Age, Biography and Wiki

Rainer Weiss was born on 29 September, 1932 in Berlin, Germany. Discover Rainer Weiss's Biography, Age, Height, Physical Stats, Dating/Affairs, Family and career updates. Learn How rich is He in this year and how He spends money? Also learn how He earned most of networth at the age of 91 years old?

Popular As N/A
Occupation N/A
Age 92 years old
Zodiac Sign Libra
Born 29 September, 1932
Birthday 29 September
Birthplace Berlin, Germany
Nationality Germany

We recommend you to check the complete list of Famous People born on 29 September. He is a member of famous with the age 92 years old group.

Rainer Weiss Height, Weight & Measurements

At 92 years old, Rainer Weiss height not available right now. We will update Rainer Weiss's Height, weight, Body Measurements, Eye Color, Hair Color, Shoe & Dress size soon as possible.

Physical Status
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Dating & Relationship status

He is currently single. He is not dating anyone. We don't have much information about He's past relationship and any previous engaged. According to our Database, He has no children.

Family
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Rainer Weiss Net Worth

His net worth has been growing significantly in 2022-2023. So, how much is Rainer Weiss worth at the age of 92 years old? Rainer Weiss’s income source is mostly from being a successful . He is from Germany. We have estimated Rainer Weiss's net worth , money, salary, income, and assets.

Net Worth in 2023 $1 Million - $5 Million
Salary in 2023 Under Review
Net Worth in 2022 Pending
Salary in 2022 Under Review
House Not Available
Cars Not Available
Source of Income

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Timeline

2022

In a 2022 interview given to Federal University of Pará in Brazil, Weiss talks about his life and career, the memories of his childhood and youth, his undergraduate and graduate studies at the MIT and the future of gravitational waves astronomy.

2017

In 2017, Weiss was awarded the Nobel Prize in Physics, along with Kip Thorne and Barry Barish, "for decisive contributions to the LIGO detector and the observation of gravitational waves".

2016

In February 2016, he was one of the four scientists of LIGO/Virgo collaboration presenting at the press conference for the announcement that the first direct gravitational wave observation had been made in September 2015.

1970

Weiss also pioneered the concept of using lasers for an interferometric gravitational wave detector, suggesting that the path length required for such a detector would necessitate kilometer-scale arms. He built a prototype in the 1970s, following earlier work by Robert L. Forward. He co-founded the NSF LIGO (gravitational-wave detection) project, which was based on his report "A study of a long Baseline Gravitational Wave Antenna System".

1960

He taught at Tufts University from 1960 to 1962, was a postdoctoral scholar at Princeton University from 1962 to 1964, and then joined the faculty at MIT in 1964.

1938

Rainer Weiss was born in Berlin, Germany, the son of Gertrude Loesner and Frederick A. Weiss. His father, a physician, neurologist, and psychoanalyst, was forced out of Germany by Nazis because he was Jewish and an active member of the Communist Party. His mother, an actress, was Christian. His aunt was the sociologist Hilda Weiss. The family fled first to Prague, but Germany's occupation of Czechoslovakia after the 1938 Munich Agreement caused them to flee again; the philanthropic Stix family of St. Louis enabled them to obtain visas to enter the United States. Weiss spent his youth in New York City, where he attended Columbia Grammar School. He studied at MIT and, after dropping out during his junior year, returned to receive his S.B. degree in 1955 and Ph.D. degree in 1962 under Jerrold Zacharias.

1932

Rainer "Rai" Weiss (/waɪs/ WYSSE, German: [vaɪs]; born September 29, 1932) is an American physicist, known for his contributions in gravitational physics and astrophysics. He is a professor of physics emeritus at MIT and an adjunct professor at LSU. He is best known for inventing the laser interferometric technique which is the basic operation of LIGO. He was Chair of the COBE Science Working Group.