Oct 182020
 

I took a break from planetary imaging last night. This is a target of opportunity I ran across in between asteroid sets. NGC 891 is an edge-on spiral galaxy located in the constellation Andromeda. Also known as the Silver Sliver Galaxy, it was discovered by William Herschel in 1784.

Silver Sliver Galaxy (NGC 891)[CV:52x60s)

There is quite a bit of detail in the prominent dust lane that evenly splits the disk. There is also another edge-on spiral galaxy apparently deep in the background slightly above NGC 891’s disk. It is very small and about half way from the central bulge and the right edge.

 Posted by at 18:05
Sep 112020
 

While waiting for an asteroid to come into view, I had enough time to image a target of opportunity. NGC 7331 is a large spiral galaxy located in the constellation Pegasus. As is normally the case, there are several other galaxies visible as well. Just starting to become visible in this image assembled from thirty-one 60 second exposures are three other members of the “NGC 7331 group” (NGC 7337/7335/7336). Although visually close, all the galaxies lie extremely far from each other and only look close from Earth’s perspective.

This image shows a spiral galaxy centered in a sparce field of Milky Way stars. It is slightly tipped towards the observer with the near edge lower. There are sveral other but much cmaller, more distant galaxies.

NGC 7331 [CV: 31x60s]


In the constellation map, NGC 7331 lies at the ‘top’ of Pegasus bordering on the constellation Lacerta (the Lizard).
This is a copy of the primary image with the primary objects identified by their astronomical designations.

NGC 7331 – Annotated [CV: 31x60s]

This is a map of a portion of the northern celestial sphere. The constellation is highlited with the brighter stars connected by lines.

By IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg) via Wikimedia Commons

 Posted by at 14:11
Jun 162020
 

I am still developing the procedures necessary to process one shot color (OSC) camera images. This is the first D90 image I have processed using the color information. The steps to process an OSC camera are totally different than the steps I use to produce color images taken by my science camera. The larger FOV also adds additional complexity. This image is 2.83° wide versus my science camera having an FOV of only 24′ (arc minutes). However, the increased area makes it much easier to image multiple objects without having to assemble a mosaic of smaller images.

This picture is centered on an object in the southern constellation Sagittarius: The Lagoon Nebula. Also known as M 8, it is a large emission nebula being energized by the open star cluster NGC 6530 that lies in it. Also easily visible towards the lower right is M 20 (The Trifid Nebula) containing both emission and reflection nebulae. The small concentration of stars at the upper left is the globular cluster NGC 6544.

Lagoon Nebula (M8) [F:10x120s]


Chart generated by Cartes du Ciel (CdC)

Chart courtesy of IAU/Sky&Telescope

The vertical yellow line that runs all the way through the CdC chart is the ecliptic. Since most asteroids orbit in the plane of the solar system, the image contains a lot of them. I counted 31 identified on the chart by small green dots, but due to the image scale and the asteroid’s magnitudes I couldn’t find any of them.

Both M 8 and M 20 are just visible with binoculars. Using the constellation chart, observe just above the spout of Sagittarius’ Tea Pot asterism (heavy green lines).

 Posted by at 18:45
Jun 132020
 

While waiting for Jupiter and Saturn to clear my tree line, I did some more testing with my wider FOV scope that has a simple DSLR mounted on it. I am still manually focusing the system but it doesn’t take too long to accomplish. The recently installed flattener corrects the distortion apparent in the stars at the corners of each image.

The target for tonight’s testing was Messier 11 (The Wild Duck Cluster). Legend has it the cluster was given its name by British Admiral William Henry Smyth (1788-1865). When describing the cluster, the Admiral, a very accomplished astronomer and avid hunter, commented the V-shaped group of stars looked like a flock of wild ducks.

Classified as an open star cluster, the flock is located in the constellation Scutum (The Shield). The constellation is right in the middle of the plane of the Milky Way and towards the center of the galaxy. That is fairly apparent by the sheer number of stars in the image. North is to the right putting M 11 right on the northern edge of the Scutum star cloud. The dark area towards the bottom right side of the image is not a lack of stars. It is a large area of dust and gas dense enough to block the light of more distant stars. Several of these areas were individually cataloged as dark nebulae by American astronomer E. E. Barnard, hence the B numbers on the matching chart.

Wild Duck Cluster (M 11) [M:11x120s]

As can be seen on the constellation chart, Scutum is in the southern sky located between Aquila and Sagittarius. The image and matching chart are rotated 90° to the constellation chart.

Chart generated by Cartes du Ciel

Chart courtesy of the IAU and Sky&Telescope

Once Jupiter and Saturn cleared the trees I switched over to planetary equipment and was able to get a couple of series of both planets before wispy clouds moved in from the south. As usual, the best Jupiter image was uploaded to NASA’s JunoCam web page for mission planning.

Jupiter [(V)TR:2506×0.74ms;TG:2501×1.1ms;TB:2505×1.7ms]

 Posted by at 15:32
Apr 072020
 

I have been testing a new optical configuration to give the PTO the ability to record larger FOV images. Mounting my Nikon D90 to a 80mm f/6 apochromatic telescope gives a 2.9°x 1.9° FOV image. The resulting 5.26 sq° image is 97% larger than the standard science image used for asteroid/comet analysis. The size of the camera chip is large enough though that significant distortion is visible at the extreme corners of the image. As you can see the stars are ‘stretched out’ with each pointing towards the center of the image. This is known as pincushion distortion. A field flattener will need to be added to correct this problem.

The test target is a fairly large open cluster. It lies in the center of the constellation Cancer and is known as the Beehive cluster. The current population count is about 1,000 stars although only the brightest form the naked eye object. This is one of the first objects observed by Galileo when he first turned a telescope to the sky. He counted 40 stars.

Beehive Cluster (M 44)
[M:4x60s]

The compressed display makes the image background much brighter than it should be. Click on the image for a larger more accurate view. This will also make the corner distortion easier to see.

 Posted by at 14:24