The Heart Nebula | IC 1805

The Heart Nebula IC 1805 in Cassiopeia, imaged from a light-polluted city

THE HEART NEBULA

IC 1805 • Star-forming emission nebula • Cassiopeia • 7500 light-years from Earth


🗓️
December 2022

Overview

The Heart Nebula, also known as IC 1805, is a vast emission nebula in the constellation Cassiopeia. Spanning around 200 light years across and lying roughly 7500 light years from Earth, it is dominated by glowing clouds of hydrogen gas shaped by radiation and stellar winds from young, massive stars. This combination of scale and structure makes the Heart Nebula a popular target for astrophotography, even from light polluted locations.

Background

This attempt at the Heart Nebula was taken with a new telescope (Askar 130PHQ), and interestingly, a new set of filters: Askar Colour Magic D1 and D2. Click here for my review of these.

The Askar 130PHQ has a focal length of 1000mm, compared to my old Askar FRA400‘s 400mm. This allowed me to get a closer view of the central region, nicknamed the Heart of the Heart. In the middle of this is Melotte 15, a collection of young hot stars whose radiation is sculpting the surrounding area. Melotte 15 is only 1.5 million years old; babies, in star terms!

Using the new set of filters allowed me to not only capture Hα and OIII data, (as I usually do with narrowband imaging using filters like the Optolong L-eXtreme and, more recently the Optolong L-Ultimate) — but also SII data. This helped to create the colourful end result.

The Heart Nebula IC 1805 in Cassiopeia, imaged from a light-polluted city
Framed astrophoto taken from a light-polluted city, available to buy as a fine art print

Close-ups

  • Close-up view showing delicate nebulosity
  • Close-up view showing the Heart Nebula's central region, surrounded by stars
  • Close-up view of nebulosity meeting deep space
  • Close-up view showing subtle details

Science

Within the “heart of the Heart nebula” lies Melotte 15. This area is packed with hot, high-mass O and B-type stars, just a few million years old. They’re producing powerful stellar winds and ultraviolet radiation, carving out cavities and shaping the surrounding gas and dust in the Heart Nebula.

Some of the stars are over 50 times the mass of the Sun and are destined to live fast die young, with dramatic ends as supernova explosions.

Imaging details

Date

December 2022

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

Askar Colour Magic D1

Hα / OIII

360 x 2-minutes (12 hours)

Askar Colour Magic D2

SII / OIII

360 x 2-minutes (12 hours)

24 hours

Imaging details

Date
December 2022

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

Askar Colour Magic D1
Hα / OIII
360 x 2-minutes (12 hours)

Askar Colour Magic D2
SII / OIII
360 x 2-minutes (12 hours)

Total exposure: 24 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.

William Optics 50mm with ROTO Lock guidescope

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

Buy from Astroshop.eu
Buy from High Point Scientific

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

Example source data

Askar FRA400 image

I first imaged the Heart Nebula back in December 2020, using my wide-field Askar FRA400 telescope. Here’s version 1, and then version 2 from my Reprocessing Bonanza 2022, then version 3 that I reprocessed in August 2025.

Imaging details

Date

December 2020

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

102 × 5-minutes

8.5 hours

Askar FRA400 image

I first imaged the Heart Nebula back in December 2020, using my wide-field Askar FRA400 telescope. Here’s version 1, and then version 2 from my Reprocessing Bonanza 2022, then version 3 that I reprocessed in August 2025.

Imaging details

Date
December 2020

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

102 × 5-minutes

Total exposure: 8.5 hours

Seestar S50 image

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






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4 thoughts on “The Heart Nebula | IC 1805

  1. Michael Brennan says:

    I have a question for you, I have been considering getting on the narrowband “band-wagon” and have been doing some researching.

    This is my current setup (I have 2 sites Class 6 and Class 4 Bortle):
    Celestron Edge 11HD + 0.7 Reducer/flatner on CGX mount + off-axis guder
    ZWO ASI2600MC PRO (I only have the IDAS LPS-D2-48 light polution filter)

    I have been thinking about getting either the “Optolong L-eXtreme 7nm” or the “Optolong L-Ultimate 3nm” and wieghing the pros vs cost.
    Another thing that I was thinking of is a filter wheel with SHO set (cost would be higher for filters of course and I was thinking of getting a filter wheel anyways)

    I am just wondering if the extra cost of the SHO set vs “Optolong L-Ultimate 3nm” would net me better images?

    What’s your option … Thanks

    Reply
    1. Lee says:

      Hi Michael, thanks for your message. I’ve written an article on OSC vs Mono that you might find interesting. It’s geared towards astroimagers from a city, but is still relevant for you even with your darker skies.

      To directly answer your question though, mono plus SHO filters will give you higher image quality than OSC and a dualband filter, but by how much and how noticeable it will be is harder to answer. My personal opinion is that an image’s total integration time and an astroimager’s processing skills are more important factors. Also note that with a mono camera you’d likely want a set of LRGB filters as well, for imaging broadband targets.

      You mentioned the L-eXtreme and L-Ultimate. I compare these in this review. The L-Ultimate is the best, so I recommend it over the L-eXtreme. (Previously I used an L-eXtreme but have now upgraded to an L-Ultimate).

      Another option to throw into the mix is the Askar D2 filter (review here). That collects SII & OIII, and during processing you can combine that with Optolong L-Ultimate data (Ha & OIII) to create SHO images. See my Heart Nebula and Soul Nebula photos for examples of end products using this method. Would the final images have been better if I’d used a mono camera and SHO filters? Possibly yes, but I’m certainly happy with the images I produced, and the data acquisition was more straightforward than with mono.

      So, I think you have three options: mono and filters; OSC and Optolong L-Ultimate; or OSC and Optolong L-Ultimate plus Askar D2. (The latter option is what I’m currently using). There’s no straightforward answer, and they all have different costs associated with them.

      Instead of thinking about what would net you the best images, think about what you’d find most fun to use. If you want to go really deep into the hobby, and you’ve got the time and budget to accommodate a complex set-up, then mono is likely the answer. If you want a straightforward rig that’s still capable of producing good images (and is also much cheaper than mono), then it’s OSC plus Optolong L-Ultimate. Add an Askar D2 filter and then you’ve got a middle-ground between those two options.

      Good luck with whatever you choose, and feel free to ask more questions if you think I can help further.

      Reply

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