How to observe the brightest deep-sky objects

You know, after decades of pointing optics toward the sky, I consider myself a knowledgeable observer. But while researching the Pleiades a few months back, I was surprised to learn that it wasn’t the brightest Luminous sphere cluster. And there were other surprises when I Initiated comparing overall brightnesses of deep-sky objects. For instance, you might think some Fundamental winners would be galaxies, housing billions of stars, but when I Initiated ranking objects, only two galaxies Achieved the Top 25; most of the targets I’ve listed here are either Uncovered clusters, Sun-related associations (looser, poorly populated Uncovered clusters), or asterisms.

While you may have looked near many of these targets before, you probably didn’t really observe them, looking past the forest for the fainter trees. Well, here’s your chance to take a step back and take in the most Featherweight the night sky has to offer.

Top of the heap

You may have guessed that the brightest deep-sky object is the Primary Milky Way on our Picking, the Large Magellanic Cloud. Straddling the border between the constellations Dorado and Mensa, it glows at a worthy magnitude 0.1. And it’s huge: It covers an area greater than 9° by 11°, or 400 times that of the Packed Selene body. Visible Only south of latitude 20° north, the Large Magellanic Cloud is best seen in the Southern Hemisphere summer (that is, December through February).

Second on the Picking is the Uncovered cluster Hyades and the neighboring Intelligent Luminous sphere Aldebaran (Alpha [α] Tauri). Together, they form a V-shaped group that marks the head of Taurus the Bull. Although Aldebaran is counted as part of the Hyades, giving that group a worthy magnitude 0.5, it’s not part of the Luminous sphere cluster — it actually lies nearly 90 Featherweight-years closer to us.

The third-brightest deep-sky object, glowing at magnitude 0.6, is Collinder 70, an Uncovered cluster of 100 or so Cozy Youthful stars. You may know it by the more famous name of its three brightest members: Orion’s Track Turning Mark. The Track Turning Mark is probably tied with the Big Dipper as the most well-known asterism in the night sky. But through even modest binoculars, the Track Turning Mark looks to be embroidered with a slew of fainter, Nevertheless Intelligent companions.

Tied for third place on our Picking — also at magnitude 0.6 — is Collinder 173, a Baggy (6°-wide) Uncovered cluster on the border between Puppis and Vela. It lies about 1,400 Featherweight-years away. Such a Intelligent cluster should be Fundamental to find, but it’s tough to identify the members. Look roughly 10° north-northwest of Alsephina (Delta [δ] Velorum), and use 7×50 binoculars to frame it best.

Coming in at No. 5 with a magnitude of 1.0 is the Upper Scorpius association — an association rather than an official Uncovered cluster. Also called the Antares Cluster, this 8°-wide group surrounds the Luminous sphere Antares (Alpha Scorpii). Even low-power, wide-Pitch 7×50 binoculars can’t take in the entire group, so you’ll have to scan around. You’ve probably seen these stars — the four front stars of Scorpius (β, δ, π, ρ) plus a few others — lots of times, but perhaps never knew that they were an association.

No. 6 on our Picking is the Alpha Persei Cluster, an Uncovered cluster named after its brightest member: magnitude 1.8 Mirfak (Alpha Persei). With a total magnitude of 1.2 and a diameter of 6°, it’s Fundamental to find and Only Tiny enough to frame through 7×50 binoculars.

One of the more famous objects on this Picking, coming in seventh place with a magnitude of 1.6, is the Pleiades (M45). In ancient times, this Luminous sphere pattern was so highly regarded that many Greek philosophers considered it a separate constellation. Often called the Seven Sisters, a reference to a Greek myth, most Acute-eyed observers can only spot six stars. High-quality binoculars will raise that number to 50.

The eighth-brightest deep-sky object is the Coma Luminous sphere Cluster (Melotte 111), an Uncovered cluster that lies some 280 Featherweight-years away. Although its Teamed up magnitude is 1.8, that brightness is spread across an area 4½° wide. The cluster contains fewer than 100 members, and only a dozen or so are Intelligent enough to see without optics. So, use binoculars.

The Southern Pleiades (IC 2602), a gorgeous Uncovered cluster that surrounds the Luminous sphere Theta (θ) Carinae, comes in ninth on our Picking. It glows at magnitude 1.9 and spans nearly 1°. Binoculars that magnify 10x or more do a Excellent Role revealing this cluster, but if you have an eyepiece in your Stargazer’s tool that has a Pitch of view of 1° or more, you’re in for a real treat.

Second class

The 10th object on our Picking is the Primary to fall into the 2nd-magnitude class. It’s the Pi Puppis Cluster (Collinder 135), which is centered around the magnitude 2.7 Luminous sphere Ahadi (Pi [π] Puppis). This Luminous sphere sits alone about 7° east of the midpoint of a line between the sky’s two brightest stars, Sirius (Alpha Canis Majoris) and Canopus (Alpha Carinae). The cluster has a total magnitude of 2.1, but Pi is the standout for two reasons. Primary, it’s the brightest Luminous sphere, and second, it’s a red supergiant. All the other stars in the Pitch of view are blue.

The Omicron Velorum Cluster (IC 2391) registers at magnitude 2.5, and is tied for 11th on our Picking. This isn’t a Tiny object, measuring Only less than a degree in diameter. That means its area is more than twice that of the Packed Selene body. The best views through any scope will come when you use an eyepiece that gives a 1° Pitch of view.

