Double Cluster - a dazzling twin set of star clusters in Perseus
Rising high in the autumn and winter skies of the Northern Hemisphere, the Double Cluster in Perseus is a stunning pair of open star clusters that offers one of the most visually rewarding views in the night sky. Officially cataloged as NGC 869 and NGC 884, these two dense clusters lie side by side, separated by only about half a degree — close enough to appear together in the same field of view with binoculars or a wide-field telescope.
The Double Cluster sparkles with hundreds of hot, young blue-white stars, many of them less than 15 million years old. Each cluster is impressive on its own, but when viewed together, they form a symmetric, jaw-dropping display that appears almost like a cosmic jewel box. With a low-power eyepiece, you’ll see a river of faint stars connecting them, and each cluster has its own character and arrangement of brighter stars.
They lie in the rich Milky Way region between Cassiopeia and Perseus, and are easily visible with the naked eye from dark skies as a faint, fuzzy patch. Through binoculars or a small scope, they explode into a shimmering star field — a perfect target for beginners, yet still a favorite of seasoned observers. No filters are needed — just a clear sky and a comfortable chair.
Whether you’re showing the night sky to friends or enjoying a solo observing session, the Double Cluster is a must-see — a timeless favorite for its beauty, accessibility, and starry abundance.
Double Cluster
Rating: 🟣 Showpiece Target
Level: 🟣 Very Easy
How:
When: Sep - Feb
🌟 Two Clusters in One View The Double Cluster gives you two rich open clusters side by side in the same field—each filled with hundreds of stars and separated by a narrow dark space. It’s a rare and beautiful pairing.
🌟 Spectacular in Binoculars and Small Telescopes Both clusters are bright, large, and well-spaced, making them ideal for binoculars and wide-field scopes. In modest apertures, they sparkle like celestial gemstones.
🌟 A Stunning Visual Scene NGC 869 and 884 are set against the Milky Way’s backdrop, creating one of the most awe-inspiring starfields in the northern hemisphere—perfect for casual viewing and star parties.
🌟 A Favorite for Beginners and Outreach The Double Cluster is always impressive, and requires no filters or complex equipment—making it a go-to target for stargazing newcomers.
🌟 Easy to Locate in Perseus Located between Cassiopeia and Perseus, it’s easily found using the “W” of Cassiopeia as a guide—high overhead in autumn and winter evenings.
🌟 Young, Hot, and Bright These clusters are only about 13 million years old, full of blue-white supergiants—offering a vivid example of young stellar populations.
Open cluster: a loose group of a few dozen to a few thousand young stars that formed together and are loosely bound by gravity.
Double Cluster
Find the constellation Cassiopeia. Look for the distinctive 'W' or 'M' shape in the northeaster sky in the fall, or overhead in winter. The two end stars in the "W" are Ruchbah and Segin -- these will help guide you in the next step.
Draw a triangle from Segin and Ruchbah downward toward Perseus about 7° on a side -- a bit less than the width of your fist. Look for the glow of the Double Cluster -- it should be visible in Bortle 1-4 skies. If you don't see it, simply estimate the location.
Using a binocular or telescope finder, point to the location of the Double Cluster. If you are using a telescope, scan the area with a low-powered eyepiece until you find the Double Cluster. Then explore.
Double Cluster
✅ Use binoculars for an ideal wide-field view. In 7x50 or 10x50 binoculars, both clusters appear as brilliant concentrations of stars, framed by the dense Milky Way. This is one of the best binocular objects in the sky.
✅ Use a low-power, wide-field eyepiece in a telescope. To fit both clusters in the same view, use magnifications of 40x to 70x with a wide field of view. This shows both groups with rich detail and the starry background between them.
✅ Observe from dark skies for maximum star contrast. Although the Double Cluster is bright enough for suburban skies, dark skies enhance the contrast and bring out more faint stars, giving the view a three-dimensional feel.
