MPC 476 Grange Observatory
The Grange Observatory from 1993 lies atop a private house in Bussoleno (50 km W
from Turin, Italy), in Susa Valley near the French border; Grange comes from the
name of the town's suburb.
The observatory's roll-off roof opens in two parts
and covers a 3 m by 3 m room; the homemade telescope is a 0.3-m Newton/Cassegrain reflector.
The optical instrumentation at Grange Obs. is permanently mounted on a concrete pillar and is
independent from the room's floor; the observing site can be reached via a
foldable ladder from a room devoted to laboratory / library.
The fork mount of the 0.3-m telescope was built at the Turin Observatory workshop with the secondary optics supports; the 10 kg main mirror 9 points cell and the foci common, anti-rotation bronze focuser were built in-house, as well as the support optics tube quest, choosing the Bakelite, a pristine composite material, for thermal isolation and for structural reasons. All the optics were built by Costruzione Ottiche Zen of Venice, and the optics in their supports were precisely integrated on the observatory proprietor's own, being graduated in structural engineering at the time, and employed in a well-known Aerospace Company in Turin since 1989. In the '80 in Italy it was absolutely common to (partly or entirely) BUILD a large astronomical telescope.
originally had a DOS based SXL8-P CCD camera, peltier cooled, and connected to a 486 DX2 computer with CD-ROM drive, this one
being useful for having a quick access to huge star catalogues and sky surveys
such as GSC-ACT, Tycho 2 and USNO A2.0 . The field given by the camera at the Newton focus was 22x22 square arcmin, being the stars recorded about magnitude 15, reached with 1 minute exposure.
The SXL8-P camera is still mounted at the 0.3-m telescope's Cassegrain focus, used for astrometry and star photometry at f/8.3 through the ASTROART 5 plug-in working with Windows XP on a ASUS laptop having a parallel port. This system can give a tri-dimensional view of stellar objects in selected photometric wavelengths. A DSLR Nikon D3000 and is present at the 0.14-m astrograph at f/5.7 with a pointing eyepiece .
The camera SXL8-P has an HR star field of 10.5x10.5 arcmin, and it is used for Sloan visual photometry.
A flip mirror is also used for mounting eyepieces from 125x to 333x at the Cassegrain focus of the telescope to point the CCD camera field.
The astrograph's main research activity is stellar photometry, although astrometry is still performed being one of the observatories appointed by IAU past Commission 20 which send their measures to the Central Bureau for
Astronomical Telegrams/Minor Planet Center, located at Smithsonian
Astrophysical Observatory, Cambridge, MA (U.S.A.). Up to date, more than 400 astrometric measures were sent in about 30 years.
Grange Obs. was also one of
the observing sites of Gruppo Italiano
Astrometristi, the Italian Astrometry Group, which at the time coordinated all the
astrometric activity done in Italy by amateur astronomers, and was a proud member
Currently the privately granted MPC 476 Grange Observatory is making researches on fundamental astronomy, such as astrometry and photometry; the instruments of the observatory can measure the distance, the temperature and the spectral class of the stars. For the observatory's technical news click here.
If interested in the researches and products of the Grange Obs. laboratory, or GOlab, please have a look of the spin off page.
- OBSERVATORY DATA
- Minor Planet
Center code = 476
- Latitude = 45° 08' 31.8" N
- Longitude = 7° 08' 26.7" E
- Height = 512 m WGS84 ell. (490 m a.s.l)
- CCD CAMERAS
- A 12-bit Starlight Xpress SXL8-P mono camera
(chip 'frame transfer' Philips FT-12, 508x512, temp. -30°C) mounted on the 0.3-m telescope is mainly used for astrometry and photometry with a field of 10.5 x 10.5 arcmin. The camera has Sloan g/r photometric channels and a filter against the local heavy LED light pollution. A neutral density channel is also present for lunar or daily imaging and for bright stars flux measuring.
- A 14-bit camera DSLR Nikon D3000, mounted at the 0.14-m astrograph focus (f/5.7), has a larger field of 101x67 square arcmin on a 3872x2592 squared pixels of 6 microns (used in mono mode in BIN2 with IRIS program, and a Shott GG495 2" filter to approximate the photometric Johnson V band).
- HOW TO CONTACT GRANGE OBSERVATORY
Go to the AAS
homepage, the local amateur association (in Italian).
Return to Grange Obs. homepage.