COPYRIGHT, PLEASE NOTE

All the material on this website is copyrighted to J-P Metsavainio, if not otherwise stated. Any content on this website may not be reproduced without the author’s permission.

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Wednesday, May 21, 2014

An animated zoom in series to the Bubble Nebula



I have shot many targets with a several focal lengths and instruments.
Due to that, I'm able to publish some of my photos as an image set, with a different field of view and detail levels. The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

Zooming into the Bubble Nebula
An animated GIF, 3MB




A closeup picture of the Bubble formation

More info about this image HERE
Buy a photographic print from HERE


An animated 3D study of the Bubble Nebula can be seen HERE


A study about the apparent scale in the sky
Note. an apparent size of the Moon is marked as a circle.
Moon has an angular diameter of ~0,5 degrees, that's ~30 arc minutes.

Click for a large image




Thursday, May 15, 2014

The largest Fine Art print in Finland




About three weeks ago I posted about my astronomical photo as a public artwork.
This very large, 10x3m, photographic print on aluminium was produced by a Finnish company Dialab.
They made an inquiry from the Finnish Museum of Photography about this print. The museum confirmed, that this is the largest photographic fine art print in Finland. The photo is located in main lobby of The "Oulu Region Joint Authority for Education" in Haukipudas

Cirrus of Cygnus
The largest fine art photo in Finland

The photo is printed on aluminium and it has a glossy finishing. This is the largest fine art print in Finland. 
The size of the photographic prin is over 3 x 10 meters (= 10 x 33 feet) Even in that size, the image is very sharp, since the original image is in very high resolution due to mosaic technique used.

More info about the print and the image HERE






Monday, May 12, 2014

Cepheus, an animated zoom in series to the IC 1396



I have shot many targets with several focal lengths.
Due to that, I'm able to publish some of my material as an image sets, with different field of view and detail levels. The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.

An animated zoom in series to an Elephant's Trunk Nebula

An animated GIF, 2MB


A closeup picture of  the Elephant's Trunk Nebula in IC 1396

More info and technical details HERE
Buy a photographic print from HERE

A study about the apparent scale in the sky
Note. an apparent size of the Moon is marked as a circle.
Moon has an angular diameter of ~0,5 degrees, that's ~30 arc minutes.

Click for a large image


Sunday, May 11, 2014

Heart Nebula, an animated zoom in series to the Melotte 15



I have shot many targets with several focal lengths.
Due to that, I'm able to publish some of my material as an image sets, with different field of view and detail levels.
The fractal nature of our universe stands out nicely by this way and it will make the orientation more easy.


An animated zoom in series to a Melotte 15 cluster

An animated GIF, 1,9MB

A closeup picture of Melotte 15 in the heart of the Heart Nebula

More info and the technical details HERE
Buy a photographic print from HERE

A collection of  Heart Nebula images HERE


An experimental 3D-study of the Melotte 15

More animations and info can be seen HERE

A study about the apparent scale in the sky
Note. an apparent size of the Moon is marked as a circle.
Moon has an angular diameter of ~0,5 degrees, that's ~30 arc minutes.

Click for a large image



Friday, May 9, 2014

Simeis 147 supernova remnant in Taurus, with and without stars



Now and then I'm publishing some experimental material of mine. This time I made an animated image about Simeis 147 SNR in Taurus. In this animation, the supernova remnant can be seen with and without stars. Human brains has a tendency to form quasi shapes from a random cloud of dots, like stars in this case. This is a very effective method to show the actual nebula and its details.

I'm planning to use the star removal procedure to hunt down some old and very diffused planetary nebulae, located at a dense star field in the Milky Way. They might have a very large angular dimensions and the surface brightness is extremely low. Due to that, they get easily buried under a dense star field.

Simeis 147 (Sh2-240)

Stars vs Starless
Buy a photographic print from HERE

Original image of the Simeis 147

More images and the technical details can be seen here:

PS.

You might know, that I lost my imaging setup at last January. Due to some serious electrical problems all the components are fried beyond any repair. Least it'll cost more than a new scope.

I haven't been able to find a corporate sponsors yet, for the new telescope and the mount. I do have couple of sponsors for the cameras though. I'll inform more about them later. Please contact, if you are interested to become a sponsor! astroanarchy (at) gmail.com
The sponsor will have lots of positive visibility for a many years.  

