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M35 Cluster - a brilliant, star-packed cluster with a hidden bonus
Our Milky Way Galaxy is full of groups of stars known as open clusters. These are stars that formed together from giant clouds of gas and dust. Some of these clusters are so close to us that they’re big in our sky and can be seen with the naked eye. Here are four super-close clusters:

            ● Hyades in Taurus, 150 light-years away
            ● Coma Star Cluster in Coma Berenices, 280 light-years away
            ● Pleiades in Taurus, 444 light-years away
            ● Beehive Cluster in Cancer, 577 light years away

This leads us to the open cluster Messier 35 in Gemini (M35). This cluster is much further away, at 2,800 light-years, so we wouldn't expect to be able to see it with the naked eye. But under very dark skies, we can. Amazing! It looks like a dim patch in the sky as big as the Full Moon.

But the true beauty of this cluster is revealed in binoculars and, especially, in telescopes where one can see lots of bright and colorful stars, including some that are double stars (two stars that orbit each other).

Another cool thing about M35 is that there’s a bonus cluster nearby, NGC 2158. NGC 2158 is smaller, dimmer, hazier and harder to see. Is it related to M35? No, NGC 2158 is much further away, about 11,000 light-years. It just happens to be in the same line of sight and makes for a fun add-on challenge for stargazers with telescopes.


