Destination pluto: New horizons performance during the approach phase
S. H. FlaniganGabe RogersYanping GuoMadeline KirkH. A. WeaverW. M. OwenC. JackmanJeremy BaumanFrédéric PelletierDerek NelsonDale StanbridgeP. DumontB. G. WilliamsS. A. SternC. B. OlkinL. A. YoungKimberly Ennico
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Imagine a future spacecraft following New Horizons’ trailblazing path to Pluto, but instead of flying past its target – as New Horizons did to explore Pluto and beyond – the next visitor touches down in the midst of tall mountains on the icy plains of Pluto’s heart.
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With just two weeks to go before its historic July 14 flight past Pluto, NASA’s New Horizons spacecraft tapped the accelerator late last night and tweaked its path toward the Pluto system.
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The flyby of Pluto and its moon Charon by the New Horizons spacecraft generated news coverage around the world. Now Stern et al. report the first scientific results from the high-speed encounter. The surface of Pluto is surprisingly diverse, with large regions of differing
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In reference to Jupiter south polar quasi-periodic 40-50 min (QP-40) activities and the model scenario for global QP-40 oscillations of the Jovian inner radiation belt (IRB), we validate relevant predictions and confirmations by amassing empirical evidence from Ulysses, Cassini, Chandra, Galileo, XMM-Newton, and Advanced Composition Explorer for Jupiter north polar QP-40 activities. We report ground 6cm radio observations of Jupiter by Urumqi 25m telescope for synchrotron intensity bursty variations of the Jovian IRB and show their likely correlations with the recurrent arrival of high-speed solar winds at Jupiter.
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