The Skinakas Observatory has been built and operates as part of a scientific research collaboration between the University of Crete, the Foundation for Research and Technology-Hellas (FORTH) and the Max-Planck-Institut fur Extraterrestrische Physik of Germany. The site of the
Observatory, chosen on scientific and functional grounds, is the Skinakas summit of Mount Ida (Psiloritis), at an altitude of 1750 m and 60 km from Heraklion.
The Observatory has two telescopes: a Modified Ritchey-Chrétien telescope with a 1.3m aperture (focal ratio of F 7.6) and a 30cm telescope (focal ratio F 3.2). The building for the small telescope was built in 1986, and observations started in 1987. The 1.3μ telescope commenced its observations in October 1995 and remains the largest operational telescope in Greece to date. The optical system was manifactured by Carl Zeiss, and the mechanical parts by DFM Engineering.
The instrumentation of the 1.3 Telescope includes:
- A Focal Reducer which more than doubles the field of view of the telescopel it also allows low resolution spectroscopic measurements
- Autoguider
- Three optical CCD cameras: one with 1024x1024 pixels and two with 800x2000 pixels.
- A wide field near-infared camera
Under construction are:
- A high resolution (R=35000) Echelle Spectrograph.
- An Adaptive Optics system for the reduction of the atmospheric seeing
The main ongoing astronomical projects at the Observatory of Skinakas include the study of:
- Galaxies and Active Galactic Nuclei- Planetary nebulae
- Supernovae remnants
- Globular clusters
- Binary systems where the compact object is either a white dwarf, a neutron star, or a black hole
A Google map with driving directions from the city of Heraklion to Skinakas Observatory is available here.
For more information visit:
- Official website of Skinakas Observatory.
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