Some info about my work as an astronomical photographer

J-P Metsavainio 

- Born 1964
- studies Art, Architecture, experienced in telecommunication manufacturing and development.
- Specialized in the astrophotography since 1998, I love to reveal some of the hidden beauty of the universe around us.

Some publications:

- Eight NASA APOD's at the moment (Astronomy Picture Of the Day)
- Many images in National Geographic image portfolio and several astronomical images of the week.
- Many images in the Science Photo Library archive in London
- The astronomer Phil Plait collected an annual list of the best astronomical images for the year 2012.
(My experimental image of IC 1396 was selected to this list. Nuber sixth from the top.) http://www.slate.com/articles/health_and_science/bad_astronomy/2012/12/best_astronomy_images_2012_see_the_most_beautiful_images_of_the_universe.html
- My photo of the constellation Cygnus was selected as one of the best amateur astronomy photographs of the past four years by the Daily Telegraph 2014.
http://www.telegraph.co.uk/science/picture-galleries/9622374/The-best-amateur-astronomy-photographs-of-the-past-four-years.html?frame=2374492
- Lots of publishing by many printed and online magazines, some logos are shown at top right corner here in my blog. 

I'm also a regular speaker in astromical happenings like NEAIC New York (North East Astro Imaging Conference) and the European version of it CEDIC (Central european Deepsky Imaging Conference)

My photos

Image portfolio:
http://astroanarchy.zenfolio.com/


Blog, works mostly as an imaging diary and a publishing channel for some of my experimental work:
http://www.astroanarchy.blogspot.fi/


Facebook, I'm publishing only an astrophotography related materila here:
https://www.facebook.com/jp.metsavainio


Best regards and clear skies,
J-P Metsavainio, Astro Anarchy Observatory, Finland


Tuesday, April 29, 2014

My astroimages converted to 3D, a collection of movie clips



I have converted my astronomical images to a various 3D-formats. This time I made a video collection out of my experimental nebula 3D-models.

My astronomical images as an experimental 3D-conversions
This is a looped 14 min video, click to start and stop. Original movie is in HD720p resolution.


Click the Youtube logo at lower right corner to see this video in Youtube.
Then, please, click the gear symbol, to see the video at 720p HD-format.


3D-stereo images from my astrophotos can be seen HERE

All my astronomical images can be seen HERE

How the 3D-models are done?

Due to enormous distances of cosmic objects, no real parallax can be imaged to get a 3D-information. I have developed a method to turn my images to a 3D-models.
Here is a short and simplified explanation, how 3D images are done:

My 3D-experiments are a mixture of scientific data, deduction and an artistic impression. 

I collect distance and other useful scientific information before I do my 3d-conversion.
Usually there are known stars, coursing the ionization, so I can place them at right relative distance. If I know a distance to the nebula, I can finetune distances of the stars so, that right amount of stars are front and behind of the object. I use a "rule of thumb" method for stars, brighter is 
closer, but if a real distance is know, I try to use it. 

Many shapes can be figured out just by looking carefully the structures in nebula. Like dark nebulae must be at front of the emission ones to show. The general structure of many star forming regions are very same. There is a group of newly born stars, as an open cluster inside of the nebula. The stellar wind from the stars is then blowing the gas away around the cluster and forming a kind of gavitation, a hole, around it. The pillar like formations in the nebula must point to a source of stellar wind, for the same reason.

Since nebulae are practically transparent and the gas itself is emitting light, the thickness of the gas can be estimated by its brightness. Emission of ionized Oxygen, O-III, needs lots of energy. For that reason, Oxygen emission seen in the photo must be at close proximity of the ionizing star(s).  

The processing workflow itself is kind of sculpting and the result is always an approximate reality.

I turned the original 2D-image to 3D by using a surface modeling software.
Image is first divided to layers by its content in a image processing software. Each layer is then projected to a 3D-surface. To build the 3D-surfaces and to have a good and realistic forms, I'm using a software, that converts the shades in the image to a 3D-form. I have semi automated the whole process, so it doesn't take too much time to make a 3D-conversion.

The nice thing about the final 3D-model is, that only image elements from the original 2D-image are used!

A typical surface model without textures




Saturday, April 26, 2014

Astro Anarchy get published


Yesterday was an opening ceremony for the new facilities of The "Oulu Region Joint Authority for Education" in Haukipudas. One of my images was selected there as a public artwork in a main lobby.

