Jaehan Bae
Postdoctoral Fellow

Jaehan Bae

Research Interests

protoplanetary disks; planet-disk interactions; planet formation; hydrodynamic/magnetohydrodynamic instabilities; accretion disks; FU Orionis objects; exoplanets


B.S., Astronomy, Seoul National University (2006); M.S., Astronomy, Seoul National University (2008); Ph.D. Astronomy & Astrophysics, University of Michigan (2017)

Contact & Links

  • 202-478-8863 | fax: 202-478-8821
  • jbae at carnegiescience.edu
  • Department of Terrestrial Magnetism
    Carnegie Institution of Washington
    5241 Broad Branch Road, NW
    Washington, DC 20015-1305
  • curriculum vitae
  • Publications
  • Personal Website


A movie of the surface density evolution of a circumstellar disk with a Jupiter-mass planet at (X, Y) = (-1, 0), showing that one planet can create multiple concentric rings and gaps in the background disk through shocks at spiral arms.

Jaehan Bae is interested in the dynamics of planet-forming, young circumstellar disks. He uses numerical simulations to model signatures of forming planets in circumstellar disks, aiming to interpret high-resolution observations from new-generation facilities and to guide future observations to uncover forming planets.

Recently, Jaehan has been working on various aspects of spiral waves -- one of the outcomes of planet-disk interactions --, including (1) the formation of multiple spiral arms from a planet; (2) the formation of multiple concentric rings and gaps through spiral shocks; and (3) an instability of spiral waves that dissipates the spiral waves themselves. Developing upon these theoretical underpinnings, Jaehan hopes to provide a more complete picture of the evolution of planet-forming circumstellar disks including our own proto-solar nebula.