An Astrophotography Journey Using Scrum

An Astrophotography Journey Using Scrum

A story of learning in the complex domain

In my Astrophotography Journey, I have embraced the Scrum framework to tackle a complex problem. Through iterative sprints and failed experiments, I have gained valuable insights into what works and what doesn’t. This iterative approach has brought me closer to capturing my first picture of the Great Orion Nebula, incrementally adding value and realising my vision.

First picture of the Great Orion Nebula using Sony Alpha A7RIII IMX-455
My first picture of the Great Orion Nebula using a Sony Alpha A7RIII IMX-455

My first telescope

What was I thinking? Biting off more than I could chew for my first sprint. Long-running experiments and big mistakes are costly at this stage of learning. Time for smaller easier experiments. The mount was faulty. I didn’t know what I was doing so I had no idea that it would only move in Declination and limited Right Ascension.

CGX-L Mount with Celestron Edge HD
CGX-L Mount with Celestron Edge HD

Solving complex problems can feel almost impossibly frustrating sometimes. It’s the passion to achieve your vision one small step at a time that gives you the energy to keep pursuing it. Mastering new technical skills that emerge through solving complex problems creates strong foundations and growth.

Vision: Enable people to Explore the Universe from the comfort of their own home

Product Goal: Just get something working

I love learning through experimentation. There’s nothing like failing fast and setting up your next experiment. When it works it’s pure glee. Every night was a new experiment.

I worked in one-week sprints. Even if the weather is poor there is always something to be done.

I swapped to a simpler faster lower focal length refractor telescope to use as a learning platform. Namely, the William Optics FLT132 f7 gives a 920mm focal length. It’s basically a big zoom lens. The lens of the latest iPhone for instance is f1.8 and 26mm focal length so very fast and wide angle.

Astrophotography Journey - William Optics FLT132 f7

For starters set up the mount and telescope. Level, balanced, polar aligned, aligned to multiple stars to build a navigation model for the mount.

Every telescope needs polar-aligning to align to the rotation of the earth. In my case the north celestial pole. Once aligned it makes it easier to find stuff in the night sky. This means learning a solid understanding of the earth’s rotation. Right ascension and declination act as coordinates for finding stuff in the night sky. The sky at night is constantly changing due to the Earth’s tilt of 23.5 degrees.

Product Goal: Photographing the night sky

At night our eyes adjust to the dark using peripheral vision. Everything looks black and white and most of the detail in the night sky can be hidden from our poor human vision. I need to collect more photons! That means new experiments. Each image is constructed from at least 50 sub-frame images. This way the signal will out way the noise and provide lovely images. Lots more experiments to understand how this works.

Now that I had understood how to set up and operate the telescope and mount from a computer it was time to start experimenting with taking pictures.

Understanding how stuff works

Many sprints discovering astrophotography

  • Discover what a flattener is. Fit the camera and flattener to the telescope at the correct distance. 1mm out in any direction results in image distortion.
  • Understanding focal length and back focus distance
  • Creating a flat image. The lens is curved but the camera’s sensor is flat! That means correcting with additional lenses
  • Exposure time and gain
  • Dew, Dew, Dew – experimenting with heating. Space is cold so staring at it chills the lens. When that gets to below dew point you get dew. Dew is evil. Dew is bad.
  • Guiding to make corrections to telescope position during long exposures. Basically using a second camera to track a star and correct the mount’s position. The better the alignment and model the better the images
  • Then there’s also understanding, creating, and using flat, dark, and biased images. As it happens camera sensors create noise. Not all the pixels work some pixels are hot and white and some are cold and black. Because the lens is curved light does not fall on the sensor evenly and is darker towards the edges. In a daytime image with lots of light, you would not notice these issues. But when the signal from targets is very low then every photon counts.

Product Goal: Eliminate Annoying Issues


As it happens camera sensors get hot during long exposures of 5 – 20 minutes. This creates noise. Noise means bad pictures, especially in summer. High gain means faster images but lost detail.

A cooled astro camera can cool the sensor to 35 degrees below the ambient temperature. There’s a learning curve here too. Experimenting with full well depth (yes, literally electron buckets) , gain, temperature, monochrome or colour, pixel size, dynamic range low noise, seeing conditions, arcsecs/pixel, and pixel size enabled me to fully understand the capabilities and limitations of these complex cameras.

