My original Astro Journal with my Equipment and Astro Automation pages: https://SaltwaterWitch.com/astronomy
Electronics project for the day: prototyping the drive system for a direct-drive star tracker. This will be driving a 100:1 ratio Harmonic Drive gearhead. For this test I'm using a NEMA 11 stepper motor, also geared down, and a cheap A4988 stepper driver, but I will be experimenting with others.
The dust and hydrogen gas of NGC 2327 "Parrot Nebula" and IC 2177 "Seagull Nebula" span 100 lightyears between the constellations Monoceros and Canis Majoris. This is another one from last night (New Years Day). After shooting the Flaming Star Nebula for several hours, I dropped down to IC 2177 for the remaining clear skies (up to around 1am). Neither of these targets are strong--or have anything showing up--in the oxygen bandpass. I ended up cutting the OIII frames and going with bi-color Ha and SII. Exposures: 28 x 300 seconds of Ha, 26 x 360 seconds of SII. Equipment: William Optics GT81 APO refractor, ZWO ASI1600MM-Pro monochrome 16MP camera (unity gain 139/21), Astronomik filters, iOptron CEM25P mount, INDI/Ekos/KStars running in Stellarmate/Raspberry Pi 3b+
The star at the core of this nebula is the "Flaming Star", AE Aurigae, in the constellation Auriga (The Charioteer), and all the surrounding dust and clouds of hydrogen is called the Flaming Star Nebula (IC 405). This emission nebula is around 1500 lightyears away and it's fairly large, about 5 lightyears across (roughly 47 trillion kilometers or 30 trillion miles across).
What's interesting is that even though AE Auriga is lighting up the nebula, it was not formed there, but rather is a "runaway star" that was probably ejected several million years ago from the star formation furnace in the core of the Orion Nebula. The star is moving quickly through the nebula, producing a violent bow shock with a wave of high energy electromagnetic radiation.
Frames: 23 x 300 seconds of Ha, 5 x 300 seconds of OIII (I was not picking up oxygen at all!), and 20 x 360 seconds of SII. Equipment: William Optics GT81 APO refractor, ZWO ASI1600MM-Pro monochrome camera (unity gain 139/21), Astronomik filters, iOptron CEM25P mount, INDI/Ekos/KStars running in Stellarmate/Raspberry Pi 3b+.
I put together a batch of images from my astrophotography sessions over the last year. This isn't in order, because a wanted a nice mix of color, narrowband, hydrogen-alpha only, wide-field, moon shots, along with some of my astro gear setups for some of these sessions.
My purpose was to avoid running another USB cable from the iOptron hand controller to the Raspberry Pi3B+, using iOptron's Wifi-to-serial adapter, "StarFi". Here's the basic setup: you plug in the hand controller normally. The adapter comes with two short cables with RJ jacks. The four lead RJ11 cable goes from the RS232 port on the StarFi to the serial port on the hand controller, and the 6 lead RJ-12 runs from the StarFi "Port" to the "iOptron Port" on the CEM25P mount. The instructions guide your through adding the device to your network and using it with ASCOM. I had no problem setting it up with Ekos/INDI, using an IP address instead of a serial port.
Want to see what I do when I setup my wide-field narrowband astro gear for the night? I shot this with a GoPro on a headband, so it's kind of fun to watch. It's like playing a first-person game where you have to install some astronomy equipment to test your patience and dexterity before they hand over the more lethal hardware. This is close to real time, and my goal with setting up the 4x4 post in the ground and using drilled 4" x 6" aluminum plates was to allow me to spend the minimum time outside. I started using this a little over a year ago--to avoid being outside when it's really cold, and so far it's worked well. I have both mounts (iOptron and Orion Atlas) with the same size and format base plate, and I have mounting plates on the backyard "pier", tripod I can carry anywhere, and a rolling cart that I can set up in the driveway.
NGC 1499, California Nebula in bi-color narrowband hydrogen-alpha and sulfur 2. I captured this data on the 25th, but didn't have time to capture oxygen 3 frames with high clouds moving in and the moon rising. Even so, I like the way this turned out with the two bandpasses, almost fluorescent. NGC 1499 is about 1000 lightyears away, and if you haven't guessed, it's called "California Nebula" because if you flip this image 90 degrees counterclockwise it looks like the state.
The clouds and icy rain are here, and I've had time to process some of the data I captured over the last two nights. Here's IC 1805 and neighboring nebulae and star clusters in hydrogen-alpha, oxygen 3, sulfur 2 using the Hubble palette (SHO mapped to RGB). The Heart swings around the north celestial pole below the "W" asterism of Cassiopeia, and with trees to the north and the house blocking the view west I don't have all night to capture data. So, I went with the 11 x 300 seconds of Ha, 21 x 300 seconds of OIII, and 13 x 300 seconds of SII. Equipment: William Optics ZS61 APO refractor, ZWO ASI1600MM-Pro monochrome camera (unity gain 139/21), Astronomik filters, iOptron CEM25P mount, INDI/Ekos/KStars running in Stellarmate/Raspberry Pi 3b+.