Category: H II nebula

NGC 6888 Crescent Nebula

Crescent Nebula, also known as NGC 6888, is a HII region, hot ionized hydrogen gas cloud. The nebula got the shape by high speed stellar wind of Wolf-Rayet star, which is colliding with slow moving mass, ejected by this star during transformation into a red giant. The nebula is approximately 5000 light-years away from us and it can be located in constellation Cygnus.

The picture is the last one from 6.9.2018. In the evening I captured Omega nebula, M80. As a last deep space object I pointed on Crescent Nebula, started auto guiding and went to sleep. Therefore the picture is a stack of 64 pictures; each has 3 minutes of exposure time, thus total integration time 192 minutes.

Technical details:

TelescopeNewton 150/600 mm
Aperture150 mm
Focal length660 mm
MountiOptron CEM25P
AutoguidingQHYCCD miniGuideScope 130 mm f/4.3, ZWO 174 MM
CameraZWO 071 Pro @-10C
CorrectorExplore Scientific HR coma corrector
FiltersAstronomik L-1 - UV IR Block Filter
Exposure64x180s, Gain 134, bin 1x1,
Date2018-09-06

M17 Omega Nebula M18 Open Cluster

Due to moderate focal length of my telescope (660 mm) I managed to capture two Messier’s object in one shot. Specifically it was Omega nebula M17 (on the right) and open cluster M18 (on the left). I already captured Omega nebula some time ago, but due to its very low declination, the picture was not that nice. I was really happy that I got the opportunity on island Milos to capture it again. The cluster M18 is approximately 4200 light-years away from Earth and it has diameter 17 light-years.

Technical details:

TelescopeNewton 150/600 mm
Aperture150 mm
Focal length660 mm
MountiOptron CEM25P
AutoguidingQHYCCD miniGuideScope 130 mm f/4.3, ZWO 174 MM
CameraZWO 071 Pro @-10C
CorrectorExplore Scientific HR coma corrector
FiltersAstronomik L-1 - UV IR Block Filter
Exposure37x180s, Gain 134, bin 1x1,
Date2018-09-06

IC 1318 Butterfly Nebula, Barnard 347

IC 1318 is an emission nebula, sometimes called Sadr region, located in constellation Cygnus, surrounding bright star Sadr. The star Sadr didn’t fit into the field view of my telescope/camera, but left the trace in form of diffraction spike at the top of the picture. The nebula contains many dark nebulae and the biggest in the middle of the picture is called Barnard 347.

The picture is another demonstration of dark skies of Milos and it is an integration of 77 pictures, each 3 minutes exposure, which means nearly 4 hours of integration time.

Technical details:

TelescopeNewton 150/600 mm
Aperture150 mm
Focal length660 mm
MountiOptron CEM25P
AutoguidingQHYCCD miniGuideScope 130 mm f/4.3, ZWO 174 MM
CameraZWO 071 Pro @-10C
CorrectorExplore Scientific HR coma corrector
FiltersAstronomik L-1 - UV IR Block Filter
Exposure77x180s, Gain 134, bin 1x1,
Date2018-09-05

M8 Lagoon Nebula

Lagoon nebula (sometimes called Messier 8) is a giant intergalactic cloud of ionized Hydrogen. The nebula is located in constellation Sagittarius and it’s 4100 light-years away from Solar System. It belongs to one of the brightest nebulas visible from northern hemisphere.

I have to admit, this nebula was the main reason and target of the trip to Milos and it was the first deep space object captured there. When I processed the picture I was so happy that the nebulosity is so clearly visible without any narrow band filters. Well, mission accomplished.

Technical details:

Telescope:Newton 150/600 mm
Aperture:150 mm
Focal length:660 mm
MountiOptron CEM25P
AutoguidingQHYCCD miniGuideScope 130 mm f/4.3, ZWO 174 MM
Camera:ZWO 071 Pro @-10C
Corrector:Explore Scientific HR coma corrector
Filters:Astronomik L-1 - UV IR Block Filter
Exposure39x180s, Gain 134, bin 1x1,
Date:2018-09-01

NGC281 Pacman nebula

NGC281 is a HII region, which reminds a head of the main character in very popular game from nineties. It is located in constellation Cassiopeia and it 9500 light-year far from us. This nebula was discovered long time ago by Edward Emerson Barnard and it is possible to observe this nebula by reasonable sized telescope under dark skies. Well, I wouldn’t see probably anything, because I live in light polluted area, therefore I had to use narrow band filters, which block the light pollution.

