Photography

A Galaxy of Dynamic Gases

The success of n-body numerical simulation to predict the motion of planets and stars cannot be denied. At the same time, the erroneous application of these model to intra-galactic objects and galaxies themselves have led to a popular narrative that is full of magic and other non-sense. In this ambitious posting, I have put together the astrophysical data in a different way – one that looks at objects from a more scientific and engineering point of view. This data has been used to show that the various objects in space should be considered as continuum bodies, rather than collections of particles. Classical physical laws and concepts are used to show how and why many of the phenomenon we see and

Anatomy of the Orion Nebula – Imaging and imagining 3-D Gas Bodies

It is easy to forget that our 2-D images are actually representations of 3-D gas bodies, that are acting according to 4-D dynamics. In day to day life, we have many clues that we can rely upon including parallax views, perspective rules, lights and shadows, and actual physical interaction that we can use to assess the nature of objects in 3-D and 3+1 space. Unfortunately many of these clues are absent or confusing in our deep space objects. In this post, we analyze a 2-D image of the Great Orion Nebula and stellar nursery including its shape and orientation in 3-D space. Along the way, we will present an understanding of the three principle gas types in deep space photography

The Sunflower Galaxy and Dynamic Complexities

At first glance, Messier 63 (M63 for short or aka “the Sunflower Galaxy”) appears to be a break from the traditional spiral structure of galaxies and represent a new type of galaxy termed a “flocculent” class. It was thought that the stars formed clumpy clouds gathered together as clumps, like strands of wool form clumps of wool – even on the sheep. In chemical engineering, we often use agents that make particles suspended in a fluid clump together to form larger particles ,so that gravity can overcome the suspension and separate the particles from the fluid. I like to thing that the word flocculate (or its sorter “floc”) comes from the word “flock”, as in a flock of sheep,

The Anatomy of a Stellar Nursery

Introducing the Rosette Nebula / Stellar Nursery When I first started to image stellar nurseries, I really didn’t know anything about them. I was told that stars are being born there – that is pretty awesome, but I was curious what was it about these light generating molecular clouds (MCs) that made them prolific star builders. Sure, stars are also created in turbulent dark molecular clouds, but stellar nurseries really churn out the stars at a much higher level – often creating whole open clusters of stars. Many of the stellar nurseries get very large and can even be mapped from their Halpha light signal in other galaxies. Ok, so my interest was piqued – I had to figure out

The Hidden Galaxy – Now you see it

IC342/Caldwell 5 – The Hidden Galaxy in LHaRGB Planewave CDK 12.5in; AP 1100GTO AE; QHY600M, – Baader Cmos Opt Broadband and 6.5nm Ha FiltersL: (50 x 180s, Bin 1, Gain 100); H: (29 x 720s Bin 1, Gain 100); R,G,B: (25,23,22 x 210s, Bin 1, Gain 100)Total integration time = 12.4 hrs (Feb 10-12, 2025) Maple Bay, BC, Canada For full resolution, downloadable image, visit my gallery at Victoria RASC Zenfolio or Astobin The Hidden Galaxy gets its name from its position in the sky, near the Milky Way and partly obscured by our galaxy’s dust. If not for the dust, IC342 would be visible with the naked eye and occupy about the same size as the moon. In reality

Its Supersonic! – But it’s complicated

The massive explosion of a supernova sends material (and light) outwards in all direction, at velocities greater than the speed of sound. The speed of sound is another way of saying the speed that pressure or density waves can travel or disperse through the medium that it is moving through. The particles ejected by the supernova are moving so fast and so much momentum that they don’t disperse but act like a moving wall of material, bulldozing and sweeping up any additional material in its path. Along the way, the particles that make up this moving wall, or shock front involves a lot of friction between particles so that it heats up to extreme temperature (million of degrees) and the wall emits light that we see as the remnants or remains of a supernova.
This wall, known as a shock-front, eventually runs out of momentum due to is expanding spherical geometry and sharing of momentum, but remains visible to our cameras long afterwards, until it fades through cooling. The patterns of emitted light are both beautiful and distinctive from other subsonic flow patterns, and these patterns enable us to identify these objects as supernova remnants. or leftovers from the supernova explosion.

The Whirlpool Galaxy (M51) – In for Questioning

The M51 Galaxy or “The Whirlpool Galaxy” definitely strikes an awsome pose, with its two apparent “centres”, and multiple star fuzzies emanating from its extremes. I decided to get all Sherlock Holmesy on it in my desire to figure out what was going on. Yes it is two glalaxies interacting, but what is the nature of this interaction. What happened to its bottom arm? – it looks like it was bitten off. The upper arm looks more intact, but also exhibiting Halpha starburst too. Is the bottom of the galaxy connected to the top with stars circling the left hand side? Can infrared light help us? Can it potentially reveal something? I recommend reading more to find out.

« Previous