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MISSION PLAN - PDS Small Bodies Node

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yaw, while continuing to meet solar array shadow constraints. The second strategy is a<br />

reduction to the amount of daily tracking required to support these maneuvers. Post-<br />

DSM-1 and pre- and post-TCM-3, daily tracking is reduced from 2 weeks to 1 week.<br />

Mission operations are slightly more complex during actual execution of DSM’s and<br />

TCM’s. During the maneuvers, the attitude of the spacecraft is such that solar power and<br />

telemetry will most likely not be available. The rechargeable battery will be the source<br />

of power. The two large DSM’s (1 and 3) cannot be executed in a single burn due to<br />

insufficient battery capacity. The current plan is to implement DSM-1 in three segments<br />

and DSM-3 in two. Each burn is separated by two days to provide sufficient time for<br />

battery recharging. No ∆V updates between each cluster of burns is planned. However,<br />

receipt of telemetry and radiometric data (>1 hr) for burn reconstruction may be possible<br />

during battery recharging.<br />

At solar ranges beyond 2.5 AU, second (L+1014 to 1320) and third (L+1942 to 2219)<br />

aphelion, the spacecraft operational capabilities are power limited such that a full 4 hour<br />

pass may not be supportable. The duration of tracking passes at these solar ranges will<br />

be reduced from 4 hours to the maximum allowable, down to a minimum of 2 hours (if<br />

required) at aphelion. The second DSM and a TCM are scheduled during second and<br />

third aphelion, respectively. A reduced tracking frequency and track duration is imposed<br />

in support of these maneuvers.<br />

Three TCM’s are planned during the cruise phase. Two of them are performed 30 and 7<br />

days after DSM-1 and -3, respectively, to correct execution errors. The third is<br />

performed at third aphelion and provides an opportunity for early targeting of the return<br />

trajectory.<br />

Table 4.3-1.a Cruise Phase Mission Operations<br />

Mission Operation Description<br />

Communications 4 (1) hrs / week, antenna: MGA<br />

4 (1) hrs / month, antenna: HGA, can replace navigation tracking<br />

TCM/DSMs (overlay changes for DSM 1,2 / TCM 3,16 below)-<br />

Two - 4 hr pass/week - MGA Comm, -14 to -28, +14 to +28d<br />

4 hrs /day - MGA Comm, ± 14 d of first/last segments<br />

1 hr / between seg. - HGA Comm, DSMs only - if possible<br />

DSM 1 / TCM 3 (overlap with ISP-1) - overlay changes:<br />

4 hrs /day - HGA Comm, 0 to +7 d, DSM-1<br />

Two - 4 hr pass/week - HGA Comm, +7 d DSM-1 to -7 d TCM 3<br />

4 hrs /day - HGA Comm, -7 to 0 d, TCM 3<br />

Two - 4 hr passes/week - MGA Comm, +7 to +28 d, TCM 3<br />

DSM 2 / TCM 16 (aphelion maneuvers) - overlay changes:<br />

4 (1) hrs / every other day - MGA Comm, ± 14 d<br />

Navigation L+398-402 d: DSM-1 (TCM 2)<br />

L+432 d: TCM 3<br />

L+1130 d: DSM-2 (TCM 7)<br />

L+1609-1611 d: DSM-3 (TCM 8)<br />

L+1618 d: TCM 9<br />

L+2063 d: TCM 16<br />

1. Or maximum allowable at solar ranges greater than 2.5 AU Minimum of 2 hours for radiometric tracking.<br />

Table 4.3-1.b Cruise Phase Mission Operations - DSN Profile<br />

62

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