Grove Creek Observatory's Telescopes & Equipment:
Short Summary:
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14" (36cm) Celestron Schmidt Cassegrain (SkyLive Internet Telescope - SBIG ST-8 CCD) | |
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14" (36cm) Meade RCX-400 f/8 GOTO Ritchey-Chrétien (Wheaton Internet Telescope - SBIG STL-1001E CCD) | |
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12" (30.5cm) Meade LX-200 f/10 GOTO Schmidt Cassegrain (SkyLive Internet Telescope - SBIG ST-10 CCD) | |
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10" (25.4cm) Meade LX-200 GPS f/10 GOTO Schmidt Cassegrain (Wheaton Internet Telescope - SBIG STL-1001E CCD) | |
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10" (25.4cm) Meade LX-200 f/10 GOTO Schmidt Cassegrain - (Viewing Instrument) | |
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8" (20.3cm) Newtonian f/7 German Equatorial | |
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4" (10cm) f/4 Pentax Astrograph | |
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Jove Riometer | |
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2.3m steerable dish Radio Telescope |
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THE CELESTRON C-14 SCHMIDT
CASSEGRAIN:

Celestron Pacific C14 Schmidt Cassegrain Telescope
Aperture: 36cm (14") Focal Length:
3,910mm Focal Ratio: f/11
(Pictured with Steven Williams)
A very unique telescope with
somewhat of a unique history....
Viewing
through the C14 Telescope:

Light Path through a
Schmidt Cassegrain Telescope
Housed in our main motorised 3.2 meter (10 foot) dome, is our massive Celestron C14. This is our main viewing instrument and with a focal length of 3,910mm (154"), this telescope is used for high resolution objects. Being a Schmidt Cassegrain, it provides a higher contrast than even larger Newtonian telescopes. The C14 was built in 1971 and was the second model made by the "Celestron Pacific" telescope company, using the original sturdy "sand-cast" rigid fork. Its 36cm (14") primary mirror is of an exceptional high optical standard - going beyond testing equipment that could measure an accuracy of 1/10 wavelength of light. The C14 can operate visually at f/11 or f/7 and can be configured with huge a variety of combinations for different types of astrophotography and CCD imaging. The C14 is mounted on a home made equatorial wedge, that is made out of 23mm (0.9") thick stainless steel. This is attached to a huge pier, which is driven 6 metres (19.5 ft) into the ground and is totally isolated with no part of the building touching it. The pier is 50cm (20") diameter and constructed with a solid steel core of 18cm (7") diameter, surrounded by concrete, sealed with a large gas pipe on the outside.
The C14 at Grove Creek has its own fame, as many live astronomical events were recorded with special video cameras attached, including live images of the Shoemaker-Levy Comet hitting Jupiter, that were shown throughout the world on Australian and international TV, including CNN, and the BBC, in July 1994. Well over 10,000 people viewed Halley's Comet through this telescope when it was installed at Grove Creek in 1985.
In 1998, extensive upgrades were made to replace the old original Right Ascension AC clock tracking and DC slewing motor (abbrev. "RA" - the east/west movement) and the DC Declination motor (abbrev. "DEC" - the north/south movement) with a home-made Z-80 processor controlled stepping motor control system, designed and built by electronics expert Chris Ralph and astronomer Steven Williams. For the first time on such an old mount, high magnification "auto-guiding" astrophotography and the early days of astronomical CCD imaging was then made possible with this system. Along with the electronic tracking upgrades, a Celestron Astro-Master computerised digital setting circle was also installed, to make finding objects a breeze. An innovation that was never even dreamed of, when the mount was designed 30 years ago! Previously, tedious sightings had to be read from old mechanical setting circles attached to the mount. Grove Creek was one of the first observatories to purchase a SBIG ST-4 CCD autoguider and stunning film photos were achieved as a result.
Then two disasters struck... In 1999, one of the most severe storms ever seen in the area totally blew the entire 300kgs dome off its rails, driving it into the telescope's mount and destroyed the delicate RA gearing system and mounting hardware for the optical encoders. However, even with such amazing force, the optics of this ruggedly built telescope didn't even loose collimation! Fortunately (and very generously) Celestron, understanding that this particular telescope was of special vintage, re-built the RA gear system at no charge and the dome was modified so such an horrible incident could never happen again. However, to the complete dread of everyone involved with Grove Creek, a violent electrical strike directly hit the C14 in 2002, which not only caused massive damage to most of the electrical devices and appliances throughout the observatory but totally destroyed both the home-made drive controller, Astro-Master and optical encoders! Parts for the previous home-made drive system were no longer available, so it was replaced with a third-party commercial computerised duel stepping motor drive system. The Celestron Astro-Master was replaced with a Argo Navis digital setting circle computer, with RS2-232 planetarium control functions from Wildcard Innovations.
In May 2008, the C14 was removed from the dome and installed on a Astro-Physics GTO-1200 mount, in our sliding roof Middle Observatory. This enabled us to put it online for everyone to use, via our SkyLive remote internet telescope system.

