The Merope Nebula (also known as Tempel’s Nebula and NGC 1435) is a diffuse reflection nebula, possibly a supernova remnant, in the Pleiades star cluster, surrounding the 4th magnitude star Merope. It was discovered on October 19, 1859 by the German astronomer Wilhelm Tempel. John Herschel, in his New General Catalogue (NGC), described it as a very faint nebula about the size of the full moon.
The Merope Nebula has an apparent magnitude starting at 13 and quickly dimming by a factor of about 15, making most of the nebula dimmer than magnitude 16. It is illuminated entirely by the star Merope, which is embedded in the nebula. It contains a bright knot, IC 349, about half an arcminute wide near Merope. It appears blue in photographs because of the fine carbon dust spread throughout the cloud. Though it was once thought the Pleiades formed from this and surrounding nebulae, it is now known that the Pleiades nebulosity is caused by a chance encounter with the cloud.
A small and unique nebula which is close to Merope was discovered by Edward Emerson Barnard in November 1890. It is naturally very bright but is almost hidden in the radiance of Merope.
Imaging telescopes or lenses: Stellarvue SVQ100
Imaging cameras: QSI 683 ws
Mounts: Losmandy G-11/Gem II
Guiding telescopes or lenses: Stellarvue SV80ST
RA center: 56.278 degrees
DEC center: 23.709 degrees
Pixel scale: 1.920 arcsec/pixel
Orientation: 161.423 degrees
Field radius: 0.851 degrees
Locations: Remote Site, Near Rodeo, New Mexico, United States