Björn Benneke
Assistant Professor at Université de Montréal
The next five years present a truly unique opportunity in the history of planetary astrophysics. For the first time, the observational techniques, the theoretical models, and a sufficient number of known exoplanets orbiting nearby stars are available to spectroscopically characterize a wide diversity of planets. Planets ranging from blazingly hot giant planets to temperate Earth-sized planets in the habitable zone of their host stars.
Many unanswered questions remain: How and where do planets form? What materials make up their interiors? What gases are in their atmospheres? What role do clouds and hazes play? How big can a terrestrial planet be? How small can a gaseous planet be? And finally, what planets are capable of hosting life?
Professor Benneke’s team is currently in an exceptional position to address many of the questions above because they are currently conducting several unprecedented large observational programs using the Hubble Space Telescope, the Spitzer Space Telescope, and the 10-meter Keck observatories. They have developed powerful analysis and modeling framework to interpret these unique data sets. The main areas that Professor Benneke’s group is working on are:
- Exploring the diversity of planetary atmospheres on super-Earths and exo-Neptunes using Hubble Space Telescope transit spectroscopy. Professor Benneke is the principal investigator of the largest Hubble Space Program in the world to characterize small exoplanets.
- Probing the formation of giant planets using high-resolution near-infrared spectroscopy from 10-meter Keck telescopes
- Atmospheric characterization and mapping of exoplanets using the upcoming James Webb Space Telescope (JWST)
- Understanding the exotic cloud types on exoplanets
- Discovery and initial characterization of prime targets for future JWST characterization using K2, TESS, and ground-based follow-up
Professor Benneke is arriving at Université de Montréal from Caltech where he completed a 4-year postdoctoral fellowship focused on exoplanet observation and modeling. He previously received his PhD at MIT supervised by Sara Seager.
- Caroline Piaulet (PhD 05/2019-, Trottier intern summer 2018, Université de Montréal)
- Stefan Pelletier (PhD 09/2017, Université de Montréal)
- Louis-Philippe Coulombe (MSc 05/2019-, Université de Montréal)
- Prashansa Gupta (Msc 09/2017-, Université de Montréal)
- Steven Rogowski (MSc 09/2017, Trottier intern summer 2017, Université de Montréal)
- Jonathan Chan (MSc 09/2017-, Université de Montréal)
- Merrin Peterson (MSc 05/2018, Trottier intern summer 2017, Université de Montréal)
Former graduate students
- Ian Wong (PhD 2013-2018 at Caltech, co-supervised with Heather Knutson)
- Danielle Piskorz (PhD 2014-2018 at Caltech, co-supervised with Geoffrey Blake)
- Marta Bryan (PhD 2014-2018 at Caltech, co-supervised with Heather Knutson)
- Peter Gao (PhD 2014-2016 at Caltech)
In the media
- http://news.yahoo.com/super-earth-mini-neptune-technique-probe-exoplanet-habitability-104951891.html
- http://www.space.com/23079-alien-planets-super-earth-mini-neptune.html
- http://www.nature.com/news/cloudy-skies-on-nearby-super-earth-1.14450
- http://www.spiegel.de/wissenschaft/weltall/neuer-planetentypus-hubble-enthuellt-ferne-wasserwelt-a-816771.html
- http://www.nature.com/news/wet-exoplanet-has-clear-skies-1.15973
- Based on interview of me: http://www.heise.de/tp/artikel/42/42893/2.html
- http://www.welt.de/wissenschaft/weltraum/article132592830/Wasserdampf-auf-kleinem-Exoplaneten-entdeckt.html
- http://www.astrobio.net/exclusive/5714/super-earth-or-mini-neptune-telling-habitable-worlds-apart-from-lifeless-gas-giants
Contact
Phone : 514-578-2716
Office Phone: 514-343-6111 x 5816
Email: bbenneke@astro.umontreal.ca
Office : Roger-Gaudry Building, D-446