Friday, August 27, 2010

The Other Side of the Veil Nebula

Click on the image for a large view
As you read in my last post, the "Witches Broom" is one part of a very large supernova remnant.  To the east of the Witches Broom, 3 degrees away, is the other half of this beautiful complex of gas expelled from an exploded star.  The remaining pieces of the star formed a shell of material similar to a bubble.  Just like a bubble, we can see right through the middle.  The shock wave that created the shell is expanding the filamentary matter out, away from where the star was located.  Only along the edges of the shell, where we see it edge on, can we see the fine branches of seemingly intertwining nebulosity.  The colors come from the presence of oxygen, sulfer and hydrogen made to glow from the energy of starlight.

There is another part of this wonderful nebula in between these two images called Pickering's (Fleming's) Wisp.  It is much fainter, but I am hoping to photograph it during the next new moon phase in a week or so.

The beautiful, delicate lacework is a wonderful sight in large telescopes.  Since the nebula is so large, one has to move the telescope along the wispy tendrils of gas to catch it all in the eyepiece.

Sunday, August 15, 2010

The Witches Broom

Click on image for a larger view
Just got back from one hell of a hot camping trip.  I spent eight days in 100 degree weather with a few amateur astronomer friends at the Astronomical Society of Kansas City's Dark Sky Site (near Butler, MO).  Thankfully, night time temperatures were in the 70's and night time is why I was there.  Six out of those eight nights were clear and therefore I got a chance to image several deep sky objects with my telescope.  The image above is one of those objects.

The Veil Nebula image is only part of a much larger complex of nebulosity also known as the Cygnus Loop.  This part is on the west side of the "loop", so it is also called the "Western Veil".  A much more descriptive name is the "Witches Broom".   It's true identity, however, is the leftover remnants of a supernova explosion. some 5000 to 8000 years ago.  The remnants have since expanded to a circular area some 3 degrees in diameter.  An area this big would fit 6 full moons across.  Even though it covers an area so big in the sky, it is rather faint and requires optical aid to see it.  The bigger the telescope, the brighter it gets.  Even getting images of this object is not easy.  I haven't been happy with previous images, but this time using my 7.5" Mak-Newt telescope, I took 10 images, each image 15 minutes long, for a total of 2.5 hours combined, calibrated those images with "Bias, Flat and Dark" images, then spent a few hours bringing out the details with Photoshop.  Not a simple "click", but hours of work for one image.

Technical Details:
* Telescope: 190mm (7.5") Orion Maksutov-Newtonian
* Focal Length: 1007mm
* Focal Ratio: f/5.3
* Mount: Celestron CGE
* Exposures:
> 10 Lights, 15 minutes long
> 20 Biases
> 20 Flats
> 1 Dark
* Calibration: Removed bad pixels on Lights using the single Dark with "Nebulosity" software
* Processing: Aligned and Stacked using "DeepskyStacker" software
* Finished: Photoshop CS3

Saturday, July 31, 2010

Baby Stars

Click on Image for a larger view
On the right side of the above picture is the famous "Double Cluster", one of the all-time favorites for amateur astronomers.  If you know where to look in the constellation Perseus, its a hazy patch of light to your unaided eyes, and in a pair of binoculars each cluster is resolved into a tight knot of stars against a starry backdrop.  For small telescopes, it is one of the finest clusters in the heavens, with many stars of contrasting colors.  Its existence was noted by Hipparchus and Ptolemy around 150 BC, but to them it was a nebula and its true nature had to wait until the invention of the telescope.

At the upper left of the image is another cluster of stars called Stock 2, but these are much more open, spread out and not as bright.  Through a pair of binoculars, Stock 2 looks like a headless stick man.  With your imagination running wild, you can even imagine one of his up raised arms holding a leash of curving stars that go down to the double "puffs" of a poodle.  Binoculars do not show as many stars as this photograph so seeing the stick man and the poodle will require you to go out and look for yourself.  To see it look about 15 degrees above the Northeast horizon soon after it gets dark.  By Midnight, it is about 25 degrees high.

