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http://dbpedia.org/ontology/abstract Kanehekili Fluctus is a lava flow field onKanehekili Fluctus is a lava flow field on Jupiter's moon, Io. This fluctus (terrain covered by outflow of liquid, used on Venus, Io and Titan) is located in the sub-Jovian hemisphere at 17°41′S 33°34′W / 17.68°S 33.56°W as shown in the picture on the right. Also in the picture is the Kanehekili volcanic center located at 18°13′S 33°36′W / 18.21°S 33.6°W.This lava field covers roughly 34,500 square kilometres (13,300 sq mi). The hotspot was detected by the Galileo Solid State Imaging experiment (SSI) on orbits by Galileo. The Kanehekili and Janus Patera region are of interest because there are indications that it contains an active, overturning lava lake. Based on thermal emission data, this area is almost identical to the Pele region which is believed to be the site of an active, overturning lava lake. These two regions are the only sites where thermal emissions are identical to terrestrial active, overturning lava lakes, and this feature makes it a high priority target for a future space craft mission. Ionian flucti are areas of lava flow. They are named after fire and thunder gods of various mythologies or after locations in Greek mythology associated with Io. Kanehekili Fluctus is possibly a silicate lava flow. The darkest and youngest area of the fluctus is about 16,500 square kilometres (6,400 sq mi). Observation of thermal emission leads to the inference that Kanehekili Fluctus is subject to episodic volcanism that has periods of explosive activity followed by less active periods of time. It is possible that detection of the cooled flows may become more difficult as time goes on.may become more difficult as time goes on. , Il Kanehekili Fluctus è una struttura geologica della superficie di Io. , 卡涅赫基里熔岩流(Kanehekili Fluctus)是木星的卫星—木卫一上的一处卡涅赫基里熔岩流(Kanehekili Fluctus)是木星的卫星—木卫一上的一处熔岩流场,该熔岩流 (被流体覆盖的陆地,该术语主要用于金星、木卫一和土卫六的地貌)位于南纬17.68度、西经33.56度处,如右图所示,图中还有位于中间的卡涅赫基里火山口,坐标南纬18.21度、西经33.6度。该熔岩场约覆盖了34500公里2(13300英里2)的区域,伽利略探测器的固态成像设备(SSI)在轨道上探测到了该热点。 卡涅赫基里和(Janus Patera)区之所以受到关注,是因为有迹象表明那里存在一座活跃、翻腾的熔岩湖。根据热排放数据,该区域与佩莱区几乎完全相同,而佩莱区被认为是一座活跃、汹涌的熔岩湖所在地。木卫一上的熔岩流区被以各种神话中的火神和雷神或是希腊神话中与伊娥有关的地点命名。卡涅赫基里熔岩流可能是一种硅酸盐熔岩流,其中最黑、最年轻的区域大约有16500公里2(6400英里2)。通过对热辐射观察得出的结论,卡涅赫基里熔岩流属于间歇性火山活动,即在经过一段时间的爆炸性喷发后,接下来会进入一段不活跃期,随着时间的推移,对冷却熔岩流的探测可能变得更困难。喷发后,接下来会进入一段不活跃期,随着时间的推移,对冷却熔岩流的探测可能变得更困难。
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http://dbpedia.org/property/mapCaption This image is clipped from the USGS Io Global Mosaic . Green stars denote the position of hot spots detected by Galileo SSI.
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rdfs:comment Il Kanehekili Fluctus è una struttura geologica della superficie di Io. , Kanehekili Fluctus is a lava flow field onKanehekili Fluctus is a lava flow field on Jupiter's moon, Io. This fluctus (terrain covered by outflow of liquid, used on Venus, Io and Titan) is located in the sub-Jovian hemisphere at 17°41′S 33°34′W / 17.68°S 33.56°W as shown in the picture on the right. Also in the picture is the Kanehekili volcanic center located at 18°13′S 33°36′W / 18.21°S 33.6°W.This lava field covers roughly 34,500 square kilometres (13,300 sq mi). The hotspot was detected by the Galileo Solid State Imaging experiment (SSI) on orbits by Galileo.ing experiment (SSI) on orbits by Galileo. , 卡涅赫基里熔岩流(Kanehekili Fluctus)是木星的卫星—木卫一上的一处卡涅赫基里熔岩流(Kanehekili Fluctus)是木星的卫星—木卫一上的一处熔岩流场,该熔岩流 (被流体覆盖的陆地,该术语主要用于金星、木卫一和土卫六的地貌)位于南纬17.68度、西经33.56度处,如右图所示,图中还有位于中间的卡涅赫基里火山口,坐标南纬18.21度、西经33.6度。该熔岩场约覆盖了34500公里2(13300英里2)的区域,伽利略探测器的固态成像设备(SSI)在轨道上探测到了该热点。 卡涅赫基里和(Janus Patera)区之所以受到关注,是因为有迹象表明那里存在一座活跃、翻腾的熔岩湖。根据热排放数据,该区域与佩莱区几乎完全相同,而佩莱区被认为是一座活跃、汹涌的熔岩湖所在地。木卫一上的熔岩流区被以各种神话中的火神和雷神或是希腊神话中与伊娥有关的地点命名。卡涅赫基里熔岩流可能是一种硅酸盐熔岩流,其中最黑、最年轻的区域大约有16500公里2(6400英里2)。通过对热辐射观察得出的结论,卡涅赫基里熔岩流属于间歇性火山活动,即在经过一段时间的爆炸性喷发后,接下来会进入一段不活跃期,随着时间的推移,对冷却熔岩流的探测可能变得更困难。喷发后,接下来会进入一段不活跃期,随着时间的推移,对冷却熔岩流的探测可能变得更困难。
rdfs:label Kanehekili Fluctus , 卡涅赫基里熔岩流
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