The Wendelstein Observatory
Universitäts-Sternwarte München / Observatorium Wendelstein|
Scheinerstr. 1, D-81679 München, Deutschland
Telefon +49-89-2180-6001 Telefax +49-89-2180-6003
Wendelsteingipfel, D-83735 Bayrischzell, Deutschland
Telefon +49-08023-8198-0 Telefax +49-08023-8198-29
The Wendelstein Observatory is situated on the summit of Mount
Wendelstein, a prominent, 1838 m high mountain in the bavarian Alpes.
It is operated by the University Observatory of the University of Munich.
University Observatory Munich
Telephone (0049 8023) 81980
Fax (0049 8023) 819829
||47o 42' 13.1" North
||12o 00' 43.4" East
Only 75 km south-east of Munich, after one hour care drive this site can
easily be reached via cable car (8 min) or by means of a cog rail road
(25 min.). Final access to the very top is achieved by an elevator
climbing up 100 m within the mountain. The observatory was first installed
to survey the solar activity. In the mid-1980, it was redirected to night
observations of stars and galaxies, but it still owns a
20 cm Zeiss solar coronograph.
Nowadays, the coronograph is used only for eduction and public outreach.
For first the night time activites, an 80 cm DFM-telescope
was installed which was operated until spring 2008 for scientific observing
programs every clear night. It was equipped with high-tech focal
instruments like high-speed multichannel photometers or a direct
imaging CCD-Camera. This instrumentation has often been involved
in international observing programs since. The scientific focussed
started with stars, especially binary stars. Later on, galaxies were added.
In 2007, a 40 cm telescope
was installed to bridge the gap for the students lab until
a 2 m telescope
took over on the old site of the 80 cm telescope. The pier and dome of
the 80 cm telescope have been demolished and replaced by a new building
with an 8.5m Baader dome (2010).
The new 2 m telescope was installed shortly before chrismas
2011 and went into regular observations mid 2013. It offers up to
four instruments. The science focus ranges from exo-solar planets, star
formation regions, nearby galaxies towards distant cluster of galaxies.
Its observing program reflects the scientific topics of the astronomer
groups at the university observatory
of the faculty of physics which is part of the Ludwig-Maximilians-University in Munich.
In 2016, the 40 cm telescope was shipped to the Munich host institute and
a 43 cm Planewave astrograph was mounted in the 3.2m Baader dome. The new
instrument continues the student lab support and offers a wider field of
The weather conditions at Wendelstein are highly seasonal with
sometimes more than 1m of snow in winter time and decent warmth in
summer. But cold weather may occur at any time of the year.
Above the clouds at sunset
Compared to other sites in Germany the meteorological conditions at
Wendelstein have turned out to be fairly good. During typical years
about 120 nights with less than 2/8 cloud cover can be used for
astronomical observations. Extremely dark nights often occur in
autumn when the upper cloud layers may reach altitudes of 1500 - 1800
m thus preventing light pollution by some nearby small villages. Seeing conditions have been studied
in April through December 1998 using a copy of the ESO Paranal Seeing
Monitor kindly made available by ESO. (e.g. ESO La Silla and Paranal
Telescope and Instrumentation:
The 2 m m Fraunhofer telescope
The telescope was installed during the second half of 2011 by Kayser-Threde GmbH (München, meanwhile
OHB Systems Wessling bei München)
Astelco System GmbH (Martinsried). A
8.5 m diameter dome of
Baader Planetarium (Mammendorf)
protects the telecope again bad weather conditions. The three mirrors of
the telecope were produced by Lytkarino Opical Glass Factory (LZOS, Moskau). Its control system was designed and
produced by tau-tec GmbH Tübingen entwickelt.
. Instruments were build at the university observatory in Munich.
The telecope has a compact Ritchey-Chrétien design with a free aperture
of 2.0 meters and a focal ratio of f/7.8. The incoming light is redirected
by a movable third plane mirror to one of the two Nasmyth-focal stations.
