The Observatory

My observatory is located at 33° 59' 50" N, 117° 33' 47" E at an elevation of 1,600 feet. I named the observatory Santana in honor of the 40 - 70 mph Santana winds that blow through the area several times a year.

The Completed ObservatoryUnder the theory that telescopes are a compromise that you look through, this observatory is a compromise that gets used - up to 100 nights a year.  It is in the worst possible place, the middle of a light polluted city, yet the best possible place, off my family room next to the big screen T.V. It is designed to operate automatically. I just have to go through a start-up routine and load that night's observing run.  The results have to be monitored several times during the night for focus and pointing accuracy, a process that only takes a few minutes.

The observatory itself started out life as a 12' by 12' patio enclosure built by a local contractor. The walls are 2-1/2" foam with hard siding on each side, which stand 8' to 10' high. The roof is 3" foam with metal facing. As such, the structure met all local building codes and sailed through the Planning Committee of Rancho Cucamonga - one of the toughest cities in Southern California.

Stephens1_small.jpg (20070 bytes)Through pre-arrangement with the builder, the roof was attached with only 4 screws. Let the modifications begin!

Besides missing the fact the roof was only held on by 4 screws, the inspectors didn't see the 14" square hole cut in the concrete pad into which I eventually dumped 600 lbs. of concrete on which to mount the pier. The pier's foundation is insulated from the house foundation and the pier was filled with sand and oil to further dampen vibration.

Kurt Sutton, also a member of the Riverside Astronomical Society, helped me build the rolling mechanism that allows the roof to roll aside onto the top of a pre-existing patio cover. The roof rolls on 10 ball-bearing wheels locked in opposite facing aluminum C-channel tracks. Eight more wheels keep it in place laterally. This mechanism slides so smoothly that I can open it with one finger.

One over-riding criteria was that the roof had to hold up to the 40 - 70 mph Santana winds that rip through the area in the Fall.  I didn't want my observatory to be featured in some remake of the Wizard of Oz! These winds are strong enough to tip over semi-trailers and can quickly shred a roof of poorly attached tile or single. I attached tie-downs as a sanity check and can report that the roof has stood up to the strongest of gusts - and I have even imaged during lesser winds with good results.

The Telescope

The telescope is a Celestron C11 on a Losmandy CG11 mount. The mount's electronic package was removed and retrofitted with a SkyWalker GOTO drive system manufactured by Astrometric Instruments.

The telescope has sprouted an electronic focuser made by Lumicon that is controllable from the computer inside the house.  It also has a 80mm finder with a .4 lux video camera sold by SuperCircuits. This camera feeds a live image to a small 5" black and white television mounted next to the computers. With this system, I can see 8th magnitude stars which greatly assists in the alignment process.

I can image at the telescope's normal F/10 - 110" focal length or at F/6.3 using a focal reducer manufactured by Celestron.   I also can image at F/5 or F/3.3 using special focal reducers manufactured by Optec, Inc. 

This telescope has been temporarily pushed aside in favor of a Celestron C14 on a Paramount mount.  That telescope is residing in the back of the observatory while it is being tested and awaiting the construction of an observatory at the Riverside Astronomical Society’s observing site in Landers, California.

Filters

Wanting to be able to do tri-color imaging as well as photometry, I mounted Optec's MAXfilter 2" automatic filter selector.  This filter slider allows for the extra large filters needed for their F/5 or F/3.3 focal reducers. 

I purchase two filter holders.  In one I mounted the standard Tri-Color RBG filter set.  In the other, I have mounted a Johnson B filter and a Johnson V filter in order to due photometry.

The CCD Camera

Previously hanging off the back end of this is an SBIG ST-9e made by Santa Barbara Instruments Group. At my location, the CCD camera can usually reach 17th magnitude when the Full Moon is in the sky, and can reach 18.5 magnitude under good conditions. Recently, I acquired an SBIG ST-9e.  Its primary benefit is the larger chip size that allows me to operate at a longer focal length while keeping the same field of view.

Software

The telescope is operating using Astrometric Instruments' SkyGuide software. This software controls the basic functions of pointing and slewing the telescope as well as focusing the camera. To provide a more robust database of objects including any asteroid, for which an orbit has been determined, I use Software Bisque's TheSky software using its LX200 interface to talk to SkyGuide.

Brian Warner's MPO Connections is used to control the CCD camera and to provide a software script to run an automated observing run.

I use Brian Warner's Canopus to analyze asteroid photometric data and to do astrometric measurements of asteroid positions.

Computers

Two computers networked together control the observatory. One, a 166 MHz, runs SkyGuide and talks to the telescope. The other, a 450 MHz, runs TheSky, CCDSoft, MPO Connections, and Canopus.

 

email: rstephens@foxandstephens.com