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Despite extensive searches and the relative proximity of solar system objects(SSOS) to Earth, many remain undiscovered and there is still much to learnabout their properties and interactions. This work is the first in a seriesdedicated to detecting and analyzing SSOs in the all-sky NOIRLab Source Catalog(NSC). We search the first data release of the NSC with CANFind, aComputationally Automated NSC tracklet Finder. NSC DR1 contains 34 billionmeasurements of 2.9 billion unique objects, which CANFind categorizes asbelonging to "stationary" (distant stars, galaxies) or moving (SSOs) objectsvia an iterative clustering method. Detections of stationary bodies for propermotion (mu) less than 2.5"/hr (0.017 degrees/day) are identified and analyzedseparately. Remaining detections belonging to hi-mu objects are clusteredtogether over single nights to form "tracklets". Each tracklet containsdetections of an individual moving object, and is validated based on spatiallinearity and motion through time. Proper motions are then calculated and usedto connect tracklets and other unassociated measurements over multiple nightsby predicting their locations at common times forming "tracks". This methodextracted 527,055 tracklets from NSC DR1 in an area covering 29,971 squaredegrees of the sky. The data show distinct groups of objects with similarobserved mu in ecliptic coordinates, namely Main Belt Asteroids, JupiterTrojans, and Kuiper Belt Objects. Apparent magnitudes range from 10-25 mag inthe ugrizY and VR bands. Color-color diagrams show a bimodality of trackletsbetween primarily carbonaceous and siliceous groups, supporting prior studies.

Exploring the Solar System with the NOIRLab Source Catalog I: Detecting Objects with CANFind