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Thursday, November 28, 2024

Beauty and the Beast, Tulip Nebula and a Black Hole

I started to collect exposures for this photo back in 2014, now I have shot new high resolution material for this amazing target with my new imaging platform. 

I see several layers in my photos and that makes them to tell a story beyond any imagination.

First

A visual layer, that's naturally very important to me as a visual artist, revealing the hidden cosmic beauty and poetry is my passion.

Second 

The physical layer, how emission of the nebulae works, radiation pressure, nuclear fusion of the star, gravitational phenomes, etc... all that is extremely beautiful in its own class.

Third 

An existential layer, where we are coming and where we are going in a cosmic scale.
Practically all of the heavier elements in our bodies are coming from supernova explosion's, iron in our blood, oxygen, carbon, etc... We are children of the stars
When our Sun will die after few billion years and turn to a planetary nebula, it'll vaporize the Earth and our remains on it and blows them to the outer space. After aeons our remains are going to end up to a building blocks for a new generation of stars.
We all have been stars and one day we going to be stars again.

This is the beauty and poetry I'm after my photos


BEAUTY AND THE BEAST

Tulip Nebula and a Black Hole 
Click the photo to see a high resolution photo, it's worth it 

A two frame mosaic from a light emitted by an ionized elements,
sulfur=red, hydrogen=green and oxygen=blue


One frame


Black Hole Cygnus X-1
Click the photo to see a high resolution photo, it's worth it 


Black Hole, Cygnus X-1, is marked in the photo


INFO

The complex and beautiful Tulip Nebula, Sharpless 101,  blossoms about 8,000 light-years away toward the constellation of Cygnus the Swan. Ultraviolet radiation from young energetic stars ionizes the atoms and powers the emission from the Tulip Nebula.  

Also in the featured field of view is the black hole Cygnus X-1, which is also a microquasar because it is one of strongest X-ray sources in planet Earth's sky. The powerful jets from the black hole can't be seen in this photo since they glow light in X-ray wave length. Faint bluish curved shock front, visible at up center, is coursed by the X-ray jet when it hits to a interstellar gas and dust. 

Why we can see the black hole in this image as a star like object?

We can't see the actual black hole but we can see how the material is twirling in the black hole. The speed become so high that the matter starts to turn to an energy emitting light trough the whole spectrum up to X-ray and gamma radiation. 


Photo in Visual Colors
Click the photo to see a high resolution photo, it's worth it 

A two frame mosaic from a light emitted by an ionized elements,
sulfur=red, hydrogen=red and oxygen=blue

Technical details

Processing workflow

Image acquisition, MaximDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 27 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics, Celestron EDGE 14" with 0.7 Focal reducer

Mount, MesuMount Mark II

Cameras, Imaging camera Apogee Alta U9000M and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AO Active Optics @ 5hz

filters, Astrodon 5nm H-alpha, 3nm S-II and 3nm O-III

Total exposure time 20h
H-alpha, 15 x 1200 s, binned 1x1 = 10 h
O-III, 45x 1200 s, binned 1x1 = 5 h 
S-II, 9 x 1200 s. binned 2x2 = 5h


A single, full scale, 20 min H-alpha exposure, Bin 1x1
 Click for a full scale image.



A single, full scale, 20 min S-III exposure, Bin 2x2
 Click for a full scale image.



A single, full scale, 20 min O-III exposure, Bin 1x1
 Click for a full scale image.







Saturday, November 23, 2024

Astro Anarchy get published

 After about three years without shooting new material from the night sky I'm finally back in business.
I had some health issues and after three operations I'm starting to be good as new again. I have also built a new imaging system, it took about two years to get it up and running. 

I was really amazed about the amount of publicity my work got after I publish my first photos from the new setup. Here are some of the publication, couple of them are in finish only, sorry.


My TV-interview in a live talk show, 
Arto Nyberg (Finish)
You can see the show here: https://areena.yle.fi/1-70235645






PETA PIXEL
World's leading independent photography, videography, and imaging technology publication

"This Astrophotographer Captures the Universe Unlike Anyone Else"
JEREMY GRAY

You can read the article here: 







MY MODERN MET
5 million visitors coming to our site each month, looking for articles on art, design, photography, architecture, science, technology, environmental issues, and more.

"Remarkable Astrophotography Captures the Sublime Beauty of Universe"
Jessica Stewart on November 11, 2024

You can read the article here: 







AN INTERVIEW BY RADIO KALEVA

"Olemme kaikki su­per­no­vien lapsia" 

Haastattelun voi kuunnella täältä sivun lopusta: (Finish)
https://www.kaleva.fi/olemme-kaikki-supernovien-lapsia-oululainen-tahtik/11396012

Kuva: Maiju Pohjanheimo




Tuesday, October 29, 2024

Methuselah Nebula, MWP1, project finalized

Planetary Nebulae are like candy of the cosmos, small and colorful treats to the eye.
MWP1 is a Planetary Nebula in constellation Cygnus, the Swan, it's rarely imaged and now I know why.

