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Henrietta Leavitt's Cosmic Yardstick

How a quiet astronomer cataloging stars on photographic plates created a tool that measured the universe and changed astronomy forever.

Chapter 1

The Human Computer

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In 1895, Henrietta Swan Leavitt began work at the Harvard College Observatory. She was a 'computer,' one of several women hired by Director Edward Pickering to perform the painstaking calculations male astronomers were too busy for. Initially an unpaid volunteer, she was eventually hired at 30 cents per hour, less than half the salary of a man. Her task was to study variable stars, whose brightness fluctuates over time, by analyzing thousands of glass photographic plates. Leavitt undertook this meticulous work while suffering from progressive hearing loss that would eventually leave her profoundly deaf. She was assigned a specific patch of sky to study: a faint, fuzzy object known as the Small Magellanic Cloud.

Frequently Asked Questions

Who was Henrietta Leavitt?

Henrietta Swan Leavitt was an American astronomer who worked at the Harvard College Observatory in the early 20th century. Hired as a 'computer,' she meticulously analyzed photographic plates of stars. Despite suffering from profound deafness, her work led to a groundbreaking discovery about the universe.

What is Leavitt's Law?

Leavitt's Law, or the period-luminosity relationship, is the discovery that for a certain type of pulsating star, its brightness is directly related to the time it takes to pulse. This means by timing a star's pulse, astronomers can determine its true brightness. This allows them to calculate its distance from Earth.

Why was Henrietta Leavitt's discovery so important?

Her discovery provided the first 'standard candle' to measure cosmic distances far beyond what was previously possible. Astronomer Edwin Hubble used her law to prove that the Andromeda Nebula was a separate galaxy, not a gas cloud in our own. This discovery revealed the true, vast scale of the universe.

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