Monday, June 14, 2010
Dumbbell Nebula (M27)
This image consists of 10-4 minute exposures taken on June 12, 2010 at the Plateau Observatory in Abbotsford.
The Dumbbell was the first planetary nebula discovered and gets its name from its dumbbell like shape when viewed though an eyepiece. It is about 6 arc minutes in diameter, much larger than its neighbour the Ring Nebula. It is located in the constellation Vulpecula and its age is estimated at 3,000 to 4,000 years.
Saturday, May 15, 2010
Plateau Observatory Imaging Set Up
Top: Looking East
Bottom: Looking South
This is the imaging set up on the back deck in Abbotsford. I have a clear view of the sky from ENE through to the SSW and a restricted view elsewhere over the roof. Fortunately Polaris is visible to the North, which facilitates telescope alignment. The downtown area of Abbotsford is situated to the South. The Clear Sky Chart lists the light pollution level as "red". I use a Baader UHC-S filter which does an excellent job of removing any colour effects of the city lights.
The photo shows:
Stellarvue 115T20 Apo Triplet Refractor
HEQ-5 Mount
Orion Star Shoot Pro One-Shot Colour Camera
7.8X7.8 micrometer pixels
~2.01 arc sec/pixel resolution
102x68 arc min field of view
KW Telescope Guide Scope (QHY-5 Camera) (mounted on the telescope rings)
9X50 scope, ~210mm focal length
QHY-5 camera, 5.2X5.2 micrometer pixels
1280X1024 pixels
~5.1 arc sec/pixel resolution
109X87 arc min field of view
Ring Nebula (M57)
This image was captured on May 14, second clear sky night in a row. The image is composed of 15 4-minute exposures with my normal set up (see preceding post). The Ring Nebula is very tiny - 1.4X1 arc minute but still visible through the eye piece as a faint grey ring. It is located in the constellation Lyra, south of Vega. The Ring is a Planetary Nebula. In this case a torus of bright light-emitting gas surrounding its central star (at 15th magnitude to faint to be seen by my 115 mm telescope). The inner ring of green is light emitted from exited oxygen and the red outer ring from excited hydrogen. Its distance and age is estimated at 2,300 ly and 6,000 to 8,000 years respectively. The Ring is the remainder of a Sun-like star which has blown away its outer envelope of gas after its hydrogen fuel has been exhausted in its inner core.
Friday, May 14, 2010
M13 The "Great Hercules Cluster"
This image was captured on May 13th from my deck in Abbotsford. It was the first clear night for several weeks. The image is segment of a larger image and is composed of 15, 4 minute exposures. M13 is 25 thousand ly distant, has a diameter of 145 ly (about 20 arc minutes in the image) and contains several 100,000 stars.
Monday, April 26, 2010
Whirlpool Galaxy (M51)
This photo comprises images taken on April 15th (previous post) and April 22nd, a total exposure time of 153 minutes. The set up on the 22nd was the same as that on the 15th. The increased exposure time yields improved detail.
Saturday, April 17, 2010
Whirlpool Galaxy (M51)
This photo was taken on April 15th, the first clear night since returning from Arizona. It is the first photo from the Plateau Observatory. The photo consists of 30 3-minute exposures with the UHC-S filter and is somewhat grainy. More exposure time is needed.
The photo shows two interacting galaxies NGC 5194 (the Whirlpool) and NGC 5195 (the smaller eliptical) located in Canes Venatici just to the west of Alkaid (the final star in the handle of the Big Dipper). The spiral structure of the Whirlpool is thought to be due to the interaction with 5195. The galaxies may be in the process of merging - perhaps over the next billion years. They are about 23 million light-years away from Earth. The angular diameter is is about 11 arc-minutes. The bright circular disc at the center of 5194 has a radius of about 38,000 light-years.
The Whirlpool was discovered by Charles Messier in 1774 (using a 3 inch diameter refractor telescope), but it was not until 1845 that it was recognized as a spiral (by Lord Rosse using a 72 inch Newtonian telescope).
No change in equipment from the previous images.
Friday, March 26, 2010
Pin Wheel Galaxy (M101)
(click the image for full screen view)
This photo was taken on Mar. 25th from a vacant lot in Tucson AZ. It is composed of 33-3 min. exposures. A Baader UHC-S filter was used. It was a cloudless night but the seeing and transparency conditions were poor. The moon was waxing gibbous 82% full! This is the beauty of CCD photography - an image is possible when you can't see anything through the eye piece.The Pin Wheel Galaxy is a spiral galaxy in Ursa Major and is about 27 million ly from Earth. It has a linear diameter of about 170,000 ly. The image field is about 40 arc min. wide.
