Nobel Prizes
in
Astrophysics & Cosmology
A Twelve Part Series
Part 1 - Overview
It
is my express wish that in awarding the prizes no consideration be given to the
nationality of the candidates, but that the most worthy shall receive the
prize.
-
Alfred Nobel
Introduction
Since their inception at the beginning of the
last century, Nobel prizes have become symbols of the highest achievement in select
fields of human endeavour – Physics, Chemistry, Physiology/Medicine, Literature
and Peace.
This is the curtain raiser to a series of eleven
articles to follow, outlining the history of the Nobel prize awarded to outstanding
work related to Astronomy/Astrophysics/Cosmology within the broader field of
Physics. The proposed series has been inspired by a book recently published in
Kannada by Prof P Venkataramiah on ‘Nobel Laureates in the Family’ which I have
reviewed in an earlier blog article here.
These articles, one for each year of the award,
will draw material from the Nobel archives and other sources, with some
assistance from AI. Each will present a
detailed account of the award to the recipient/s, including an elucidation of
the work involved from a physics perspective, and a biographical sketch.
Here is a summary of the eleven occasions when
the award was made to work directly or indirectly related to Astronomy/Astrophysics/Cosmology:
|
Year |
Recipient/s |
Nationality |
Citation |
1 |
1967 |
Hans A Bethe (1906-2005) |
German-American |
“For his contributions
to the theory of nuclear reactions, especially his discoveries
concerning the energy production in stars.” |
2 |
1974 |
1) Martin Ryle (1918-1984) 2) Antony Hewish (1924-2021) |
British
British
|
“For their pioneering
research in radio astrophysics… Ryle for aperture-synthesis
techniques, Hewish for a decisive role in the discovery of pulsars.” |
3 |
1978 |
1) Arno A Penzias (1933-2024) 2) Robert W Wilson (1936- ) |
American
American |
“For their discovery
of cosmic microwave background radiation.” |
4 |
1983 |
1) Subrahmanyan
Chandrasekhar (1910-1995) 2) William A Fowler (1911-1995) |
Indian-American
American |
“For studies…
important to the structure and evolution of the stars” (Chandrasekhar)
and “for… nuclear reactions of importance in the formation of the
chemical elements in the universe” (Fowler) |
5 |
1993 |
1) Russell A Hulse (1950- ) 2) Joseph H Taylor
Jr (1941- ) |
American
American |
“For the discovery of
a new type of pulsar, a discovery that has opened up new possibilities
for the study of gravitation.” |
6 |
2002 |
1) Raymond Davis Jr (1914-2006) 2) Masatoshi
Koshiba (1926-2020) 3) Riccardo
Giacconi (1931-2018) |
American
Japanese
Italian-American |
“For pioneering
contributions to astrophysics, in particular for the detection of cosmic
neutrinos” (Davis & Koshiba) and “for pioneering contributions to
astrophysics, which have led to the discovery of cosmic X-ray sources”
(Giacconi). |
7 |
2006 |
1) John C Mather (1946- ) 2) George F Smoot (1945- ) |
American
American |
“For their discovery
of the blackbody form and anisotropy of the cosmic microwave background
radiation.” |
8 |
2011 |
1) Saul Perlmutter (1959- ) 2) Brian P Schmidt (1967- ) 3) Adam G Riess (1969- ) |
American
American-Australian American |
“For the discovery of
the accelerating expansion of the Universe through observations of
distant supernovae.” |
9 |
2017 |
1) Rainer Weiss (1932- ) 2) Barry C Barish (1936- ) 3) Kip S Thorne (1940- ) |
German-American American
American |
“For decisive
contributions to the LIGO detector and the observation of gravitational
waves.” |
10 |
2019 |
1) James Peebles (1935- ) 2) Michel Mayor (1942- ) 3) Didier Queloz (1966- ) |
Canadian-American Swiss
Swiss |
Half to James Peebles
“for theoretical discoveries in physical cosmology”; the other half
jointly to Mayor & Queloz “for the discovery of an exoplanet orbiting
a solar-type star.” |
11 |
2020 |
1) Roger Penrose (1931- ) 2) Reinhard Genzel (1952- ) 3) Andrea Ghez (1965- ) |
British
German
American
|
Penrose: for work
showing GR predicts black-hole formation; Genzel & Ghez: “for the
discovery of a compact object (supermassive black hole) at the centre
of our galaxy.” |
This list excludes the following three awardees whose achievements relate only marginally to the areas of interest here:
- Victor F Hess, Austrian-American physicist, who got the 1936 Nobel Prize in Physics ‘for his discovery of cosmic radiation’,
- P M S Blackett, British physicist, who got the Nobel award in 1948 ‘for his contributions to his development of the Wilson Cloud Chamber method and its use in discovering cosmic ray interactions’, and
- Hannes Alfven, Swedish Engineer and pioneer of magnetohydrodynamics and plasma physics, who got the Nobel award in 1970.
