Brian G. Marsden’s orbit calculation indicated that on January 22, 2002, Comet LINEAR, C/2000 WM1, would pass just 0.55 astronomical unit (82 million kilometers) from our star. As it begins to draw away from Earth, we might expect the comet to fade. But the effect is almost perfectly offset by its brightening as it approaches the Sun. The net result is that from early in December until the first days of February the magnitude should remain close to 5. All the while, the comet’s coma should steadily shrink in angular extent and look progressively more condensed.Throughout this interval Comet LINEAR’s elongation from the Sun in the evening sky will be diminishing. Even so, it will never become lost in the Sun’s glare. Around the date of perihelion passage, January 22nd, the gossamer little visitor to our solar neighborhood is in the constellation Indus, well south of the Sun. Southern Hemisphere observers can catch sight of it twice each night, first during evening twilight and then again toward dawn.
February finds the comet marching northward once again, but its elongation from the Sun is slow to increase, so that it hovers near the dawn’s glow. Now in a rapid retreat from the Sun, Comet LINEAR will quickly become a binocular object and then a purely telescopic one. It also slowly returns into view for midnorthern observers during the second week of March. If all plays out as I expect, the comet could well stay within reach of quite modest telescopes throughout the spring.
One week after passing perihelion, Comet LINEAR brightened dramatically from magnitude 6.2 to 2.3 — a 35-fold increase over a 3-day period. Although it’s fading again, the details are available in this News item.