Click picture for full resolution.
Above: The C14 installed on
a Astro-Physics GTO-1200 mount in our
Middle Observatory, as a fully remote internet controlled telescope.
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Meade 36cm (14") RCX-400
Ritchey-Chrétien
Telescope:

Dedicated SBIG STL-1001E CCD Internet remote controlled
system
1024 x 1024 pixels @
24 microns. f/8 (FL=2,844mm) FOV = 30^min square. Image scale = 1.74^sec/pixel
Installed on January 29th, 2007, this is the new telescope for the Wheaton College internet telescope project. It upgraded a previous 30cm (12") Meade LX-200 and is a dedicated CCD imaging system with a SBIG Large Format STL-1001E CCD camera - it is not for viewing through. A fast (f/8) RC design produces a large, coma-free field of view from edge-to-edge, providing users with the latest in imaging technology, to capture tack sharp images over a wider field. For full details on this project, please visit our Wheaton Telescope web page. Currently, this telescope has some hardware problems and a personal Meade 10" LX-200 GPS is operating as a back-up.
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30cm (12") LX-200 Schmidt Cassegrain
Telescope:

Mounted on the central pier in the Western Observatory
Aperture 30.5 (12") Focal Length: 2,500mm Focal Ratio: f/5.88
Dedicated SBIG ST-10 CCD Internet remote controlled system.
Field of View = 19.5 x 28.9^mins. Image
Scale =0.788^secs/pixel
R V B C I Photometric filters Installed
We use the LX-200 12" for remote CCD imaging. The 12" was upgraded in November 2007 and is now online, as part of the Skylive project at Grove Creek. These telescopes have highly sophisticated software and electronics with "GOTO" ability, automatically moving the telescope to any of thousands of different astronomical objects with very high precision - simply with the click of a mouse! "T-Point" error mapping software lands any desired object in the field of view, every time.
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25cm (10") LX-200 Schmidt Cassegrain Telescope:

Aperture: 25.4cm (10") Focal Length: 2,000mm Focal Ratio: f/10
Mounted on the pier in the Main Dome
As all our telescopes are mostly dedicated CCD imaging instruments and can not be viewed through, we have this telescope available for viewing use in the main dome. In January 2009, a special pier adaptor plate was installed by Brett Soames to enable a LX-200 Wedge base, Paramount ME mount or to put back the original C-14 fork on the main pier. The previous C14 was moved into the middle observatory for robotic use in May 2008. A CCD camera for personal use can be easily installed, operated from a PC in the control room.

CCD Imaging Setup on the 10" LX-200 Telescope.
Shown above, is the 10" LX-200 telescope and SBIG ST-9XE CCD camera. This provides a field of view of 14 arc minutes square (nearly a quarter of a degree or half a moon's width). This is perfect for imaging galaxies, globular clusters and planetary nebulae. The CCD camera is so sensitive, that 13th magnitude galaxies can be imaged in less than a minute! It is fitted with an SBIG Adaptive Optics AO-7 guiding system and also has remote controlled rear cell focussing.
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20cm (8") f/7 Newtonian
Telescope
(Mounted on "Samson" Equatorial Mount
LEFT, Sturdy wooden Dobson Mount RIGHT)
The 8" (20cm) f/7 Newtonian telescope provides a nice contrast and compliments the larger telescopes at Grove Creek. Being one of the most common type and size of a serious amateur telescope, this telescope is provided as a "learning tool" for visitors at Grove Creek, who may be thinking of starting the hobby of astronomy and what they can expect from a (comparably affordable) and portable instrument. This telescope can be placed on an German Equatorial Mount (which tracks the movements of stars) or on a common Dobson Mount, to enable those people that are not used to a telescope, to just roam the skies with. A telescope like this with a Dobson (non-tracking) mount, is a good "starter telescope" and simple models can start from around AUD$700, without accessories.
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Pentax - 10cm (3.9") SDUF II f/4 APO
Astrograph:
This stunning wide field refractor is mostly used for wide-field deep sky viewing, CCD imaging and astrophotography. It has a SDP 4-lens/two group design with integrated corrector, which offers excellent image quality over the entire field of view. Even at very high magnifications, the colour correction is superb. Due to its short 400mm focal length, this telescope makes a wonderful wide field viewing instrument. It can accept both film SLR and CCD cameras, as well as 2" eyepieces (like our Naglars). It is fantastic for large comets. It sports a clear aperture of 83mm, which easily covers a large 6 X 4.5 film format. This instrument used to be "piggy-back" mounted on our C14 telescope but is now installed on a Astro-Physics 1200-GTO mount, with a SBIG ST-10 CCD Camera. These instruments are well prized in the astronomical community and are available from OPT Telescopes in the USA.
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Radio Telescopes:
Andrew Mattingly and Greg Ford run and own these
instruments, which are
installed at the Grove Creek Observatory and operated over the internet
remotely.

The S.R.T
The Small Radio Telescope (S.R.T) uses a 2.3m
diameter dish driven by an altitude/azimuth computer control drive system with
an FFT based radio spectrometer receiver operating between 1370 - 1800 MHz to
make various radio astronomy observations including the 21 cm (1420 MHz) spin
flip line of atomic hydrogen. The receiver uses digital technology with a 8-bit
analogue to digital down converter, digital signal processor (DSP) and is
controlled remotely using a STAMP microprocessor and RS-232 communications. It
is run exclusively over the internet by Andrew Mattingly and Greg Ford. Greg &
Andrew also run projects which have been submitted by others in the astronomical
community, where the resulting data is passed on over the internet for further
study.

Jove Riometer
Our Radio Jove Riometer operating at 20.1 MHz is used to study both Jupiter and Solar radio emissions to better understand their magnetic fields and their plasma [charged particle] environment.
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