The story of Galileo Galilei versus the Catholic Church is usually told as a simple drama: enlightened science crushed by religious prejudice. We know this narrative is wrong, as I discussed previously on my blog (Revisiting the Galileo Affair).
But did you know that Galileo tried to measure stellar parallax to prove the Copernican heliocentric system, that his experiment failed, and that he did not tell anyone? – This really struck me.
Here is the story:
In 1617, Benedetto Castelli asked Galileo to observe Mizar, a star that appears single to the naked eye but reveals itself as a double star when seen through a telescope.

Galileo was an important figure, and so was Castelli. He was a Benedictine monk, mathematician, and astronomer — first a student and later a close friend of Galileo. He defended Galileo and the Copernican system throughout Galileo’s troubles with Church authorities. In 1613, when Galileo decided to defend himself publicly against some of his accusers, he chose to do so by means of an open letter addressed to Castelli.
Galileo realized that the double star Mizar could be used to observe stellar parallax and thus confirm heliocentrism. “He observed them [both stars] meticulously for a year, but saw no parallax. He recognized this as observational evidence, given the state of astronomical knowledge at the time, that Earth does not go around the sun,” explains Tim Thompson, former physicist at NASA’s Jet Propulsion Laboratory in California [1].
What Galileo did not know was that the real distances of these stars from us are orders of magnitude greater than his calculations suggested. “Nobody understood optics well enough to realize that the apparent stellar disk they saw in telescopes was just an optical artifact (the Airy disk). They thought it was the physical disk of the star, and therefore all of them, Galileo included, seriously underestimated the distances to the stars, assuming they must be nearby and therefore must also show parallax,” says Thompson.
Galileo could not observe stellar parallax, and this was strong counter-evidence against heliocentrism. What did Galileo do? “He hid his observations and never told anyone what he had discovered.”
Hide observations and tell nobody? Scientists perform experiments and make observations to test their hypotheses, and based on these results, they refine their hypotheses in order to arrive at a strong theory. I told this at various occasions to my high-school students during my recent 18-month assignment teaching Biology and Chemistry. I used this graph for illustration of the scientific method:

And if Galileo hid his results, how do we know?
Several historians of astronomy [2] investigated Galieo’s notes and the correspondence between Galilei and Castelli and found reasonable evidence that Galileo tried for several years to find stellar parallax, not only looking at Mizar but also other double stars between 1617 and 1627, on his own and upon Castelli’s request.
But there is even more to say about Galileo’s lack of scientific transparency. In 1632, Galileo wrote:
“I do not believe that the stars are spread over a spherical surface at equal distances from one center; I suppose their distances from us vary so much that some are two or three times as remote as others. Thus if some tiny star were found by the telescope quite close to some of the larger ones, and if that one were therefore very very remote, it might happen that some sensible alterations would take place among them.”
Chris Graney, astronomer and historian of science from the Vatican Observatory, indicates [3] that Galileo proposes — using the word “if” — that parallax might be observable with double stars at different distances from each other. Yet, he does not mention that he had already found such a pair in 1617 and had not observed any differential parallax. He says, “Should Galileo have published his double star observations? Certainly. From a scientific standpoint, if he is going to promote the ideas that Earth circles the sun, and that the stars are sun-sized bodies at varying distances from Earth — and that for these reasons a double star might reveal differential parallax and thus appear in court to give witness that Earth does in fact move — then, yes, he should also mention that he has already observed exactly the sort of double star system that he describes, and that those observations contradict the ideas he is promoting. When Galileo wrote in the Dialogue about how ‘if some tiny star were found by the telescope’ close to a large star, he was sitting on exactly that sort of observation, right in his notebooks. Scientifically speaking, that’s definitely not cool.”
And he concludes: “Galileo was a great scientist. He should be honored as one of the greats. But, in trying to prove that the Earth moved, he did stuff that scientists are not supposed to do. Galileo was not punished for proving that Earth moved. But some of the things he did while trying to prove Earth’s motion would get him in trouble in the scientific world today.”
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Stellar parallax was first measured by Friedrich Bessel in 1838. In 1851, the Earth’s rotation was demonstrated with Foucault pendulum. The decisive evidence Galileo sought did exist — but it required instruments, theoretical insight, and physical understanding that lay beyond his century.
Galileo was right about the Earth’s motion. He was wrong about the distances of the stars. And when his own careful observations failed to support his expectations, he chose silence instead of transparency.
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[1] Tim Thompson on facebook (16 Feb 2026)
[2] Umberto Fedele (1949). Le prime osservazioni di stelle doppie. Leos Ondra (1999), A New View of Mizar.
Overview articles: Harald Siebert (2005). The Early Search for Stellar Parallax: Galileo, Castelli, and Ramponi. Journal fothe History of Astronomy, 36(3), 251–271. doi:10.1177/002182860503600301; Christopher Graney (2017). Strange Tales of Galileo and Proving: Telescopic Evidence for Earth’s Immobility through Double Stars, on the blog of Vatican Observatory. Christopher Graney (2024). The View of the Double Star Mizar, Twenty Years Later, on the blog of Vatican Observatory
[3] Christopher Graney, (2017), op.cit.







