
Nobel Prize in Physics · 2017
Rainer Weiss
A refugee from Nazi Berlin, he designed the laser detector that first heard gravitational waves from colliding black holes.
The Nobel citation: “for decisive contributions to the LIGO detector and the observation of gravitational waves”
- Born
- September 29, 1932, Berlin, Germany
- Died
- August 25, 2025, Cambridge, MA, USA
- Shared with
- Barry C. Barish, Kip S. Thorne
- Affiliation at the time
- LIGO/VIRGO Collaboration; Massachusetts Institute of Technology (MIT), USA
Physics prize
2017
Shared with 2 other laureates.
Age that year
85years
Born in 1932.
Sources cited
17
Fact-checked September 24, 2026.
- He flunked out of MIT as a junior, by his own account over a failed romance, then worked there as a lab technician and went on to earn an MIT PhD.
- The idea behind LIGO began as a way to explain gravitational waves to students in a general relativity course he taught at MIT in the late 1960s.
- His family reached New York in January 1939, two months before German troops occupied Prague, with help from a St. Louis family that posted bond for Jewish refugees.
- As a teenager he built and sold hi-fi systems from war-surplus parts and from speakers salvaged after a fire in a Brooklyn movie theater.
- LIGO senses changes in length smaller than one ten-thousandth the width of a proton, along arms 4 kilometers long.
The breakthrough
Designing the laser detector that caught gravitational waves
Einstein's theory of gravity predicted that when heavy objects speed up, such as two black holes whirling around each other, they send out ripples that stretch and squeeze space itself. These gravitational waves are incredibly faint, and Einstein doubted anyone could ever measure them. In 1972 Weiss worked out how it could be done, building on a classroom thought experiment from the late 1960s. His design is an L-shaped instrument. A laser beam is split in two and sent down both arms, where it bounces off hanging mirrors and comes back. Normally the two returning beams cancel each other out. When a gravitational wave passes, one arm gets slightly longer while the other gets slightly shorter, so the beams fall out of step and a flicker of light reaches a detector. Think of two runners racing out and back on identical tracks: they always tie, until one track secretly stretches. Weiss's key contribution was listing every kind of noise that could drown out a signal, from ground vibrations to the jiggling of atoms in the mirrors and the graininess of light itself, and showing how each could be beaten. His analysis showed the arms would need to be kilometers long. LIGO's two detectors, in Washington state and Louisiana, have 4-kilometer arms and can sense a change in length smaller than one ten-thousandth the width of a proton. On 14 September 2015 they recorded waves from two black holes that had merged 1.3 billion years earlier.[4],[5],[10],[11]
“People say, 'I failed out of college! My life is over!' Well, it's not over. It depends on what you do with it.”
What it meant for humanity
LIGO gave people a new way to sense the universe. Until 2015, almost everything known about the cosmos came from light, other radiation and a few kinds of particles. Gravitational waves carry news of events that give off little or no light, such as black holes colliding. The Nobel committee described them as a completely new window on the most violent events in space. The payoff came quickly. In 2017 LIGO and the European Virgo detector caught two neutron stars colliding, and some 70 observatories on the ground and in space joined in. Telescopes saw freshly made gold and platinum, which helped solve a long-standing puzzle about where about half of the elements heavier than iron are made. By 2025 the LIGO, Virgo and KAGRA detectors had recorded about 300 black hole mergers, some still awaiting confirmation, and were catching roughly one every three days. A very clear 2025 signal gave the strongest evidence yet for Stephen Hawking's 1971 prediction that the total surface area of black holes cannot shrink. To reach this sensitivity, LIGO's teams had to improve lasers, mirror coatings, vibration isolation and quantum measurement methods, techniques that LIGO scientists say also apply to quantum sensors and quantum computers. Weiss's influence also came through people. An MIT colleague called him the creator of two fields, measurements of the Big Bang's leftover microwave glow and of gravitational waves, and noted that his students went on to lead both. He used his Nobel Prize money to fund a fellowship for MIT physics students.
