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May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996xmm..pres...11.&link_type=abstract
XMM Press Release INFO 11-1996
Other
Scientific paper
LASCO is a joint project between NRL (USA), the Max Planck Institut für Aeronomie (Germany), the Laboratoire d'Astronomie Spatiale (France), and the School of Physics and Space Research at the University of Birmingham (UK).
"Such observations require a special instrument in space to suppress the glare of the Sun and reveal the comet and its tails", said Dr. Guenter Brueckner, NRL's principal investigator for LASCO. Scattering of sunlight in the Earth's atmosphere prevented good views from the ground during the comet's "perihelion passage" when it was closest to the Sun. The orbital period of Comet Hyakutake has been estimated to be 10,000 years. Hyakutake is called a "new" comet because it was not seen when, and if, it last visited the solar system. As Hyakutake approaches the Sun, it is being heated enormously. If this is the first visit of the comet, it could be broken into pieces, according to scientists.
Images captured by the LASCO instrument have shown that this did not happen when the comet was in LASCO's field of view, which is approximately the size of the constellation Orion. "Comet Hyakutake could have passed through the solar system many times before", said Dr. Brueckner, who is also head of the NRL's Solar Physics Branch. "How many times remains a mystery".
Hyakutake's orbit carries it back into the so-called "Oort Cloud" a vast collection of billions of comets that is located 1.4 light years away from the solar system. These comets are presumably the remnants of the cloud from which the solar system were formed billions of years ago.
When the comet enters the outer atmosphere of the Sun, it begins to react with the Sun's environment and can be used as a "probe" of the solar corona. LASCO images show the head of the comet, and clearly visible are three separate tails that behave differently as Hyakutake swings around the Sun. These tails are made of different materials ; dust of different sizes, perhaps chunks of ice and atomic particles, each of which reacts differently with their environment. The heavy particles follow the comet in its orbit without being redirected by an outside force while the light dust particles are lining up away from the Sun and are driven by the Sun's intensive radiation. Finally, the atomic particles are repelled from the comet by the solar wind and presumably line up with the magnetic field of the solar corona.
As the comet speeds through the corona at 37 miles per second, these forces have direct influence on its tails, which could clearly be seen changing their relative direction over the seven-day observation period.
Coronal mass ejections were also observed by LASCO, in which hot gases were expelled and accelerated by the corona's magnetic field to travel through the interplanetary medium. A strong reaction between such a solar high-speed cloud and the portion of the comet's tails made of atomic particles is expected when Hyakutake crosses the equatorial plane of the Sun. The comet was out of LASCO's field of view during this crossing, but the scientists will have another opportunity when Hyakutake reappears from behind the Sun and can be seen later in the southern hemisphere's night sky with ordinary telescopes.
Researchers expect to learn more about the tails of the comet and the surrounding solar corona with more detailed analysis.
SOHO is a project of international cooperation between ESA and NASA. More information can be found on the LASCO Comet Hyakutake page on the World Wide Web http://lasco-www.nrl.navy.mil/b2-1996.html and on the SOHO home page http://sohowww.nascom.nasa.gov.
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