Here Comes Comet Linear
Comet LINEAR-S4 was discovered on September 27, 1999, by the Lincoln Near-Earth Asteroid Research program in New Mexico. It appears to be a first-time visitor to the inner solar system traveling in an orbit that will return it beyond distant Pluto after it passes 114 million km from the Sun on July 26, 2000.
Right: This time-lapse sequence of Comet LINEAR-S4 was taken on July 2, 2000, from Arizona and shows the comet's movement over only 19 minutes. Credit & Copyright: Wil Milan
"Estimating how bright this comet will become is tricky," says an astronomer at the NASA Marshall Space Flight Center. "Comet LINEAR hasn't been here before so we can't use past experience as a guide."
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Nevertheless, comet LINEAR-S4 could be a beautiful sight as it moves through the relatively star-poor area around the Big Dipper in late July. In fact, if the comet reaches 4th magnitude it will probably resemble another popular fuzzy blob, our nearest neighboring galaxy, the Andromeda Nebula. Experts stress that predicting what LINEAR-S4 will do is more of an art than hard science. The comet might fail to develop or it could be far more striking than expected.
Above: Comet LINEAR-S4 is expected to reach peak brightness around July 23, 2000. Skywatchers in the northern hemisphere should look for the comet near the Big Dipper around 9 p.m. local time approximately 30 degrees above the northern horizon. Although the comet will appear to be stationary when viewed for a short time, it is actually moving 8 degrees per day with respect to background stars. (The bowl of the Big Dipper is 10 degrees across.) The comet will move past the Big Dipper in just a few days. To view finder charts for other dates, visit Sky & Telescope and CometLinear.com. Note for Southern Hemisphere observers: when comet LINEAR is brightest on July 23 it will be impossible to view from most southern latitudes as it rises just a few degrees above the horizon during the day. In August the fading comet will be a good target for southern telescopes for a few hours after sunset.
LINEAR-S4 is expected to become a naked-eye object around July 17, 2000, when it brightens to 6th magnitude. Even if the comet eventually reaches 4th magnitude, it will be invisible in light polluted urban areas. Dark skies are essential. For comet watchers, this is a good time for a vacation in the country!
The comet will fade after its closest approach to our planet on July 23rd and by the end of July, LINEAR-S4 it will be too dim for naked-eye observations. It will remain a good target for binoculars and small telescopes well into September. On August 20th, telescopic observers in the southern hemisphere will be treated to a rare sight when the 7th magnitude comet passes almost directly in front of the Sombrero galaxy M104. [See Sky & Telescope for more information.]
Right: This 10-minute exposure of comet LINEAR S4 was captured in Austria on June 28, 2000. Copyright © 2000 by Michael Jäger and Gerald Rhemann.
Although we probably won't see comet LINEAR-S4 again after this summer, it's almost certainly not the last "Comet LINEAR." The LINEAR project has discovered more than 40 new comets since 1998 and shows no signs of slowing.
Will this Comet LINEAR be worth watching? Only time will tell. The best way to find out is to go outside and look!
Science@NASA readers are invited to send their descriptions and photos of Comet LINEAR to the editor for possible inclusion in future articles about this comet.
Right: This image of Comet Halley's nucleus was taken by the European Space Agency Giotto spacecraft during a flyby on March 13, 1986. Scientists estimate that about 10% of the surface was boiling off into space. The stuff that boiled off Halley in 1986 may one day be seen again during an eta Aquarid meteor shower.
Above: This photograph of Comet Hyakutake highlights different components of the tail. The gold and red tail features are dust, made predominately of little bits of rock and carbon. The dust tail shines by reflecting sunlight. Extending past the dust tail is the comet's ion tail, shown here glowing in blue. The ion tail is composed mostly of ions of water, carbon monoxide, and cyanogen. The ion tail glows by emitting light when elections re-combine with electrically charged ions to make uncharged molecules.
Orbital Elements of C/1999 LINEAR S4 - from the Harvard Center for Astrophysics
Daily Ephemeris for C/1999 LINEAR S4 - from the Harvard Center for Astrophysics
CometLinear.com -pictures, updates, and a discussion board for observers of comet Linear.
Comet LINEAR's Summer Show - from Sky & Telescope, includes detailed finder charts and ephemerides.
C/1999 S4 (LINEAR) -- images and historical highlights from Gary Kronk's popular Comets & Meteors web site.
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|For lesson plans and educational activities related to breaking science news, please visit Thursday's Classroom||Author: Dr. Tony Phillips
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