EAA Observing Session December 2024
 

EAA is "Electronically-assisted" astronomy.  With this type of observational astronomy, the camera substitutes for your eyeballs at the telescope:

  • Typically the observer live-streams and stacks together many short-exposure sub-frames of around 5-10 seconds exposure time for each subframe, for a total stack time of 10-20 minutes for each object before moving on in the sky to the next object to be observed.  The full stack of subframes is then saved onto the pc hard drive out at the telescope as a single Master Frame for further basic software processing later if desired.

  • You then slew to the next object on your observing list and repeat the process.

  • There are several multiple software apps available to automate these EAA routines.  SharpCap is one of the primary apps used to image the objects shown on these EAA webpages.

Click here to go back to EAA home page.

The following objects shown below were imaged and observed from 12/2/2024 through 12/4/2024 using the EAA techniques described above and listed below.

EAA Image Acquisition:

  • Telescope:  Vixen VMC260L Modified Klevtsov Cassegrain OTA with Astro-Physics CCDT67 focal reducer, shooting at f/7.8 and a focal length of 2044 mm
    Image Acquisition Software used:  SharpCap latest version
    Mount:  Rainbow Astro RST300, used in Equatorial Mode on Supermount CYG54G carbon-fiber tripod
    Camera:  ASI071 MC-Pro One-shot-color camera
    Autoguiding:  ASCOM software driver for mount used to connect mount to telescope control pc.  No 2nd camera was needed or used for autoguiding due to the short 5-10 second sub-exposures and precise polar alignment of the mount using the SharpCap Polar Alignment Tool, as well as the tracking quality of typical Rainbow Astro motor drives for short-exposure imaging.

Post-Processing Steps Used:

PixInsight software was used to lightly post-process the accumulated and saved single master frames from each object's image stack.  Typically, the steps used for processing were:

  • Removal of light-pollution gradients:  DBE (1 iteration only)
    Color calibration of the master image:  SPCC
    Deconvolution, sharpening, fix star elongation, and Noise Reduction using the RC Astro BlurXTerminator tool from inside PixInsight can also remove star elongation from the final images that was caused by tracking errors or optical errors from focal reducer spacing and minor telescope optical defects such as coma, astigmatism, soft focus, etc...  BXT will also help correct soft focus caused by poor atmospheric conditions or jet-stream turbulence over your observing site.
    Curves Transformation:  adjust image for any remaining residual noise or light pollution gradients, object detail enhancement, color channel or color saturation boosting or reducing of the image, and to adjust the white, mid and black points of the images for best overall appearance on a pc screen.
    Final Noise Reduction:  RC Astro NoiseXTerminator to reduce camera signal background noise or leftover color artifact noise, and clean up the overall image quality of the saved and processed master frames.

NOTE:  the above processing steps for EAA are much less in-depth and very fast compared with full-processing of true traditional long-exposure images.  Again, the goal is to just produce a logbook permanent record of your observing and not to produce publish-worthy pretty pictures.

EAA Objects Observed and Saved for this session:  (all image information and links are courtesy of Wikipedia and NASA).

