Philosophy
Leonard Searle
October 23rd, 1930 to July 2nd, 2010
"Leonard Searle dies at 79; astronomer's work provided key information on the Big Bang"
The former director of the Carnegie Observatories also played a crucial role in the construction of the twin 6.5-meter Magellan telescopes at Carnegie's Las Campanas Observatory in Chile.
by
Thomas H. Maugh II
July 30th, 2010
Los Angeles Times
Astronomer Leonard Searle, a former director of the Carnegie Observatories whose observations provided crucial information in determining the conditions of the Big Bang that created the universe and helped explain how heavy elements are produced in stars, has died. He was 79.
Searle died July 2 at his home in Pasadena, according to the Carnegie Institution for Science in Washington, D.C. No cause of death was released.
Searle also played a crucial role in the construction of the twin 6.5-meter (255-inch) Magellan telescopes at Carnegie's Las Campanas Observatory in Chile, which opened in 2000 and are generally considered to be the best natural imaging telescopes in the world.
He was "a thoughtful man who chose his problems carefully," said astronomer Robert Preston, a director emeritus of the Carnegie Observatories. "The things that he accomplished were of lasting value; they're still used today."
The Big Bang was a singularity that started the formation of the universe and researchers have been curious about the precise conditions that existed during the explosion. That event produced massive numbers of elementary particles that, as the gas expanded and cooled, condensed to form hydrogen, helium and trace amounts of lithium and beryllium. All the rest of the elements in the universe were subsequently created in the nuclear furnaces of stars.
To calculate the temperature and pressure that existed in the Big Bang, it is crucial to know the ratio of helium to hydrogen that existed immediately afterward, and that was a problem Searle and Wallace Sargent attacked.
Most old stars are too cool to cause helium to fluoresce, so it is not possible to measure their helium-to-hydrogen ratio. And in even the hottest old stars, helium has diffused inward to the core, diluting the concentration at the surface and providing a false value for the ratio.
Ultimately, the pair identified small galaxies with slow star formation rates whose helium-to-hydrogen ratios were probably very similar to those at the creation of the universe. The values they obtained are still used in modeling the conditions of the Big Bang.
"That was typical of Leonard," Preston said. "He didn't write lots of papers. He settled on issues of fundamental importance, studied them carefully and then wrote them up. He produced a relatively small number of papers whose impact on the field is large."
Searle and Sargent also developed a model of how hydrogen and helium in the nuclear reactors of stars fused to form all the other heavier elements, a process called chemical evolution. Others termed it the "simple model" because of its clarity and it is still used today to characterize the way a galaxy produces elements and transforms gases into stars.
Searle may be best known for his work, with Robert Zinn, now at Yale University, on how galaxies are formed. Most astronomers had originally believed that galaxies condensed from massive clusters of gas in a uniform process. But by studying small galaxies near the outer fringes of our own Milky Way galaxy, the pair concluded that galaxies grew by swallowing smaller galaxies, so-called primordial fragments.
That process is now the accepted mechanism for galaxy formation and has been verified in many other experiments.
Leonard Searle was born Oct. 23, 1930, in the London suburb of Mitcham. He received his bachelor's degree from the University of St. Andrews in Scotland and his doctorate in theoretical physics from Princeton University.
His first post was at the University of Toronto, but he left in 1960 to join Caltech. Three years later, he joined the faculty of the Mount Stromblo Observatory in Australia. Finally, in 1968, he returned to Pasadena to join the Carnegie Observatories, where he spent the rest of his career.
Searle's wife of 47 years, the former Eleanor Millard, died in 1999. He has no surviving relatives.
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Cecilia Helena Payne-Gaposchkin May 10th, 1900 to December 7th, 1979 Cecilia Helena Payne-Gaposchkin was an English-born American astronomer who was the first to apply laws of atomic physics to the study of the temperature and density of stellar bodies,...
Philosophy
Deceased--Leonard Searle
Leonard SearleOctober 23rd, 1930 to July 2nd, 2010
"Leonard Searle dies at 79; astronomer's work provided key information on the Big Bang"
The former director of the Carnegie Observatories also played a crucial role in the construction of the twin 6.5-meter Magellan telescopes at Carnegie's Las Campanas Observatory in Chile.
by
Thomas H. Maugh II
July 30th, 2010
Los Angeles Times
Astronomer Leonard Searle, a former director of the Carnegie Observatories whose observations provided crucial information in determining the conditions of the Big Bang that created the universe and helped explain how heavy elements are produced in stars, has died. He was 79.