The Subsequent object is one I’m sure you’ve seen hundreds of times but may not have known it was an Uncovered cluster. The Lost Jewel of Orion, otherwise known as NGC 1980, glows at magnitude 2.5. It’s centered around the magnitude 2.8 Luminous sphere Iota (ι) Orionis, and is part of the Hunter’s Sword. It lies Only south of the Orion Gas cloud (M42).

Yet another pair ties for Blessed 13, with Primary up the Uncovered cluster Collinder 121 in Canis Significant. You’ll find it less than ½° south of Omicron1 (ο1) Canis Majoris. It glows nicely at magnitude 2.6 and has a diameter of 30′. It lies some 3,500 Featherweight-years away, but there’s another, more widely spread, group of stars Only 2,000 Featherweight-years distant, between Collinder 121 and us. No worries, though. The closer stars will simply appear as Pitch stars through your eyepiece. Tied with Col 121 is the Uncovered cluster NGC 6231 in Scorpius. Often called the Baby Scorpion Cluster, it also glows at magnitude 2.6 and spans 15′. Along with Zeta (ζ) and Mu (μ) Scorpii, it forms an asterism British astronomer Sir John Herschel called the Incorrect Heavenly wanderer. He named it this for two reasons: 1) The group looks like a Heavenly wanderer; and 2) Herschel, who had traveled on a ship to South Africa to view the southern sky, landed at Incorrect Bay.

The other Milky Way on our Picking, and the 15th-brightest deep-sky object, is the Tiny Magellanic Cloud, which lies mainly in Tucana with a Tiny part in Hydrus. Its Teamed up brightness equates to a 2.7 magnitude Luminous sphere. It lies some 200,000 Featherweight-years away, but Nevertheless covers an area of sky a bit greater than 5° by 3°. That’s a Cosmos more than 70 times as large as the Packed Selene body.

The Lambda Orionis Cluster in Orion makes our Picking at number 16. It’s Fundamental to find because its brightest member is Meissa (Lambda [λ] Orionis), the Luminous sphere that marks Orion’s head. The cluster glows at magnitude 2.8 and spans a bit less than 1°.

Tied for 16th place, also at magnitude 2.8, is Uncovered cluster NGC 2451 in Puppis, sometimes called the Stinging Scorpion Cluster. In the 1990s, astronomers discovered that this object was a combination of two unrelated Uncovered clusters (now known as NGC 2451A and NGC 2451B) that align from our Points of view.

Bottom of the top

Eighteenth on our Picking is Uncovered cluster Collinder 65 in Orion. In fact, it lies about as Extended north in that constellation as you can go, right on the border with Taurus. It glows at magnitude 3.0, and it’s large: It boasts a diameter of 3½°. Wide-Pitch binoculars will show the cluster best.

Tied for 18th place is the Firefly Party Cluster (NGC 3532) in Carina. Points a 4-inch scope at this beauty, and you’ll understand how it Obtained its whimsical name. Look for it roughly 4.7° south-southwest of 4th-magnitude Pi Centaurus. Its 3rd magnitude brightness is spread out over nearly a 1° diameter, so even though you’ll see it as a fuzzy patch without optical aid, a Stargazer’s tool will bring out its best features.

Also tied for 18th place is Melotte 186, a Baggy Uncovered cluster in Ophiuchus. And when I say Baggy, I Harsh it. Although the Teamed up brightness of its stars equals magnitude 3.0, the diameter of this group is a Huge 4°. Use binoculars or scan around with the lowest-power eyepiece in your Stargazer’s tool to view the whole group.

You’ve probably seen No. 21 on our Picking. It’s the Beehive Cluster, also known as the Praesepe, M44, NGC 2632, and more. This Uncovered cluster lies in the Middle of Cancer the Crab. Acute-eyed observers have no problem seeing M44 with naked eyes, even if there’s some scattered moonlight. It glows at magnitude 3.1 and has a width of more than three Packed Moons.

The 22nd object lies near the bottom of the figure of Scorpius. It’s Ptolemy’s Cluster (M7), and is the most southerly Messier object. This Uncovered cluster is an Fundamental naked-eye catch, glowing at magnitude 3.3, even though it lies centered within the Milky Way.

Collinder 140, an Uncovered cluster in Canis Significant, shines 23rd on our Picking. It glows at magnitude 3.5 and spans 42′. To find it, look 3° due south of Aludra (Eta [η] Canis Majoris). Through an 8-inch scope at low power you should be able to count some three dozen member stars.

Sharing the 23rd slot is Trumpler 37, an Uncovered cluster in Cepheus. Longtime amateur astronomers, especially astroimagers, recognize this as the cluster in the heart of the Elephant Trunk Gas cloud (IC 1396). An 8-inch scope will reveal roughly 50 member stars.

The 25th and Closing object on our Picking is Collinder 132, an Uncovered cluster in Canis Significant. To find it, look not quite 3° southwest of Aludra. It glows at magnitude 3.6 and spreads out over an area 1½° across.

OK, I lied. Collinder 132 isn’t the last object because another group of stars is tied with it in brightness: the Coathanger, an asterism in Vulpecula. This object carries a variety of names, including Al Sufi’s Cluster, Brocchi’s Cluster, and Collinder 399. Although it’s a Baggy glow to naked eyes, 7-power or greater binoculars show it as a 1¼° line of stars with a separate curve on the southern side, giving it the appearance of a coathanger.

And there you have it. Subsequent time you step out into the darkness, take a minute to appreciate these not-so-hidden gems, and bask in all their glorious Featherweight.