The Soul Nebula is a complex structure of emission nebulae and open clusters, packed full of detail and contrast. I managed to get 5 hours on it last night.
It’s usually processed with either deep red colors or the mix of blue and gold from the HOO palette. I always like to go soft on these targets and try to create a “warmer shade of red.”
I won’t be imaging for a few weeks now. Incoming clouds is one of the reasons but it’s mainly because I’ll have some maintenance done on my HEQ5 mount. I will replace the gears with the belt mod which will hopefully future proof the mount for whatever equipment I might combine it with over the next few years.
My HEQ5 has been amazing though and with the exception of some issues last winter it has been working flawless for me.
I’ve started doing some research on new projects but the next targets will be the “low late fall targets” in the Orion & Monoceros region.
Autumn means rapidly changing weather forecasts, foggy mornings, high humidity and lots of dew but also nebula season, which means some of the most fascinating and popular astrophotography targets can be observed.
We’re nearing that time of the year, where clear skies become a rare event so I can only hope to be lucky this year and get some good imaging time, we’ll see.
Here are some of the finished projects from summer and early autumn: the Triangulum Galaxy, Capella, The Lion Nebula and The Ghost of Cassiopeia.
Eris is a dwarf planet located 14.5 billion km away in the so-called Scattered disc, an area beyond the Kuiper Belt. Once you star tracking objects beyond Neptune, light becomes obscure and distances become immense. 14.5 billion kilometers is about 3 times the distance between the sun and Pluto. This makes Eris probably the furthest object in our solar system we can image with our amateur equipment.
Eris is also very dim at +18 magnitude. On top of that it’s currently located in Cetus which is a constellation that is not getting very high up in my northern skies. Eris will stay in Cetus for a while during its 557 year orbit around the sun.
Preparation
Astrophotography is not that complicated. We basically look up targets in our astronomy software, figure out the framing, exposure times and which filters to use and we’re set. Once the scope is set up and polar aligned, we slew to the target and start shooting exposures. Those are then calibrated, stacked and post-processed, all of which can be done today in a semi-automated way without too much effort. The only thing we really depend on is clear skies and a stable atmosphere.
For more peculiar objects it’s a bit more complicated. Trans Neptunian Objects, small galaxies, peculiar stars, asteroids, comets etc. require more preparation and active involvement.
The first issue is that objects like Eris are not accurately tracked in most of the available (free) astronomy software. To find its precise location I had to find it in the Nasa Horizons Systems database. The second challenge is in tracking the object, this means figuring out where the object will be in the future, preferable in the same image frame and making sure there is ample clear sky available to shoot the object twice in the required time slot. The end result is hopefully two images that show the movement of Eris.
Results
In total I had 5 sessions on this object. My first session was fruitless due to the September super moon event but I did manage to clearly capture Eris on the second try. Sessions 3 & 4 were interrupted by clouds but yesterday I finally managed to find Eris again
Eris as a faint spot on the night of the 29th of September in the constellation Cetus under a near new moon. This is 1 hour of integration time with 5 minute subs.
Eris again, now moved close to galaxy PCG1139116 on the 11th of October.Even with more integration time it remains very, very faint.
