Astronomy - February 2014

(John Hannent) #1
62 ASTRONOMY t FEBRUARY 2014

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THE TRUMPLER


classes of clusters


SKYGAZING


F


rom earliest times, observers
have gazed at loose collections of
stars, grouping them into amor-
phous forms that they correctly
assumed were moving through
space together. But no organization of these
objects existed until one meticulous astron-
omer imposed his classification scheme

upon them. Who he was and what he
accomplished makes a fascinating sidebar
— and a fun observing project — for
today’s amateur astronomers.

The man behind the plan
Robert Julius Trumpler was born in Zurich
on October 2, 1886, the third in a family of
10 children. At age 12, he took the competi-
tive examination for entrance to the Gym-
nasium (high school) and was first in his
class. His interest in astronomy began when

he heard a classmate speak about the origin
of the solar system.
Trumpler entered the University of
Zurich to study astronomy in 1906. Two
years later, he started advanced work at the
University of Göttingen, where he received
his Ph.D. in 1910.
At the meeting of the Astronomische
Gesellschaft in Hamburg in 1913, Trumpler
met Frank Schlesinger, director of the
Allegheny Observatory in Pittsburgh. They
discussed a program for determining the

Since 1930, astronomers have divided the thousands of open
clusters into 36 types. Find out what makes them diferent.
text by Michael E. Bakich; images by Bernhard Hubl

Michael E. Bakich is a senior editor of Astron-
omy. Bernhard Hubl is a highly accredited
astroimager who lives in Schlierbach, Austria.

NGC 6791 has a Trumpler classification of II3r. That means it’s a cluster that stands out against the background, shows a bit of central condensation, contains
both bright and faint stars, and ranks as a rich cluster with more than 100 suns.
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