M31 (And)

M31 (And)

Click on the image for a larger version

Date/Site: 14. and 15. September 2023. Remote observatory on the AAR club's site in Presberg
Exposure/
Filter:
RGB: 6 x 12 x 300 seconds (-10°C)
Camera/
Optics/
Instrument:
Touptek 294CP on 150mm f/5 Newton with 2" Skywatcher Comacorrector
Data acquired remotely with N.I.N.A.,
Guiding: ASI120 attached to a 61mm-finder,
Focusing with Microtouch,
Calibration and processing: PixInsight 1.8 and ICE (Image Composite Editor, Microsoft)

In August 2023 a disastrous failure of the power supply in my observatory caused damage in several electrical devices, including the main camera, the Moravian G3-16200. It had to be sent to Moravian and as repair dragged on for many weeks, I decided to image with the 6"-Newton and the Touptek colour camera alone objects containing no or few emission nebulae, that I normally would not have chosen during late summer/early autumn.
Collecting frames with the fast colourcamera alone is comparatively easy. And as planning and realizing a mosaic in N.I.N.A. is a mere child's play, I ventured to create a mosaic of the great galaxy of Andromeda, M31.
Close inspection of the completed 6-panel-image showed I could better have planned an additional row of panels in the northeast-southwest-direction, because the spiral arms of M31 reach out even further. Also I underestimated the brightness of the core regions of M31 and M32, which are burned out after 5 minutes because of the Touptek's 14-bit.
Nevertheless I am quite satisfied with my first mosaic.
During the presentation of the image my astronomy-friends from the AAR identified in it the Mira-variable, by which Edwin Hubble (almost exactly 100 years earlier on a plate exposed with the 100-inch Hooker-telescope on Mount Wilson) proved that galaxies are independent systems far outside our local galaxy.

© Friedhelm Hübner, last revision:  03.12.2023