Stars are born in cold clouds of gas known as the Giant Molecular Clouds. These stellar nurseries determine the rate stars are born, yet what controls their evolution is less clear. My research group models their formation in different environments, using the astrophysics simulation code Enzo. Enzo is known as a hydrodynamical, adaptive mesh refinement code. In more sensible terms, this means the code models the gas on a series of grids whose cell size changes depending on what resolution is required.
My more recent work on planet formation focusses on understanding exoplanet diversity. At the moment, our data on exoplanets is usually limited to size and insolation level (the amount of radiation the planet receives from the star). The fact this is a poor indication of planet conditions can be easily demonstrated within our own Solar System: Venus is very close to the Earth in size and mass and receives only slightly more radiation from the Sun. A guess at the surface temperature if we saw Venus as an exoplanet might be in the region of 27 Celsius: perfect beach weather temperature! Yet, Venus's true surface temperature exceeds 450 Celsius; lead-melting conditions that point to a wildly different evolution.
In my current projects, I have been exploring trends in the current data to try and impute missing data values using neural networks. With my student, Ngan Nguyen, we have also been looking at how planets migrate during the early years of their formation, changing their orbits such that planets found on similar paths may not have similar histories.
[2016 - ] Japan Aerospace Exploration Agency (JAXA), Institute for Space and Astronautical Sciences (ISAS)
Associate Professor in the Division of Solar System Sciences
[2011 - 2016] Hokkaido University, Japan
Assistant/Associate Professor in the Department of Physics, Faculty of Science
[2009 - 2011] McMaster University, Canada
CITA National Postdoctoral Fellow
[2006 - 2009] University of Florida, USA
Theoretical Astrophysics Postdoctoral Fellow
 University of Oxford, UK
D.Phil in computational astrophysics
 Durham University, UK
M.Sci (Hons) Theoretical Physics
From 2012 - 2016, I taught two physics courses at Hokkaido University. These lectures covered core physics topics for first year undergraduates, including classical mechanics, vibrations, waves, optics, thermodynamics, electromagnetism and a touch of quantum mechanics.
Since most of my students were not native-level English speakers, my courses used keynote presentations that included many graphics and movies. I also used the clicker system for in-class questions (keeps students awake and allows me a 5 minute break!). Three or four times during the semester, we watched short movies and read science news stories to see physics beyond the first year syllabus.
I was delighted to be awards the Hokkaido University President's Award for Education in 2014, 2015 and 2016 and be listed as an Excellent Teacher for those last three years.
Recent Journal Papers
- On the effective turbulence driving mode of molecular clouds formed in disc galaxies,
Jin, Keitaro; Salim, Diane M.; Federrath, Christoph; Tasker, Elizabeth J.; Habe, Asao; Kainulainen, Jouni T.
- The language of exoplanet ranking metrics needs to change,
Tasker, Elizabeth; Tan, Joshua; Heng, Kevin; Kane, Stephen; Spiegel, David; Brasser, Ramon; Casey, Andrew; Desch, Steven; Dorn, Caroline; Hernlund, John; Houser, Christine; Laneuville, Matthieu; Lasbleis, Marine; Libert, Anne-Sophie; Noack, Lena; Unterborn, Cayman; Wicks, June.
Nature Astronomy, 02/2017
- Star formation and ISM morphology in tidally induced spiral structures,
Pettitt, Alex R.; Tasker, Elizabeth J.; Wadsley, James W.; Keller, Ben W.; Benincasa, Samantha M.