Age, Biography and Wiki
Christopher McKee was born on 1942, is a Christopher Fulton McKee is astrophysicist astrophysicist. Discover Christopher McKee'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 82 years old?
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82 years old |
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1942, 1942 |
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1942 |
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We recommend you to check the complete list of Famous People born on 1942.
He is a member of famous with the age 82 years old group.
Christopher McKee Height, Weight & Measurements
At 82 years old, Christopher McKee height not available right now. We will update Christopher McKee's Height, weight, Body Measurements, Eye Color, Hair Color, Shoe & Dress size soon as possible.
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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.
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Christopher McKee Net Worth
His net worth has been growing significantly in 2023-2024. So, how much is Christopher McKee worth at the age of 82 years old? Christopher McKee’s income source is mostly from being a successful . He is from . We have estimated Christopher McKee'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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Not Available |
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Christopher McKee Social Network
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Timeline
Christopher Fulton McKee (born 1942) is an astrophysicist.
McKee attended Phillips Academy and Harvard University, and obtained a Ph.D. from the University of California, Berkeley (UCB) in 1970 under advisor George B. Field.
McKee performed the first simulations of relativistic counter-streaming plasmas as part of his Ph.D. thesis at Berkeley (1970).
He began his study of the interstellar medium by pointing out the existence of reverse shocks in young supernova remnants, and he then analyzed the interaction of a supernova blast wave with interstellar clouds.
In 1974, he was appointed Professor of Physics and Astronomy, University of California at Berkeley.
He is a member of the National Academy of Sciences and has been chair of the UCB Physics Department.
Since joining the Physics and Astronomy Departments in Berkeley in 1974, he has devoted much of his research to studying processes in the interstellar medium, including evaporation of clouds, the structure of shock waves in atomic and molecular gas, and the dynamics of blast waves in both homogeneous and inhomogeneous media.
In collaboration with Jeremiah Ostriker (Columbia University), he developed the three-phase model of the interstellar medium, which has been widely used to organize and interpret observational data.
His research on quasars has included development of the relativistic blast wave model for variability, introduction of reverberation mapping to analyze variable emission line profiles, the two-phase model for quasar emission line regions, and the development of the theory of coronae and winds from accretion disks.
He has developed a self-regulated model for the structure and evolution of molecular clouds, and for the rate of star formation within these clouds.
He established the Berkeley Astrophysical Fluid Dynamics Group with Richard Klein to develop the technique of adaptive mesh refinement for numerical simulations of astrophysical fluid dynamics.
In his three decades as a professor at UCB, he has advised many graduate students and postdoctoral research fellows.
He is a former member (1990) and chairman (2000) of the NASA Astronomy and Astrophysics Survey Committee (the "decadal review") and former Director of the Space Sciences Laboratory (SSL) at UCB.
He was elected a Legacy Fellow of the American Astronomical Society in 2020.