Perhaps understandably, the list is dominated by one single nationality.
The Unlucky Lot
As it is now, the early 20th century was a golden age
for astronomy, astrophysics, and cosmology, with many scientists making
groundbreaking contributions that fundamentally reshaped our understanding of
the universe. Several key figures did not receive a Nobel Prize in
Physics despite their monumental work, often because their fields were not yet
recognized by the Nobel Committee or because the scope of the prize was more
traditionally focused on laboratory and theoretical physics. Here are some of
the most deserving candidates:
1. Edwin Hubble (1889–1953) who discovered the
expansion of the universe (Hubble's Law, 1929), providing the first
observational evidence for the Big Bang theory and showed the existence of
galaxies beyond the Milky Way.
[The Nobel Committee did not consider Astronomy a
part of Physics at the time. Hubble justifiably aspired for a Nobel prize, but sadly
none was awarded for Astronomy until the 1970s.]
2. Arthur Eddington (1882–1944) who provided
experimental confirmation of Einstein's General Relativity during the 1919
solar eclipse, pioneered stellar structure theory (e.g., the Eddington limit
for radiation pressure in stars), and also did some early work on nuclear
fusion in stars.
[His work was more theoretical/observational than
experimental, and the Nobel Committee was slow to recognize Astrophysics.]
3. Georges Lemaître (1894–1966) who proposed
the "primeval atom" theory (later called the Big Bang) in 1927–1933,
and independently derived Hubble's Law before Hubble.
[Cosmology was not yet a Nobel-recognized field,
and his work was initially overshadowed by Hubble’s observations.]
4. Fred Hoyle (1915–2001) who formulated the theory
of stellar nucleosynthesis, and was one of the authors of the path breaking B2FH
(Margaret Burbridge, Geoffrey Burbridge, William Fowler and Fred Hoyle) paper
on the origin of chemical elements.
[His outspoken opposition to the Big Bang theory
may have been a dampener.]
5. Cecilia Payne-Gaposchkin (1900–1979) who discovered
that stars are primarily composed of hydrogen and helium (her 1925 thesis is
one of the most important in astrophysics), and laid the foundation for stellar
composition studies.
[Gender bias in science was pronounced at the time;
her work was initially dismissed by senior astronomers like Henry Norris
Russell (who later acknowledged her findings).]
6. Henrietta Swan Leavitt (1868–1921) who discovered
the period-luminosity relation for Cepheid variables (1912), allowing Hubble to
measure galactic distances.
[She was a "computer" (not a formally
recognized scientist) at Harvard, and women were rarely considered for high
honors. Nobel Prizes are also not given posthumously.]
7. Fritz Zwicky (1898–1974) who proposed the
idea of dark matter (1933) through galaxy cluster dynamics, and pioneered
supernova and neutron star research.
[His ideas were too ahead of their time, and his
abrasive personality may have hindered recognition.]
8. Karl Schwarzschild (1873–1916) who gave the first
exact solution to Einstein's field equations (Schwarzschild metric, 1916),
predicting black holes.
[He died young, and black holes were not yet
experimentally confirmed.]
9. Milton Humason (1891–1972) who provided
critical spectroscopic data supporting Hubble's Law.
[Seen as an observer rather than a theorist, and
Nobel prizes were rarely given to non-PhDs at the time.]
10. Vesto Slipher (1875–1969) who first
measured galactic redshifts (1912–1917), laying the groundwork for Hubble’s
expansion discovery.
[His work was overshadowed by Hubble’s later
synthesis.]
11. Vera Rubin (1928–2016) who pioneered work on
galactic rotation rates that produced the first widely accepted evidence for
the existence of dark matter.
[The recently inaugurated Vera C Rubin Observatory in
Chile is some consolation to her memory.]
12. Jocelyn Bell Burner (1943- ) who discovered
the first radio pulsars in 1967.
[She was a mere ‘student’ at the time of the
discovery and, as such, not a credible candidate for the award which went to
her ‘teacher’ Anthony Hewish. However, the lucrative Breakthrough Prize bestowed
upon her later was adequate compensation.]
These scientists reshaped our cosmic understanding,
and many later prizes in astrophysics (e.g., for cosmic microwave background,
exoplanets, black holes) owe a debt to their foundational work.
[It makes as much sense to write about these
pioneers, who were unlucky not to get the award, as about the ones who did. I
intend to feature them separately in a follow up series of articles.]