Light Noise Demonstration

The scourge of light pollution

It’s a sad truth, but according to a study done by Italian and American scientists, one-third of the world’s population and 80% of Americans cannot see the Milky Way. The Milky Way is an awesome cosmic wonder to behold and ponder. Even more, experiments are needed to remove gradients created by street lighting in the UK. Most of the lighting is not required. With modern technology, LED lighting can be switched on only when somebody approaches. LEDs are way worse than the old streetlights. LED light produces light across the whole visible spectrum so difficult to filter out.

Next experiment using various filters to try and tackle the UK’s terrible light pollution and learn about narrowband filters.

The scourge of satellites

Say no more. Thanks to projects like StarLink and zero regulation of night skies, Earth-based astronomy science is at risk forever. The only way to remove this is to use image processing to remove the noise.

Product Goal: Stay warm using Automation

I want to be warm. Winter is cold. At this point, I need to be with my equipment to move targets and take sequences of images of a target. Experimenting with automation using an industrial computer strapped to the telescope via Wi-Fi or ethernet. No laptop in the garden all night. Full Remote Control 🙂

Product Goal: More Advanced Telescopes

Refractors have great resolution but if you want more zoom then a reflector is better. Basically, this is a mini-Hubble. They are difficult to use and require more advanced collimation using a laser to line up two mirrors. This required going back to basics with experimenting. Getting more advanced too quickly can feel like a backward step. It’s a risk that delays value but can be necessary to achieve the vision. It took three months to master the Ritchey Chretien.

Ritchey Chretien on a CEM60EC2 mount

Product Goal: Professional Image processing with PixInsight

Using a professional software package for processing data is a daunting prospect. The results are great, however after a few hundred experiments I’m just kind of becoming a little more proficient and consistent. The image here was constructed from 240 monochrome Hydrogen Alpha and Oxygen sub-frames

Product Goal: Think Bigger

During all my experimentation and getting creative I had become very proficient in setting up and consistently taking some great images. But everything was limited by light pollution, the wrong kind of airflow, the wrong type of weather and humidity, and seeing conditions that limit image resolution.

After much research moving equipment and setting up in a dark area in Spain or Chile at a site used by Astro professionals and amateurs alike was possibly the answer. Fregenal de la Sierra in Spain has an excellent Bortle scale and everything I need. It’s also closer than Chile if I need to visit. Chile is still on the list though.

It felt great setting up in Spain knowing exactly what I’m doing. Using best practices discovered through many explorations to my advantage. Roll-off roof, dual telescope setup, with industrial computer control and remote access. 250 cloudless nights a year and very low light pollution and good seeing conditions.

Product Goal: Diagnosing issues remotely

Ah yes, something always goes wrong. When you can be there it’s easier to diagnose and confirm issues. Experience but more likely intuition comes into play in solving problems remotely. Autofocus slipping, filter wheel broken, camera moisture levels too high to name a few.

Creating my own software to analyze image quality in real-time

With all that I had learned I was able to start to solve a few automation problems that professional packages lack. I have had some great fun analysing the quality of images in real-time including curvature and sensor tilt and correction during sprinting towards this goal.

Experimenting creates waste! Not experimenting creates nothing good at all

Best advice. Keeping experiments small, goal-focused, and lightweight creates less waste and optimisation of value vs cost.

Product Goal: Automation for customers targets

Bringing it all together. These sprints were about enabling public access requests to professionally photograph targets of their choice delivering raw data and automated processed images. The images enclosed in the blog are much smaller than the real thing. A real single processed image may contain a gigabyte of HDR data. To reproduce these results starting from scratch could cost 10’s of thousands. With this service, results are guaranteed for a fraction of the cost.

Vision achieved

This is why I embrace the Scrum Framework in my current Astrophotography Journey. Through small iterations and increments, I maximize value, accelerate learning, and optimize my investment. It took 18 months to bring this vision to life!

Now, I have established a viable business model where individuals can request a target and receive a fully automated dataset along with a processed image of their desired target. Scrum has played a pivotal role in achieving these milestones in my Astrophotography Journey.

Next Vision: Different focal length telescopes and Southern Hemisphere

How will you bring your curiosity and creativity to play through experimentation to solve problems in the complex domain and have fun doing it? Discover new possibilities with our course or contact us to discuss agile and team coaching, and ignite your journey of growth and enjoyment.

The Great Orion Nebula a year after the first
The Great Orion Nebula a year after the first
Veil Supernova Remnants
Veil Supernova Remnants

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