- In August 2017, LIGO and Virgo detected two colliding neutron stars. Some 70 observatories joined the observation, and telescopes saw newly made gold and platinum, helping explain where about half of all elements heavier than iron come from.[12]
- By September 2025 the LIGO-Virgo-KAGRA network had recorded about 300 black hole mergers, some still awaiting confirmation, and LIGO was observing roughly one every three days.[11]
- Before LIGO, his balloon-borne instruments showed in 1973 that the Big Bang's leftover microwave glow has the peak expected of heat radiation. He later chaired the science team of NASA's COBE satellite.[3],[9]
- With his Nobel Prize money he set up the Barish-Weiss Fellowship to support student research in MIT's physics department.[7]
Impact in numbers
Weiss's contribution is knowledge and a new kind of instrument, not a product, so we record no quantified claims. His 1972 design study became the blueprint for LIGO, which opened gravitational-wave astronomy: a way to study black holes and neutron stars through the shaking of space itself rather than through light. The field has since tested predictions of Einstein and Hawking, helped reveal where heavy elements such as gold are made, and catalogued hundreds of black hole mergers. Earlier, his balloon measurements and leadership of COBE's science team helped turn the Big Bang's afterglow into precise evidence about the early universe. LIGO's drive for precision also advanced lasers, mirror coatings and quantum measurement, but no credible figure links a dollar value or a count of lives to Weiss's own work, and inventing one would be dishonest. Much of his impact also lives on in people: the students he trained now lead both fields he helped found.
Fundamental scienceSpaceTechnologyEducation
No number is given here on purpose. Some contributions cannot be counted honestly, and we would rather describe them than invent a figure.
The double edge
No harms are documented from Weiss's discovery itself. It is basic research with no military or commercial product. The controversies concern money and credit. Science magazine called LIGO the most costly project in the history of the US National Science Foundation. Physicists first asked for nearly $300 million, and the cost estimate later rose by about 40 percent, all for an instrument that might never detect anything. Weiss recalled that people thought his team was crazy, and that some astronomers considered LIGO premature and a possible waste of funds. Credit is the second issue. The prize went to three people, while Weiss himself said the three represented about 1,000 scientists, engineers, technicians, students and administrators. LIGO co-founder Ronald Drever died in March 2017, months before the prize was announced.
- Minor
A costly gamble on uncertain science
Science called LIGO the most costly project in the National Science Foundation's history. Physicists first asked for nearly $300 million, and the cost estimate later rose about 40 percent. Some astronomers considered it premature and a possible waste of money. Construction began in 1992, and no gravitational waves were seen until 2015.[4],[10],[13]
- Minor
Three prizewinners for the work of a thousand
The Nobel Prize honored three founders and leaders, but LIGO's discoveries rested on about 1,000 people. Co-founder Ronald Drever died in March 2017, before the prize was announced. Weiss said he saw the award as a symbol of the many others who worked on LIGO.[5],[6],[7],[17]
Against the odds
Weiss was born in Berlin in September 1932, four months before Hitler took power. Berlin had Germany's largest Jewish community, about 160,000 people in the mid-1920s. From 1933 the Nazi state issued hundreds of anti-Jewish laws and decrees, including 1933 measures that curtailed the work of Jewish doctors and lawyers. Weiss's father was a Jewish neurologist and a Communist. In 1932, while Weiss's mother was pregnant, his father reported a Nazi doctor at the workers' hospital where he worked and was seized by a Nazi gang. His mother's family got him released and he was pushed over the border to Czechoslovakia; mother and baby followed to Prague. Czechoslovakia was a refuge only until September 1938, when the Munich agreement handed its border region to Hitler. The family heard the news on the radio while on vacation and rushed to Prague to seek visas to any country that would accept Jews. Few would. With the backing of a St. Louis family, the Stixes, they reached New York in January 1939, two months before German troops occupied Prague. The Germans and their collaborators later killed about 263,000 Jews from prewar Czechoslovakia. In New York his father spent years qualifying to practice medicine again, while his mother worked store counters and odd jobs. Weiss went to private school on a refugee-relief scholarship.
