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Transferral of the Refurbished Primary Mirror to the BTA Dome

On May 18, the renovated primary mirror was transferred to the BTA cupola. Before this event in the first half of May, the mounting supports of the former mirror were deinstalled, and on May 16 it was demounted from the telescope. During May 17, preparatory works were carried out, in particular: the old mirror was washed in the specialized washing chamber and prepared for transportation to the container outside the dome.

Under the supervision of two highly-experienced SAO staff members: the leading engineers of the BTA technical-support team (BTA TST) Yu.M. Mametiev and A.M. Pritychenko, the immensely complicated work on swapping the mirrors was conducted. The works began at 7 a.m. in order to use as much as possible the favorable "weather window" in a rainy season typical of this region. The former mirror that had worked at the telescope for 40 years was loaded to the container though the shutter of the cupola, then the refurbished one was transferred to the dome, put on the frame, and fitted into the centering sleeve. The whole procedure took us about nine hours. The mirror was installed at a specified position in the frame at the first attempt. The mirrors' weight is greater than 40 tons each; they were transferred using the crane with a lifting capacity of 100 tons able to move above the telescope cupola along the rail track. Most of the time was taken by lifting and installing extremely heavy glass mirrors at a specified position with maximum accuracy and safety. The replacement was "open", i.e., the mirrors were carried without containers which allowed us to save time needed for loading works.

The crane was once used in Lytkarino in 2007 before transportation of the mirror and after its arrival to the observatory in February this year; however, at that time the mirror should be lifted to a small height in order to take it from the vehicle platform. For reference, its transferral to the telescope dome, as well as the whole process of the mirror replacement itself, was last time performed in 1979. As distinguished from the past years, now the operator's cabin was equipped not only with the two-way communication but also with the video broadcast from the dome.

The following was told by Yury Yu. Balega, the SAO RAS scientific supervisor, the first vice-president of RAS, the former SAO RAS director from 1993 till 2015, and primary initiator and organizer of mirror reconstruction works: "In 2003, an idea has started up to replace the 6-m mirror for an 8-m one. In the workshop of the SCHOTT Company in Mainz (Germany), a cast workpiece, the copy of the VLT (Very Large Telescope) mirrors, was kept. I had several trips to Mainz for negotiations. The cost of works on the mirror replacement was six million euros. Besides the fact that the 8-m mirror is much bigger than the 6-m one, it also has a shorter focal length, thus, the whole BTA telescope should have been reconstructed.

In 2006 at a meeting, at which the participants besides me were: Yu.S. Osipov (the president of RAS), A.A. Boyarchuk (the member of the Academy of Sciences) and A.F. Andreev (the member of the Academy of Sciences and acting secretary of general physics and astronomy department of RAS), it was decided that the original BTA mirror should be repolished. In the federal budget of Russia, there was a separate line for a sum of 159 million rubles. The mirror was transported to the Lytkarino factory in 2007. Unfortunately, the budget was sequestered and the sum was reduced to 90 million rubles. Due to underfunding, the works at the Lytkarino Optical Glass Factory extended over 10 years. At the last stage of reconstruction, the Federal Agency for Scientific Organizations (FASO Russia) allocated money in two tranches by 50 million rubles to complete works.

The main problem about the primary mirror operating from 1979 was in the fact that the considerable part of its surface (about 40%) was damaged owing to numerous coatings with aluminum. These damaged areas of the mirror scattered the light rather than concentrated it in the focus. The quality of the original mirror installed on a telescope in 1975 and used until 1979 was extremely low due to the fact that during the figuring in the 1970s, a polishing machine made large dishings on it around bubbles that opened when forming a surface. The first four years of working with this mirror, we had to shield these areas with opaque dark screens. Then, in 1979, SAO received the second mirror.

