Grove Creek Observatory's Telescopes & Equipment:


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                      Short Summary of Telescopes at Grove Creek:

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           14" (36cm) Celestron f/10 or f/7 Schmidt Cassegrain (main viewing instrument)

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           14" (36cm) Meade RCX-400 f/8 GOTO Ritchey-Chrétien (Internet Telescope - SBIG STL-1001E CCD)

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           12" (30.5cm) Meade LX-200 f/10 GOTO Schmidt Cassegrain (Internet Telescope - SBIG ST8 CCD)

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           10" (25.4cm) Meade LX-200 f/10 GOTO Schmidt Cassegrain

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            8" (20.3cm) f/7 Newtonian German Equatorial or Dobson Mounted

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            4" (10cm) f/4 Pentax Astrograph mounted on a Astro-Physics 1200-GTO Mount  (Internet Telescope - SBIG ST8 CCD)

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            Jove Riometer

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            2.3m steerable dish Radio Telescope

THE CELESTRON C-14 SCHMIDT CASSEGRAIN:

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

Watch our video about our C14

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 piggy backed telescopes, with its Losmandy dovetail system. We have the best available eyepieces - including a full range of Tele Vue Naglars and a huge range of adaptors for astrophotography, rear-cell remote focusing and CCD imaging for this instrument. The telescope pier itself, is driven 6 metres (19.5 ft) into the ground and is totally isolated with no part of the building touching it and is 1metre (3.2 ft) in diameter and constructed with a solid steel core, filled with concrete, sealed with a large gas pipe on the outside. The mount's wedge is home made out of 2cm (3/4") thick stainless steel, that makes the C14 very stable. 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. Along with proper equatorial alignment of the telescope mount, the "timing pulses" of the RA stepping motor is very critical - as the earth rotates from west to east, the telescope has to track the stars as they pass overhead from east to west, otherwise the stars would quickly move out of the field of view and also cause the stars to "trail" in a long exposure photograph. 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 with encoders, was 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.

The new upgrades where very much being enjoyed by both staff and visitors, as it sped up finding objects ten fold - until 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 original drive system were no longer available, so it was replaced with a third-party versatile computerised duel stepping motor drive system (which was extensively programmed to work with the unique C14's stepping motors), enabling 7 different speeds to move the telescope, depending on the magnification selected and where the telescope was pointing (as a fork mount is moved further south near the celestial pole, it requires a faster RA speed to slew the telescope.)


The C-14's "brain" - The Argo Navis

A newer and very powerful Australian made Argo Navis digital setting circle computer, with RS2-232 planetarium control functions was then purchased from Wildcard Innovations. This amazing system guides the user to over 29,000 astronomical objects in its own database, using very high resolution 10,000 step optical encoders. It is very easy to learn and use. The Argo Navis can also interface with our PC in the control room, using Software Bisque's "The Sky" program which constantly updates the telescope's position on the computer screen with extreme accuracy - identifying any object being viewed and further allowing millions of objects to be found by a simple mouse click on the PC! The Argo Navis on the C14 then displays arrows, to guide the user to move the telescope manually and with the hand paddle, to any astronomical target. The Argo navis now supports TPAS™ - a telescope pointing analysis system, which measures, models, computes and analyses the very small various values of systematic fabrication errors in the C14 mount, which assists with improving the pointing accuracy performance of the C14 to as close as 5^mins - a very small part of "astronomical real estate". The Argo Navis can even give you an automatic electronic tour of the Southern Skies! For example, you can set the system to "show me all galaxies brighter than magnitude 12" and it will point the way for you, with one rotational click on the main dial! We now have two Argo Navis systems - the other one is installed on our 12" f/4 Newtonian. In our view, there is no better DSE (Digital Setting Circle) on the market and they are now used on many thousands of telescopes throughout the world.

With what the C14 has been through and with the new upgrades, it still remains a powerful telescope with stunning optics and user-friendliness. Under Grove Creek's wonderful night skies, it still out performs even larger telescopes that are coming out on the market (previous to 1990, it was the largest commercial telescope available in the world). Sure, it hasn't got the "GOTO" control like some of the modern systems but the vibration free fork mount beats the newer systems "hands down". As the old saying goes - "they don't make 'em like the used too" and the Celestron C14 is certainly a wonderful and very much valued instrument at the Grove Creek Observatory.


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.

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. Staff have Local LAN and remote internet access before midnight. After midnight, use of this internet telescope is provided for Wheaton College faculty and students only.

 Meade 25cm (10") and 30cm (12") LX-200 Schmidt Cassegrain Telescopes:
   

10": Aperture: 25.4cm (10") Focal Length: 2,000mm Focal Ratio: f/10
12": Aperture 30.5 (12") Focal Length: 2,500mm Focal Ratio: f/10

We use the LX-200 12" and 10" for remote CCD imaging. Staff are able to control these telescopes, operated over our Local Area Network to the comfort of the control room, 30m (100ft) east of the sliding roof observatory, where they are installed. 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.


CCD Imaging Setup on the LX-200 Telescopes

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.

Equatorial   Dobson ALT/AZ Mount
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.

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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