We describe a low-cost compact grism spectrometer for use with small astronomical telescopes. The system can be used with existing charge-coupled device (CCD) cameras and filter wheels. The optical design consists of two prisms, a transmission grating, a collimating lens, and a focusing lens, all enclosed in a 3D-printed housing. The system can be placed inline, typically in an unused filter wheel slot. Unlike conventional spectrometers, it does not require the target to be precisely positioned on a narrow slit. The mean resolving power (R 300) is sufficient to resolve the spectral lines of many astronomical objects discussed in undergraduate astronomy labs, such as stellar absorption lines along the main-sequence, emission lines of early type hot stars and galactic novae, and redshifts of bright quasars and supernovae.

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