| Nomination Letters
November 29, 1963
Dr. Albert E. Whitford, Director
Lick Observatory
Mount Hamilton, California
Dear Albert:
I am writing as a member of the Vetlesen Award Committee
of Columbia University to ask for your advice in connection
with the award of the Vetlesen Prize in 1964.
The Vetlesen Prize, first awarded in 1960, was established
by the G. Unger Vetlesen Foundation as an award "for
outstanding achievement in the sciences resulting in a clear
understanding of the earth, its history or its relation to
the universe". The Foundation was formed in 1955 by
the late George Unger Vetlesen who was president and chairman
of the Norwegian-American Line Agency, Inc. and one of the
founders of the Scandinavian Airline System, Inc.
The Award is to be made every two years provided a worthy
candidate in the opinion of the Award Committee is presented.
Any person in any country may be nominated for the prize.
It is the intention of the foundation, which asked Columbia
University to administer the Award, that the prize shall
rank in dignity and significance with others that now recognize
the achievements of the world's leading scholars and scientists
in other fields. In terms of material reward, the Vetlesen
Prize consists of a gold medal, a sum of $25,000, and support
for the publication of the recipient's papers.
The recipient of the Vetlesen Prize in 1960 was Dr. Maurice
Ewing. In 1962 Professor H. Jeffreys and Professor F. A. Vening
Meinesz shared the Prize.
Although it is expected that the Prize will normally be awarded
for research in the fields of the Earth Sciences it can also
be awarded for research in Astronomy.
To me it would seem that Professor J. H. Oort is eminently
qualified for the reward. His work on the structure and dynamics
of our galaxy, on the properties of interstellar matter and
on the origin of comets is an outstanding contribution, and
one that in my opinion contains results that are of decisive
importance in reaching a "clear understanding of the
earth, its history or its relation to the universe".
At the coming meeting of the Vetlesen Award Committe on December
17, 1963,
I wish to nominate Professor Oort for the Award. I should
be most grateful to you if you would let me know your reaction
in this connection. In particular, I should also welcome suggestions
of other names to be considered for the Award.
May I ask you to regard the contents of this letter as strictly
confidential. This would seem particularly important in view
of the fact that the Vetlesen Award Committee may decide,
in spite of Professor Oort's eminence as an astronomer, that
the Award should go to someone whose work is more central
in the area of research than is recognized through the Vetlesen
Prize.
Sincerely,
Bengt Stromgren
THE INSTITUTE FOR ADVANCED STUDY
PRINCETON, NEW JERSEY SCHOOL OF MATHEMATICS December 12,
1963
Dr. Maurice Ewing
Vetlesen Award Committee
Torrey Cliff
Palisades, New York
Dear Dr. Ewing:
Referring to the discussion at the last meeting of the Vetlesen
Award Committee, I am herewith writing to you with regard
to the 1964 Vetlesen Prize.
I wish to propose for discussion at the meeting on December
17, 1963, that the 1964 Prize, or one-half of it, be awarded
to Professor J. H. Oort, Director of the Leiden Observatory.
In proposing that the award be given to J. H. Oort I would
like to refer, first, to the conditions by which the Vetlesen
Award Committee is guided, namely that the Vetlesen Prize
is awarded "for outstanding achievement in the sciences
resulting in a clear understanding of the earth, its history
or its relation to the universe".
If, today, we have a clearer understanding of the history
of the earth and its relation to the universe than we had
three or four decades ago, we owe this partly to astronomers
who, through their research work, have provided some of the
foundations for the investigations in question, namely a detailed
knowledge of the structure, kinematics, and dynamics of our
galaxy with respect to its stellar as well as interstellar
component and insight into the nature of the forces of evolution
at work in every part of the galaxy. Among the astronomers
who have thus contributed, Professor Oort in my opinion ranks
highest.
