Age, Biography and Wiki
Diana Valencia is a Colombian physicist and professor at the Universidad Nacional de Colombia. She was born in Bogota, Colombia in 1978. She obtained her PhD in Physics from the Universidad Nacional de Colombia in 2006.
Valencia is an expert in the field of nanotechnology and has published several papers in the field. She is also a member of the Colombian Academy of Sciences and the Colombian Association of Physics.
Valencia has been awarded several awards for her work in nanotechnology, including the National Science Award in 2011 and the National Prize for Science and Technology in 2012. She is also a member of the National System of Researchers in Colombia.
Valencia is married and has two children. She currently resides in Bogota, Colombia.
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45 years old |
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, 1978 |
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Bogota, Colombia |
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Colombia |
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She is a member of famous with the age 45 years old group.
Diana Valencia Height, Weight & Measurements
At 45 years old, Diana Valencia height not available right now. We will update Diana Valencia's Height, weight, Body Measurements, Eye Color, Hair Color, Shoe & Dress size soon as possible.
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Dating & Relationship status
She is currently single. She is not dating anyone. We don't have much information about She's past relationship and any previous engaged. According to our Database, She has no children.
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Diana Valencia Net Worth
Her net worth has been growing significantly in 2022-2023. So, how much is Diana Valencia worth at the age of 45 years old? Diana Valencia’s income source is mostly from being a successful . She is from Colombia. We have estimated
Diana Valencia's net worth
, money, salary, income, and assets.
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$1 Million - $5 Million |
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Pending |
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Under Review |
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Diana Valencia Social Network
Timeline
Valencia, with her Ph.D. advisory team of Richard J. O'Connell and Dimitar D. Sasselov at Harvard University, coined the term Super-Earths to describe extra-solar planets (solid) with masses up to ten times Earth’s mass. Valencia’s research characterizes planets with masses between gas giants and Earth’s.
"Can a Machine Learn the Outcome of Planetary Collisions?", published 2019, explores improved methods of predicting the outcome of planetary collisions thought to be important in the last stages of planet formation. This machine learning approach seems a promising avenue. The methodology identifies variables needing further investigation to build better predictive models as large ratio of target to impactor masses and low velocities.
2018’s "Habitability from Tidally Induced Tectonics" introduced the mechanism of vertical recycling of carbon through a planet's volcanic activity and sequestered carbon onto, and with, the basaltic oceanic crust settling ("foundering") and re-entering the mantle. This heat-pipe tectonism is equivalent to Earth's plate tectonics, enabling carbon-silicate cycling, thereby maintaining Earth habitable for billions of years.
In 2013, "Bulk Composition of GJ 1214b and Other Sub-Neptunian Exoplanets", attempts to show an atmospheric exoplanet's composition was attained based on planetary mass and radius, and its evolution and internal characteristics.
2007's publication, "Radius and Structure Models of the First Super-Earth Planet", recognized that exoplanets of different compositions would have different mass and radius measurements as quantified by degeneracy pressures, including exoplanets with iron cores, rocky mantles, and icy/liquid shells.
Recognizing that human interest in the habitability of extra-solar planets drives much of their investigation, and that plate tectonics plays an important role in life on Earth, another 2007 publication, "Inevitability of Plate Tectonics on Super-Earths", was the first published investigation to propose that larger-massed terrestrial planets should experience plate tectonics due to thinner, weaker lithospheres and higher stresses.
In 2006, Valencia's first major publication, "Internal Structure of Massive Terrestrial Planets", proposed the first mass-radius relationship for rocky exoplanets that associated mass, radius, and internal structure of solid planets more massive than Earth.
Diana Valencia (born 1978) is a Colombian planetary scientist and astrophysicist. She is Assistant Professor of Physics and Astrophysics, University of Toronto, Scarborough, and of Astronomy & Astrophysics, University of Toronto.