Alfred Nobel, the man behind the prizes
Alfred Bernhard Nobel (1833 – 1896) after whom these
famous awards are known was a Swedish chemist, engineer, inventor,
industrialist and philanthropist. His father, Immanuel Nobel, was an inventor
and industrialist who eventually moved to Russia for work. Alfred received a
broad education in natural sciences, literature, and languages. He was fluent
in Swedish, Russian, French, English, and German. In Paris, Nobel
studied chemistry under the famed chemist Théophile-Jules Pelouze, where he
encountered Ascanio Sobrero, the discoverer of nitroglycerin—a highly volatile
explosive compound.
In 1867, Nobel discovered how to stabilize
nitroglycerin by combining it with absorbent materials like kieselguhr,
creating "dynamite." This invention revolutionized construction,
mining, and warfare. Eventually he was to hold 355 patents. Nobel's inventions
extended to blasting caps, gelignite, and ballistite (a precursor to smokeless
gunpowder).
Nobel established an industrial empire consisting of 90
armaments factories and laboratories in over 20 countries.
Despite the immense wealth he had amassed, Nobel led a
relatively isolated personal life. He never married and was known to be
introspective, a lover of literature, and a pacifist at heart. He maintained a
long correspondence with Austrian pacifist Bertha von Suttner, who would later
win the Nobel Peace Prize in 1905.
Nobel’s Will
One year before his death, Nobel signed a handwritten
will at the Swedish–Norwegian Club in Paris. Its contents shocked his family
and the public: He wrote in part: “The whole of my remaining realizable estate
shall be dealt with in the following way: the capital... shall constitute a
fund, the interest on which shall be annually distributed in the form of prizes
to those who, during the preceding year, have conferred the greatest benefit on
mankind…”. This requirement underwent major re-interpretations and adaptations in
course of time.
Nobel specified five fields: Physics, Chemistry,
Physiology or Medicine, Literature, and Peace (to the person or society that
promotes peace and fraternity between nations).
[Note: The Nobel Prize in Economic Sciences was added
later, in 1968, by the Swedish central bank.]
Nobel’s action led to a lot of unpleasant reactions
and consequences. His relatives were unhappy, and the will was challenged in
court. It took four years to resolve the attendant disputes and establish the
Nobel Foundation in 1900.
Nobel’s handwritten will
Nobel specified that the Peace Prize be awarded by a Norwegian committee, while others were to be awarded by Swedish institutions—a symbolic gesture, as Sweden and Norway were in a union at the time.
The Nobel Prizes, first awarded in 1901, remain among
the most prestigious awards in the world.
Nobel’s name, once associated with explosives, became
a global symbol of peace, progress, and human achievement. He left about 31
million Swedish kronor (equivalent to over USD 250 million today) to fund the
prizes.
Alfred Nobel was a paradoxical figure—an inventor of
deadly explosives who chose to dedicate his fortune to honoring those who
advance humanity. His actions led to an eventual global recognition of
scientific, literary, and humanitarian excellence, and his name endures as a
beacon of peace and progress.
Nobel Physics Awards
Physics was the prize area which Alfred Nobel
mentioned first in his will from 1895. At the end of the nineteenth century,
many people considered physics as the foremost of the sciences, and perhaps
Nobel saw it this way as well. His own research was also closely tied to
physics.
The Nobel Prize in Physics has been awarded 118 times
to 227 Nobel Prize laureates between 1901 and 2024. John Bardeen is the only
laureate who has been awarded the Nobel Prize in Physics twice, in 1956 and
1972. This means that a total of 226 individuals have received the Nobel Prize
in Physics.
The Nobel Foundation, a private
institution established in 1900, has ultimate responsibility for fulfilling the
intentions in Alfred Nobel’s will. The main mission of the Nobel Foundation is
to manage Alfred Nobel’s fortune in a manner that ensures a secure financial standing
for the Nobel Prize over the long term and that the prize-awarding institutions
are guaranteed independence in their work of selecting recipients.
The Foundation is also tasked with strengthening the
Nobel Prize’s position by administering and developing the brands and
intangible assets that have been built up during the Nobel Prize’s history,
which spans well over a century.
The Nobel Foundation also strives to safeguard the
prize-awarding institutions’ common interests and to represent the Nobel organization
as a whole. In the past two decades a number of outreach activities have been
developed with the aim of inspiring and disseminating knowledge about the Nobel
Prize.
Who selects the Nobel Prize laureates?
In his last will and testament, Alfred Nobel
specifically designated the institutions responsible for the prizes he wished
to be established: The Royal Swedish Academy of Sciences for the Nobel Prize in
Physics and Chemistry, Karolinska Institutet for the Nobel Prize in Physiology
or Medicine, the Swedish Academy for the Nobel Prize in Literature, and a committee
of five persons to be elected by the Norwegian Parliament (Storting) for the
Nobel Peace Prize.
By the terms of Alfred Nobel’s will, the
Nobel Prize in Physics has been awarded by the Royal Swedish Academy of
Sciences since 1901.