J. H. Oort made an outstanding contribution when he showed
in 1927, through an analysis of the radial velocities of relatively
distant high-luminosity stars, that our galaxy rotates around
an axis at right angles to the plane of the milky way and
determined the speed of rotation and the direction to the
center of rotation. Also in the 1920's, he investigated the
properties of high-velocity stars; he was the first to recognize
the great importance of the clues provided by these stars
and initiated studies of the galactic-halo stars that have
been decisive for the formation of our ideas of the evolution
of our galaxy.
In the 1930's, J. H. Oort carried out a penetrating and comprehensive
analysis of the observational material then available for
the determination of the stellar distribution in our galaxy
and in the 1940's he extended his investigations of the structure
of the galaxy with emphasis on the properties of the interstellar
medium.
During the 1950’s and up to present, J.H. Oort has
been engaged in work on the 21 cm radio radiation emitted
by interstellar hydrogen in our galaxy. Through this work
and very extensive investigations carried out by J.H. Oort's
associates under his leadership, very great advances have
been made in the knowledge of our galaxy. Spiral-arm structure
has been revealed and studied in detail to much greater distances
than had been reached through optical-astronomy investigations.
The center of the galaxy has been located with high accuracy
and detailed studies of the structure and dynamics of the
central regions of our galaxy have been made. Altogether,
these investigations have yielded results of crucial importance
to nearly every field of stellar astronomy and astrophysics.
In addition to his work on galactic problems, J. H. Oort
has carried out a very important investigation of the orbits
of comets. Through an analysis of the distribution of the
semi-major axes of the original orbits of comets (before they
are appreciably perturbed by the planets during passage through
the inner parts of the solar system), Oort showed convincingly
that a very considerable fraction of all comets when seen
are passing through the inner regions of the solar system
for the first time. This conclusion led to a study of the
distant reservoir of cometary material in the outskirts of
the solar system and the nature of its changes under the influence
of the gravitational perturbations from nearby stars.
In a previous letter to you I mentioned that I had written
to a number of astronomers in this country and in Europe to
obtain their advice in connection with the award of the Vetlesen
Prize in 1964. To date I have received replies from the great
majority of those to whom I wrote. I enclose photostat copies
of all the replies received.
I should like to add that I fully realize that the Vetlesen
Prize will normally be awarded for outstanding achievement
in the Earth Sciences. However, in my opinion the contributions
of J. H. Oort are such that they justify an award for achievements
in the field of Astronomy. In this connection I would like
to refer in particular to the letters by Dr. N. U. Mayall,
Director of the Kitt Peak National Observatory, and Dr. A.
E. Whitford, Director of the Lick Observatory of the University
of California.
Sincerely yours,
Bengt Stromgren
December 9, 1963
Dr. Bengt Stromgren
Insititute for Advanced Study
Princeton, New Jersey
Dear Bengt:
This is the first letter I write upon my return to Tucson,
following my very pleasant visit with you and Sigrid yesterday
and the evening before. I am very glad to respond to your
request to express my views about your proposal to recommend
Dr. J. H. Oort for the Vetlesen Award.
Jan Oort's contributions to our knowledge of the relationship
of the earth as an astronomical body to our own stellar system, in
my opinion, constitute the most significant work of our generation.
In fact, I believe that his work on the dynamics, structure,
and composition of the Galaxy, and on the nature of comets
in the solar system, rank along with those of Edwin Hubble
for the extragalactic universe.
One cannot think of such properties of the Galaxy as its
rotation, dynamics of the several stellar population subsystems,
spiral structure, and properties of its nuclear region without
connecting our first firm knowledge, and its most penetrating
interpretation, with the name of Oort. Also, the most important,
major advance in our knowledge of galactic structure, which
is related to the use of the radio region radiation from neutral
hydrogen, is largely due to Oort's work and his inspired leadership.
It is safe to say that for many years Oort and his group of
radio astronomers in Holland has led the rest of the world
in this field by a considerable margin.
