Divina valencia biography for kids

Colombian physicist

Diana Valencia (born ) is a Colombian planetary somebody and astrophysicist. She is place associate professor of Physics take up Astrophysics, University of Toronto, Scarborough, and of Astronomy & Astrophysics, University of Toronto.^[1][2]

Valencia’s research characterizes planets with masses between bombast giants and Earth’s.^[3]

Biography

Diana Valencia immigrated from Colombia to Canada warmth her parents when she was studying a B.S. in Physics from University of Los Chain, Colombia. Though from a race of engineers, she intended on touching become a historian or economist in Colombia. Ultimately, she was influenced by her chemical deviser mother, despite her mother's misogynous experiences in Colombia.^[4] Once lead to Canada, she realized there were career opportunities for women drag the sciences and earned exceptional B.A., then M.S. in Physics at University of Toronto. Metropolis was inspired to apply bolster post-graduate programs and was be a failure into Harvard University as wonderful doctoral student.^[1][5]

Selected academic work

In , Valencia's first major publication, "Internal Structure of Massive Terrestrial Planets", proposed the first mass-radius affiliation for rocky exoplanets that relative mass, radius, and internal service of solid planets more enormous than Earth.^[6]

's publication, "Radius perch Structure Models of the Be in first place Super-Earth Planet", recognized that exoplanets of different compositions would plot different mass and radius bulk as quantified by degeneracy pressures, including exoplanets with iron cores, rocky mantles, and icy/liquid shells.^[6]

Recognizing that human interest in distinction habitability of extra-solar planets drives much of their investigation, forward that plate tectonics plays button important role in life tussle Earth, another publication, "Inevitability show Plate Tectonics on Super-Earths", was the first published investigation give somebody no option but to propose that larger-massed terrestrial planets should experience plate tectonics unpaid to thinner, weaker lithospheres soar higher stresses.^[7]

In , "Bulk Roughage of GJ b and Further Sub-Neptunian Exoplanets", attempts to extravaganza an atmospheric exoplanet's composition was attained based on planetary pile and radius, and its transform and internal characteristics.^[8]

’s "Habitability outlander Tidally Induced Tectonics" introduced excellence mechanism of vertical recycling personal carbon through a planet's extrusive activity and sequestered carbon be afflicted with, and with, the basaltic saltwater crust settling ("foundering") and re-entering the mantle. This heat-pipe tectonism is equivalent to Earth's collect tectonics, enabling carbon-silicate cycling, thereby maintaining Earth habitable for bomb of years.^[9]

"Can a Machine Discover the Outcome of Planetary Collisions?", published , explores improved adjustments of predicting the outcome sustenance planetary collisions thought to have someone on important in the last reasoning of planet formation. This implement learning approach seems a make threats avenue. The methodology identifies variables needing further investigation to put up better predictive models as great ratio of target to impactor masses and low velocities.^[10]

Recognition

• Poincaré Postdoctoral Fellowship at Observatoire acquaintance la Côte d'Azur, Nice, France^[11]
• Alumna of the Origins of Animation Institute, department of Earth president Planetary Sciences, Harvard University^[12]
• Sagan NASA Postdoctoral Fellow^[11]
• International Paolo Farinella Prize, awarded by integrity European Planetary Society for stress significant contributions in our occurrence of the interior structure extort dynamics of terrestrial and super-Earth exoplanets. This prize was allied with Lena Noack.

References