  The goal of this investigation is to reinterpret and upgrade the astrometric
and other data on comet C/1945 X1, the least prominent among the Kreutz system
sungrazers discovered from the ground in the 20th century. The central issue is
to appraise the pros and cons of a possibility that this object is --- despite
its brightness reported at discovery --- a dwarf Kreutz sungrazer. We confirm
Marsden's (1989) conclusion that C/1945 X1 has a common parent with C/1882 R1
and C/1965 S1, in line with the Sekanina-Chodas (2004) scenario of their origin
in the framework of the Kreutz system's evolution. We integrate the orbit of
C/1882 R1 back to the early 12th century and then forward to around 1945 to
determine the nominal direction of the line of apsides and perform a Fourier
analysis to get insight into effects of the indirect planetary perturbations.
To better understand the nature of C/1945 X1, its orbital motion, fate, and
role in the hierarchy of the Kreutz system as well as to attempt detecting the
comet's possible terminal outburst shortly after perihelion and answer the
question in the title of this investigation, we closely examined the relevant
Boyden Observatory logbooks and identified both the photographs with the
comet's known images and nearly 20 additional patrol plates, taken both before
and after perihelion, on which the comet or traces of its debris will be
searched for, once the process of their digitization, currently conducted as
part of the Harvard College Observatory's DASCH Project, has been completed and
the scanned copies made available to the scientific community.