The Cirrus of Cygnus
A very large photographic print on aluminium, 3x10m

The photo is printed on aluminium and it has a glossy finishing. This is one of the largest art prints I have ever seen. The size of the photographic prin is over 3 x 10 meters (= 10 x 33 feet) 
Even in that size, the image is very sharp, since the original image is in very high resolution due to mosaic technique used. An info board for the artwork can be seen next to the door at middle right.

An opening ceremony

Yours truly at left in a red shirt. Photo copyright OSAO

About the photo
Click for a very large image, 3000 pixels wide and 4,5MB

A mapped color image from the emission of ionized elements,
R=Sulfur, G=Hydrogen and B=Oxygen.

The image above spans about 15 degrees of sky horizontally, that's 30 fool Moons side by side in a sky!
There are nine panels seamlessly stitched together. Each panel has been shot three times for a color image by using emission line filters for Hydrogen, Oxygen and Sulfur. A camera lens, Canon EF 200mm f1.8, was used with a cooled astronomical camera, QHY9. Original image is about 20000 pixels wide . Total exposure time is around 90h.

The "Cirrus of Cygnus" is a part of a much large image of this area. 
Note! a very large image, 2300 pixels wide and 4,7MB
The Cirrus formation can be seen at upper part of the image above.


More info in this blog post: http://astroanarchy.blogspot.fi/2011/12/cygnus-mosaic-18-panels-and-22-x-14.html

Couple of closeups from a mosaic image above

The propeller nebula, this area can be seen at middle of bottom edge in the topmost image.
Original blog post about the Propeller Nebula: http://astroanarchy.blogspot.fi/2011/10/first-light-for-autumn-season-2011.html

Sharpless object 112 can be seen as a dim batch at left, near a bottom edge, next to a brighter blue area, in a topmost image.

Orientation in constellation Cygnus



It does look like a Cirrus cloud





Thursday, April 10, 2014

Tone Mapping V2.0, my lecture at NEAIC conference, New York




Click the image to download a PDF-tutorial

Click the image to download a PDF-tutorial

I'm offering my development work for free.
Donations are welcome especially since I don't have any equipments to continue my imaging work.









Saturday, April 5, 2014

Two collections of planetary nebulae in scale


Since I don't have any equipment to continue my imaging work, I have organized my image archives. This time I made an image collection out of the planetary nebulae imaged by me. I'm trying to show here, how large they appear to be in the sky. There is an image of the Moon as a scale in the posters. The Moon has an angular diameter of about 30 arc minutes, that's equal to 0,5 degrees. I have made a similar poster out of the supernova remnants, it can be seen HERE.


A collection of planetary nebulae as a poster
Click for a full resolution image




A collection of very large planetary nebulae as a poster
Click for a full resolution image. Please, read the NOTE under the image!


NOTE!

A friend of mine, Sakib Rasool, contacted me for this posters. There is an error in second one.
Sh2-223 is actually an emission nebula. You can read a paper about it here: http://www.aanda.org/articles/aa/abs/2006/29/aa4881-06/aa4881-06.html



INFO

For more information about palnetary nebulae: http://simple.wikipedia.org/wiki/Planetary_nebula
All images are emission line images shot with a Baader narrowband filter set, cooled astronomical camera QHY and Meade LX200 GPS.

Links to my original photos with technical details

Poster 1


Poster 2




Tuesday, April 1, 2014

Best amateur astronomy photos of the past four years, by the Telegraph




My photo of the constellation Cygnus was selected as one of the best amateur astronomy photographs of the past four years by the Telegraph. The collection of images can be seen HERE, my image is a number 09.

A mosaic image of constellation Cygnus 
Reprocessed, NOTE. a large image 2300 pixels wide and 4.3MB

Image is in mapped colors from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen. Native size of  this image is over 15.000 x 10.000 pixels.

More information and images HERE




Monday, March 24, 2014

A collection of large supernova remnants as a poster



Since I don't have any equipment to continue my imaging work, I have organized my image archives. This time I made an image collection out of the supernova remnants with a large angular scale. I'm trying to show here, how large they really are in the sky. There is an image of the Moon as a scale in the poster. The Moon has an angular diameter of about 30 arc minutes, that's equal to 0,5 degrees.


