Outstanding in planet Earth's sky [
http://www.spacewea
gallery_mcnaught_pag e23.php ] early this year, Comet McNaught [
http://en.wikipedia
] is captured in this view from the STEREO [
http://stereo.gsfc.
] A spacecraft. McNaught's coma [
http://www.nasa.gov
] is so bright, it blooms [
http://www.cs.duke.
faq.html#blooming ] into the long horizontal stripe at the bottom of the field. Brilliant Venus, near the top left corner, also produces a severe horizontal blemish in the digital image. But the sensitive camera does accurately record the striations in McNaught's famous dust tail [
http://antwrp.gsfc.
] along a region stretching over 30 million kilometers toward the top right of the field of view. A separate, fainter, arching tail just to the left of the dust tail was initially thought to be an example of a common ion tail [
http://www.ifa.hawa
], formed by electrically charged atoms [
http://www.chem4kid
] carried away from the comet by the solar wind [
http://www.phy6.org
]. However, detailed [
http://www.swissedu
] modeling indicates that tail is actually due to neutral iron atoms pushed out by the pressure of sunlight [
http://www.phy6.org
] -- the first ever detected neutral iron tail from a comet. The iron atoms are thought to originate in dust grains [
http://stardust.jpl
] from the comet nucleus [
http://antwrp.gsfc.
] that contain the iron-sulfur mineral troilite [
http://www.mindat.o
] (FeS).
Explanation
Outstanding in planet Earth's sky [
http://www.spacewea
gallery_mcnaught_pag e23.php ] early this year, Comet McNaught [
http://en.wikipedia
] is captured in this view from the STEREO [
http://stereo.gsfc.
] A spacecraft. McNaught's coma [
http://www.nasa.gov
] is so bright, it blooms [
http://www.cs.duke.
faq.html#blooming ] into the long horizontal stripe at the bottom of the field. Brilliant Venus, near the top left corner, also produces a severe horizontal blemish in the digital image. But the sensitive camera does accurately record the striations in McNaught's famous dust tail [
http://antwrp.gsfc.
] along a region stretching over 30 million kilometers toward the top right of the field of view. A separate, fainter, arching tail just to the left of the dust tail was initially thought to be an example of a common ion tail [
http://www.ifa.hawa
], formed by electrically charged atoms [
http://www.chem4kid
] carried away from the comet by the solar wind [
http://www.phy6.org
]. However, detailed [
http://www.swissedu
] modeling indicates that tail is actually due to neutral iron atoms pushed out by the pressure of sunlight [
http://www.phy6.org
] -- the first ever detected neutral iron tail from a comet. The iron atoms are thought to originate in dust grains [
http://stardust.jpl
] from the comet nucleus [
http://antwrp.gsfc.
] that contain the iron-sulfur mineral troilite [
http://www.mindat.o
] (FeS).
Explanation