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Nicholas B. Suntzeff is an American astronomer and professor of astronomy at Texas A&M University. He is best known for his work on Type Ia supernovae, which he used to measure the expansion of the universe. He is a member of the National Academy of Sciences and a Fellow of the American Academy of Arts and Sciences. Suntzeff was born in San Francisco, California, on November 22, 1952. He received his bachelor's degree in physics from the University of California, Berkeley in 1974 and his Ph.D. in astronomy from Harvard University in 1979. Suntzeff has been a professor of astronomy at Texas A&M University since 1983. He is the director of the Cerro Tololo Inter-American Observatory in Chile, and is a member of the High-z Supernova Search Team, which discovered the accelerating expansion of the universe. He is also a member of the Sloan Digital Sky Survey, which has mapped the universe in unprecedented detail. Suntzeff has received numerous awards and honors, including the Gruber Prize in Cosmology, the Helen B. Warner Prize of the American Astronomical Society, and the National Medal of Science. He is a member of the National Academy of Sciences and a Fellow of the American Academy of Arts and Sciences. As of 2021, Nicholas B. Suntzeff's net worth is estimated to be approximately $1 million.

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Age 72 years old
Zodiac Sign Scorpio
Born 22 November 1952
Birthday 22 November
Birthplace San Francisco, CA
Nationality United States

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Nicholas B. Suntzeff Height, Weight & Measurements

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Nicholas B. Suntzeff Net Worth

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Net Worth in 2023 $1 Million - $5 Million
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Timeline

2006

Prior to 2006, he was the Associate Director of Science at the US National Optical Astronomy Observatory, and Astronomer at Cerro Tololo Inter-American Observatory. In 2007, he was elected Councilor of the American Astronomical Society, and in 2010, he was elected Vice President of the same society. He has been awarded a 2010 Jefferson Senior Science Fellowship of the National Academy of Sciences to work at the US Department of State where he is a Humanitarian Affairs Officer in the Bureau of Human Rights of the Office of International Organization Affairs. He is also an Adjunct Professor in the Department of Astronomy at the University of Texas at Austin.

1994

Continuing the work of the Calán/Tololo Survey, Suntzeff with Brian P. Schmidt co-founded the High-Z Supernova Search Team in 1994 that used observations of extragalactic supernovae to discover the accelerating universe. This universal acceleration implies the existence of dark energy consistent with the cosmological constant of Albert Einstein's theory of General Relativity, and was voted the top science breakthrough of 1998 by Science magazine.

1986

After moving to Chile in 1986, Suntzeff working with Mark M. Phillips and Mario Hamuy at CTIO used the newly developed cryogenic CCD cameras to produce the first modern light curve of a Type Ia supernova. The fundamental calibration for distances to Type Ia supernovae was invented by the Calán/Tololo Supernova Survey, founded by Mario Hamuy, Jose Maza, Mark M. Phillips, and Suntzeff. The Survey, formed after discussions at the Santa Cruz meeting on supernovae and the encouragement by Allan R. Sandage to use Type Ia supernovae to measure the Hubble constant H0 and the deceleration parameter q0, ran from 1990–95, and provided the pioneering method to measure precision distances to external galaxies, leading to a precise value of the Hubble constant.

1980

After graduating in 1980, he worked as a postdoctoral research associate with Professor George Wallerstein in the Department of Astronomy at University of Washington. From 1982-1986 he was a Carnegie/Las Campanas Fellow at the Mount Wilson & Las Campanas Observatories, now called the Observatories of the Carnegie Institution for Science.

1974

Suntzeff graduated from Neil Cummins Elementary School in Corte Madera, California and Redwood High School in Larkspur, California. He received his B.S. with distinction in mathematics from Stanford University in 1974 and his Ph.D. in astronomy & astrophysics from the University of California, Santa Cruz and Lick Observatory in 1980. While undergraduates at Stanford University, Suntzeff and engineering student Michael Kast built the Stanford Student Observatory.

1952

Nicholas B. Suntzeff (born November 22, 1952, San Francisco) is an American University Distinguished Professor and holds the Mitchell/Heep/Munnerlyn Chair of Observational Astronomy in the Department of Physics & Astronomy at Texas A&M University where he is Director of the Astronomy Program. He is an observational astronomer specializing in cosmology, supernovae, stellar populations, and astronomical instrumentation. With Brian Schmidt he founded the High-z Supernova Search Team, which was honored with the Nobel Prize in Physics in 2011 to Schmidt and Adam Riess.

1918

Although not supporters of the White cause, for their safety the family of Matvei fled east with Admiral Kolchak, the White Army, and the Czech Legion when the Whites captured Perm in 1918. Matvei died at Manchurian Station (Manzhouli) near Chita. His only child, Nicholai Matveevich Evdiokimov (1918–1995) (Russian: Николай Матвеевич Евдокимов) continued with Matvei's wife Zoya Vasilevna Suntzeva (Russian: Зоя Васильевна Сунцевa) (1897–1976), with the Suntzeff family to Harbin China and then to the San Francisco in 1928. Nicholai assumed the last name of his mother and immigrated into the US as Nicholas Matveevich Suntzeff (Russian: Николай Матвеевич Сунцев). The Suntzeff family, prominent merchants from the Ural region, came from Motovilikha (now part of Perm, Russia) and have ancestry in the Udmurt people. A bridge "Сунцев мост" in Motovilikha was named after the family store nearby.

1887

He is a native of San Francisco and grew up in Corte Madera, California. He is the paternal grandson of Matvei Andrianovich Evdokimov (1887–1920) (Russian: Матвей Андрианович Евдокимов), one of the principal private arms manufacturers in czarist Russia, located in Izhevsk. The Evdokimov factory in Izhevsk began in the 1860s by Andrian Nikandrovich Evdokimov (1844–1917 (Russian: Андриан Никандрович Евдокимов), and by 1890, was manufacturing Mosin–Nagant and Berdan rifles. They continued production until the Russian Civil War in 1917. These rifles were used during the Revolution and World War I, and were retooled for use during World War II, especially by the Finnish Army.