Ankara University Kreiken Observatory
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The Ankara University Observatory (AUG) (), is a ground-based astronomical observatory operated by the Astronomy and Space Sciences Department at
Ankara University Ankara University () is a public university, public research university in Ankara, the capital of Turkey. It was the first higher education institution founded in Turkey after the History of the Republic of Turkey, formation of the Turkish republ ...
's Faculty of Science. Established in 1959 by
Dutch Dutch or Nederlands commonly refers to: * Something of, from, or related to the Netherlands ** Dutch people as an ethnic group () ** Dutch nationality law, history and regulations of Dutch citizenship () ** Dutch language () * In specific terms, i ...
astronomer
Egbert Adriaan Kreiken Egbert Adriaan Kreiken (1 November 1896, Barneveld, Gelderland – 16 August 1964) was a Dutch teacher and astronomer. He was born at Barneveld in the Netherlands, to a family of teachers. After being awarded his Ph.D. in 1923, he would ...
in Ahlatlıbel,
Ankara Ankara is the capital city of Turkey and List of national capitals by area, the largest capital by area in the world. Located in the Central Anatolia Region, central part of Anatolia, the city has a population of 5,290,822 in its urban center ( ...
. Currently, it consists of nine
optical telescope An optical telescope gathers and focus (optics), focuses light mainly from the visible spectrum, visible part of the electromagnetic spectrum, to create a magnification, magnified image for direct visual inspection, to make a photograph, or to co ...
s and a
radio telescope A radio telescope is a specialized antenna (radio), antenna and radio receiver used to detect radio waves from astronomical radio sources in the sky. Radio telescopes are the main observing instrument used in radio astronomy, which studies the r ...
, which is currently taken out of service. Old instruments are displayed in a museum at the observatory.


History

Ankara University's Faculty of Science decided in 1954 to establish an observatory to begin with astronomical studies. Ahlatlıbel in
Gölbaşı, Ankara Gölbaşı is a municipality and Districts of Turkey, district of Ankara Province, Turkey. Its area is 1,364 km2, and its population is 150,047 (2022). It is south of the city of Ankara. Its elevation is . The district includes the Lake Moga ...
was chosen as the ideal site, a location with dark skies far from the city's downtown to avoid the effects of
light pollution Light pollution is the presence of any unwanted, inappropriate, or excessive artificial Visible spectrum, lighting. In a descriptive sense, the term ''light pollution'' refers to the effects of any poorly implemented lighting sources, during the ...
, having an average 300 clear nights per year and also offering easy transportation from the campus. It is situated south of Ankara at an altitude of . Groundbreaking of the main building and the three domes took place in 1959. The observatory was officially inaugurated on August 26, 1963, accompanied by an international astronomy conference. The scientific studies were carried out in the beginning with a radio telescope produced by the Dutch PTT, a 5 cm
astrograph An astrograph (or astrographic camera) is a telescope designed for the sole purpose of astrophotography. Astrographs are mostly used in wide-field astronomical surveys of the sky and for detection of objects such as asteroids, meteors, an ...
, a 15 cm
Coudé A reflecting telescope (also called a reflector) is a telescope that uses a single or a combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century by Isaac Newton as an alternati ...
telescope of
Zeiss Zeiss or Zeiß may refer to: People *Carl Zeiss (1816–1888), German optician and entrepreneur *Emil Zeiß (1833–1910), German Protestant minister and painter * Juan Pablo Zeiss (born 1989), Argentine rugby union player * Mary Zeiss Sta ...
from Germany for solar observations, a Hilger and Watts microphotometer and a Cuffey Iris
photometer A photometer is an instrument that measures the strength of electromagnetic radiation in the range from ultraviolet to infrared and including the visible spectrum. Most photometers convert light into an electric current using a photoresistor, ...
.


