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Zamama is an active volcanic center on Jupiter's moon Io. This volcanic center erupted after the Voyager 1 flyby in 1979, making it one of the few planetary volcanoes known to have activated during this generation's lifetime. Further analysis and study by the Galileo spacecraft helped with the overall study of Io's volcanism. Galileo located it on Io at 21°N 173°W / 21°N 173°W. Zamama has a fissure-fed-type flow that is 150 km (93 mi) long with temperatures of 1,100 K (830 °C; 1,520 °F), and the volcanic center site has explosive and effusive eruption characteristics. The flow appears to be emanating from the Promethean-type volcano.

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  • Zamama (it)
  • Zamama (volcano) (en)
  • 札巴巴火山 (zh)
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  • Zamama è un centro eruttivo presente sulla superficie di Io. (it)
  • 札巴巴火山 （Zamama）是木星的卫星-木卫一上一座活跃的火山中心，该火山中心于1979年“旅行者1号”飞掠后爆发，成为此代人一生中少数所知的外星复苏火山之一。“伽利略号探测器”进一步的分析和研究有助于全面了解木卫一的火山活动。根据“伽利略探测器”定位，札巴巴火山位于木卫一北纬21度、西经173度处，包括一道长150公里（93英里）、温度1100 K（摄氏830度、华氏1520度）的“裂隙补给型”熔岩流。该火山中心具有爆炸性喷发和溢流式喷发的特点，它的熔岩流似乎源于“普罗米修斯型”火山。 “伽利略探测器”安装了一系列收集和分析木卫一表面火山活动的遥感仪-近红外测图光谱仪(NIMS)、固态成像仪(SSI)、偏振光辐射计(PPR)等。由于没有从木卫一采集到样本，因此，所有的解释都是通过研究“伽利略”数据中的反照率效应、形态和/或光谱变化等得出的。此外，地貌分析被谨慎地应用于这类特殊行星结构的研究。1979年，国际天文联合会以巴比伦神话的基什守护神—“札巴巴”（Zababa），又称作“札玛玛”（Zamama）命名该火山。 (zh)
  • Zamama is an active volcanic center on Jupiter's moon Io. This volcanic center erupted after the Voyager 1 flyby in 1979, making it one of the few planetary volcanoes known to have activated during this generation's lifetime. Further analysis and study by the Galileo spacecraft helped with the overall study of Io's volcanism. Galileo located it on Io at 21°N 173°W / 21°N 173°W. Zamama has a fissure-fed-type flow that is 150 km (93 mi) long with temperatures of 1,100 K (830 °C; 1,520 °F), and the volcanic center site has explosive and effusive eruption characteristics. The flow appears to be emanating from the Promethean-type volcano. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Eruption_styles_and_volumetric_eruption_rates_of_Zamama,_and_comparison_with_terrestrial_volcanoes..jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Lava_flow_field_on_Zamama,_image_is_captured_using_Solid-State_Imaging_during_the_Galileo_Mission.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Thermal_emission_variability_of_Zamama,_eruption_rate_and_power_output_flux_of_Zamama.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Zamama_region_on_Io_showing_three_volcanoes_(Zamama_A,_B,_and_C)_marked_by_White_arrows._Zamama(A)_shield_volcano_and_the_dark_main_flow_comples_spreading_eastward..jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Zamama_volcanic_center,_Galileo,_July_1999_(PIA02504).jpg
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  • Zamama è un centro eruttivo presente sulla superficie di Io. (it)
  • Zamama is an active volcanic center on Jupiter's moon Io. This volcanic center erupted after the Voyager 1 flyby in 1979, making it one of the few planetary volcanoes known to have activated during this generation's lifetime. Further analysis and study by the Galileo spacecraft helped with the overall study of Io's volcanism. Galileo located it on Io at 21°N 173°W / 21°N 173°W. Zamama has a fissure-fed-type flow that is 150 km (93 mi) long with temperatures of 1,100 K (830 °C; 1,520 °F), and the volcanic center site has explosive and effusive eruption characteristics. The flow appears to be emanating from the Promethean-type volcano. Remote sensing instruments built on the Galileo spacecraft—the Near-Infrared Mapping Spectrometer (NIMS), Solid-State Imager (SSI), Photopolarimeter-Radiometer (PPR)—collect and analyze volcanism on Io's surface. Since there are no samples collected from Io, all of the interpretations are made by studying albedo effects, morphology and/or spectral variations in Galileo data. Furthermore, Geomorphologic analysis is strictly used to study such specific planetary structures. (en)
  • 札巴巴火山 （Zamama）是木星的卫星-木卫一上一座活跃的火山中心，该火山中心于1979年“旅行者1号”飞掠后爆发，成为此代人一生中少数所知的外星复苏火山之一。“伽利略号探测器”进一步的分析和研究有助于全面了解木卫一的火山活动。根据“伽利略探测器”定位，札巴巴火山位于木卫一北纬21度、西经173度处，包括一道长150公里（93英里）、温度1100 K（摄氏830度、华氏1520度）的“裂隙补给型”熔岩流。该火山中心具有爆炸性喷发和溢流式喷发的特点，它的熔岩流似乎源于“普罗米修斯型”火山。 “伽利略探测器”安装了一系列收集和分析木卫一表面火山活动的遥感仪-近红外测图光谱仪(NIMS)、固态成像仪(SSI)、偏振光辐射计(PPR)等。由于没有从木卫一采集到样本，因此，所有的解释都是通过研究“伽利略”数据中的反照率效应、形态和/或光谱变化等得出的。此外，地貌分析被谨慎地应用于这类特殊行星结构的研究。1979年，国际天文联合会以巴比伦神话的基什守护神—“札巴巴”（Zababa），又称作“札玛玛”（Zamama）命名该火山。 (zh)
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