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61 Cygni Trivia Questions

How much do you really know about 61 Cygni? Below are 8 true or false statements. Click each one to reveal the answer and explanation.

1.

61 Cygni is visible to the naked eye from suburban skies under good conditions.

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Easy
✗ FALSE

Its apparent magnitude of about 5.2 makes it faintly visible only from very dark rural skies; it's easily lost in suburban light pollution.

2.

61 Cygni was the first star to have its distance measured via parallax.

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Medium
✓ TRUE

In 1838, Friedrich Bessel used parallax to measure 61 Cygni's distance, making it the first star (besides the Sun) with a known distance.

3.

61 Cygni has a high proper motion, moving across the sky faster than most naked-eye stars.

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Medium
✓ TRUE

Its rapid proper motion (about 5.2 arcseconds per year) earned it the nickname 'the Flying Star' and made it famous for early astrometry.

4.

61 Cygni was the first star (other than the Sun) to have its distance measured by parallax.

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Medium
✓ TRUE

In 1838, Friedrich Bessel successfully measured its parallax, making 61 Cygni the first star beyond the Sun with a known distance.

5.

61 Cygni's two stars are so close that they exchange material and erupt as novae every few centuries.

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Hard
✗ FALSE

They are a wide binary (about 85 AU apart) and do not exchange mass. No novae have been observed from this system.

6.

In the 1940s, 61 Cygni was suspected to have a planet based on wobbles in its motion.

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Hard
✓ TRUE

Early astrometric data suggested a planetary companion, but later observations using better instruments disproved it—a classic false positive.

7.

61 Cygni will make its closest approach to the Sun in about 20,000 years, passing within 9 light-years.

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Hard
✓ TRUE

Due to its high proper motion and radial velocity, it will reach perihelion around 20,000 AD at about 9 light-years, still a safe distance.

8.

61 Cygni is actually a triple star system, consisting of two K-type stars and a white dwarf companion.

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Hard
✗ FALSE

61 Cygni is a binary system of two K-type main-sequence stars (A and B). No white dwarf companion has been confirmed; a suspected third star was disproven.

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