Whenever questions as to the most reliable values of the
size of the Galaxy, the distance of the sun from its center,
the speed of the sun in its galactic orbit, the galactic mass,
the average density of matter in space, and the systematic
motions of the stars are desired, one always turns to the
most recent work and discussions by Oort. The reason, of course,
is that he has not only contributed much of this information
by his own work, but that he has also convinced astronomers
throughout the world that he has the soundest judgment in
appraising the current situation with respect to the most
accurate and reliable numerical data relating to these characteristics.
The detailed documentation of all his work would be most impressive,
and I imagine that this will be done for the Vetlesen Award
Committee.
In conclusion, I should like to use this opportunity to point
out what I think is an unfortunate situation with respect
to the fullest and proper recognition for the kind of astronomical
research that has been done by Hubble and by Oort. This is
the fact that the conditions establishing the Nobel Prizes
preclude their award to astronomers. It is my opinion, which
I know is shared by many of my colleagues, that Hubble definitely
deserved such recognition. In the case of Oort, I think the
Vetlesen Award Committee has a fine opportunity to adopt a
liberal interpretation of the Award conditions, in order to
place it on a par with that of a Nobel Prize, by awarding
it to Oort. His contributions to astronomy are so numerous
and fundamental that it is no exaggeration to state they compare
equally well with those achievements in chemistry and physics
that have been recognized by Nobel Prizes.
I hope that you will successfully plead the case for our
very distinguished colleague, Jan Oort, when the Vetlesen
Award Committee meets in the near future.
With best wishes, and many thanks to you and Sigrid for your
recent generous hospitality.
Sincerely yours,
N. U. Mayall
Observatory Director
UNIVERSITY OF CALIFORNIA
LICK OBSERVATORY
MOUNT HAMILTON, CALIFORNIA December 4, 1963
Dr. Bengt Stromgren
The Institute for Advanced Study
Princeton, New Jersey
Dear Bengt:
If the Vetlesen Award Committee is disposed to consider candidates
who have made outstanding contributions toward the understanding
of the relation of the earth to the universe, I can think
of no one more worthy than J. H. Oort. You have summarized
his achievements very well in your letter, and I cannot add
to the list of the significant contributions he has made.
In any formal statement of his work that would accompany the
actual award many details could be filled out, but the topics
you have mentioned are certainly the important ones.
I therefore support your suggestion strongly. It is fortunate
that the Vetlesen Award has been set up in terms which recognize
an important area of scientific endeavor and intellectual
achievement in a broad enough manner so that outstanding candidates
in the fields of both the earth sciences and astronomy can
be recognized. These areas have been excluded from the deliberations
of the Nobel Committees. If a case is to be made for an astronomer
in one of the early years of the awards, I think you have
chosen the right person and the right time.
Sincerely,
Albert
A. E. Whitford
UNIVERSITE DE LIEGE
INSTITUT ASTROPHYSIQUE
COINTE-SCLESSIN (BELGIQUE)
December 4, 1963
Dr. Bengt STROMGREN,
The Institute for Advanced Study
School of Mathematics
PRINCETON, New Jersey
U. S. A.
Dear Stromgren:
Your letter of November 29 regarding the Vetlesen Prize of
1964 has been the object of my very careful attention. I fully
agree with you that Professor J.H. Oort is eminently qualified
for the reward. I share your view that certain of Professor
Oort's contributions are of deep significance with regard
to the relation of the earth to the universe. Among the astronomers
and geophysicists whom I know well I could mention the names
of several eminent scholars who would also qualify for the
Vetlesen Prize. However I personally feel that Professor Oort's
results in the field covered by the Vetlesen Prize are the
most outstanding. Hence I am happy to learn that you plan
to nominate Professor Oort for the Award, You may make my
comments on this matter known to the Vetlesen Award Committee
if you wish.
Very sincerely yours,
P. SWINGS.
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