The picture is composed out of 66 narrow band exposures, which means slightly more than one hour per channel. First one is bi-color composition of hydrogen and oxygen, the others are in Hubble palette (hydrogen in green, oxygen in blue and sulfur in red).

Technical details

Telescope:Newton 254/1000 mm
Aperture:254 mm
Focal length:1000 mm
MountGemini G53f
AutoguidingTS 60 mm, ZWO 174 MM
Camera:Moravian instruments G2 8300M @-30C
Corrector:GPU coma corrector
Filters:Baader narrow band
Exposure:8x22xHa, 22xOIII, 22xSII 180 s, bin 1x1,
Date:2018-01-13

 


IC1848 Soul nebula

Soul nebula is a beautiful HII region, where new stars are being born. It’s located in the constellation Cassiopeia and it’s 7500 light-years from Earth. The nebula has a neighbor Heart Nebula (IC1805). One can say that in this constellation the heart and soul are close to each other.

As usual, I used narrow-band filters to capture this spectacular nebula. It didn’t fit into my field of view; this means I would need a shorter focal length.

Update 2023-05-07. I returned to this data and reprocessed it, using the latest post-processing know-how. I learned a lot in the last few years, and Pixinsight got very useful plugins. For example, Blur Exterminator sharpens the data, but it still looks realistic without any artifacts. However, the biggest difference is the white balance of the picture. I used the rainbow SHO technique published by
lukomatico.

Technical details

Telescope:Newton 150/600 mm
Aperture:150 mm
Focal length:438 mm
MountGemini G53f
AutoguidingTS 60 mm, ZWO 174 MM
Camera:Moravian instruments G2 8300M @-30C
Corrector:ASA 0.73 reducer
Filters:Baader narrow band
Exposure:8x77xHa, 77xOIII, 77xSII 180 s, bin 1×1,
Date:2017-11-23

IC5070 Pelican nebula

Pelican nebula is large cloud of hydrogen gas, where many stars are being born, located in constellation Cygnus (Swan). The nebula is approximately 2000 light-years away from Earth. If you use bit of an imagination, you will be able to see the pelican in the dark cloud surrounding the brighter center of the nebula – good luck with searching.

The picture was taken completely by narrow band filters. The first one is in “fake” Hubble palette and second one as a bi-color image (Ha in red channel, OIII in green and blue channel).

Technical details

Telescope:Newton 150/600 mm
Aperture:150 mm
Focal length:438 mm
MountGemini G53f
AutoguidingTS 60 mm, ZWO 174 MM
Camera:Moravian instruments G2 8300M @-30C
Corrector:ASA 0.73 reducer
Filters:Baader narrow band
Exposure:8x32xHa, 32xOIII, 32xSII 180 s, bin 1x1,
Date:2017-12-15


IC1396 Elephant trunk nebula

Elephant trunk nebula is visually one of the biggest deep space objects in the sky. It covers more than 6 times the diameter of the Moon. I had to use the telescope with the shortest focal length and use focal reducer ASA 0.73. Recently, I managed to improve the picture quality of this reducer by adjustment of the tilt. The nebula can be located in constellation Cepheus, but it cannot be spotted visually because it’s very dim.

I spent 4 nights capturing these photos. In total, there is nearly 19 hours of exposure time. Probably this is my longest integration time I have ever made. The first picture is in fake Hubble colors, second one in more or less visible spectrum colors.

 

Technical details

Telescope:Newton 150/600 mm
Aperture:150 mm
Focal length:438 mm
MountGemini G53f
AutoguidingOrion Mini Autoguider
Camera:Moravian instruments G2 8300M @-30C
Corrector:ASA 0.73 reducer
Filters:Baader narrow band
Exposure:8x125xHa, 125xOIII, 125xSII 180 s, bin 1x1,
Date:2017-10-17


M20 Trifid nebula

Trifid nebula is a combination of emission, reflection and dark nebula – pretty unique. It got its name from 3 dark lines across emission (red) part. The lines are dust clouds blocking the light emitted by ionized hydrogen.  It’s possible to observe this nebula, but one needs dark skies and a telescope with aperture at least 120 mm. The nebula can be found in constellation Sagittarius and it’s 5200 light-years far from Earth.

The picture was taken in Gavdos during my first dark sky chasing. The total integration time is only one hour, which is remarkable for such portable setup.