Imaging Setup:
Stellarvue 115T20 Apo Triplet
Stellarvue Field Flattener
HEQ-5 Mount
Orion Star Shoot Pro One-Shot Colour Camera
KW Telescope Guide Scope (QHY-5 Camera)
PHD Guiding
Nebulosity 2 – Image Capture
Deep Sky Stacker 3.3.2
Adobe Photoshop CS2 – Image Processing
Sunday, March 21, 2010
The Crab Nebula (M1)
(click image for full screen)
This image consists of 6 6 min. exposures taken on Jan. 7 from a vacant lot in Tucson. M1 is a supernova remnant located near the southern "horn" of Taurus, about 6,300 ly from Earth. It is 6x4 arc minutes in size. This is one of my first images and I was still experimenting with exposure time. I plan to re-shoot with greater exposure time, which should reveal greater detail.
According to the SEDs Data Base (http://seds.lpl.arizona.edu/messier/data2.html) Chinese astonomers observed and recorded the supernova in 1054 AD as a "guest star. The records show that the supernova was so bright that it was visible in the daylight for 23 days. The nebulous remnant was found by Charles Messier in 1758 and became the first item in his catalogue.
According to the SEDs Data Base (http://seds.lpl.arizona.edu/messier/data2.html) Chinese astonomers observed and recorded the supernova in 1054 AD as a "guest star. The records show that the supernova was so bright that it was visible in the daylight for 23 days. The nebulous remnant was found by Charles Messier in 1758 and became the first item in his catalogue.
Imaging Setup:
Stellarvue 115T20 Apo Triplet
Stellarvue Field Flattener
HEQ-5 Mount
Orion Star Shoot Pro One-Shot Colour Camera
KW Telescope Guide Scope (QHY-5 Camera)
PHD Guiding
Nebulosity 2 – Image Capture
Deep Sky Stacker 3.3.2
Adobe Photoshop CS2 – Image Processing
Saturday, March 20, 2010
Leo Triplet (M65, M66, NGC3628)
(click image for full screen)
This photo consists of 45 3 min. (135 min. total) exposures taken on Mar. 15 and 18 from a vacant lot in Tucson, AZ. It is a work in progress. I am hoping that more exposure time will reveal more detail in the galaxies. NGC3628 (upper left) is edge-on and is bisected by a dust lane. M65 is a tight spiral galaxy (upper right). M66 is a spiral galaxy (lower right). The galaxies are about 35 million ly from Earth. The image size is about 65x65 arc minutes.
Imaging Setup:
Stellarvue 115T20 Apo Triplet
Stellarvue Field Flattener
HEQ-5 Mount
Baader UHC-S Filter
Orion Star Shoot Pro V2.0 One-Shot Colour Camera
KW Telescope Guide Scope (QHY-5 Camera)
PHD Guiding
Nebulosity 2 – Image Capture
Deep Sky Stacker 3.3.2
Adobe Photoshop CS2 – Image Processing
Flame Nebula (NGC 2024) & Horsehead (IC 434)
(click image for full screen)
This photo consists of 12 8 min. exposures taken on Feb. 17 from a vacant lot in Tucson, AZ. I am surprised that a total exposure of 96 min. was sufficient to capture this detail. The Flame nebula is located to the left of the star Alnitak, one of the Orion's belt stars. The Horsehead can be seen in the lower right. The image size is about 65x65 arc minutes.Imaging Setup:
Stellarvue 115T20 Apo Triplet
Stellarvue Field Flattener
HEQ-5 Mount
Baader UHC-S Filter
Orion Star Shoot Pro One-Shot Colour Camera
KW Telescope Guide Scope (QHY-5 Camera)
PHD Guiding
Nebulosity 2 – Image Capture
Deep Sky Stacker 3.3.2
Adobe Photoshop CS2 – Image Processing
Rosette Nebula (NGC 2237)
(click image for full screen)
This photo consists of 35 exposures taken on Feb. 13, 15 and 16 from a vacant lot in Tucson, AZ. The total exposure time is 260 minutes. The Rosette nebula is located in Monoceros just west of Orion. The open cluster NGC2244 is embedded in the centre of the nebula. The image is about 100x68 arc minutes.Imaging Setup:
Stellarvue 115T20 Apo Triplet
Stellarvue Field Flattener
HEQ-5 Mount
Baader UHC-S Filter
Orion Star Shoot Pro One-Shot Colour Camera
KW Telescope Guide Scope (QHY-5 Camera)
PHD Guiding
Nebulosity 2 – Image Capture
Deep Sky Stacker 3.3.2
Adobe Photoshop CS2 – Image Processing
Orion Nebula (M42 & M43)

(click image for full screen)
This photo consists of 47 exposures taken on Jan. 3, 5 and 13, and Feb. 18 from a vacant lot in Tucson, AZ. The total exposure time is 194 minutes. M42 and its smaller companion M43 (right centre) are about 1400 ly from Earth. The open cluster NGC1977 is on the right. The dark lanes in the nebulosity are called "the Running Man" (here shown up-side down). The image size is about 100x67 arc minutes.Imaging Setup:
Stellarvue 115T20 Apo Triplet
Stellarvue Field Flattener
HEQ-5 Mount
Orion Star Shoot Pro One-Shot Colour Camera
KW Telescope Guide Scope (QHY-5 Camera)
PHD Guiding
Nebulosity 2 – Image Capture
Deep Sky Stacker 3.3.2
Adobe Photoshop CS2 – Image Processing
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