Click on Image for a larger view
The Double Star Cluster look like they are neighbors, but the distance to this great swarm of stars is not identical.  The lower cluster, also known as NGC 884, is further away at 7600 light years. The upper cluster, NGC 889, is 6800 light years. 884 is also the older of the two.  However, when we consider the age of stars, these clusters are one of the youngest in our Milky Way galaxy, 3.2 million years old for 889 and 5.6 million years old for 889.  Millions of years may seem like a long time for us humans, but in astronomical terms, its very young.  Our own Sun is about 2.5 billion years old.  At the other extreme, are globular clusters, which are more than 10 billion years old.

Another interesting fact about these "baby stars".  If you were on a planet orbiting one of these stars and you looked toward our Sun, you would be hard pressed to see it.  This is because the brightest stars in these clusters are all great blazing supergiants of amazing brilliance compared to the Sun.  The brightest stars are 60,000 times brighter then the Sun.  Not only that, they are unimaginably large.  Placing of these supergiant stars in place of the Sun, it's diameter would go out beyound Earth's orbit.  Of interest is the presence of M-type red supergiant stars.  Some of these are located in the image below.
 Click on the Image for a larger view
One more interesting fact.  The Perseid meteor shower, which this year peaks during the evening of Aug 12 and morning hours of Aug 13, is near the radiant point of this shower. 
n other words, these "shooting stars" appear to come from this part of the night sky.

Sunday, July 11, 2010

Storm Panorama

 Click on Image to see a larger view and scroll to see the whole image
Traveling west across Kansas to Colorado we came across a huge thunderstorm.  It looked like three storms racing across the wide open spaces.  We drove on I-70 right between two sheets of rain and extreme winds.  The sun low behind the storm adds background light adding nice color to the scene.  The panorama is made from six individual images.

Monday, May 24, 2010

Whirlpool Galaxy

Click on Image for a larger view
One of most popular galaxies for amateur astronomers is the Whirlpool Galaxy, a grand spiral in the consetllation Canes Venatici.  Even though it is 23 million light years away, it can be seen as a fuzzy spot of light in a pair of binoculars, although you will need dark skies away from the city lights and know exactly where to look.  In a telescope, the spiral structure starts to be seen along with a smaller galaxy seemingly attached to one of the spiral arms of the larger galaxy.
Click on Image for a larger view
But only through long exposure photographs can we see detail that is too faint for our eyes.  The top image is a view of the whole area covered by my 1000mm focal length telescope.  Back in March, 2009, I took an image of this galaxy with my 300mm telephoto lens.  Compare this view with the much wider view of that lens by clicking on this link: http://tomjmartinez.blogspot.com/2009/03/galaxies-near-far-and-really-far.html
The bottom image is a close-up view showing the interaction taking place between the two galaxies.  Radio astronomers have been able to show that the smaller galaxy has merged with the larger one at least twice before.  The faint extensions seen around the galaxies are caused by material from both galaxies being flung out by the gravitational forces during the interactions.

The image is a combination of five 10-minute exposures with my 190mm f/5.3 telescope.

Thursday, May 20, 2010

Great Balls of Fire

 Click on Image for a larger view
Not the Jerry Lee Lewis rock 'n' roll rendition, but it really is a great ball of stars.  Some 500,000 stars, this is a Globular Cluster named M3.  This is because it is the 3rd object in a catalog of 110 objects created by Charles Messier in the late 18th century.  Like bees around a hive, these stars orbit around each other.  50% of the mass is within the central 22 light years, but there are stars rotating the main mass out to about 750 light years.  As we look at this cluster from a distance of some 34,000 light years, it seems that stars are touching each other, but they are not.  They are still very far apart, but if the Earth were inside M3, our sky would be very bright with no night sky.
***
Imaging Telescope: Orion Mak-Newt, 190mm, f/5.3, 1000mm focal length mounted on a Celestron CGE mount.
Guide Camera and Guidescope: CCD-Labs Q-Guider on a 50mm finderscope.
Acquisition Camera: CCD-Labs Q-453.
Exposures: Ten frames, 1 minute each.
Calibration Software:  DeepSkyStacker was used to stacked 20 Bias frames and 20 flat frames, then the 10 light frames were calibrated.
Final Process: Photoshop CS3

Monday, May 17, 2010

Venus and Moon

Click on Image for a larger view
The crescent Moon and Venus put on a fine show from my daughter's front yard in Castle Rock, Colorado this evening (05-16-2010).

Two second exposure on my tripod mounted Canon digital XTi at ISO 800 with my 18-55mm lens set at 31mm and f/5.6.