The Telescopes at the Grove Creek Observatory
Short Summary: (click links to go direct to each telescope)
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THE
CELESTRON C-14" (36cm) SCHMIDT CASSEGRAIN
A very unique telescope with a unique history!
Celestron Pacific C14 Schmidt Cassegrain Telescope
Aperture: 36cm (14") Focal Length:
3,910mm Focal Ratio: f/11
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| The
original fork mount, installed in the main dome 1985 - 2008 and seen through by thousands of people, when Grove Creek used to run public tours. This mount had no GOTO capability, only digital setting circles and upgraded stepping motors. |
The C14 now installed on
a Astro-Physics GTO-1200 mount in
the Middle Observatory, a fully remote internet controlled telescope. The C14 was moved to this mount in May 2008. See our Middle Observatory Web Page for full details. |
Click here to watch a video about our C14

Light Path through a
Schmidt Cassegrain Telescope
This is the most outstanding instrument at the Grove Creek Observatory. With a focal length of 3,910mm, 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 (with the original three paint scheme of white, grey and light blue tube). Its 36cm 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 was mounted on a home made 60kgs equatorial wedge, constructed from 23mm stainless steel plates. This was attached to our massive pier in the main dome, driven 6 metres into the ground and totally isolated with no part of the building touching it. The pier is 50cm in diameter and constructed with a solid steel core of 18cm 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 in July 1994, that were shown via a live satellite feed throughout the world on Australian and international TV, including CNN, the BBC and Channel 7. Well over 10,000 people viewed Halley's Comet through this telescope when it was installed at Grove Creek in 1985. Many professional and amateur astronomers that visited Grove Creek, when we used to run public tours, often commented on how amazing the optics of this telescope was.
In 1998, extensive electrical upgrades were made by Steven Williams and Christopher Ralph, 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. 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. The periodical error of the mount was only 8 arc seconds, which was remarkable, considering its age and that it was never designed for such a role. 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 in the late 60's! 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 from 2002 until 2008.
As Grove Creek closed to public tours in September, 2007, the C14 was able to be configured as a dedicated CCD imaging internet remote controlled instrument. Therefore, In May 2008, the C14 was removed from the dome and installed on a Astro-Physics GTO-1200 mount and pier, in our new robotic sliding roof Middle Observatory. This enabled us to put it online on the internet for everyone to use.
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Meade 30.5cm (12") LX-200 "Classic
Model":

Dedicated Photometric SBIG
ST-9XE CCD Internet remote controlled system
Focal Length = 1,770mm
Aperture = 300mm Focal Ratio = f/5.9
FOV: 19.9x19.9^min.
Image Scale=2.339^secs/pixel Bin1x1
We use the LX-200 12" for remote photometric CCD imaging. The 12" was upgraded in November 2007 after Prof. Tim Barker from Wheaton College very kindly donated it to Grove Creek. It was sitting in a box broken, left over from the Wheaton Internet Telescope Project after many problems with blown electronics, GOTO motors and a faulty secondary mirror holder. This is a totally re-built Meade 12" LX-200 - the electronics and software allow it to be "parked" (tracking turned off) without loosing position of the known sky and many other enhancements and upgrades have been made, to enable this to operate remotely over the internet. Still, however, it is probably the most difficult internet telescope to maintain due to the design of the original "classic" model GOTO motors, that still cause considerable problems and down-time. In October 2009, this telescope was moved to a new pier (donated by Greg Ford) into our Middle Observatory.
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Meade
25cm (10") LX-200 GPS Model.

Dedicated SBIG STL-1001E CCD Internet remote controlled
system
AP=250mm FL= 2,760mm FR=f/11.04
FOV=30.6^min square.
Array= 1024x1024 @ 24microns/pixel. Image Scale=1.79^sec/pixel
See our Wheaton Telescope
Web Page for further details
This telescope is installed in the Western Observatory at Grove Creek. Please go to our Wheaton Project Web Page for full details about this dedicated CCD remote internet telescope. This is the next model above the "classics" - and the GOTO motors are a lot more reliable and sturdy.
14"
Meade RCX-400 Telescope:

Currently under repair - Please go to our
Wheaton Project Web Page for details
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Meade 25cm (10") LX-200 "Classic" Model:

Aperture: 25.4cm (10") Focal Length: 2,000mm Focal Ratio: f/10
Mounted on the pier in the Main Dome on the
multi-use adaptor plate
This telescope is owned by Steven Williams and is used as a personal viewing instrument at Grove Creek, as most of the other telescopes are dedicated CCD imaging instruments only. This telescope is currently installed in the main dome and is a non-modified "classic" model. In January 2009, a special pier adaptor plate was installed to enable a LX-200 Wedge base, Paramount ME mount or a Astro-Physics Mount, as the previous C14 was moved into the Middle Observatory in May 2008. A CCD camera for personal use can be easily installed, operated from a PC in the control room (see right image).
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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. The equatorial mount shown is known as a "Samson Mount" are no longer made any more but used to be a very popular mount available from Astro Optical, in Sydney, Australia. Please note that despite the many offers we receive via email, this mount is NOT for sale at any price, as it has a suburb low periodical error and is owned by Jim Lynch.
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Pentax - 10cm (3.9") SDUF II f/4 APO
Astrograph:

Having won many astrophotography prizes at Grove Creek, 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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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. Projects are submitted by users in the astronomical community, where the resulting data is passed on over the internet for further study.

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. Both the Riometer and the Radio Telescope are projects run and owned by Andrew Mattingly and Greg Ford.
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