**Click on any  image to view full-screen** 

Click on image for full-screen version
Image Information:
M27, also known as the "Dumbbell Nebula", is the remnant of an exploded star.  The explosion happened about 10,000 years ago The nebula lies 1360 light-years from Earth and is roughly 1 light-year diameter in actual physical size.  The nebula is receding from Earth at a rate of approximately 42 km/second.
8 second livestream exposures x 450 total sub-frames for total exposure time of 60 minutes
Click on image for full-screen versionImage Information:
M31 is "The Great Andromeda Galaxy".  It is a spiral galaxy 2.6 million light-years from Earth.  The galaxy is 220,000 light-years in diameter, about double the diameter of our own Milky Way Galaxy.  This image shows the central nucleus of the galaxy but it actually extends outward to a much wider field of view than this frame and its limited exposure time shows.
8 second livestream exposures x 150 total sub-frames for total exposure time of 20 minutes
Click image for full-screen version
Image Information:
M32 is an elliptical companion galaxy to M31 (seen in image above).  M32 is gravitationally bound to M31, so it lies at roughly the same distance from Earth of 2.6 million light-years.  M32 is very small in relation to M31 at a diameter of only 6,500 light-years.  The extreme edge of the M31 galaxy can be seen at the far left of this frame.
8 second livestream exposures x 150 total sub-frames for total exposure time of 20 minutes
Click image for full-screen version
Image Information:
M110, like M32, is a companion galaxy gravitationally bound to the Great Andromeda Galaxy seen above.  Notable in this frame are a couple of dark splotches that are gigantic gas and dust clouds near the nucleus of the galaxy.  M110 is approximately double the size of M32 at about 12,000 light years in diameter.  M110 also contains a large halo of globular clusters visible in very large telescopes.
5 & 8 second livestream exposures x 390 total sub-frames for total exposure time of 40 minutes
Click image for full-screen versionImage Information:
M34 is an open cluster in our Milky Way Galaxy.  It is located about 1400 light-years from Earth.  The cluster has a diameter of approximately 15 light-years.  It is notable for its very hot, young blue stars, several of which are optical double stars from Earth's line of sight.  Many of the background stars farther out from the cluster's center are also members of this large bright cluster.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen version
Image Information:
M52 is a very dense open cluster packed full of about 200 stars.  It lies at a distance from Earth of approximately 5000 light-years.  M52 has a diameter of 15 light-years.  Its predominant star members are yellow giants similar to our Sun, as well as several younger blue-white very hot stars.  It is nearly stationary in angular velocity with the Earth inside our Milky Way Galaxy.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen version
Image Information:
Messier 103 is a compact open cluster in our Milky Way galaxy.  It lies at a distance from Earth of approximately 9200 light-years and has a diameter of 15 light-years.  It is populated by about 172 stars, many of which are about 25 million years old.   It has a notable large, bright red-giant star near its center and a physically-bound double star is also visible in the upper right of the frame.
5 second livestream exposures x 84 total sub-frames for total exposure time of 7 minutes
Click on image for full-screen version
Image Information:
NGC457 is an open cluster in our Milky Way galaxy that contains about 100 stars.  It lies at a distance from Earth of 7900 light-years and has a physical diameter of about 15 light-years.  It is also known as the "ET Cluster" due to it's two very bright stars that look like a pair of eyes staring back at you.  The brightest stars is a foreground star and not physically bound to the cluster.
5 second livestream exposures x 120 total sub-frames for total exposure time of 10 minutes
Click on image for full-screen version
Image Information:
NGC884 is a beautiful, bright open cluster in our galaxy that is comprised of many hot, young blue-giant stars,  It contains about 150 stars and lies at a distance from Earth of 7000 light-years.  The cluster is approximately 3.2 million years old which is very young by galactic standards for objects of this type and mass.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen version
Image Information:
NGC 869 is the other half of the famous "Double-Cluster" in the constellation Perseus.  This cluster is only a few hundred light years distant from NGC884 (see image to left) and also is at a distance of approximately 7000 light-years from Earth.  It appears to be significantly older than NGC884, despite their relatively close spacing together in our galaxy.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen version
Image Information:
NGC663 is an open cluster in our Milky Way galaxy.  It is approximately 20 million years old.  It is approximately 7000 light years distant from Earth.  It contains at two bright Red Supergiants (upper right of cluster).  The cluster is receding away from Earth at approximately 32km/second.  It is thought to be part of a larger group of adjacent clusters that are all gravitationally bound.
5 second livestream exposures x 118 total sub-frames for total exposure time of 9.8 minutes
Click on image for full-screen version





Image Information:
NGC6826 is a planetary nebula in our Milky Way galaxy.  Like most planetary nebulae, it is gas shell remnant of a violent exploding, then collapsing star that has expended all its fuel and has reached the end of its life cycle.   It lies at a distance of 4200 light-years from earth and is known as the "Blinking Eye" nebula.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen version
Image Information:
NGC6946 is a spiral galaxy located at a distance from Earth of 10 million light-years.  It is known as the "Fireworks Galaxy" due to its pinwheel appearance and brightness of its spiral arms.  It's physical diameter is 40,000 light-years, less than half the size of our own Milky Way galaxy.  This galaxy is undergoing an unusually high amount of new-star formation in its spiral arms.
8 second livestream exposures x 225 total sub-frames for total exposure time of 30 minutes
Click on image for full-screen versionImage Information:
NGC7293, also known as the "Helix Nebula" is another exploded-star planetary nebula gas shell.  It is known for its excellent color from hot, ionized gas and dust that originated from the star explosion approximately 10,600 years ago.  It lies at a distance from Earth of 650 light-years and has a physical diameter of approximately 2.5 light years.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen versionImage Information:
M33 is a spiral galaxy commonly known as the Triangulum Galaxy.  It is a member of the Local Group of galaxies along with our own Milky Way galaxy and the Great Andromeda Galaxy,   It lies at a distance from Earth of 2.9 million light-years.  M33 has a physical diameter of 50,000 light-years, or about half the size of our own galaxy.
8 second livestream exposures x 342 total sub-frames for total exposure time of 45.6 minutes
Click on image for full-screen versionImage Information:
NGC 7331 is a spiral galaxy with an associated cluster of smaller fainter elliptical galaxies and one spiral galaxy just visible below the main galaxy.  It lies at a large distance from Earth of 49 million light-years and has a physical diameter of 30,000 light years, or less than a third the diameter of our own Milky Way galaxy.  View full size by clicking the image for best views of these objects.
8 second livestream exposures x 450 total sub-frames for total exposure time of 60 minutes
Click on image for full-screen versionImage Information:
NGC7662, also known as the "Blue Snowball" nebula, is a planetary nebula in our Milky Way galaxy.  It lies at a distance from Earth of 4500 light-years.  It has a physical diameter of approximately 0.5 light-years.  It has a distinctive blue-green appearance in larger telescopes.  Click  on image to see more details in the object's structure.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes
Click on image for full-screen versionImage Information:
NGC7789, also known as "Caroline's Rose", is a beautiful large and very dense open star cluster in our Milky Way galaxy.  It lies at a distance from Earth of 8000 light-years, and has a diameter of about 60 light-years.   The cluster is estimated to be 1.6 billion years old which is unusually old for an open star cluster and compares similarly to much older globular clusters in our galaxy.
5 second livestream exposures x 240 total sub-frames for total exposure time of 20 minutes

 

wcv
12/11/2024