At those stations, scientific equipment of up to 350 kg and a flat field of
view of up to über 0.7 degree can be mounted. One station operates
an optical CCD-based wide field imager making full use of this large field of
view , the other one supports some field of view instruments without additional
lens systems. The telescope can be opearted remotely.
The scientific instruments build at the host institute in Munich:
- WWFI, (operational since July 2013)
- 3KK, (operational since January 2016)
- VIRUS-W, (on loan to the 2.7 McDonald teleskop)
- FOCES (in commissioning).
Wendelstein 2 m Fraunhofer telescope dbuild by Kayser-Threde (München)
and Astelco (Martinsried)
equipped with the wide field CCD camera WWFI (left) and the optical-near-infrared 3-chanal-camera (right).
Exposure of the spiral galaxy NGC 891 (Andromeda)
taken with the Wendelstein 2 m Fraunhofer Teleskops
and its WWFI camera. Individual exposures in
u′, g′, und r′ filters were
combied to a so-called true-color image. NGC 891 resembles our
own Milky Way galaxy in size and structure and is about 30 Mio.
Shortly before end of the years 2013 to 2017, pseudo thrue color images of
nice astronomical objects were produced. They are based on data taken
with the 2m Fraunhofer telescope and its wide field CCD camera WWFI.
2013, the neighboring spiral galaxy M33 (far left) was selected. In 2014,
a portrait of the Perseus cluster of galaxies (2nd from left) was published.
2015 followed a picture of the galaxies M65 and M66 which are central in a
small group of galaxies (3th from left). In 2016, we produced an image
of the great Orion nebula M42 (4th from left). 2017, the pair of interacting
galaxies M51(=NGC5194) and NGC5195 was selected (far right). The newest picture
in this series by end of 2018 is at top under
Aktuelles (german web page).
Technically, the images are produced in the same manner as the on for NGC891,
but for all images, the full field of view of WWFI is used (corresponding
to the full moon diameter). Click on the images for higher resolution.
43 cm Teleskop
Since 2017, a CDK17-Planewave telescope with a corrector for 0.75 degree field
of view is operated in the small 3.2 m Baader dome and a CCD camera for
imaging is mounted. The telescope is designed as a Dall-Kirkham astrograph.
The telecope can be controlled remotely. Besides its imaging capability, it
can also serve a small spectrograph for student lab work.
Technically, the images are produced in the same manner as WWFI frame for NGC891. Click on the images for higher resolution and larger size.
|Wendelstein 40 cm Planewave telescope (rotating dome during
night time - picture by M. Kluge
||Total lunar eclipe 27.7.2018 as observed with the 40cm Planewave at Wendelstein. SBIG CCD camera with g, r, and i filters.
Observer: M. Schmidt, datareduction: C. Goessl.
|| The great Orion nebula M42 as observed with the Wendelsteinn 40cm Planewave through filters g, r, L, i, <[OIII]>and Halpha (Data reduction Ch. Obermeier).
Done in the course of the student lab.
||Supernova remnant 'cygnus loop' (also known under 'Cirrus nebula' or 'Veil nebula') taken with the Planewave astrograph at Wendelstein and g, r, L, andHalpha
filters (data reduction by Chr. Obermeier). The picture shows only a cut-off of the full data set (extend roughly 3 by 2 degree).
20 cm Coronograph
A special 20 cm refracor, built by Zeiss-Oberkochen, was used until 1988 to
observe the activity of the sun in white
light, Haplha, and spectra. On can place
special light stops (the so-called coronographic design which
produces artificial solar eclipses) into the telecope light path
allowing to observe the solar
atmosphere under excellent atmospheric conditions. The telescope
is still used for public outreach and student eduction.
Solar activity data taken at Wendelstein have been digitzed for the years
1947 to 1982 and are availabel from the
Solar Data Services of the National Geophysical Data Center
20 cm Coronograph and solar protuberances
The telescopes at Wendelstein support the science topics of the astronomers
of the university observatory in Munich which range from the exo-solar planets towards distant cluster of galaxies.
Results can be found in the publication list of the observatory, which also includes the results of student work
(OhD, master/diploma, bachelor). The telscopes also support the education of
the Munich students.
(in German, many pictures)