CCD image of the bright diffuse reflection nebula M78, taken with the MIT/Lincoln Labs CCD camera on the 3.9-meter Anglo-Australian Telescope.
The two brightest illuminating stars are well visible within the blueish reflection nebula, as are NGC 2064 to the WSW (lower right) and faint but larger NGC 2067 to the North-West (upper right), separated from M78 by a dark band. Note the fine detail within the nebula and particularly on its edges, especially to the North and south.
This image was created by David Malin. It is copyrighted and may be used for private purpose only. For any other kind of use, including internet mirroring and storing on CD-ROM, please contact the Photo Permissions Department of the Anglo Australian Observatory.
Reflection nebula M78 in Orion, as photographed by Ylla and Calvin Pratt, on
December 18, 2000, from Kitt Peak near Tucson, Arizona. They took this photo
when participating in the Advanced
Observing Program of the
Kitt Peak National Observatory (KPNO) Visitor Center. This image was
obtained with AOP's Meade 16in LX200 telescope operating at f/6.3 and SBIG
ST8E CCD camera with color filter wheel, and processed by Adam Block. It is a
composite of four CCD images: Luminance = 42 min, Red = 10 min, Green = 10
min, and Blue = 20 min. The weaker neighboring reflection nebulae NGC 2064
and NGC 2067 are well visible in this image.
Credit: Ylla and Calvin Pratt/Adam Block/AURA/NOAO/NSF
2MASS image of reflection nebula M78. Much detail and many stars become visible in this 2-micrometer wavelength IR image which are hidden behind the dust in above and other visible-light images of this nebula. The two brightest stars illuminating M78, HDE 38563A and 38563B, are prominently visible, together with a cluster of fainter and presumably lower-mass young stars which recently formed in this nebula, from the associated part of the giant Orion Molecular Cloud. This image was cropped from a huge mosaic, created by S. Van Dyk (IPAC). A number of the young stellar objects in this region are highlighted dramatically by their Herbig-Haro outflows; in 1999, 17 Herbig-Haro objects were known in M78.
In the IR, NGC 2064 can well be traced, but only a small part of NGC 2067 is visible just around the star above (N of) NGC 2064 and right of (preceding, west of) M78. In the IR, the optically dark southern edge appears as a bright and much structured part of the nebula.
As all 2MASS Atlas representations, this is a false-color IR image, mapping 3 IR wavelength bands into colors: J light (1.2 micron) into blue, H light (1.6 micron) in green, and Ks light (2.2 micron) into red. Thus the blueish region is brightest at shortest wavelengths (closest or "nearest" to visible), the more grey or white outlayers are about equally bright throughout this part of the IR spectrum, and the brown-reddish regions to the south and in NGC 2064 are brighter to the cooler, longer-wavelength ("farther" IR) part of the spectrum.
Last Modification: 17 Aug 2001, 17:50 MET