M35 Cluster
Rating: 🟣 Showpiece TargetLevel: 🔵 EasyHow: When: Nov to mid-Mar
🌟 Bright, Big, and Easy to See
M35 is a bright, large open cluster that’s easily visible in binoculars and stunning in small to medium telescopes, even from suburban skies.
🌟 A Rich and Sparkling Field
It contains over 200 stars, including many bright, blue-white members. The cluster fills the eyepiece with a dense, glittering field, making it one of the richest open clusters in the winter sky.
🌟 Looks Great at Low Magnification
M35 spans over 30 arcminutes (about the size of the full Moon), making it ideal for low-power, wide-field views—a relaxing and beautiful deep-sky object to sweep across.
🌟 Companion Cluster Nearby
Just 0.4° away lies the compact and older open cluster NGC 2158, offering a striking contrast—M35’s youthful sparkle versus NGC 2158’s tight, golden glow—two clusters in one view!
🌟 Easy to Find in Gemini
Located near the feet of the Gemini twins, M35 is easy to star-hop to from Eta Geminorum and well-placed for winter evening viewing.
🌟 Great for Beginners and Outreach
Bright, pretty, and instantly rewarding, M35 is perfect for public star parties, beginners, and kids, offering an impressive field without needing dark skies or filters.
M35 Cluster
NamesMessier 35 (M35),NGC 2168ConstellationGeminiDistanceM35: 2,800 ly, NGC 2158: 11,000+ ly
RA, Dec06h 10m 27s, +24° 19′ 48″Angular SizeM35: 28’x28’, NGC 2158: 5’x5’MagnitudeM35: +5.09, NGC 2158: +8.60
Angular
Size
vs
Moon
DSO TypeOpen cluster: a loose group of a few dozen to a few thousand young stars that formed together and are loosely bound by gravity.
M35 Cluster
Find the constellation Gemini with bright Castor (+1.58) and Pollux (+1.22). Find two much dimmer stars in Gemini: Propus (+3.29) and 1 Geminorum (+4.17).
Using a binocular or telescope finder, point to M35. It forms a triangle with Propus and 1 Geminorum. Using a telescope with a low-power eyepiece, search for the cluster. Explore!
M35 Cluster
Use binoculars to spot its hazy glow.
In 7x50 or 10x50 binoculars, M35 appears as a small, misty patch with a few bright stars resolved. It’s easily found from a dark site and stands out nicely from the background.
Start with low power to frame the whole cluster.
At 30x–50x, a telescope will show the entire cluster, filled with dozens of stars forming arcs, chains, and knots. The field is dense and lively, especially in 4-inch and larger scopes.
Switch to medium magnification to increase star resolution.
At 100x or so, many of the fainter stars become visible and the view becomes more three-dimensional. The outer edges resolve more cleanly, revealing depth and structure.
Observe from dark skies to enhance contrast.
Though M35 is bright enough for suburban skies, dark skies allow you to see more background stars and improve the view of NGC 2158 nearby.
Look for the companion cluster NGC 2158.
Just southwest of M35 lies a faint, compact cluster—NGC 2158. It appears as a hazy, grainy patch in small scopes and begins to resolve in 8-inch telescopes under dark skies.
Let your eyes adapt fully to see more stars.
As your night vision improves, more of the cluster’s stars—especially the fainter ones—will emerge, creating a richer, more layered view.
Scan slowly to appreciate the star patterns.
M35 is full of subtle groupings and star chains. Slowly panning through the field can reveal patterns that aren’t obvious at first glance.
Compare it with other open clusters.
Try viewing M37, M36, or M38 in Auriga during the same session. Comparing their structure and richness with M35 adds context and depth to your observing experience.
M35 Cluster
⚠️ Naked Eye
Messier 35 is not visible to the naked eye from most locations, though under dark skies it may appear as a faint, unresolved patch in the constellation Gemini.
Binoculars
Through binoculars, it shows up as a misty glow, loosely defined but clearly different from the surrounding star field, hinting at a dense group of stars.
Small Telescope
In a small telescope, M35 becomes a bright, richly populated open cluster, filling the field of view with dozens of sharp stars of varying brightness, arranged in a wide, irregular pattern that feels lively and expansive.
Medium Telescope (4–8”)
A medium telescope enhances the contrast and resolution, revealing fainter members and adding depth to the field, while also making nearby NGC 2158—its compact, more distant companion cluster—just visible as a small, hazy knot at the edge of the view.
Large Telescope
In a large telescope, M35 remains wide and brilliant, with hundreds of stars resolved across the field, and the contrast with the tightly packed, golden-hued NGC 2158 becomes even more striking, offering a beautiful juxtaposition of two very different clusters in a single view.
M35 Cluster
Messier 35 is a bright, rich open cluster in the constellation Gemini, located near the feet of the Twins. Its stars are widely spaced but numerous, giving it a sparkling, textured appearance. Because of its brightness and relatively high surface star density, M35 holds up well in moderate light pollution, but its richness, star count, and background contrast are strongly affected by sky darkness.
🟣 In Bortle 1–2 skies, Messier 35 is a dazzling spray of starlight. Dozens to hundreds of stars are visible across a broad field, many forming graceful arcs and curved lines. The brightest stars shine crisply against a deeply black sky, while the fainter members add fine texture throughout. The nearby, denser open cluster NGC 2158 is also visible in the same field, appearing as a faint, concentrated patch that provides a beautiful contrast with M35’s more open structure. The overall view is immersive, dynamic, and rich with detail.
🔵 In Bortle 3–4 skies, M35 remains an impressive cluster. The brightest stars still sparkle clearly, and much of the fine structure is preserved. The star field is a little less dense, and some of the faintest members begin to disappear, but the sense of richness remains. NGC 2158 may still be detectable, though with less contrast. The cluster continues to appear full and vibrant, offering an enjoyable and rewarding view.
🟢 In Bortle 5–6 skies, the cluster becomes flatter and sparser. The core stars are still visible and form a recognizable pattern, but many of the fainter stars fade into the skyglow. M35 begins to lose its sparkling quality, and the surrounding star field appears dimmer. The nearby cluster NGC 2158 becomes difficult or impossible to detect. The overall appearance is still pleasing, but less intricate and immersive than in darker skies.
🟡 In Bortle 7+ skies, Messier 35 is still visible, but it loses much of its richness. Only the brightest stars remain prominent, and the cluster’s full extent becomes difficult to trace. The star pattern appears loose and isolated, and the background sky lacks the supporting stars that give it context and depth. The cluster appears washed-out and less cohesive, with its subtle structure entirely flattened.