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.

BUY A MUSEUM QUALITY POSTER

Wednesday, February 16, 2011

IC 1848, the "Soul Nebula", finalized





IC 1848, the "Soul Nebula"
Ra 02h 51m 36.24s Dec +60° 26′ 53.9"



Image is in HST-palette, (HST=Hubble Space Telescope)
from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.

This is a final version of IC 1848. I shot more H-alpha, 15 x 20min., since the first set was ruined by the orthogonality problem between the optical path and CCD. Now all stars are pinpoints at a whole field of view.

Soul Nebula, (Sh2-199, LBN 667) is an emission nebula in constellation Cassiopeia. IC 1848 is a cluster inside Soul Nebula. Distance is about 7.500 light years. This complex is a Eastern neighbor of IC 1805, the "Heart Nebula" and they are often mentioned together as Heart and Soul.


Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.

A closeup

Not a bad resolution for a 300mm camera lens.


Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack. 
Deconvolution with a CCDSharp, 20 iteration, added at 50% weight.
Levels, curves and color combine in PS CS3.

Equipments:
Tokina AT-a 300mm f2.8 @ f2.8
Platform and guiding, Meade LX200 GPS 12" @ f5
Camera, QHY9
Guider, Lodestar
Image Scale, 3,79 arcseconds/pixel

Exposures:
Baader H-alpha 7nm 15x1200s, binned 1x1
Other channels are from an older image



Older images from the same target


Image shows both, Soul and Heart, nebulae
Colors for a new image are taken from this older one.






Tuesday, February 15, 2011

Caldwell 49, the "Rosette Nebula", as a Stereo Pair 3D






Parallel vision 3D




Cross vision 3D


Original 2D:





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

Caldwell 49, the "Rosette Nebula" as an anaglyph Red/Cyan 3D




You'll need Red/Cyan Eyeglasses to be able to see this image right.
Note, if you have a Red and Blue filters, you can use them! Red goes to Left eye.



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

Caldwell 49, the "Rosette Nebula"



"Rosette Nebula"
Ra 06h 33m 45s Dec +04° 59′ 54″






Image is in HST-palette, (HST=Hubble Space Telescope)
from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.
Star colors are mixed from the NB channels, Red=H-a, G=O-III and B= 85%O-III + 15%H-a.

This image is from two nights, 09.02 and 13.02. It was very cold, about -25C, at both nights.
I had an orthogonality problem with QHY9 and the Tokina AT-X 300mm f2.8 lens. The problem is now fixed and the optical axle and the CCD are now perfectly perpendicular to each others.

The Rosette Nebula (also known as Caldwell 49) is a large, circular H II region located near one end of a giant molecular cloud in the Monoceros. The open cluster NGC 2244(Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula's matter. The cluster and nebula locates at a distance of about 5,200 light years from Earth. The diameter is about 130 light years. 
The radiation from the young stars ionized the atoms in the nebula, causing them to emit light, typical to each element, producing the visible nebula. Stellar winds, radiation pressure, from a group of stars cause compression to the interstellar clouds, followed by star formation in the nebula. This star formation is currently still ongoing.



Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.

The scale

In this image, there is a full Moon placed as a scale.
The diameter of the full Moon is about 30', 0.5 degrees.
Image area is about 193', 3,2 degrees, wide.



An older, wider view, mosaic image of the Rosette area.

Colors for the new image are taken from this older capture.
Technical information in original blog post:

Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack. 
Deconvolution with a CCDSharp, 20 iteration, added at 50% weight.
Levels, curves and color combine in PS CS3.

Equipments:
Tokina AT-a 300mm f2.8 @ f2.8
Platform and guiding, Meade LX200 GPS 12" @ f5
Camera, QHY9
Guider, Lodestar
Image Scale, 3,83 arcseconds/pixel

Exposures:
Baader H-alpha 7nm 15x1200s, binned 1x1 (5h)
Other channels are from an older image:




A closeup of the Rosette Nebula from Spring season 2010

Original blog post with a technical details: