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在高日食度度处测量尘埃.

M Baguhl, D P Hamilton, E Grün

    Science (New York, N.Y.)
    |May 19, 1995
    PubMed
    概括

    乌利塞斯航天器的数据揭示了星际尘埃撞击以及在高南度的小颗粒的额外流动. 这些较小的粒子可能是从太阳系内部喷射出的β流星.

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    科学领域:

    • * 太阳系探索研究
    • * 宇宙尘埃研究
    • * 星际介质 星际介质

    背景情况:

    • *"乌利塞斯"号航天器穿越了从木星到日食南极的区域.
    • *了解尘埃的组成和起源对于太阳系和星际介质研究至关重要.

    研究的目的:

    • *分析乌利塞斯航天器收集的尘埃撞击数据.
    • * 为了确定检测到的尘埃颗粒的来源和特征.
    • * 为了研究在高南度观察到的不同寻常的尘埃流的性质.

    主要方法:

    • *利用了来自"乌利塞斯"号航天器的车载尘埃探测器数据.
    • *分析了尘埃撞击率和方向信息.
    • * 与航天器轨迹和太阳系现象相关的尘埃流变化.

    主要成果:

    • * 测量了尘埃撞击速率的缓慢变化 (每天0.2-0.5次撞击).
    • * 确定了一个主导的尘埃流组成部分,来自星际方向 (100°日食度,280°日食经度).
    • * 观测到 - 45°度以南的额外的小粒子流,与星际和生肖尘埃不同.

    结论:

    • * 检测到的主要尘埃成分具有星际起源.
    • * 额外的微粒流可能代表β-流星.
    • * 贝塔石可能被太阳辐射压力和电磁力加速.