The Jellyfish Nebula | IC 443

The Jellyfish Nebula IC 443 in Gemini, imaged from a light polluted urban sky

THE JELLYFISH NEBULA

IC 443 • Supernova remnant • Gemini • 5000 light-years from Earth


🗓️
Jan – Feb 2025

Overview

The Jellyfish Nebula (IC 443) was formed around 30,000 years ago, when a high-mass star reached the end of its life and exploded as a supernova. The material that the star was made from — plus new elements forged in the extreme temperatures of the explosion — blasted outwards. Fast-forward to today, and we see the remnants as the Jellyfish Nebula.

It’s a tricky target to image through the haze of light pollution, but if you can use filters to isolate specific wavelengths of light then it’s possible to produce striking photos.

Background

My plan for this target was to use a variety of filters in order to capture Hα, SII, and OIII wavelengths of light, plus RGB stars. Unfortunately, bad weather and technical issues meant I needed to cut the project short, with just 20 hours of Optolong L-Ultimate data. This gave me enough Hα and OIII to create an interesting image, although I had to apply a lot of noise reduction during processing.

The Jellyfish Nebula IC 443 showing tangled supernova remnant filaments, captured from an urban location
Framed astrophoto taken from a light-polluted city, available to buy as a fine art print

Close-ups

  • Close-up of the Jellyfish Nebula revealing complex filamentary structure within IC 443
  • Detailed view of IC 443 highlighting overlapping shock fronts from a supernova explosion
  • Inner filaments of the Jellyfish Nebula showing turbulent ionised gas
  • Close-up of the Jellyfish Nebula emphasising fine arcs of supernova remnant material
  • Detailed view of IC 443 highlighting overlapping shock fronts from a supernova explosion

Science

We know that the Jellyfish Nebula is the remains of a star that exploded as a supernova; but was anything left of the star? It turns out yes, the dense core was left and became a neutron star. This is a sphere about 20km across (twice the size of my home city of Bristol), but with more mass than the Sun. In terms of density, it’s second only to a black hole. This particular neutron star is likely to be spinning very rapidly, meaning it is in fact a pulsar.

The pulsar itself is moving through space at a break-neck speed of 800km every second. The reasons for this aren’t known for sure. The original star could have been careening through space when it went supernova, or perhaps the explosion itself blasted the remains of the star, in effect giving it a cosmic kick!

The pulsar is leaving a trail of high-energy particles in its wake as it hurtles through space. These have been observed by astronomers using the Chandra X-Ray space telescope and Very Large Array radio observatory in New Mexico. (More info here).

My telescope and camera can’t detect light in these wavelengths, so the neutron star is invisible to me. Still, I managed to track its location down on my image. It’s a good example of how multi-wavelength astronomy reveals a universe normally hidden from view:

Use the slider below to compare my image with the multi-wavelength professional image.

Composite image credit — Chandra X-ray: NASA/CXC/B.Gaensler et al; Radio Detail: NRAO/AUI/NSF; Optical: DSS.

Imaging details

Date

15 January – 28 February 2025 (six weeks)

Location

Bristol, UK (Bortle 8)

Telescope

Askar 130PHQ Flatfield Astrograph

Camera

ZWO ASI 2600MC Pro

Mount

Sky-Watcher EQ6-R Pro

Guiding

WO 50mm + ZWO ASI 120MM Mini

Control

ASIAIR Plus

Software

PixInsight, Lightroom

Image by

Lee Pullen

Filter

Channels

Exposure

Optolong L-Ultimate

Hα / OIII

240 × 5-minutes (20 hours)

20 hours

Imaging details

Date
15 January – 28 February 2025 (six weeks)

Location
Bristol, UK (Bortle 8)

Telescope
Askar 130PHQ Flatfield Astrograph

Camera
ZWO ASI 2600MC Pro

Mount
Sky-Watcher EQ6-R Pro

Guiding
WO 50mm + ZWO ASI 120MM Mini

Control
ASIAIR Plus

Software
PixInsight, Lightroom

Image by
Lee Pullen

Filters

Optolong L-Ultimate
Hα / OIII
240 × 5-minutes (20 hours)

Total exposure: 20 hours

Kit list

This is the equipment I used to capture the image.
Affiliate links help support the site at no extra cost to you.

Guidescope: William Optics 50mm with ROTO Lock

Guidescope: William Optics 50mm with ROTO Lock
Read my review

Buy from Astroshop.eu
Buy from High Point Scientific

Processing walkthrough

I used a few SetiAstro PixInsight processes, including to stretch the image from non-linear. The trickiest thing was dealing with large halo around the bright star Propus. I used Photoshop’s Generative Fill to remove this.

Example astrophotography image promoting one-to-one online astrophotography masterclasses

Example source data

Here are example single subframes and freshly integrated stacks, just with simple stretches applied.

Askar FRA400 image

I first imaged the Jellyfish Nebula back in January 2022, using my wide-field Askar FRA400 telescope.

Imaging details

Date

January 2022

Location

Bristol, UK (Bortle 8)

Telescope

Askar FRA400 f/5.6 Quintuplet APO Astrograph

Camera

ZWO ASI 2600MC Pro

Mount

Orion Sirius EQ-G

Guiding

William Optics 32mm; ZWO ASI 120MM Mini

Control

ASIAIR Plus

Software

PixInsight, Lightroom

Image by

Lee Pullen

Filter

Channels

Exposure

Optolong L-eXtreme

Hα / OIII

600 × 2-minutes

20 hours

Askar FRA400 image

first imaged the Jellyfish Nebula back in January 2022, using my wide-field Askar FRA400 telescope.

Imaging details

Date
January 2022


Location
Bristol, UK (Bortle 8)


Telescope
Askar FRA400

Camera
ZWO ASI 2600MC Pro

Mount
Orion Sirius EQ-G

Guiding
WO 32mm; ZWO ASI 120MM Mini

Control
ASIAIR Plus

Software
PixInsight, Lightroom

Image by
Lee Pullen

Filters

Optolong L-eXtreme
Hα / OIII

600 × 2-minutes (20 hours)

Total exposure: 20 hours

Seestar S50 image

This photo of the Jellyfish Nebula was taken using my Seestar S50 telescope.






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