These dark nebulae were found from visual inspection of the Palomar
Sky Survey photographic plates.
Not exact matches
Achieving this goal required a huge step up from the 1950s - era Palomar
Sky Survey, whose
photographic plates have guided astronomers to celestial curiosities for decades.
This color image is based on data coming from 33
photographic plates taken between 1987 and 1995 through the Palomar Observatory's 48 - inch (1,2 - meter) Samuel Oschin Telescope as a part of the second National Geographic Palomar Observatory
Sky Survey (POSS II).
So Jewitt and Luu carried out two parallel
surveys: they used the Palomar Observatory's Schmidt telescope equipped with conventional glass
photographic plates to scan large areas of the
sky for the very faintest objects, while also watching a narrow field of view in the plane of the planets for rare but slightly brighter objects using MIT's 1.3 - metre telescope fitted with a CCD.
The DASCH
survey is based on thousands of
photographic plates taken by Harvard astronomers between 1890 and 1989 as part of a regular
survey of the northern
sky.
This wide - field view of the
sky around the bright star Alpha Centauri was created from photographic images forming part of the Digitized Sky Survey
sky around the bright star Alpha Centauri was created from
photographic images forming part of the Digitized
Sky Survey
Sky Survey 2.