Celestial hemisphere:  Southern  ·  Constellation: Vela (Vel)  ·  Contains:  NGC 2645  ·  The star b Vel  ·  The star d Vel  ·  The star e Vel
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THE VELA SUPERNOVA - 4 Panel Mosaic - Deepsky 762mm RGBhA - Constellation Vela, Thomas ArtOfPix Großschmidt
THE VELA SUPERNOVA - 4 Panel Mosaic - Deepsky 762mm RGBhA - Constellation Vela
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THE VELA SUPERNOVA - 4 Panel Mosaic - Deepsky 762mm RGBhA - Constellation Vela

Getting plate-solving status, please wait...
THE VELA SUPERNOVA - 4 Panel Mosaic - Deepsky 762mm RGBhA - Constellation Vela, Thomas ArtOfPix Großschmidt
THE VELA SUPERNOVA - 4 Panel Mosaic - Deepsky 762mm RGBhA - Constellation Vela
Powered byPixInsight

THE VELA SUPERNOVA - 4 Panel Mosaic - Deepsky 762mm RGBhA - Constellation Vela

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Description

THE VELA SUPERNOVA
- 4 Panel Mosaic
- Deepsky 762mm RGBhA
- Constellation Vela

The Vela Supernova Remnant (also known as Vela-SNR) is a remnant of a supernova explosion that took place about 11,000 to 12,000 years ago. It is located in the southern hemisphere of the sky in the constellation Vela (Sail of the Ship).
The Vela-SN remnant covers an area of about 8 degrees in the sky, which is about 16 times the size of the full moon. It consists of various components, including a series of filaments, shock waves and pulsar wind nebulae.
The supernova that produced the Vela SN remnant was one of the closest known supernovae to Earth, leaving behind a large amount of matter that is expanding at high speed. The shock wave from the explosion collides with the interstellar medium, creating characteristic shock fronts and filaments.
At the center of the Vela-SN remnant is the Vela pulsar, a high-energy neutron star that spins extremely fast and emits regular pulses of electromagnetic radiation. The pulsar has an influence on the surrounding matter and produces the pulsar wind nebula, which is visible as a bright, high-energy structure.

VelaSupernova_LRGBHOO_RemoteTelescope_4PanelMosaik_762mm-SW-web4096.jpg
VelaSupernova_LRGBHOO_RemoteTelescope_4PanelMosaik_762mm_Starless-web4096.jpg

Optic |Takahashi TOA-130, Reducer, 762mm, f/5.9 (T10 iTelescope)
Camera|FLI Proline 16803, Astrodon 2 Gen E-Series Luminance/Red/Green/Blue/H-Alpha 3nm
Filter|Astrodon 2 Gen E-Series R, G, B, hA, OIII 3nm
LUM |Superluminance from hA & OIII
RGB |5xRed/5xGreen/5xBlue each 180s Bin1x1 per panel
NB |12xhAlpha/12xOIII each 1200s Bin1x1 per panel
EBV |4 Panel Combination SuperLUM RGB HOO
Loc |Siding Spring Observatory Australia 

Premium imageset, taken by iTelescope, Image Processing - Thomas ArtOfPix Großschmidt
Date: 26.05.2023

Image processing:
Mainly Pixinsight, Photoshop, Lightroom, GraXpert, BTX Blur Terminator, Noise Terminator, Star X Terminator

#velasupernova #supernova #universe #artofpixastro #astrophotography #itelescope

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