Jorge Fernández Fernández
I am a third year PhD student in the Astronomy and Astrophysics group at the University of Warwick. My supervisor is Prof. Peter Wheatley. I am studying how the evolution of close-in exoplanets is affected by the high energy radiation coming from their host stars.
The Kepler mission has uncovered a surprising number of planets between Earth and Neptune in size that are not present in our Solar System. The masses and sizes of some of these planets are consistent with a solid rocky core surrounded by a large H-rich envelope (mini-Neptunes) that can double the planet's radius and yet comprise less than a percent of its mass; whereas others are most likely entirely rocky (super-Earths). These two populations appear as two distinct peaks in the radius distribution of Kepler planets, the Radius Gap, which is though to arise due to the evaporation of these envelopes. This phenomenon has been directly observed in Lyman-α and Helium triplet transits, in which the extended atmosphere occults a larger amount of stellar photons than expected given the planet's optical radius.
Photoevaporation is a proposed mechanism for evaporation, where high energy radiation emitted by their host stars, namely X-rays and extreme ultraviolet radiation (together XUV), is readily absorbed by the upper layers of the planet's atmospheres. This causes the envelopes to heat-up and expand, with the subsequent escape of material from the planet's gravitational well.
My research focuses on studying the extent to which photoevaporation influences the evolution of young close-in mini-Neptunes and super-Earths.
- Proceedings article. X-ray irradiation of three planets around Hyades star K2-136Link opens in a new window. J. Fernández Fernández and P. J. Wheatley, 2021, doi:10.1002/asna.20210076.
- The young mini-Neptune HD 207496b that is either a naked core or on the verge of becoming oneLink opens in a new window. Barros, S. C. C. ; Demangeon, O. D. S. ; Armstrong, D. J. ; Delgado Mena, E. ; Acuña, L. ; J. ; Fernández, Fernández;
Discovery of an Edge-on Circumstellar Debris Disk Around BD+45° 598: a Newly Identified Member of the β Pictoris Moving Group. S. Hinkley et al., 2021, The Astrophysical Journal, Volume 912, Issue 2, id.115,
- Astrophysics, PhD. University of Warwick (2020-2024). "Studying the extent to which X-ray photoevaporation affects the evolution of exoplanet atmospheres". Supervised by Prof. Peter Wheatley.
- Physics with Astrophysics, MPhys. University of Exeter (2016-2020). Integrated Masters program, combining a 3-year bachelors degree with a final year masters dissertation. "Direct Imaging of Exoplanets & Circumstellar Discs". Supervised by Dr. Sasha Hinkley.
Conferences / Workshops
- New Results in X-ray Astronomy (Leicester, May 2022). The evaporation history of three planets around K2-136.
- XMM-Newton 2021 Science Workshop (Online, May 2021). Analysis of X-ray driven atmospheric loss on three-planet system K2-136.
- STFC Introduction to Astronomy (Online, January 2021). Analysis of X-ray driven atmospheric loss on multiplanetary system K2-136. Link to presentation here.
- National Astronomy Meeting (University of Warwick, 2022)
- UKEXOM (Edinburgh, 2022)
- Athena UK Science Meeting (Leicester, May 2022)
- ESCAPE Data Science Summer School (Online, June 2021)
- UKEXOM (Online, April 2021)
- PX129 (Physics Tutorial)Link opens in a new window, PX146 (Key Skills for Physicists) - First year physics problem classes (2020-2023). Marking problem sheets, assessing the progress of undergraduate students, and delivering a teaching session twice a week both in online and face-to-face formats.
Jorge Fernández Fernández,