Age, Biography and Wiki

Brian Schmidt was born on 24 February, 1967 in Missoula, Montana, United States, is an American-born Australian astrophysicist and Nobel Laureate. Discover Brian Schmidt'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 57 years old?

Popular As Brian Schmidt
Occupation N/A
Age 57 years old
Zodiac Sign Pisces
Born 24 February, 1967
Birthday 24 February
Birthplace Missoula, Montana, United States
Nationality American

We recommend you to check the complete list of Famous People born on 24 February. He is a member of famous with the age 57 years old group.

Brian Schmidt Height, Weight & Measurements

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Who Is Brian Schmidt's Wife?

His wife is Jennifer M. Gordon

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Brian Schmidt Net Worth

His net worth has been growing significantly in 2023-2024. So, how much is Brian Schmidt worth at the age of 57 years old? Brian Schmidt’s income source is mostly from being a successful . He is from American. We have estimated Brian Schmidt's net worth, money, salary, income, and assets.

Net Worth in 2024 $1 Million - $5 Million
Salary in 2024 Under Review
Net Worth in 2023 Pending
Salary in 2023 Under Review
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Timeline

1967

Brian Paul Schmidt (born 24 February 1967) is a Distinguished Professor and astrophysicist at the Australian National University's Mount Stromlo Observatory and Research School of Astronomy and Astrophysics.

1985

Schmidt attended Bartlett High School in Anchorage, Alaska, and graduated in 1985.

He has said that he wanted to be a meteorologist "since I was about five-years-old [but] ... I did some work at the USA National Weather Service up in Anchorage and didn't enjoy it very much. It was less scientific, not as exciting as I thought it would be—there was a lot of routine. But I guess I was just a little naive about what being a meteorologist meant."

His decision to study astronomy, which he had seen as "a minor pastime", was made just before he enrolled at university.

Even then, he was not fully committed: he said "I'll do astronomy and change into something else later", and just never made that change.

1989

He graduated with a BS (Physics) and BS (Astronomy) from the University of Arizona in 1989.

1992

He received his AM (Astronomy) in 1992 and then PhD (Astronomy) in 1993 from Harvard University.

Schmidt's PhD thesis was supervised by Robert Kirshner and used Type II Supernovae to measure the Hubble Constant.

While at Harvard, he met his future wife, the Australian (Jenny) Jennifer M. Gordon who was a PhD student in economics.

1993

Schmidt was a postdoctoral research Fellow at the Center for Astrophysics | Harvard & Smithsonian (1993–1994) before moving on to the ANU's Mount Stromlo Observatory in 1995.

1994

In 1994, they moved to Australia.

In 1994, Schmidt and Nicholas B. Suntzeff formed the High-Z Supernova Search Team to measure the expected deceleration of the universe and the deceleration parameter (q0) using distances to Type Ia supernovae.

1995

In 1995, the HZT at a meeting at the Center for Astrophysics | Harvard & Smithsonian elected Schmidt as the overall leader of the HZT.

1998

Schmidt led the team from Australia and in 1998 in the HZT paper with first author Adam Riess the first evidence was presented that the universe's expansion rate is not decelerating; it is accelerating.

The team's observations were contrary to the then-current models, which predicted that the expansion of the universe should be slowing down, and when the preliminary results emerged Schmidt assumed it was an error and he spent the next six weeks trying to find the mistake.

But there was no mistake: contrary to expectations, by monitoring the brightness and measuring the redshift of the supernovae, they discovered that these billion-year old exploding stars and their galaxies were accelerating away from our reference frame.

This result was also found nearly simultaneously by the Supernova Cosmology Project, led by Saul Perlmutter.

The corroborating evidence between the two competing studies led to the acceptance of the accelerating universe theory and initiated new research to understand the nature of the universe, such as the existence of dark energy.

The discovery of the accelerating universe was named 'Breakthrough of the Year' by Science in 1998, and Schmidt was jointly awarded the 2011 Nobel Prize in Physics along with Riess and Perlmutter for their groundbreaking work.

Schmidt is currently leading the SkyMapper telescope Project and the associated Southern Sky Survey, which will encompass billions of individual objects, enabling the team to pick out the most unusual objects.

Schmidt and the other members of the High-Z Team (the set defined by the co-authors of Riess et al. 1998) shared the 2007 Gruber Cosmology Prize, a $500,000 award, with Saul Perlmutter of the Lawrence Berkeley National Laboratory and the Supernova Cosmology Project (the set defined by the co-authors of Perlmutter et al. 1999) for their discovery of the accelerating expansion of the universe.

2000

Schmidt has received the Australian Government's inaugural Malcolm McIntosh Prize for achievement in the Physical Sciences in 2000, Harvard University's Bok Prize in 2000, the Australian Academy of Science's Pawsey Medal Medal in 2001, and the Astronomical Society of India's Vainu Bappu Medal in 2002.

2005

He was the Marc Aaronson Memorial Lecturer in 2005, the same year he received an ARC Federation Fellowship, and in 2006 he shared the Shaw Prize in Astronomy with Adam Riess and Saul Perlmutter.

2006

Schmidt shared both the 2006 Shaw Prize in Astronomy and the 2011 Nobel Prize in Physics with Saul Perlmutter and Adam Riess for providing evidence that the expansion of the universe is accelerating, making him the only Montana-born Nobel laureate.

He was previously an Australian Research Council Laureate Fellow.

Schmidt, an only child, was born in Missoula, Montana, where his father Dana C. Schmidt was a fisheries biologist.

When he was 13, his family relocated to Anchorage, Alaska.

2009

In 2009, he was awarded an Australian Laureate Fellowship.

2011

Schmidt, along with Riess and Perlmutter, jointly won the 2011 Nobel Prize in Physics for their observations which led to the discovery of the accelerating universe.

2012

He currently holds an Australian Research Council Federation Fellowship and was elected a Fellow of the Royal Society (FRS) in 2012.

In July 2012 Schmidt was given a three-year appointment to sit on the Questacon Advisory Council.

2014

In 2014 they announced the discovery of the first star which did not contain any iron, indicating that it is a very primitive star, probably formed during the first rush of star formation following the Big Bang.

He is the chairman of the board of directors of Astronomy Australia Limited, and he serves on the management committee of the ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO).

2015

On 24 June 2015 it was announced Schmidt would replace Ian Young as the 12th Vice-Chancellor of the Australian National University, to commence his tenure on 1 January 2016.

The Chancellor of the ANU, Professor Gareth Evans, said, "Brian Schmidt is superbly placed to deliver on the ambition of ANU founders – to permanently secure our position among the great universities of the world, and as a crucial contributor to the nation ... We had a stellar field of international and Australian candidates, and have chosen an inspirational leader. ... Brian's vision, vitality, global stature and communication skills are going to take our national university to places it has never been before."

On 2 February 2023, Schmidt announced that he would be stepping down as vice chancellor at the end of the year.

The publicity that came with winning the Nobel Prize has given Schmidt the opportunity to help the public understand why science is important to society, and to champion associated causes.

2016

He was the Vice-Chancellor of the Australian National University (ANU) from January 2016 to January 2024.

He is known for his research in using supernovae as cosmological probes.

2017

As of March 2017, Schmidt serves as a member of the Bulletin of the Atomic Scientists' Board of Sponsors.