The Royal Swedish Academy of Sciences
in Stockholm
The Academy was founded in 1739 and has today about 440 Swedish and 175 foreign members. Membership in the Academy constitutes exclusive recognition of successful research achievements. The Academy appoints members of the Nobel Committee, the working body, for a three-year term.
Nomination to the Nobel Prize in Physics is by
invitation only. The names of the nominees and other information about the
nominations cannot be revealed until 50 years later.
The right to submit proposals for the award of a Nobel Prize in Physics is, by statute, enjoyed by:
- Swedish and foreign members of the Royal Swedish Academy of Sciences;
2 Members of
the Nobel Committee for Physics;
3 Nobel
Prize laureates in physics;
4 Tenured
professors in the Physical sciences at the universities and institutes of
technology of Sweden, Denmark, Finland, Iceland and Norway, and Karolinska
Institutet, Stockholm;
5 Holders of
corresponding chairs in at least six universities or university colleges
(normally, hundreds of universities) selected by the Academy of Sciences with a
view to ensuring the appropriate distribution over the different countries and
their seats of learning; and
6 Other scientists from whom the Academy may see fit to invite proposals.
Decisions as to the selection of the scientific
scholars referred to in paragraphs 5 and 6 above are taken each year before the
end of the month of September.
The Royal Swedish Academy of Sciences is responsible for the selection of the Nobel Prize laureates in physics. The Academy appoints a working body, the Nobel Committee for Physics, which screens the nominations and presents a proposal for final candidates. The committee consists nominally of five voting members, but since many years, it also includes voting adjunct members. The Committee’s proposal is discussed in a larger body, the Physics Class of the Academy, who may suggest a modification or forward a different proposal to the Academy. Finally, additional proposals may be raised at the final Academy meeting. It is in principle possible to suggest that no prize be given the current year, but that is a seldom used choice.
Who is eligible for the Nobel Prize in Physics?
The candidates eligible for the physics prize are
those nominated by qualified persons who have received an invitation from the
Nobel Committee to submit names for consideration. No one can nominate himself
or herself.
How are the physics laureates selected?
The nomination process for Nobel Prize laureates in physics.
© Nobel Prize Outreach. Ill. Niklas Elmehed
Below is a brief description of the process involved in selecting the Nobel Prize laureates in physics.
September – Nomination forms are sent out. The
Nobel Committee sends out invitations for proposals for Nobel Prize nominees to
thousands of specially selected university professors and other scholars, all
around the globe. Members of the Royal Swedish Academy of Sciences as well as
Nobel Prize laureates may also propose candidates. It is not possible to
nominate oneself or to spontaneously submit a proposal without receiving an
invitation.
February – Deadline for submission. The completed
nomination forms must reach the Nobel Committee no later than 31 January of the
following year. The Committee screens the nominations and selects the
preliminary candidates.
March-May – Consultation with experts. The
Nobel Committee sends the names of the preliminary candidates to specially
appointed experts for their assessment of the candidates’ work.
June-August – Writing of the report. The Nobel
Committee puts together the report with recommendations to be submitted to the
Academy. The report is signed by all members of the Committee.
September – Committee submits recommendations.
The Nobel Committee submits its report with recommendations on the final
candidates to the members of the Academy. The report is discussed at two
meetings of the Physics Class of the Academy.
October – Nobel Prize laureates are chosen.
In early October, the Academy selects the Nobel Prize laureates in physics
through a majority vote. The decision is final and without appeal. The names of
the Nobel Prize laureates are then announced.
December – Nobel Prize laureates receive their
prize. The Nobel Prize award ceremony takes place on 10 December in
Stockholm, where the Nobel Prize laureates receive their Nobel Prize, which
consists of a Nobel Prize medal and diploma, and a document confirming the
prize amount.
Are the nominations made public?
The statutes of the Nobel Foundation restrict
disclosure of information about the nominations, whether publicly or privately,
for 50 years. The restriction concerns the nominees and nominators, as well as
investigations and opinions related to the award of a prize.
10 December – A magic date
Since 1901, the Nobel Prizes have been presented to
Nobel Prize laureates at ceremonies on 10 December, the anniversary of Alfred
Nobel’s death.
As stipulated in Nobel’s will, the Nobel Prizes in
Physics, Chemistry, Physiology or Medicine and Literature are awarded in
Stockholm, Sweden, while the Nobel Peace Prize is awarded in Oslo, Norway.
A typical Nobel awards ceremony in Stockholm, Sweden on Dec 10
Looking forward
By now the selection process for the 2025 awards should be well under way, with the names of the winners scheduled to be announced early in October. Considering that Astrophysics and Cosmology continue to be at the cutting edge of current scientific research, another award in this field his highly probable. If it happens, the number of my blog articles in the present series will swell by one!