Cosmos Week
Check out the Double Cluster in Perseus on October evenings
Earth scienceEnglish editionScience journalismJournalistic coverage

Check out the Double Cluster in Perseus on October evenings

The Double Cluster in Perseus is a breathtaking pair of open star clusters, easy to see in October. Here's how to find it in your sky.

Original source cited and editorially framed by Cosmos Week. EarthSky
Editorial signatureCosmos Week Editorial Desk
Published11 Oct 2026 08: 00 UTC
Updated2026-10-11
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: The Double Cluster in Perseus is a breathtaking pair of open star clusters, easy to see in October
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

The Double Cluster in Perseus is a breathtaking pair of open star clusters, easy to see in October. Here's how to find it in your sky. The post Check out the Double Cluster in Perseus on October evenings first appeared on EarthSky. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

It is relevant because Earth science becomes stronger when local observations can be placed inside a broader physical pattern that spans time and geography. The planet operates as a coupled system in which atmospheric, oceanic, cryospheric and solid-Earth processes interact across timescales from days to millions of years. A measurement that captures one variable at one location and one moment has limited interpretive value until it is embedded in the longer series and wider spatial coverage that allow natural variability to be separated from forced change. Subscribe to EarthSky’s free daily newsletter for the latest in science, stars, planets and more. These two star clusters are located about 7, 500 light-years away.

Scan the area between them with binoculars and you’ll find the 2 glittering star clusters. Of course, Charles Messier (1730-1817) was looking for deep-sky objects that could be mistaken for comets.

The position of h Persei is Right Ascension: 2h 19m. 57 o 9′ north The position of chi Persei is Right Ascension: 2h 22.4m.

57 o 7′ north The Double Cluster from our EarthSky Community View at EarthSky Community Photos. | Makrem Larnaout in Tunisia made this 34-hour telescopic exposure of the Double Cluster in Perseus with surrounding nebulosity on October 1, 2024.

The broader interest lies in linking the observation to climatic, geophysical or environmental dynamics that extend well beyond the immediate event or location. Earth science is unusual in that its most important questions operate on timescales that no single research career can observe directly, making the archival record, whether in ice, sediment, rock or satellite data, as important as any new measurement. Results that can be embedded in that record, and that either confirm or challenge the patterns it reveals, carry disproportionate scientific weight.

Here’s a new image of the stunning Double Cluster in the constellation Perseus, captured over several nights with the Skywatcher ED80 Esprit and ZWO ASI 2600MC. | Jeremy Likness in Newport, Oregon, captured this telescopic view of the Double Cluster in the constellation Perseus on November 24, 2023.

Because this item comes through EarthSky as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to place the result inside longer time series and to compare it with independent instruments and independent sites. Earth system observations gain most of their interpretive power from network density and temporal depth, not from any single measurement however precise. Model simulations that assimilate the new data will help clarify whether the observation fits comfortably within known natural variability or represents a shift that existing models do not reproduce.

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