Technical details

Telescope:RC 154/1370
Aperture:154 mm
Focal length:917 mm
MountiOptron CEM25P
AutoguidingQHYCCD miniGuideScope 130 mm f/4.3, ZWO 174 MM
Camera:ZWO 1600 MC @ -15C
Corrector:Astro Physics CCDT67
Filters:UV, IR cut
Exposure:20x 180s Gain 240
Date:2017-09-23


NGC6604 Open cluster

NGC6604 is an open cluster associated with nebulosity. It is located not far from my favorite Eagle nebula in constellation Serpens and it’s 5500 light-years far from the Earth. Since this deep space object is not that high on the skies, I rather used narrow band filters, because this part of the skies is strongly influenced by the light pollution, which is coming from the nearest town. First picture is processed in “fake” Hubble color palette, the second one should more or less look like in “true” color.


NGC2264 Cone nebula

Cone nebula is a giant cloud of ionized hydrogen gas, which includes the Christmas Tree Cluster. It’s located between two bright winter stars Betelgeuse (constellation Orion) and Procyon (Canis Minor) and it’s 2700 light-years far from the Solar System. There is a famous picture from Hubble Space telescope of the tip of the cone – star forming complex.

Bi-color picture didn’t look as I expected, therefore I decided to publish only mono version of hydrogen alpha channel.


M42 Great nebula in Orion

I don’t want to repeat myself, therefore the description of the most famous nebula visible from the northern hemisphere can be found here.

The previous picture has some strange halo around the bright star Hatsya and I was thinking why. Recently, a similar picture came out of my telescope and I realized that this strange halo is caused by the frost on the secondary mirror. I manufactured a homemade dew shield and I don’t have these problems anymore.

This picture is, as usual, composed of narrowband pictures. When I look at it I am still not happy, therefore I hope next year will be better weather and I will make a better picture.

Telescope:Newton 254/1000 mm
Aperture:254 mm
Focal length:730 mm
Mount:Gemini GF53f
Autoguiding:Orion Mini, TS 50/160 mm
Camera:Moravian instruments G2 8300M @-30C
Corrector:ASA 0.73 reducer
Filters:Baader Ha, OIII
Exposure:17xHa, 15xOIII, 240 s, 10xHa, OIII 60 s bin 1x1
Date:2017-01-07

NGC7380 Wizard nebula

Wizard nebula is an open cluster associated with nebulosity.  Visually, it has apparent size of the full Moon, but since it’s very far from the Earth (7200 light years), its real diameter is about 100 light years.

So, where is the wizard located? It took me a while to find him, but if you turn your head 90° counter-clockwise, you see two darker hands. It looks like he is trying to grab something. Then above the hands you see the wizard’s conical hat.

First picture is a composition of 3 narrow band pictures (Ha, OIII and SII) and composed in Hubble Space Telescope palette. Second one is more-or less visible spectrum.

ngc7380-wizard-2016-10-06-30c-600s-32x-haoiiisii-fl1000-dbe-proc ngc7380-wizard-2016-10-06-30c-600s-32x-haoiiisii-fl1000-dbe-rgbeq


NGC6820 Nebula

NGC6820 Nebula doesn’t have a name, so let’s call it Hidden octopus nebula (because only one tentacle is visible). Hidden octopus nebula is a giant cloud (50 light years in diameter) of ionized hydrogen alpha gas, where new stars are born. The tentacle forms a similar structure just like in the more famous M16 Eagle nebula. It’s located in the constellation Vulpecula (Little fox) not far from M27 Dumbbell nebula and it’s 6000 light years from Earth.

The picture was processed in the bi-color technique. This means I collected the photos through two filters: H alpha and OIII. H alpha was inserted into the red channel, and OIII into the green and blue one.

ngc6823-nebula-2016-08-04-300s-30c-22ha-20oiiii-fl1000-gpu

Telescope:Newton 254/1000 mm
Aperture:254 mm
Focal length:1000 mm
Mount:Gemini GF53f
Autoguiding:ZWO 174MM, TS 60/240 mm
Camera:Moravian instruments G2 8300M @-30C
Corrector:GPU
Filters:Baader Ha OIII
Exposure:22xHa 30 s, 20xOIII, bin 1x1
Date:2016-08-23


M17 – Omega Nebula

Omega Nebula is a giant cloud of the hydrogen gas where new stars are born. It’s around 5000 light years from Solar system and it has 15 light years in diameter. The nebula is located in constellation Sagittarius (The Archer) and it’s the most massive star-forming location in our galaxy. Visual observation is possible, but only with the telescope (medium or big aperture) and from the place with low light pollution.