Facilities


Telescopes

;T40 Kreiken telescope * Diameter: 406 mm (16") * Focal ratio: f/10 * Focal length: 4,000 mm * Image scale: 51 arcsec/mm * Producer:
Meade Instruments Meade Instruments Corporation (also shortened to Meade) was an American multinational corporation, multinational company (law), company headquartered in Watsonville, California, that manufactured, imported and distributed telescopes, binoculars, ...
Corp., California, USA * Focal plane instruments: Apogee ALTA U47+ CCD camera, 1024x1024 13 micron pixels E2V CCD47-10 back illuminated ccd chip, PC based data acquisition via USB 2.0 port, OPTEC IFW filter wheel (PC controlled), Johnson UBVRI – Strömgren uvbyHbeta – RGB filters, various eye-pieces. Named after Egbert Adriaan Kreiken, the founder of the observatory, it is used in general for
photoelectric The photoelectric effect is the emission of electrons from a material caused by electromagnetic radiation such as ultraviolet light. Electrons emitted in this manner are called photoelectrons. The phenomenon is studied in condensed matter physic ...
photometry Photometry can refer to: * Photometry (optics), the science of measurement of visible light in terms of its perceived brightness to human vision * Photometry (astronomy), the measurement of the flux or intensity of an astronomical object's electr ...
observations on eclipsing
binary star A binary star or binary star system is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars in the night sky that are seen as a single object to the naked eye are often resolved as separate stars us ...
s and
variable star A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes systematically with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are ...
s. ;T35 telescope * Diameter: 356 mm (14") * Focal ratio: f/10 * Focal length: 3,556 mm * Image scale: 58 arcsec/mm * Producer: Meade Instruments * Focal plane instruments : Apogee ALTA U47+ CCD camera, 1024x1024 13 micron pixels E2V CCD47-10 back illuminated ccd chip, PC based data acquisition via USB 2.0 port, OPTEC IFW filter wheel (PC controlled), Johnson UBVRI – Strömgren uvbyHbeta – RGB filters, various eye-pieces. Installed in the former Maksutov Dome ın 2011, the 356mm telescope is used for observation on binary stars and photoelectric effects of variable stars. ;T30
Maksutov telescope 250px, A 150mm aperture Maksutov–Cassegrain telescope The Maksutov (also called a "Mak") is a catadioptric telescope design that combines a spherical mirror with a weakly negative meniscus lens in a design that takes advantage of all the sur ...
* Diameter: 300 mm * Focal ratio: f/16 * Focal length: 4,800 mm * Image scale: 43 arcsec/mm * Producer : E. Popp Tele-Optik, Zurich, Switzerland * Focal plane instruments: Optec SSP-5A single channel photoelectric photometer, (containing a Hamamatsu R1414 phototube), standard 1 mm diaphragm, Johnson UBV filters, motorized filter slider, 80386 PC based data acquisition. 300mm telescope for observation on binary stars and photoelectric effects of variable stars. ;T15 Coudé telescope * Diameter: 150 mm * Focal ratio: f/15 * Focal length: 2,250 mm * Image scale: 92 arcsec/mm * Producer: ZEISS-Oberkochen, Württemberg, Germany * Focal plane instruments: Solar projection lens and screen for Sun spot observations, Contarex photo camera, Lyott H-alpha monochromator, various filters and eye-pieces. 150mm telescope of type
Coudé A reflecting telescope (also called a reflector) is a telescope that uses a single or a combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century by Isaac Newton as an alternati ...
is used for scientific observation of
sun spot Sun SPOT (Sun Small Programmable Object Technology) was a sensor node for a wireless sensor network developed by Sun Microsystems announced in 2007. The device used the IEEE 802.15.4 standard for its networking, and unlike other available sen ...
s. Popular and educational public sessions are held also at this telescope. ;Other telescopes For popular and educational activities open to public: ;
Meade LX200 The Meade LX200 is a family of commercial telescopes produced by Meade Instruments launched in 1992 with 8" (20.32 cm) and a 10" (25.4 cm) Schmidt–Cassegrain models on computerized altazimuth mounts. Two larger models, a 12" (30.4 ...
8" * Diameter: 203 mm (8") * Focal ratio: f/10 * Focal length: 2,000 mm * Producer: Meade Instruments Corp., California ; Meade ETX-125 5" * Diameter: 127 mm (5") * Focal ratio: f/15 * Focal length: 1,900 mm * Image scale: 108 arcsec/mm * Producer: Meade Instruments * Focal plane instruments : DSI-2 Color CCD camera ;TAD Bresser RB-60 (Two pieces) * Diameter: 60 mm * Focal length: 700 mm * Producer: Meade Instruments ;Bresser Mars Explorer ST-70 * Diameter: 70 * Focal ratio: f/10 * Focal length: 700 *Producer: Meade Instruments ;Radio telescope The radio telescope is not in use anymore.


Meteorological station

There is a
meteorological station A weather station is a facility, either on land or sea, with instruments and equipment for measuring atmospheric conditions to provide information for weather forecasts and to study the weather and climate. The measurements taken include tempera ...
for observing atmospheric conditions such as temperature, humidity, barometric pressure, wind speed and wind direction as well as precipitation amounts. The gathered data is published also on the internet every five minutes.


Transportation

The observatory is in Ahlatlıbel on İncek Blvd., at a distance of from Or-An Bridge (
Konya Konya is a major city in central Turkey, on the southwestern edge of the Central Anatolian Plateau, and is the capital of Konya Province. During antiquity and into Seljuk times it was known as Iconium. In 19th-century accounts of the city in En ...
Road) and can be reached by public transportation: * From Güvenpark in
Kızılay, Ankara Kızılay is the city center of Ankara Province in the municipality and district of Çankaya District, Çankaya, Turkey.Ulus, Ankara Ulus is a quarter in Ankara, Turkey and is located at the center of the capital city. It was once the heart of old Ankara. The name means "tribe, nation" in Turkish language, Turkish. It is now a predominantly a commercial and tourist area made ...
with
Dolmuş In Turkey and Northern Cyprus, a () is a share taxi that runs set routes within and between cities. Background The name is derived from Turkish language, Turkish for "seemingly stuffed", in reference to how the vehicles were often filled to the ...


References

{{reflist Astronomical observatories in Turkey
Observatory An observatory is a location used for observing terrestrial, marine, or celestial events. Astronomy, climatology/meteorology, geophysics, oceanography and volcanology are examples of disciplines for which observatories have been constructed. Th ...
Buildings and structures in Ankara Province 1963 establishments in Turkey Radio telescopes University and college astronomical observatories