because the original target was a 30 h quasi-equatorial retrograde Venus orbit optimized for tracking atmospheric super-rotation, while the recovered mission ended up in a much higher and more weakly bound Venus orbit, chosen because only the RCS was available for the second insertion attempt. From the mission timeline, the operational phases can be divided into:

  • Cruise phase from launch on 20 May 2010 to the first Venus encounter.
  • Sun-orbiting phase after the failed VOI on 7 December 2010.
  • Primary science phase starting with the successful VOI-R1 on 7 December 2015.
  • Then extended science phases. Functionally, the trajectory logic is:

Nominal design

  • Direct Earth-to-Venus transfer.
  • One critical VOI burn with the OME.
  • Injection into a 30 h retrograde, near-equatorial science orbit.

After failure

  • The spacecraft missed capture because only about 18–20% of the planned deceleration was achieved.
  • It escaped Venus and entered a heliocentric orbit with period about 203 days, perihelion about 0.61 AU, and aphelion about 0.74 AU.
  • The next natural return would have been only in early 2017, too late and with a high reinsertion cost.
  • JAXA therefore redesigned the transfer using perihelion maneuvers and a non-tangent V- Infinity Leveraging Transfer, so as to anticipate the Venus re-encounter to late 2015 and reduce the required capture energy. This is also why the recovery design is operationally more robust than the original VOI architecture: the perihelion correction can be split into several burns over days, whereas VOI must be completed within minutes during a single critical event.

2. Orbital states to define These are the orbital states to place in the reconstruction table.

A. Nominal Earth-Venus transfer arrival condition

This is the pre-VOI state at Venus arrival in December 2010. The planned capture maneuver was 748.3 m/s. The mission design papers describe the arrival as a direct transfer followed by OME braking into the science orbit.

B. Nominal target Venus orbit

The original science orbit was a 30 h elliptical, near-equatorial, retrograde orbit, with westward motion, chosen to follow the atmospheric super-rotation. Early design values are approximately 300 km periapsis altitude and 79,000 km apoapsis altitude.

C. Heliocentric orbit after failed VOI-

After the failed insertion on 7 December 2010, Akatsuki entered a heliocentric orbit with period about 203 days, perihelion about 0.61 AU, and aphelion about 0.74 AU. More precise osculating values reported in the recovery design are perihelion about 9.150 × 10^7 km and aphelion about 1.110 × 10^8 km.

D. Heliocentric orbit after the 2011 perihelion campaign

After the DOX + PHM campaign in late 2011, the recovery paper gives perihelion about 9.14 × 10^7 km and aphelion about 1.080 × 10^8 km. The orbital period became about 199 days, with Venus re-encounter initially set for 22 November 2015.

E. Real Venus orbit after VOI-R1 in 2015

After the successful RCS-only insertion on 7 December 2015, the initial orbit had apoapsis altitude about 440,000 km, inclination about 3°, and orbital period about 13 days 14 h. A later trim reduced the orbit to about 360,000 km apoapsis altitude, 1000–8000 km periapsis altitude, and about 10 days 12 h period. Useful reverse-sized check. Using rp = RV + 300 km and ra = RV + 79,000 km gives an orbital period of about 29.9 h, which is fully consistent with the nominal 30 h design.

3. Main maneuver costs and reverse sizing

3.1 Nominal VOI

For a capture burn at Venus periapsis, the standard impulsive two-body estimate is: Δv_VOI = v_p,hyp − v_p,ell v_p,hyp = sqrt(v_inf^2 + 2 μ_V / r_p) v_p,ell = sqrt[ μ_V (2 / r_p − 1 / a) ] a = (r_p + r_a) / 2 If the nominal orbit approximation h_p = 300 km and h_a = 79,000 km is used together with the literature value Δv = 748.3 m/s, the inferred arrival hyperbolic excess velocity is about v_inf ≈ 2.84 km/s. This is a reasonable reverse-sized value for the original direct transfer.

The most relevant maintained quantities are therefore mission-preserving constraints rather than generic orbital elements:

  • Periapsis altitude, to avoid atmospheric entry or impact.
  • Apoapsis altitude, because it affects both science geometry and perturbation sensitivity.
  • Orbital plane orientation relative to the Venus equator, because near-equatorial retrograde observation was a science requirement.
  • Eclipse duration and umbra time, constrained by the battery system.
  • Incident angle relative to the orbital plane, constrained by spacecraft operations. Solar radiation pressure can be mentioned, but for center-of-mass orbit maintenance it is probably secondary compared with solar third-body gravity. 5. Station keeping estimate A fully regular station-keeping budget is not explicitly tabulated in the available material, so the safest approach is to combine the perturbation logic with the actual maintenance maneuvers reported in the timeline.
  • TRM-R1 = 1.1 m/s on 11 September 2015 before VOI-R1.
  • PC1 = 2.2 m/s on 4 April 2016.
  • PC2 = 0.52 m/s on 7 October 2020. For center-of-mass maintenance after orbit establishment, a reasonable empirical bracket is about 0.1–0.6 m/s/year. The higher end comes from averaging PC1 + PC2 over about 4.8 years, while the lower end reflects the later mature correction level represented by PC2. This should be presented honestly as an estimate, because the available timeline does not report every possible maintenance event and VOI-R2 does not have a published Δv in the material used here. 6. Delta-V recap and comparison between ideal and real mission

A. Original nominal mission around 2010

  • APH-1 test = 12.2 m/s
  • TRM-1 = 2.9 m/s
  • TRM-2 = 0.27 m/s
  • TRM-3 = 0.04 m/s
  • VOI-1 planned = 748.3 m/s This gives a known pre-insertion + insertion budget of about 751.5 m/s if only the late Venus-approach trims and nominal VOI are counted, or about 763.7 m/s if the APH- engine test is also included.

B. Recovery effort after the failure

  • Failed VOI-1 actually spent = 134.8 m/s
  • DOX maneuvers = 25.7 m/s
  • PHM maneuvers = 242.7 m/s
  • DV4-1 to DV4-3 = 87.4 m/s
  • VOI-R1 = 134.8 m/s
  • PC1 + PC2 known later maintenance = 2.72 m/s This gives about 493.3 m/s for the successful recovery sequence from 2011 onward if the sunk failed 2010 VOI is excluded, or about 628.1 m/s if that failed VOI is also included. These values are lower bounds because VOI-R2 is listed in the timeline but its Δv is not reported in the material used here.

C. Interpretation

This does not mean the recovered mission was simply cheaper than the original one. The comparison is not apples-to-apples, because the recovered orbit is far less demanding dynamically than the original low-apoapsis 30 h science orbit. The real lesson is that the recovery campaign spent a substantial amount of Δv in heliocentric space to lower the later Venus arrival energy. That trade allowed a final 134. m/s RCS-only capture, which would have been impossible on the original failed-arrival geometry. Design robustness / fragility The original trajectory design was efficient but operationally brittle, because it depended on a single critical OME burn at Venus. Once that burn was interrupted after only about 18% of the planned Δv, nominal capture became impossible. At the same time, the mission was surprisingly robust at system level for three reasons:

  • Enough propellant remained to reshape the heliocentric orbit.
  • The recovery transfer lowered the Venus arrival energy dramatically.
  • The final science orbit, although degraded, still supported valuable science and improved some kinds of global imaging continuity. Overall conclusion. The original trajectory design was efficient but fragile, whereas the recovered design was less performant scientifically yet much more resilient energetically and operationally.