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Monday, March 25, 2013

The Great Globular Cluster in Hercules on a Moonlit Morning

After experimenting with iTelescope.net's remote robotic telescopes for astronomy education, imaging galaxies, and galaxy clusters, I figured it was now a good time to target another type of deep-sky object. First thing this morning around 3:00am, MDT, Telescope T-21 (Planewave 17" f/4.5 CDK) was available for imaging at New Mexico Skies. The moon's phase was near full in the western part of the sky and Messier 13 (M13), the Great Globular Cluster in Hercules was becoming high in the eastern part of the sky. This was my first attempt at imaging a deep-sky object when the moon was so bright using these telescopes. 

Image of M13 - Globular Cluster in Hercules - 300 Second Exposure
M13 - Globular Cluster in Hercules - 300-Second Exposure

After making a 5-minute exposure with only a luminance filter, the result is what you see to the left. I used the FITS Liberator and Adobe Photoshop CS6 for post-processing. I converted the FITS-processed grayscale image to RGB in Photoshop and added a blueish hue to the image for effect.

I find it absolutely amazing that when there is nearly a full moon in the night sky, observers are still able to take images of deep-sky objects with no interference from the moonlight. As I referred to the "All-Sky Camera" at New Mexico Skies to check the sky conditions before imaging, I could barely make out only a few of the brightest stars accompanied by an overexposed view of the moon. Also, because of today's technology with advanced CCD Cameras and precision mounts that track the sky so accurately, it only takes about 5 minutes to get an image like the one above.

Messier 13 (M13), also designated NGC 6205 and sometimes called the Great Globular Cluster in Hercules or the Hercules Globular Cluster, is a globular cluster of about 300,000 stars in the constellation of Hercules.M13 is about 145 light-years in diameter, and it is composed of several hundred thousand stars, the brightest of which is the variable star V11 with an apparent magnitude of 11.95. M13 is 25,100 light-years away from Earth. 13 was discovered by Edmond Halley in 1714, and cataloged by Charles Messier on June 1, 1764. The Arecibo message of 1974, containing encoded information about the human race, DNA, atomic numbers, and Earth's position, was beamed there for being picked up by a potential extraterrestrial civilization. It will reach the cluster in 25,000 years.
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Tuesday, March 19, 2013

Galaxies Galore

Since my independent discovery of SN1989B in the spiral galaxy, M66 in the constellation Leo back on February 11, 1989, I have always been fascinated with observing galaxies and galaxy clusters. Over this past weekend, Muir and I wanted to try to capture a few galaxy clusters in the spring sky using the remote robotic T-5 (Takahashi Epsilon 250mm) telescope in New Mexico Skies. Over the weekend we referenced the Stellarium astronomy program to find a field of view that may catch multiple galaxies in a single image. One group of galaxies that caught our attention in Stellarium was in the constellation of Coma Berenices. We chose one galaxy in the group that would make a good "center point" for the image. 

Image of Galaxies in the Coma Cluster - Click on Image to Enlarge
Galaxies in the Coma Cluster - Click to Enlarge


That object was NGC 4872. We scheduled a 300-second exposure at 2:45 am MDT when the galaxy was near transit. After examining the data we received post-processing, we noticed a few different galaxies in the frame. Using the Aladin Sky Atlas astronomy software, I loaded up the DSS color image of NGC 4872. As I zoomed into the Aladin image with NGC 4872 at the center, I observed numerous galaxies. Referring back to our image taken with the T-5, what I thought were faint stars were actually galaxies. After the excitement set in, I decided to use telescope T-11 (Planewave 20" CDK Astrograph) the next day to get a magnified image of the galaxy cluster. After waking up this morning around 5:00 am EDT (3:00 am MDT), I jumped on T-11 and acquired the image above. After processing the image, I magnified and saw the same detail in all of the galaxies I observed in the Aladin Sky Atlas software.