Searle died July 2 at his home in Pasadena, according to the Carnegie Institution for Science in Washington, D.C. No cause of death was released.
Searle also played a crucial role in the construction of the twin 6.5-meter (255-inch) Magellan telescopes at Carnegie's Las Campanas Observatory in Chile, which opened in 2000 and are generally considered to be the best natural imaging telescopes in the world.
He was "a thoughtful man who chose his problems carefully," said astronomer Robert Preston, a director emeritus of the Carnegie Observatories. "The things that he accomplished were of lasting value; they're still used today."
The Big Bang was a singularity that started the formation of the universe and researchers have been curious about the precise conditions that existed during the explosion. That event produced massive numbers of elementary particles that, as the gas expanded and cooled, condensed to form hydrogen, helium and trace amounts of lithium and beryllium. All the rest of the elements in the universe were subsequently created in the nuclear furnaces of stars.
To calculate the temperature and pressure that existed in the Big Bang, it is crucial to know the ratio of helium to hydrogen that existed immediately afterward, and that was a problem Searle and Wallace Sargent attacked.
Most old stars are too cool to cause helium to fluoresce, so it is not possible to measure their helium-to-hydrogen ratio. And in even the hottest old stars, helium has diffused inward to the core, diluting the concentration at the surface and providing a false value for the ratio.
Ultimately, the pair identified small galaxies with slow star formation rates whose helium-to-hydrogen ratios were probably very similar to those at the creation of the universe. The values they obtained are still used in modeling the conditions of the Big Bang.
"That was typical of Leonard," Preston said. "He didn't write lots of papers. He settled on issues of fundamental importance, studied them carefully and then wrote them up. He produced a relatively small number of papers whose impact on the field is large."
Searle and Sargent also developed a model of how hydrogen and helium in the nuclear reactors of stars fused to form all the other heavier elements, a process called chemical evolution. Others termed it the "simple model" because of its clarity and it is still used today to characterize the way a galaxy produces elements and transforms gases into stars.
Searle may be best known for his work, with Robert Zinn, now at Yale University, on how galaxies are formed. Most astronomers had originally believed that galaxies condensed from massive clusters of gas in a uniform process. But by studying small galaxies near the outer fringes of our own Milky Way galaxy, the pair concluded that galaxies grew by swallowing smaller galaxies, so-called primordial fragments.
That process is now the accepted mechanism for galaxy formation and has been verified in many other experiments.
Leonard Searle was born Oct. 23, 1930, in the London suburb of Mitcham. He received his bachelor's degree from the University of St. Andrews in Scotland and his doctorate in theoretical physics from Princeton University.
His first post was at the University of Toronto, but he left in 1960 to join Caltech. Three years later, he joined the faculty of the Mount Stromblo Observatory in Australia. Finally, in 1968, he returned to Pasadena to join the Carnegie Observatories, where he spent the rest of his career.
Searle's wife of 47 years, the former Eleanor Millard, died in 1999. He has no surviving relatives.
- Deceased--space Telescope Herschel
Space Telescope Herschel May 14th, 2009 to April 29th, 2013 "Space Telescope Herschel Ran Out of Liquid Helium Today as Planned" by Mark Hoffman April 29th, 2013 SCIENCE WORLD REPORT The crucial liquid helium coolant of ESA’s Herschel space observatory...
- Allan Sandage...a New Paper By Lynden-bell And Schweizer
Allan Sandage was an observational astronomer who was happiest at a telescope. On Hubble’s sudden death Allan Sandage inherited the programmes using the world’s largest optical telescope at Palomar to determine the distances and number counts of...
- More Stars
I suppose that this news will make one feel better...three times the chance of alien encounter[s]. Regardless, it is humbling. "How Many Stars? Three Times as Many as We Thought, Report Says" by Kenneth Chang December 1st, 2010 The New York Times It...
- Deceased--allan Sandage
Allan Sandage June 18th, 1926 to November 13th, 2010 "Allan R. Sandage dies at 84; cosmologist focused on the age of the universe" The scientist, an assistant to Edwin Hubble in the 1950s, believed the universe to be about 15 billion years old rather...
- Cecilia Helena Payne-gaposchkin...the Sun
Cecilia Helena Payne-Gaposchkin May 10th, 1900 to December 7th, 1979 Cecilia Helena Payne-Gaposchkin was an English-born American astronomer who was the first to apply laws of atomic physics to the study of the temperature and density of stellar bodies,...