NASA has announced plans to study Hale-Bopp using spacecraft, sounding rockets, and telescopes, as the giant comet approaches the Sun and brightens in the night sky.
A series of four sounding rocket launches, scheduled between March 24 and April 5, will allow observations of the comet at ultraviolet wavelengths. The launches, using two-stage Black Brant IX rockets, will take place at the White Sands Missile Range in New Mexico.
NASA will also use the Ulysses spacecraft, originally launched to study the Sun, to study the effects of the solar wind on the comet. The NASA/ESA spacecraft will examine what happens to the comet, particularly its plasma tail, as it passes through different solar wind conditions at different latitudes.
The Polar spacecraft, launched to study the magnetosphere, will also provide images of the comet in ultraviolet and visible wavelengths. Astronomers have already been using NASA's Infrared Telescope Facility (IRTF), a 3-meter (120-inch) telescope on Mauna Kea, Hawaii, to study the comet at infrared wavelengths.
One major spacecraft that will not be taking part in the study of Hale-Bopp will be the Hubble Space Telescope. The comet is currently too close to the Sun to allow the HST to safely observe the comet. The comet will not be far enough away to permit HST observations until this fall. Hubble took images of the comet from 1995 through October 1996.
The comet, which is up to 40 km (25 mi.) in diameter, is one of the largest comets ever seen. Although it will not pass close to the Earth, the comet is still a bright naked-eye object with a magnitude near zero. It is easily visible in the northern hemisphere in the eastern sky before sunrise and in the western sky just after sunset. The comet will become easier to see in the evening sky over the next several weeks.
[Editor's Note: For more information about Comet Hale-Bopp, including the most extensive list of Web sites devoted to the comet, visit http://www.seds.org/spaceviews/halebopp/ ]
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