NGC 4872 and Surrounding Galaxies in the Coma Cluster Identified with Aladin Astronomy Software
NGC 4872 and Surrounding Galaxies in the Coma Cluster Identified with Aladin Astronomy Software

There were so many galaxies in the field of view that I could not keep count. I then thought it would be a fun exercise to identify a few of the brighter and more interesting-looking galaxies using the SIMBAD Astronomical Database overlay in the Aladin Sky Atlas. I was able to successfully identify the galaxies in the image above using the technique pictured left.

A wide-field image of the Coma Cluster of galaxies taken at the   Mount Lemmon SkyCenter using the 0.8m Schulman Telescope.   Image courtesy Adam Block
A wide-field image of the Coma Cluster of galaxies taken at the 
Mount Lemmon SkyCenter using the 0.8m Schulman Telescope. 
Image courtesy Adam Block

The Coma Cluster (Abell 1656) is a large cluster of galaxies that contains over 1,000 identified galaxies. Along with the Leo Cluster (Abell 1367), it is one of the two major clusters comprising the Coma Supercluster. It is located in and takes its name from the constellation Coma Berenices. The cluster's mean distance from Earth is 321 million light-years. Its ten brightest spiral galaxies have apparent magnitudes of 12–14 that are observable with amateur telescopes larger than 20 cm. The central region is dominated by two giant elliptical galaxies: NGC 4874 and NGC 4889. The cluster is within a few degrees of the north galactic pole in the sky. Most of the galaxies that inhabit the central portion of the Coma Cluster are ellipticals. Both dwarf and giant ellipticals are found in abundance in the Coma Cluster. The image (right) shows some of the same galaxies that are in the field of view of the image (top of post) I obtained using the Planewave 20" telescope this morning.
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Sunday, March 17, 2013

Toyotas, iPads and Galaxies... Oh My!

Waiting for my vehicle to be serviced has never been so exciting! Yesterday as I waited for my Toyota Rav4 SUV to be serviced in the dealership's waiting room, I experimented with iTelescope.net on my iPad. iTelescope.net does not recommend using Safari as a web browser (only Firefox and Chrome), however, because the Toyota dealership had such good wi-fi reception, I thought I would experiment and make an attempt to image a galaxy from iTelescope.net's remote robotic telescope location at Siding Spring Observatory, Australia. 

M83 - Barred Spiral Galaxy in Hydra  - 300 sec. exposure
M83 - Barred Spiral Galaxy in Hydra  - 300 sec. exposure

The iTelescope.net remote robotic telescope "Launchpad" page in Safari worked flawlessly until I got to the "One-Click Image" page that lists a catalog of recommended objects with the exposure times already programmed. I was not able to execute the "Submit Image" button. The workaround for this was to go into the "Single Image" page and manually set the object desired as well as the exposure settings. After inputting the settings, the "Acquire Image" button worked just fine. The object I imaged was the barred spiral galaxy, M83 in the constellation of Hydra. Messier 83 (also known as the Southern Pinwheel Galaxy, M83, or NGC 5236) is a barred spiral galaxy approximately 15 million light-years away. It is one of the closest and brightest barred spiral galaxies in the sky, making it visible with binoculars and small telescopes. Six extragalactic supernovae have been observed in M83 making the object a good candidate for the part of a continued supernova search program.

The instrument I used via my iPad to capture the above image of M83 was the Medium Deep Field (T9) which is a 12.5" Ritchey-Chrétien Cassegrain with a long focal length of f/9. This telescope is typically used for imaging & some photometry. It has a selection of color imaging filters and a photometric V filter. It is teamed with an STL-11000M CCD Camera. T9 is a prime imaging platform in the southern hemisphere and is capable of brilliant narrowband imaging with several Astro Photo of the Day (APOD) prizes under its belt already. It is a highly reliable telescope that has enabled countless iTelescope.net users to capture southern glories as well as valuable science data. It has often been used in Hubble Space Telescope support missions.

After having success imaging a galaxy visible from the other side of the globe, using my iPad, I feel that making appointments that require extensive wait times just got a lot more painless!
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