A collection of large supernova remnants as a poster
Images are in mapped colors from the emission of ionized elements. NOTE a large image, 1900x2500 pixels and 6MB

All images are in Mapped colors from the emission of ionized elements,
R=Sulfur, G=Hydrogen and B=Oxygen.
Note. The Moon as a scale to show the apparent scale in the sky.


The same collection in visual spectrum
Click for a full resolution poster. NOTE a large image, 1900x2500 pixels and 6MB

Images are in Natural color palette from the emission of ionized elements,
R=Hydrogen + Sulfur, G=Oxygen and B=Oxygen + Hydrogen. This is very close to a visual colors.
Note. The Moon as a scale to show the apparent scale in the sky.

More information about SNR images above
Links to my original photos with technical details

All the images are shot with the camera optics, Canon EF 200mm f1.8 monster lens full open, Baader narrowband filters (H-a, O-III and S-II) and the QHY9, a cooled astronomical camera with the KAF 8300 CCD chip. Very long exposure times are used, 15 to 50 hours per image, to reveal dim and diffused structures buried in the dense star fields. All images are guided with the Meade LX200 GPS 12" and the Lodestar guider. Meade works also an imaging platform for the camera lens.

In this collection, there are couple of very rare images, like Simeis 147, Sharpless 224. There are also two "firs light" images out of two super nova remnants, Sharpless 221(Sh2-221) and G65.3+5.7SNR. I haven't been able to find any other color images out of them, showing the whole SNR.





Monday, February 24, 2014

Exploded stars as an experimental 3d-stereopair

Images are for two different viewing methods, the first  is for the Parallel Vision method and the second one for the Cross Vision method. Viewing instructions can be seen HERE.

Anaglyph versions, for the Red/Cyan glasses, can be found from my portfolio HERE.

NOTE! This is a personal vision about volumes and shapes, based on some known facts and an artistic impression.

Image of Sh-221 and Sh2-216 as an experimental 3D study
Two ways to end a life of the star in a same seven degrees field of view!

For Parallel Vision method



For Cross Vision Method


Original blog post about this photo can be seen HERE

INFO

Just next to Sh2-221 locates a closest known planetary nebula, Sh2-216. This is also a very rarely images target, due to its low surface brightness and large angular dimension. This mosaic image covers over seven degrees of sky vertically. (The Moon has an apparent dimension of 0.5 degrees.)  Mosaic is made out of my new data of Sh2-221 and an older material of Sh2-216. Some new exposures was taken for the Sh2-216 to match the background for a mosaic image. 

Image shows two different ways to end a life of the star. At left, as a Supernova and at right as a Planetary Nebula. (Massive stars will go to a Supernova, after burning out all of the Hydrogen. There will be a Neutron star or a Black Hole left behind. Lighter stars, as our Sun, will turn to a Planetary Nebula, after ran out of Hydrogen. There is a core of the star left behind, it's called a White Dwarf  and it will cool down gradually. ) 






Thursday, February 13, 2014

Astroa Anarchy is looking for sponsors



Business corporate sponsors needed

I recently lost my imaging system due to massive short circuit. After calculating the repair cost of the current setup, it turned to be more expensive, than a new one would be.  

I'm looking for Business Corporate sponsors to support my work as an astronomical photographer. I can offer lots of visibility in my pages. A free usage right to my photos is negotiable.

I have a plan for a new set up, the estimated cost will be around 25.000 Euros. (That's about 34.000$)
The new system will have a new telescope mount and the optics will be 14" SCT converted to a f2 astrograph, with the HyperStar system.  (The price is low for a high end system, since I have lots of usable material from my old setup and I will do the actual labor by myself.) 

How much visibility can be generated?

It's difficult to give any exact numbers, since I have Several channels to publish my images. My blog have had about 20.000 monthly visitors starting from the year 2007. My image portfolio have had about 15.000 monthly visitors, starting from the year 2010. Beside that, I have Facebook page for my photographs, it has about 1200 friends and about as many followers. Images get shared a lot by a popular Facebook pages.

Quite regularly my images get published by a very popular websites, like NASA Astronomy Picture of the Day or National Geographic, there is a collection of publishers logos at  upper right corner of this page.
Any time the photo get published by a popular page, it will get easily millions of views.


