Max Planck Institute for Astronomy - Annual Report 2005
Max Planck Institute for Astronomy - Annual Report 2005
Max Planck Institute for Astronomy - Annual Report 2005
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136 V. People and Events<br />
Lemke: I was just as interested in the astronomical<br />
problems. Elsässer had worked on zodiacal light and now<br />
wanted to observe it in the infrared and mid-UV range<br />
as well. The long-term objective was the separation of<br />
the zodiacal light from other components of the night<br />
sky brightness, and tHibse was to contribute to this. It<br />
was absolutely fascinating <strong>for</strong> me to observe the glowing<br />
gaseous nebulae, such as the Orion Nebula, with groundbased<br />
telescopes in the infrared range and to detect embedded<br />
point sources in addition to the huge extensive<br />
emission. At that time, the observation of star <strong>for</strong>mation<br />
in gas and dust clouds actually started. Today this is one<br />
of the main research fields at the MPIA.<br />
All this still took place at the Landessternwarte. How<br />
do you remember the establishment of the MPIA?<br />
Lemke: Elsässer had hired me on February 1st, 1969,<br />
together with seven more colleagues, including Thorsten<br />
Neckel, Joachim Hermann, Josef Solf, Elsässer’s secretary<br />
Traudl Filsinger as well as Bodo Schwarze, Wolfgang<br />
Hormuth, and Franz Pihale from the workshops. At that<br />
time, the <strong>Institute</strong> consisted of nine persons. In the beginning,<br />
some of the MPIA staff worked in a hut on the<br />
grounds of the Landessternwarte, and in 1975 we finally<br />
moved into the new building.<br />
The development of helios ran parallel to this.<br />
Leinert: The German participation in this space probe<br />
was the result of a meeting between the German<br />
Chancellor Ludwig Erhard and the U.S. President Lyndon<br />
B. Johnson in 1965. The question as to which kind of<br />
instruments should be contributed by Germany was<br />
entrusted to Ludwig Biermann, the most renowned<br />
German astronomer at the time. Naturally he suggested<br />
studying the solar winds he himself had discovered, but<br />
also interplanetary dust. He regarded Hans Elsässer as the<br />
Fig. V.13.3: Christoph Leinert and Dietrich Lemke at the end of<br />
the festive colloquium.<br />
specialist in this field, who then received the zodiacallight<br />
photometer project (first at the Landessternwarte,<br />
later at the MPIA).<br />
It was Germany’s first participation in an interplanetary<br />
space probe, and technologically, at least one double<br />
step <strong>for</strong>ward – there<strong>for</strong>e meaning new territory <strong>for</strong> all<br />
of us. It was a young project pursued in many areas by<br />
professional novices with great enthusiasm. I was made<br />
P.I. (Principal Investigator) <strong>for</strong> the photometer, although<br />
I didn’t even have my PhD then. It was a project worth<br />
millions – something like that would be unthinkable<br />
today. But it was another time then – in many respects.<br />
For instance, it was not so important to publish anything<br />
– only if the work on the project was proceeding well.<br />
Five years after I recieved my PhD, I still had not published<br />
a paper in a refereed journal. Can you imagine that?<br />
Technically, our instrument was state-of-the-art and very<br />
successful. We used carbon fiber material <strong>for</strong> the first<br />
time in space astronomy then.<br />
What is your present-day view of the decisions<br />
Elsässer made at that time?<br />
Leinert: With the participation in Helios, Elsässer<br />
received a great deal of funding and was able to attract<br />
PhD students to the <strong>Institute</strong>. This certainly was important<br />
<strong>for</strong> the development of the MPIA. But at the time, he<br />
very swiftly rejected participation in successor projects<br />
without consulting us, although ulysses – a space probe<br />
flying above the poles of the sun – would have been an interesting<br />
opportunity. In his opinion, the scientific problem<br />
had essentially been solved with Helios, or at least was no<br />
longer a suitable main field of research <strong>for</strong> the <strong>Institute</strong>.