Italian Spring Accelerometer measurements of unexpected Non Gravitational Perturbation during BepiColombo second Venus swing-by

Carmelo Magnafico, Umberto De Filippis, Francesco Santoli, Carlo Lefevre, Marco Lucente, David Lucchesi, Emiliano Fiorenza, Roberto Peron, Valerio Iafolla
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Abstract

The Italian Spring Accelerometer (ISA) is a three axis mass-spring accelerometer, one of the payloads of the BepiColombo joint space mission between the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA). At launch in October 2018, BepiColombo started its seven-year cruise as a stack of three different modules, overall named Mercury Composite Spacecraft (MCS). The spacecraft will provide BepiColombo the necessary Delta V to reach Mercury with its electric thrusters and along with one, two and six gravity assists, respectively with Earth, Venus and Mercury. The accelerometer is accommodated on the Mercury Planetary Orbiter (MPO) module and, jointly with the Ka-band Transponder (KaT) tracking data, will primarily serve the BepiColombo Radio Science Experiment (BC-RSE). During the second Venus swing-by, strong tidal effect and external perturbations was expected to act on the spacecraft and to become detectable by ISA. The swing-by had a closest approach of about 550 km and the gravity gradient expected on the IDA sensing elements was perfectly measured. Hence, in this paper, the first direct Gravity Gradient effect detection generated by an extraterrestrial body is shown. Nevertheless, around the closest approach, the measurements evidenced a spurious acceleration event lasting for several minutes. This work, exploiting information on the Attitude and Orbit Control System (AOCS) commanded torques, focuses and analyses this ISA acceleration signal, ascribing it to a net force really acting on the MCS spacecraft. Furthermore, using an estimation method, the application point of the force is confined to an area close to the MPO radiator.
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意大利弹簧加速度计对贝皮-科伦坡号第二次金星掠过期间意外非重力扰动的测量结果
意大利弹簧加速度计(ISA)是一个三轴质量弹簧加速度计,是欧洲空间局(ESA)和日本宇宙航空研究开发机构(JAXA)之间的BepiColombo联合太空任务的有效载荷之一。2018年10月发射时,BepiColombo作为三个不同模块的堆叠开始了其为期七年的巡航,总体命名为水星复合航天器(MCS)。该航天器将为 BepiColombo 提供必要的德尔塔 V,以便利用其电动推进器到达水星,同时还将分别为地球、金星和水星提供一次、两次和六次重力辅助。加速度计安装在水星行星轨道器(MPO)模块上,与 Ka 波段转发器(KaT)跟踪数据一起,将主要为贝皮科伦坡无线电科学实验(BC-RSE)服务。在第二次掠过金星期间,预计会有强烈的潮汐效应和外部扰动作用在航天器上,并会被国际空间站探测到。这次绕行的最近距离约为 550 公里,国际空间站传感元件上预期的重力梯度得到了完美的测量。因此,本文首次直接探测到了由地外天体产生的重力梯度效应。然而,在最近接近时,测量结果表明出现了持续数分钟的假加速事件。这项工作利用姿态和轨道控制系统(AOCS)指令扭矩的信息,聚焦并分析了这一ISA加速信号,将其归因于真正作用于MCS航天器的净力。此外,利用一种估算方法,该力的作用点被限制在靠近 MPOradiator 的区域。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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