Contact for more information

jp.metsavainio (a.t.) gmail.com


My photo portfolio







Monday, February 10, 2014

All my images from the Spring season 2014



This is a small collection of my images, shot at Spring 2014. There are not many images and new ones aren't coming anytime soon, since my main telescope system has toasted beyond any repairI'm having a hard time trying to figure out, how to restore my observatory to an imaging condition with a very limited assets. 

I managed to get some really rare images though. I think, that both supernova remnant images, Sharpless 221 and G65.3+5.7 SNR, are the first three band color images, showing the whole remnant, in the world! If someone is able to find other images, I'm very interested to hear about it. Both SNR images are kind of long projects. Exposure time for the G65.3+5.7 SNR 38 hours and for the Sharpless 221 was 33 hours, with the planetary nebula Sharpless 216, 58 hours. (Image at the bottom of the poster.)

Main work for the season was the large, ten panels mosaic of the constellation Cepheus. Every pane is shot three times to have a narrow band color composition. Total exposure time was 92 hours, it includes shots from six different years. 

All images from the Spring season -14 are shot with the Canon EF200mm f1.8 camera lens (full open), QHY9 a cooled astronomical camera and the Baader narrowband filters, H-a, S-II and O-III.

All my images from the Spring season 2014 as a poster
Click to see at full scale, 1600x2600 and 5MB

Images are in Natural color palette from the emission of ionized elements, 
R=Hydrogen + Sulfur, G=Oxygen and B=Oxygen + Hydrogen.


Ps.

All my astronomical photos can be seen HERE.




Monday, February 3, 2014

A zoom in series of the Sharpless 132



Now and then I have published some zoom in series of various objects imaged by me.
The purpose is to show the apparent scale in the sky. Beside that, this series shows nicely the fractal nature of our universe.  Series are possible to make, since I have shot many objects with various focal lengths.
Like this one is shot with 200mm, 300mm and ~2000mm  focal lengths. Images are from my large mosaic image of the constellation Cepheus.

The Sharpless 132 (Sh2-132), a study about the scale in the sky
Note. A circle, size of the Moon, in the images as a scale. (An apparent scale of the Moon is 0,5 degrees, or 30  arc minutes.)

All images are in Mapped colors from the emission of ionized elements,
R=Sulfur, G=Hydrogen and B=Oxygen.


Orientation in constellation Cepheus

An orientation in constellation Cepheus. The mosaic image covers an area of ~18x10 dgrees.






Sunday, February 2, 2014

A poster format collection from the Cepheus project



In this collection of my images, the objects shown in a large mosaic of the constellation Cepheus, are collected together. There are indicator lines to show the actual location of object in a large context. As can be seen, I have shot many objects in various focal lengths.

 The Cepheus project was my last published image before the major break down of my imaging equipment.

The Cepheus collection
Be sure to click the image to see it in full scale! (2400 x 2000 pixels and 4,5 MB)

All images are in mapped colors from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
An Original blog post of The Cepheus project can be seen HERE.


Small images clockwise, starting from the top left 
  1. Cave Nebula, a closeup: http://astroanarchy.blogspot.fi/2012/12/the-cave-nebula_9.html
  2. Cave Nebula, a wide field shot: http://astroanarchy.blogspot.fi/2011/01/sh2-155-cave-nebula-reprocessed.html
  3. Sharpless 140: http://astroanarchy.blogspot.fi/2012/02/dim-and-large-nebula-in-cepheus.html
  4. Sharpless 129: http://astroanarchy.blogspot.fi/2013/12/a-start-of-new-project-cepheus-mosaic.html
  5. Elephant's Trunk Nebula: http://astroanarchy.blogspot.fi/2012/12/elephants-trunk-nebula-reprocessed.html
  6. IC 1396: http://astroanarchy.blogspot.fi/2011/10/ic-1396-home-of-elephants-trunk-nebula.html
  7. Sharpless 132, a wide field shot: http://astroanarchy.blogspot.fi/2011/02/sh2-132-project-finalized.html
  8. Sharpless 132, a closeup: http://astroanarchy.blogspot.fi/2013/10/the-second-image-of-autumn-season-2013.html
  9. The Wizard Nebula: http://astroanarchy.blogspot.fi/2011/07/sh2-142-wizard-nebula-reprocessed.html
  10. Sharpless 157http://astroanarchy.blogspot.fi/2011/03/sh2-157-reprocessed.html
  11. Bubble Nebula: http://astroanarchy.blogspot.fi/2011/03/bubble-nebula-reprocessed.html