What the Life Cycle of a Star Can Teach Us About This School Year

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If I remember my high school science classes correctly, stars like our sun spend a good long time burning brightly at the center of their solar systems, providing the light and heat and gravity that keep everything moving and, in our case, alive. But as many a poet reminds us, all good things must come to an end. Eventually, once their hydrogen is gone and after brief explosions, most stars settle into new existences that consist of gradual cooling and general diminishing of their once radiant dominance.

I’ve been thinking about the life cycle of a star a lot in regards to this school year, as there are a few similarities. Generally speaking, the role of teacher has long been to be the undisputed sun at the center of her/his/their classroom. The classwork, class structure, and class community have all traditionally orbited around the teacher, with the students acting as satellites of sorts, satellites whose trajectory is almost wholly dependent on the sun they orbit.

But last spring after our educational systems largely exploded, many teachers faced a reality that was not unlike the reality that a star faces after it has blown up. Anyone who has spent more than five minutes on a Zoom call likely knows that even the most dynamic presenters just don’t shine as brightly on Zoom as they do in person, and the gravitational pull of a class from a distance just isn’t the same as when thirty five bodies are all crammed together in a 500 sq. ft. room.

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