k Telescope domes on Mauna Kea with HaleBo Keck I and II with comet. Composite image of comet HaleBopp seen above the Keck I and II telescope domes on Mauna Kea, Hawaii, USA. The optical telescopes of Keck I and II each have a 10 metre diameter mirror, which can be used together to provide more detailed images. Mauna Kea, an extinct volcano 4200 metres high, has several telescopes on its summit. Comet HaleBopp, seen in early 1997, was one of the brightest comets of the 20th century. Here, its two tails are seen. The gas or ion tail blue consists of ionised glowing gas blown away by the solar wind. The dust tail white consists of dust grains pushed away from the comet head by the radiation of sunlight. Stock Photo - Afloimages
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Telescope domes on Mauna Kea with Hale Bo Keck I and II with comet. Composite image of comet Hale Bopp seen above the Keck I and II telescope domes on Mauna Kea, Hawaii, USA. The optical telescopes of Keck I and II each have a 10 metre diameter mirror, which can be used together to provide more detailed images. Mauna Kea, an extinct volcano 4200 metres high, has several telescopes on its summit. Comet Hale Bopp, seen in early 1997, was one of the brightest comets of the 20th century. Here, its two tails are seen. The gas or  ion  tail  blue  consists of ionised glowing gas blown away by the solar wind. The dust tail  white  consists of dust grains pushed away from the comet head by the radiation of sunlight.
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Telescope domes on Mauna Kea with Hale-Bo

Keck I and II with comet. Composite image of comet Hale-Bopp seen above the Keck I and II telescope domes on Mauna Kea, Hawaii, USA. The optical telescopes of Keck I and II each have a 10 metre diameter mirror, which can be used together to provide more detailed images. Mauna Kea, an extinct volcano 4200 metres high, has several telescopes on its summit. Comet Hale-Bopp, seen in early 1997, was one of the brightest comets of the 20th century. Here, its two tails are seen. The gas or 'ion' tail (blue) consists of ionised glowing gas blown away by the solar wind. The dust tail (white) consists of dust grains pushed away from the comet head by the radiation of sunlight.

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