✅ Take your time exploring individual stars. Some stars in the clusters show subtle blue, gold, or orange hues. A slow, careful observation reveals these color contrasts, adding to the beauty.
✅ Let your eyes adapt fully to the dark. More stars emerge as your eyes adjust, especially in the outer halos of each cluster. Give yourself 20–30 minutes of darkness for best results.
✅ Use a small to medium telescope for optimal viewing. A 3- to 8-inch scope offers the perfect balance between field of view and resolution. Larger scopes can show even more stars but may require very low power to fit both clusters.
✅ Share it at outreach events. The Double Cluster is a crowd favorite—bright, beautiful, and easy to locate. It’s an excellent target for showing newcomers the beauty of star clusters.
Double Cluster
✅ Naked Eye
The Double Cluster, consisting of NGC 869 and NGC 884, appears to the naked eye as a faint hazy patch between the constellations Perseus and Cassiopeia, easily seen under dark skies and often mistaken for a single unresolved object.
✅ Binoculars
Through binoculars, the view transforms into two distinct, sparkling star clusters close together, suspended in a rich field of Milky Way stars; the contrast between the twin groupings and the surrounding space is both striking and beautiful.
✅ Small Telescope
In a small telescope, the Double Cluster becomes even more impressive, with dozens of individual stars coming into sharp focus, including some bright blue-white stars and subtle color contrasts that enhance its visual appeal.
✅ Medium Telescope
A medium telescope adds depth and richness, filling the field with hundreds of pinpoint stars and revealing slight differences in density, shape, and star brightness between the two clusters, while the dark lane of space separating them becomes more prominent.
✅ Large Telescope
In a large telescope, the field becomes densely packed with stars, and although both clusters remain visually distinct, the surrounding star field is so rich that the clusters almost melt into a glittering river of light—still spectacular, but best appreciated at low magnification where the full breadth and symmetry of this celestial pairing can be seen in a single, majestic view.
Double Cluster
The Double Cluster, composed of NGC 869 and NGC 884, lies between Perseus and Cassiopeia and is one of the sky’s most beloved open cluster pairings. These two clusters sit close together in the sky and are rich with bright, young stars. Their proximity and luminosity make them a striking sight even in moderate conditions, though sky darkness greatly enhances their depth, richness, and the sense of starry immersion.
🟣 In Bortle 1–2 skies, the Double Cluster is a breathtaking display of stellar brilliance. Both clusters shine as densely packed swarms of stars with a fine balance of bright and faint members. Between and around them, a dense backdrop of stars fills the view, creating a glittering river of light. Subtle color differences among the stars become noticeable—many of the brightest members appear blue-white, while a few orange or yellow stars stand out as colorful punctuation. The entire region feels deep, radiant, and full of motion, like twin beacons embedded in the Milky Way’s flow.
🔵 In Bortle 3–4 skies, the clusters remain prominent and beautiful. The brighter stars continue to shine clearly, and the overall shape and pairing are obvious. The background field is slightly dimmer, and fewer faint stars are visible, which reduces the sense of immersion slightly. Still, the Double Cluster retains much of its brilliance and charm, standing out as one of the highlights of the northern autumn and winter skies.
🟢 In Bortle 5–6 skies, the Double Cluster loses some of its delicacy. The brightest stars are still visible and the twin arrangement is still apparent, but many of the fainter stars blend into the skyglow. The field around the clusters feels thinner, and the scene flattens somewhat. The color variation among stars becomes harder to detect, and the clusters start to resemble looser patterns rather than compact, vibrant swarms.
🟡 In Bortle 7+ skies, the Double Cluster is still visible thanks to its bright core stars, but it becomes much more subdued. The richness and depth are gone, and the fainter cluster appears less defined. Without the background star field or dimmer members to complete the picture, the clusters lose their brilliance and cohesion. They appear as two modest groupings of stars in a dull sky, stripped of the sparkle that gives them their magic in darker settings.
Double Cluster
DSOs within 48° or 2 outstretched hands at arm's length