This comet was
discovered by LINEAR as a magnitude 18.8 object on
There is some dispersion in
the light curve but the comet appears to be following the predictions that have
been made of a peak brightness around 11 close to perihelion..
The data shows that the
central condensation faded slightly in late 2002, although the total magnitude
continued to brighten. After a small break in the light curve the central
condensation continued to brighten again until early March 2003 when it has
started to fade rapidly.
From mid-March 2003 the
decrease in brightness has been dramatic and the central condensation has
suddenly and very rapidly faded.
This comet has been notable for the spectacular tail that it has shown and the considerable change in form with changing presentation and major activity.
CCD observations in a 10
arcsecond aperture by:
CCD aperture photometry
in apertures of 0'.2, 0'.3, 0'.5, 0'.6, 0'.7, 1'.0, 1'.1, 1'.2, 1'.3, 1'.4,
1'.6, 3'.2 by:
Total visual magnitude
estimates by:
Última actualización 05/06/2003
Por M.R.Kidger