It was decided at the factory to cut off the 8-mm upper layer of glass from the working surface of the mirror. This allowed them to remove the areas of large air bubbles. Then the process of shaping the "rotation parabola" and polishing began. The surface's shape was controlled in the workshop by means of a special interferometer. For this purpose, the mirror was placed in a vertical position, and the control was performed at the horizontal section of the optical path. The surface roughness of the mirror was raised to 15-20 nanometers. This corresponds to the surface quality of the best mirrors in the world. Although, the problem of the general shape of the mirror remains unsolved. It can be solved only after its installation on a telescope. For this purpose, the telescope with the renovated mirror will be guided to a point source of light - a star - and from the images obtained with the help of the Shack-Hartmann wavefront sensor, the deviation of the surface from the specified shape will be determined. The supporting mechanisms on which the mirror lies will be each time adjusted from these images. The process of adjusting and forming the mirror surface can take us several months.

The new mirror will provide reducing the scattered color background in images of stars and galaxies. For astronomers, this means an advantage in the limiting magnitude of the telescope by about 0.5-1 magnitude. Scientists will be able to look into the depths of the Universe at a distance of twice as much as with the old mirror."

The next stage of the work involves adjusting the supports of the mirror to a new weight (as a result of the mirror repolishing, it became lighter by 800 kilograms) and installing them in the specialized holes at the bottom of the mirror. The adjustment of supports is a very difficult task - it takes a whole working day to adjust three pieces, and there are sixty of them. The supporting mechanism is designed to support a part of weight of the primary mirror (1/60 of weight or about 700 kg). Each mechanism combines the axial and radial supports which transmit load to the mirror varying depending on the position of the telescope tube. Installation of supports is planned to be completed in the second half of June.

Photo: Philippova E.A., Sholukhova O.N., Oborina N.A.

Commencement of Works on Replacing the Primary Mirror of the 6-m BTA Telescope

On May 3, 2018, the final stage of the project of the mirror replacement at the 6-m BTA telescope - installation of the refurbished mirror - has started.

Let us recall that the intention to replace the mirror arose in 2004, when it turned out that the quality of the operating mirror surface (used from 1979) had gradually degraded from multiple applications of fresh reflective layers which had been done every five years on average. At that time, it was decided to refurbish the original mirror which had been used from 1975 to 1979, although, due to a number of defects had been replaced and in storage for a long time in a specialized container near the BTA cupola. Expert reviews have shown that with the use of new instruments, the top layer of the mirror could be removed and the surface could be repolished. Then the reconstructed original BTA mirror should not only achieve the necessary performance but also can surpass the quality of the currently working one. The works within the project started in 2007, when the mirror was transported to the Lytkarino Optical Glass Factory (https://www.sao.ru/hq/sekbta/GZ_1/GZ_1.html). On February 14, 2018 the refurbished mirror was back at the observatory (https://www.sao.ru/Doc-en/Events/2018/Mirror/index.php). Works on its installation were planned for early May, as the procedure can be carried out only in summer under favorable temperature conditions.

Despite the identity of the original and current mirrors and simplicity of the phrase "replacement of the mirror", the installation procedure is far from a simple swapping of one part for another due to its complexity. The works would require demounting the current mirror, its unloading and then loading the renovated mirror through the shutter of the BTA dome, recalibrating 60 mechanical mounting supports on which the mirror lies in the frame, putting the reflecting coating with the specialized vacuum instrument in the BTA dome, conducting high-accuracy measurements of the quality of the surface, and precise adjustment of the mirror and telescope, then realignment of its mechanical components, as the weight and focal length of the refurbished mirror has changed due to skimming. To a great extent, the fate of the whole project will depend on successful fulfillment of the above tasks, because despite calculations, numerous measurements, and control of the surface in the workshop at the factory, the final result can be seen only after the telescope is put into operation.

The works will continue throughout the summer. Main operations are performed by the BTA operation personnel with the involvement of specialists from the Lytkarino Optical Glass Factory. At the present time, the mounting supports are being deinstalled from the frame of the mirror. The unloading of the current mirror and loading of the renovated in the dome are planned for the second half of May; the exact date will be defined more precisely depending on progress of works and weather conditions.

Photo: deinstallation of the mounting support of the BTA primary mirror.

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Last update: 24/05/2018