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Stephan's Quintet Trivia Questions

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

1.

The quintet is visible to the naked eye under dark skies as a faint smudge of light.

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Easy
✗ FALSE

The combined magnitude is around 13, far too dim for naked-eye viewing; a moderate telescope is needed to resolve the group.

2.

The galaxy group was discovered by French astronomer Édouard Stephan in 1877.

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Easy
✓ TRUE

Édouard Stephan first observed the quintet at the Marseille Observatory, making it the first compact galaxy group ever identified.

3.

Stephan's Quintet is a visual grouping of five galaxies, but only four are actually interacting.

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Medium
✓ TRUE

The fifth galaxy, NGC 7320, is a foreground interloper about seven times closer to Earth, not part of the tight group.

4.

All five galaxies in Stephan's Quintet are gravitationally bound and will eventually merge into one giant galaxy.

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Medium
✗ FALSE

Only four are bound; the fifth is a foreground galaxy not interacting. The bound four are indeed merging over billions of years.

5.

Stephan's Quintet was the first galaxy group ever photographed by the James Webb Space Telescope.

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Medium
✗ FALSE

Webb's first deep field image in 2022 included SMACS 0723, not Stephan's Quintet, though the quintet was released separately.

6.

Stephan's Quintet is the only known compact galaxy group with an interloper galaxy in the foreground.

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Hard
✗ FALSE

Several other compact groups, like Hickson 90, also contain foreground interlopers; it's not unique.

7.

The quintet is located about 40 million light-years from Earth in the constellation Pegasus.

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Hard
✓ TRUE

While some members are at 290 million light-years, the foreground interloper is about 40 million light-years away, causing common confusion.

8.

Stephan's Quintet contains a supermassive black hole actively feeding and producing powerful radio jets.

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Hard
✓ TRUE

One member, NGC 7319, harbors an active galactic nucleus with radio jets, revealed by X-ray and radio observations.

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