Since this nebula is visible in summer, there is not enough time to collect enough photons during one night (short nights in summer). Therefore I had to photograph this deep space object several nights (4 in total) and I collected 7.2 hours of the exposure time. Since the light pollution is quite high on the south, I used narrowband filters to collect three channels (H alpha, OIII and SII). I was playing with pixel math and placing partially some narrowband images into Red Green Blue channels and here are the results of my experimentations:

M17-2016-07-05-22Ha32OIII32SII-300s-30C-FL1000-01 M17-2016-07-05-22Ha32OIII32SII-300s-30C-FL1000-RGB M17-2016-07-05-22Ha32OIII32SII-300s-30C-FL1000-SCNR


NGC 6888 – Crescent Nebula

In an emission nebula located in constellation Cygnus (swan), 5000 light years from Earth. The nebula has 25 light years (!) in diameter. This constellation, as well as the nebula is lying on the plane of our home galaxy Milky Way. Therefore there are so many stars visible.

The picture was processed by bi-color technique – this means that the picture is assembled from two narrow band images: hydrogen alpha (Ha) and ionized oxygen (OIII). Ha was inserted into red channel and OIII into green and blue.

NGC6888_2015-08-23_600s_22Ha_8OIII-30C


NGC2237 Rosette nebula

Another place where the stars are born is called Rosette nebula. It is a cloud of hydrogen gas, located 5000 light years from Earth in constellation Monoceros (unicorn). The diameter of this nebula is 50 light years.

This time I processed collected data by two different ways. Basic data are three monochromatic pictures captured through narrow band filters: Hydrogen alpha, Oxygen OIII and Sulfur SII.

First technique is called Hubble pallet – natural color of H alpha is red, but it’s inserted into green channel, oxygen is blue, therefore ends in blue channel and sulfur is even more “red” than the red color, therefore lands in red channel. After many different post-processing steps the final picture looks like this:

NGC2237-Rosette-2016-02-10-360s-40C-17Ha-19OIII-10SII-FL730-Hub

Second technique is more realistic for the human eyes and brain, and requires pixel math. H alpha is red, SII even more, therefore the combination of this pictures (SII + 0.8*H alpha) will end up in red channel. Green channel is a combination of 0.075*H alpha + OIII. Finally blue channel is just OIII.

NGC2237-Rosette-2016-02-10-360s-40C-17Ha-19OIII-10SII-FL730-Tri

I am quite curious which picture you like more…


B33 Horsehead Nebula

Horesehead nebula is a dark nebula located in constellation Orion, approximately 1550 light years from Earth. The bright star is on the picture is called Alnitak (eastern star of Orion’s belt). Horsehead shape is a cloud of cold gas, blocking the light coming from ionized hydrogen in the background.

This nebula is my favorite, but it’s not so simple to photograph, due to its dimness. Even with very fast telescope (f-stop 2.8) I had to use quite long exposure times – 6 minutes. The picture was postprocessed by bi-color technique, which means putting 27 H alpha pictures into red channel and 17 OIII pictures into green and blue channel. This was done in Pixinsight software.

B33-2016-02-05-FL730-40C-360s-27Ha-15OIII-LHa


H II regions

H II regions are vast clouds of ionized hydrogen gas, where new stars are born. The clouds of the gas are being pushed by shock waves caused by supernovae and other mechanisms, which can trigger a collapse and new stars being born during this process.

Most of the observable H II regions are located in our galaxy Milky Way, but there are also visible some H II regions in our neighboring galaxies, for example in M33 Triangulum Galaxy.

The most famous H II regions are M42 Orion Nebula, M16 Eagle Nebula.


M42 Great nebula in Orion

I think everyone knows constellation Orion, but only few people know that there is Great nebula in Orion, visible even by naked eye. It’s located between his belt and legs. The nebula is approximately 1300 light years from earth and it has 24 light years in diameter. Red color shows a lot of hydrogen gas, which is essence for star formation. In fact, the Orion nebula is the closes location from Earth, where the stars are born.

Since this nebula is visible by naked eye, with help of telescope even with sub-urban area, it’s not necessary to use long exposure times. I used just 3 minutes exposures and the picture yielded in nearly overexposed photo. Small nebula on the right side is NGC1973 Running man nebula.

M42-OrionNebula-2015-12-13-30-20x180sL-12x120sRGB2x2-FL730