1932
Persecution
While his mother was pregnant, his Jewish, Communist father reported a Nazi doctor at the Berlin workers' hospital where he worked. A Nazi gang seized him and held him in a cellar. His mother's father, a judge, got him released, and he was pushed over the border to Czechoslovakia.[2],[3],[9]
1933
Persecution
Months after his birth, the Nazi regime began more than 400 anti-Jewish decrees and regulations, including 1933 laws that curtailed Jewish doctors and lawyers. Berlin, where about 160,000 Jews lived in the mid-1920s, had the country's largest Jewish community.[14],[15]
1938
Exile
After the September 1938 Munich agreement left Czechoslovakia open to Hitler, the family joined crowds seeking visas to any country that would accept Jews. Backed by the Stix family of St. Louis, they reached New York in January 1939, two months before Germany occupied Prague.[2],[3],[9],[16]
1939
Other
As refugees in New York, his father struggled for years to requalify as a doctor (about four years in Weiss's Nobel autobiography, about eight in a 2000 interview), while his mother took store-counter and odd jobs. Weiss attended private school on a refugee-relief scholarship.[2],[3],[9]
1974
Other
Vietnam-era limits on military research money cut off funding for his gravitational-wave prototype at MIT. Reviewers doubted the idea, and he spent years seeking new support.[4],[8]
Jewish background
Weiss's father, the neurologist and later psychoanalyst Frederick Weiss, came from a well-off German Jewish family in Berlin with ties to the Rathenau family that founded the electrical company AEG. He was also a committed Communist. His mother, the actress Gertrude Loesner, came from a Protestant family of civil servants and lawyers on the Rhine near Koblenz. In a 2000 interview Weiss said simply that his father was Jewish and his mother was not. NobelPrize.org describes his father as of Jewish descent. Weiss wrote that in 1938 the family sought visas to any country that would take Jews. In the sources we found, he did not discuss Jewish religious practice or his own Jewish identity.[1],[2],[3],[9]
Key dates
September 29, 1932
Born in Berlin to a Jewish neurologist father and an actress mother. That year his father is seized by a Nazi gang, then released and pushed over the border to Czechoslovakia; mother and baby follow.[1],[2],[3],[9]
September 1938
After the Munich agreement opens Czechoslovakia to Hitler, the family seeks visas to leave Europe.[2],[3],[9]
January 1939
Arrives in New York as a refugee, two months before German troops occupy Prague.[2],[3],[9]
1953
Having failed his courses and left MIT as a student, becomes a technician in Jerrold Zacharias's atomic beam laboratory at MIT.[3],[9]
1962
Earns his PhD from MIT, after completing his bachelor's degree in 1955.[1],[7]
1964
Joins the MIT physics faculty and starts a research group in cosmology and gravitation.[7]
1966
Asked to teach MIT's graduate course in general relativity; preparing a lecture, he devises a thought experiment to detect gravitational waves by timing light between free-floating masses.[3],[4],[8]
1972
Sets out his design for a laser interferometer gravitational-wave detector in an MIT laboratory progress report, identifying its main noise sources and how to overcome them.[4],[10]
1973
Balloon measurements with his student Dirk Muehlner reveal the thermal peak of the cosmic microwave background.[9]
1976
Elected chair of the science working group for NASA's COBE satellite.[3],[9]
1984
Caltech and MIT agree to design and build LIGO jointly, led by Weiss, Kip Thorne and Ronald Drever.[10]
September 14, 2015
LIGO's two detectors make the first direct detection of gravitational waves, from two merging black holes.[5],[11]
October 3, 2017
Awarded half of the Nobel Prize in Physics; the other half is shared by Barry Barish and Kip Thorne.[1],[5]
August 25, 2025
Sources
- 1.Rainer Weiss - Facts · NobelPrize.org (Nobel Prize Outreach)
- 2.Interview with Rainer Weiss (oral history conducted by Shirley K. Cohen, 10 May 2000) · Caltech Archives, 2000
- 3.Rainer Weiss - Biographical · NobelPrize.org (Nobel Prize Outreach), 2017
- 4.LIGO and the Discovery of Gravitational Waves, I (Nobel Lecture, 8 December 2017) · NobelPrize.org (Nobel Prize Outreach), 2017
- 5.Popular information: Cosmic chirps (The Nobel Prize in Physics 2017) · NobelPrize.org (Royal Swedish Academy of Sciences), 2017
- 6.Rainer Weiss - Banquet speech · NobelPrize.org (Nobel Prize Outreach), 2017
- 7.Professor Emeritus Rainer Weiss, influential physicist who forged new paths to understanding the universe, dies at 92 · MIT News, 2025
- 8.Q&A: Rainer Weiss on LIGO's origins · MIT News, 2016
- 9.Meet the college dropout who invented the gravitational wave detector (Adrian Cho; archived copy) · Science (AAAS), 2016
- 10.A Brief History of LIGO (by Kip Thorne and Rai Weiss) · Caltech, 2016
- 11.Ten Years Later, LIGO is a Black-Hole Hunting Machine · Caltech, 2025
- 12.LIGO and Virgo make first detection of gravitational waves produced by colliding neutron stars · LIGO Laboratory (Caltech), 2017
- 13.Got gravitational waves? Thank NSF's approach to building big facilities (Jeffrey Mervis; archived copy) · Science (AAAS), 2016
- 14.Anti-Jewish Legislation in Prewar Germany · United States Holocaust Memorial Museum, Holocaust Encyclopedia
- 15.Germany: Jewish Population in 1933 · United States Holocaust Memorial Museum, Holocaust Encyclopedia
- 16.Czechoslovakia · United States Holocaust Memorial Museum, Holocaust Encyclopedia
- 17.Caltech Mourns the Passing of LIGO Co-founder Ronald W. P. Drever · Caltech, 2017
Fact-checked on September 24, 2026 by a separate AI fact-checking pass that re-opened the sources, with 8 corrections made. How we check
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