Do I need my own telescope to participate?

No; you can use public datasets during the class, but bringing your own gear allows hands-on imaging practice.

What level of astronomy knowledge is required?

This is an intermediate class and assumes basic familiarity with telescopes and night-sky navigation.

Can I submit my measurements to scientific databases?

Yes; the class shows how to prepare and format photometric measurements for citizen-science projects.

Is the class suitable for teens?

Age limits are not specified, but intermediate-level concepts mean motivated teens with prior experience will benefit.

What happens in poor weather?

If clear-sky observing is impossible, instructors focus on data analysis using archival observations and public datasets.

How large are class groups?

Sessions can accommodate up to 35 participants, making them suitable for small groups and community learning.

Tracking the Light: Photometry Class at cincinnatiobservatory in Cincinnati, Ohio

Tracking the Light: An Introduction to Photometry takes place at cincinnatiobservatory in Cincinnati, Ohio, and opens a doorway from backyard stargazing into real scientific contribution. In a focused 1.5-hour session aimed at intermediate hobbyists, the class translates the flicker of distant suns into measurable data—showing how changes in brightness reveal exoplanets, variable stars, asteroids, and supernovae. Inside a compact classroom and under the observatory’s dome, instructors walk students through photometry fundamentals: precise measurements of stellar brightness, calibration frames, signal-to-noise tradeoffs, and constructing light curves from images or public datasets. The setting is urban but intentional; Cincinnati’s sky often reveals bright planets, seasonal constellations, and the isolated pinpricks needed for differential photometry. The experience emphasizes hands-on practice—participants can bring their own telescopes and cameras or work with public data to extract scientifically useful measurements that can be submitted to citizen-science projects. Key features of the session include guided use of a telescope aperture and CCD/CMOS image considerations, live demonstrations of measuring a star’s flux, and step-by-step assembly of a light curve. Unique natural elements here are the interplay between city-affected skies and sufficiently dark patches that still permit meaningful photometric work; seasonal targets shift from winter’s crisp constellations to summer’s dense Milky Way fields. Cultural notes: the class invites amateur contribution to ongoing research, continuing a long tradition of volunteer observers supporting professional astronomy. Why book this class? It’s a rare chance in a midwestern city to move beyond pretty astrophotos and learn the methods scientists use to confirm exoplanets or track asteroid brightness. For travel planners, the course is short, affordable, and scalable—up to 35 people—making it suitable for solo learners, couples, or small groups looking to add depth to a Cincinnati trip. Practical details: intermediate-level prerequisite knowledge of telescopes is assumed; the pace is brisk but approachable. Bring a laptop for data work, and a red-filtered light for night sessions. Expect a mix of lecture, guided demonstration, and hands-on analysis. The tangibility of producing a publishable light curve is rewarding; the class transforms night-sky wonder into a repeatable observational skill. Whether you want to contribute to an exoplanet transit detection or simply sharpen your astrophotography technique, this photometry introduction is a compact, high-impact way to track the light. The class also connects you with a community of local amateur astronomers—seasonal star parties, data-sharing sessions, and follow-up workshops often crop up through the same network. For visitors, combining this class with an evening walk along Cincinnati’s riverfront or a morning visit to nearby parks can turn a single lesson into a short science-focused escape. Instructors emphasize repeatable technique so participants leave able to produce comparable results on different nights and under varied sky conditions. Bring curiosity; expect immediate observational payoffs.