This is a unusually old, unusually shaped and unusually large planetary nebula, it also was one of the most difficult targets I have captured so far.

When I saw the first  20 min. exposure, it looked like there is plenty of nothing in the frame, this is dim to an extreme.  I have added full size 20 min sub frames of H-alpha and O-III at the end of this blog post so you can see yourself how much data there is. 


MWP1, Methuselah Nebula
Click for a full size image

Photo is in natural color palette from the light emitted by an ionized hydrogen (H-alpha) 
and an ionized oxygen (O-III)




MWP1 in O-III light only
Click for a full size image

The structure of MWP1 in light of an ionized oxygen (O-III)



INFO

More or less symmetric planetary nebula cataloged as MWP1 lies some 4,500 light-years away in the northern constellation Cygnus the Swan. 

This is one of the largest planetary nebulae known, it spans about 15 light-years. Based on its expansion rate the nebula has an age of 150 thousand years, a cosmic blink of an eye in the 10 billion year life of a sun-like star. But planetary nebulae represent a very brief final phase in stellar evolution, as the nebula's central star shrugs off its outer layers to become a hot white dwarf. In fact, planetary nebulae ordinarily only last for 10 to 20 thousand years. 

The central star of the nebula is on of the hottest stars known. It's so hot that it's producing large amounts of X-rays

Source NASA APOD


Scale in the Sky

The white circle show the apparent size of the Moon in the same scale, this is a large object as a Planetary nebula. Moon has a angular dimension of 30 arcminutes, that's 0.5 degrees. 




Animation

I made this small animation to show the difference between two emission lines, H-a and O-III



Technical details

Processing workflow

Image acquisition, MaximDL
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2, Positive Constraint, 27 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics, Celestron EDGE 14" with 0.7 Focal reducer

Mount, MesuMount Mark II

Cameras, Imaging camera Apogee Alta U9000M and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AO Active Optics @ 5hz

filters, Astrodon 5nm H-alpha and 3nm O-III

Total exposure time 24h
H-alpha, 21 x 1200 s, binned 1x1 = 8 h
O-III, 48x 1200 s, binned 1x1 = 16h 



A single, full size, 20 min H-alpha and O-III exposure
 Click for a full scale image.

Both images below are jpg photos of a single full size, 20 min. FIT-format 16 bit image. 
Photos are calibrated with darks and bias corrected flats and are heavily stretched to show even a hint of the actual nebula.

H-alpha




O-III








Sunday, October 20, 2024

A start of the new imaging project, MWP1, the Methuselah Nebula

MWP1 ( Motch-Werner-Pakull 1, PN G080.3-10.4, PK 080-10.1) is a very old, dim and diffused planetary nebula in constellation Cygnus, the Swan. It's one of the largest planetary nebula known, it spans about 15 light years of space. The apparent size in the sky is 15.52 x 13,13 arcminutes. (Full moon has a diameter of 30 arcminutes) The estimated age of the nebula is 150.000 years.  

MWP1 is a very usually shaped, unusually large, and unusually old, planetary nebulae. The progenitor star is also one of the hottest stars known, so hot it is producing large amounts of X-rays. There are not very many photos out of this difficult target. 

This is a start of the imaging project with my new imaging system. So far I have shot 15 hours of  light from an ionized oxygen, O-III.  I'll shoot two other emission lines, H-alpha and S-II, when ever the weather allows it. The triple ionized oxygen emits blueish light, in this image the O-III emission is colorized to blue. I can produce a real three band color image after I have collected enough light for ionized hydrogen and sulfur. 


MWP1, the Methuselah Nebula
Click for a large image

MWP1 planetary nebula in light of an ionized oxygen only.




Technical details

Processing workflow

Image acquisition, MaximDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 27 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics, Celestron EDGE 14" with 0.7 Focal reducer

Mount, MesuMount Mark II

Cameras, Imaging camera Apogee Alta U9000M and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AO Active Optics @ 5hz

filters, Astrodon 3nm O-III

Total exposure time
O-III, 45x 1200 s, binned 1x1 = 15h 



A single full scale 20 min O-III exposure
 Click for a full scale image.

MWP1 is a really dim target, a single 20 O-III exposure doesn't show much of it. The photo is calibrated with a bias corrected flat frame and dark frame.