  Despite extensive searches and the relative proximity of solar system objects
(SSOS) to Earth, many remain undiscovered and there is still much to learn
about their properties and interactions. This work is the first in a series
dedicated to detecting and analyzing SSOs in the all-sky NOIRLab Source Catalog
(NSC). We search the first data release of the NSC with CANFind, a
Computationally Automated NSC tracklet Finder. NSC DR1 contains 34 billion
measurements of 2.9 billion unique objects, which CANFind categorizes as
belonging to "stationary" (distant stars, galaxies) or moving (SSOs) objects
via an iterative clustering method. Detections of stationary bodies for proper
motion (mu) less than 2.5"/hr (0.017 degrees/day) are identified and analyzed
separately. Remaining detections belonging to hi-mu objects are clustered
together over single nights to form "tracklets". Each tracklet contains
detections of an individual moving object, and is validated based on spatial
linearity and motion through time. Proper motions are then calculated and used
to connect tracklets and other unassociated measurements over multiple nights
by predicting their locations at common times forming "tracks". This method
extracted 527,055 tracklets from NSC DR1 in an area covering 29,971 square
degrees of the sky. The data show distinct groups of objects with similar
observed mu in ecliptic coordinates, namely Main Belt Asteroids, Jupiter
Trojans, and Kuiper Belt Objects. Apparent magnitudes range from 10-25 mag in
the ugrizY and VR bands. Color-color diagrams show a bimodality of tracklets
between primarily carbonaceous and siliceous groups, supporting prior studies.
