The Owl Nebula

 
Messier Object 97, The Owl Nebula
 

 

Image Information
Date Imaged 12/28/2005
Location Imaged From

Tierra del Sol , CA

Equipment Telescope: Astro Tech 203mm RC
Mount: Losmandy G-11 w/Gemini
Camera: SBIG ST-2000XM
Focal Ratio: f/8.0
Exposure Information

LRGB 80:80:90:90

  • Data collection using:
    CCD Commander
    ASCOM POTH
    MaxPoint
    CCDSoft
    FocusMax
    PinPoint
    TheSky6 Pro
  • Image Calibration - Maxim DL
  • Image Registration - Maxim DL
  • Image Stacking - Maxim DL
  • Post processing in Adobe Photoshop CS3 Extended

 

The Owl Nebula (also known as Messier Object 97 or NGC 3587) is a planetary nebula in the constellation Ursa Major. It was discovered by Pierre Méchain in 1781.

M97 is regarded as one of the more complex of the planetaries. The 16th magnitude central star has about 0.7 solar masses and the nebula itself about 0.15 solar masses. The nebula formed roughly 6,000 years ago.

The nebula gets it name due to the appearance of owl-like "eyes" when view through a large (>200 mm) telescope under dark sky conditions with the aid of a so-called "nebula filter." The "eyes" are also easily visible through photographs taken of the nebula.