Dennis
23-10-2007, 03:20 PM
Hello,
Well, what a difference seeing and altitude make! I looked outside the window at 2:00am and saw Orion so decided to try to capture a set of images of the Trapezium stars A B C D E F G H & I.
By 3:00am the ‘scope had cooled and I estimated the seeing to be around 8/10. Using the Mewlon 180 F12, TeleVue x2.5 PowerMate and DMK21AF04.AS CCD camera I tried various exposure settings to see which would be best.
Pane 1: Limiting the exposure to 1/30 got me stars A through F, even revealing the stellar diffraction rings around the brighter components.
Pane 2: Increasing the exposure to 1/15 sec made the stars more blobby although the separation between components A to F was clear and steady due to the very good seeing and the altitude of Orion.
Pane 3: Finally, I tried exposures of 1/3 sec to see if I could dig out the fainter components G H & I.
Pane 4: After stretching the data using the histogram, it became apparent that the seeing had supported the splitting of H1 and H2. I then overlaid this stretched image of a Hubble image and the components lined up precisely.
Data from SkyTools:
Theta 1 Ori, Multiple Star System, Magnitude: 5.13
AB: 5.13+6.35 mag, In 1991: PA 312° Sep 12.87"
AC: 5.13+7.2 mag, PA 56° Sep 13.12"
AD: 5.13+7.49 mag, PA 342° Sep 16.87"
AE: 5.13+6.4 mag, PA 134° Sep 135.30"
EF: 6.4+7.5 mag, PA 92° Sep 52.50"
EG: 6.4+9.1 mag, PA 97° Sep 128.70"
BH: 6.35+11.1 mag, Sep 4.10"
AI: 5.13+11.5 mag, PA 122° Sep 4.00"
Some sources place components G, H & I at between magnitude 14 and 15.
Here is an excellent reference site: http://www.astropix.com/HTML/B_WINTER/TRAPEZ.HTM
Here is an HST reference site: http://hubblesite.org/newscenter/archive/releases/2000/19/image/a/
Here is a reference page by Glenn Schneider: http://nicmosis.as.arizona.edu:8000/TRAPESIUM/TRAP_COLOR.html
Cheers
Dennis
Well, what a difference seeing and altitude make! I looked outside the window at 2:00am and saw Orion so decided to try to capture a set of images of the Trapezium stars A B C D E F G H & I.
By 3:00am the ‘scope had cooled and I estimated the seeing to be around 8/10. Using the Mewlon 180 F12, TeleVue x2.5 PowerMate and DMK21AF04.AS CCD camera I tried various exposure settings to see which would be best.
Pane 1: Limiting the exposure to 1/30 got me stars A through F, even revealing the stellar diffraction rings around the brighter components.
Pane 2: Increasing the exposure to 1/15 sec made the stars more blobby although the separation between components A to F was clear and steady due to the very good seeing and the altitude of Orion.
Pane 3: Finally, I tried exposures of 1/3 sec to see if I could dig out the fainter components G H & I.
Pane 4: After stretching the data using the histogram, it became apparent that the seeing had supported the splitting of H1 and H2. I then overlaid this stretched image of a Hubble image and the components lined up precisely.
Data from SkyTools:
Theta 1 Ori, Multiple Star System, Magnitude: 5.13
AB: 5.13+6.35 mag, In 1991: PA 312° Sep 12.87"
AC: 5.13+7.2 mag, PA 56° Sep 13.12"
AD: 5.13+7.49 mag, PA 342° Sep 16.87"
AE: 5.13+6.4 mag, PA 134° Sep 135.30"
EF: 6.4+7.5 mag, PA 92° Sep 52.50"
EG: 6.4+9.1 mag, PA 97° Sep 128.70"
BH: 6.35+11.1 mag, Sep 4.10"
AI: 5.13+11.5 mag, PA 122° Sep 4.00"
Some sources place components G, H & I at between magnitude 14 and 15.
Here is an excellent reference site: http://www.astropix.com/HTML/B_WINTER/TRAPEZ.HTM
Here is an HST reference site: http://hubblesite.org/newscenter/archive/releases/2000/19/image/a/
Here is a reference page by Glenn Schneider: http://nicmosis.as.arizona.edu:8000/TRAPESIUM/TRAP_COLOR.html
Cheers
Dennis