The Color Images

If you came to this Web site seeking color images, this is the place for them.

Enjoy the views and please observe the copyright restriction on the homepage. If you wish to read a rather long-winded description about my observatory and photographic work, continue past the images in the Table of Contents.

The original purpose of this Web space was to show off high resolution Schmidt camera photography with TP-2415 film. However, I have recently (September, 1996) begun to play in Photoshop 3.0 with some of the few color slides I took with the Schmidt a long time ago. These images, taken on hypered Ektachrome 200 back in 1982, were the most misserable washed out low contrast pictures ever secured with an 8-inch Schmidt. Just for the fun of it, I decided to see what Photoshop could do with these 14-year-old rejects, and I was amazed. I am partially color blind, and the results I achieved can best be called "Photoshop gone wild", so the colors presented here are NOT scientifically accurate. It is just a case of a Photoshop novice pushing the program slider bars until something interesting happens. The results turned out kinda neat, I think.


North America Nebula

797 X 600 pixel 112 K .jpg


NGC 7000 and IC 5070, the North America and Pelican Nebulae in Cygnus.
Location: NGC 7000 = 20h 58m +44d 20m, IC 5070 = 20h 51m +44d 00m
Size: NGC 7000 = 120 arc/min, IC 5070 = 60 X 50 arc/min
Magnitude: ---
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
Gamma Cygnii Nebula

800 X 600 pixel 153 K .jpg


IC 1318 and NGC 6888, the Butterfly and Crescent Nebulae in Cygnus.
Location: IC 1318 = 20h 26m +40d 20m, NGC 6888 = 20h 12m +38d 23m
Size: IC 1318 = 210 X 140 arc/min, NGC 6888 = 18 X 8 arc/min
Magnitude: ---
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
The Eagle and the Swan (or Omega) Nebulae

996 X 475 pixel 152 K .jpg


IC 4703 and M 17, the Eagle and the Swan (or Omega) Nebulae in Serpens and Sagittarius.
Location: IC 4703 = 18h 19m -13d 50m, M 17 = 18h 21m -16h 10m
Size: IC 4703 = 28 X 17 arc/min, M 17 = 11 X 6 arc/min
Magnitude:---
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
The Lagoon and Trifid Nebulae

639 X 629 pixel 101 K .jpg


M 8 and M 20, the Lagoon and Trifid Nebulae in Sagittarius.
Location: M8 = 18h 04 m -24d 18m, M 20 = 18h 02m -22d 59m
Size: M 8 = 50 X 40 arc/min, M 20 = 17 X 12 arc/min
Magnitude:---
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
M 6 and M 7 Star Clusters

800 X 600 pixel 124 K .jpg


The M 6 and M 7 star clusters in Scorpius.
Location: M 6 = 17h 40m -32d 14m, M 7 = 17h 54m -34d 47m
Size: M 6 = 14 arc/min, M 7 = 80 arc/min
Magnitude: M 6 = 4.2, M 7 = 3.3
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
The 'false comet' in Scorpius

814 X 814 pixel 152 K .jpg


IC 4628 and NGC 6231, the "false comet" in Scorpius.
Location: IC 4628 = 16h 57m -40d 18m, NGC 6231 = 16h 54m -41d 47m
Size: IC 4628 = 52 X 33 arc/min, NGC 6231 = 14 arc/min
Magnitude: NGC 6231 = 2.6
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
Double Cluster

800 X 600 pixel 63 K .jpg


NGC 884 and NGC 869, the Double Cluster in Perseus.
Location: NGC 884 = 2h 21m +57d 07m, NGC 869 = 2h 19m +57d 08m
Size: NGC 884 = 29 arc/min, NGC 869 = 29 arc/min
Magnitude: NGC 884 = 6.1, NGC 869 = 5.3
5 minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.
Space Fly

666 X 800 pixel 77 K .jpg


"Space Fly", the internal reflection inside a Schmidt camera caused by a bright object reflecting off the inside of the corrector plate. In this case, the reflection is caused by the planet Venus.
One minute exposure on hypered Ektachrome 200, developed with E-6 chemistry and no push processing.

Go to next page ---- New color images on Ektachrome Elite II 100 film
Go to previous page Black & White Images -- Page 2
Back to ------------ Table of Contents