k Halleys CometFirst major approach in 76 yearsMarch 12, 1986 BTHIS PICTURE MAY NOT BE USED TO STATE OR IMPLY BROES ENDORSEMENT OF ANY COMPANY OR PRODUCT. THIS PICTURE MAY NOT BE USED TO STATE OR IMPLY ROE ENDORSEMENT OF ANY COMPANY OR PRODUCT Optical image of comet Halley taken on March 12th 1986. It derives from the composition of three plates taken at blue, green and red wavelengths. The comet is characterised by two distinct tails. The plasma tail blue at centre right is produced by the interaction between the solar wind and the molecules of gases, such as carbon monoxide, sublimated from the nucleus. The dust tail faint at top right is formed by dust particles evaporated from the cometary nucleus and repelled by the radiation pressure of sunlight. Editorial Stock Photo - Afloimages
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Halley s Comet First major approach in 76 years  March 12, 1986   BTHIS PICTURE MAY NOT BE USED TO STATE OR IMPLY  BROE S ENDORSEMENT OF ANY COMPANY OR PRODUCT.     THIS PICTURE MAY NOT BE USED TO STATE OR IMPLY   ROE ENDORSEMENT OF ANY COMPANY OR PRODUCT     Optical image of comet Halley taken on March 12th 1986. It derives from the composition of three plates taken at blue, green and red wavelengths. The comet is characterised by two distinct tails. The plasma tail  blue at centre right  is produced by the interaction between the solar wind and the molecules of gases, such as carbon monoxide, sublimated from the nucleus. The dust tail  faint at top right  is formed by dust particles evaporated from the cometary nucleus and repelled by the radiation pressure of sunlight.
ED

Halley's Comet First major approach in 76 years (March 12, 1986)

^BTHIS PICTURE MAY NOT BE USED TO STATE OR IMPLY ^BROE'S ENDORSEMENT OF ANY COMPANY OR PRODUCT. *** THIS PICTURE MAY NOT BE USED TO STATE OR IMPLY ROE ENDORSEMENT OF ANY COMPANY OR PRODUCT *** Optical image of comet Halley taken on March 12th 1986. It derives from the composition of three plates taken at blue, green and red wavelengths. The comet is characterised by two distinct tails. The plasma tail (blue at centre right) is produced by the interaction between the solar wind and the molecules of gases, such as carbon monoxide, sublimated from the nucleus. The dust tail (faint at top right) is formed by dust particles evaporated from the cometary nucleus and repelled by the radiation pressure of sunlight.

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ID
10620046

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License type
Editorial

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Creation date
19-11-2010

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