
THE BEEHIVE CLUSTER
M44 • Open star cluster • Cancer • 580 light-years from Earth
🔭
Askar 130PHQ
📷
ZWO 2600MC Pro
🌃
Bortle 8
⏱️
13 hours
🗓️
March 2025
Overview
The Beehive Cluster (officially known as Messier 44) is a sparkling swarm of stars. The name comes from views through a telescope, where the stars look like bees buzzing around a hive.
One of the nearest open clusters to Earth, the Beehive contains close to 1000 stars that formed together around 600 million years ago. If you’ve got dark skies away from light pollution then you might spot it with the naked eye. You’ve not much hope of this from a light-polluted city, although it’s a fairly easy target for urban astrophotographers.
Background
The winter night sky is filled with prime targets for astrophotographers, but as we head into spring there’s less choice (unless you’ve got the right telescope to photograph distant galaxies!) The Beehive is in a good location for me though, rising over my garden fence just as the sky gets dark enough for imaging.
Being a bright star cluster means I didn’t need the 20 / 30+ hours I normally put into a project. This image is a mere 13 hours, which is about as quick as I ever do!
I also decided to use shorter subframes this time. Normally I shoot 5-minute subframes, but I decided to lower this to one-minute, just to avoid the brighter stars becoming blown out.

Science
The Beehive is an open cluster, which means the stars formed together and and are still loosely bound by gravity. It’s around 600 – 700 million years old, and 610 light-years from Earth. For comparison, the famous Pleiades open cluster is 100 million years old, and 444 light-years away.
One of the stars within the Beehive is called Pr0211. It’s quite similar to the Sun, but is noteworthy because astronomers have discovered two planets orbiting it. These are called Pr0211b and Pr0211c. They’re gas giants that orbit close to their star; what we call “hot Jupiters”. They were discovered in 2012 and 2016, respectively. Pr0211b has the claim to fame of being the first hot Jupiter to be found within an open cluster of stars. Here’s the paper that documents this find.
Unfortunately these planets can’t be seen directly through telescopes (and especially not amateur level!) Instead, they were discovered using the radial velocity method, which is when a star can be seen to very slightly “wobble” in space due to the gravitational force of its planets. Still, I think it’s neat that the star can be seen from a city centre, and that we know it’s orbited by at least two planets.

Thanks go to my astro pal Richard Hook for pointing out that I’ve captured some quasars in my image. A quasar is a supermassive black hole “feeding” on gas and dust. As this material spirals into the black hole, it heats up due to friction and becomes incredibly bright — often outshining the entire galaxy of stars that surrounds it. They’re almost unbelievably distant though, so they’re still hard to spot.
Here’s a quasar, with the catchy name J083857.85+193335.7. It’s 7 billion years old, meaning the photons of light recorded in my image travelled through space for half the age of the entire universe before they hit my camera sensor! That’s quite a journey…

Kit list
This is the equipment I used to capture the image.
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Telescope: Askar 130PHQ
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Camera: ZWO ASI 2600MC Pro
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Mount: Sky-Watcher EQ6-R Pro
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Guidescope: William Optics 50mm with ROTO Lock
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Guidecam: ZWO ASI 120MM Mini
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Control: ASIAIR Plus
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Filter: Optolong L-Quad Enhance
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Processing walkthrough
Example source data
Here are example single subframes and freshly integrated stacks, just with simple stretches applied.


Seestar S50 image
Seestar S50 telescope coming soon…
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