SCL Seminar by Marija Janković

You are cordially invited to the SCL seminar of the Center for the Study of Complex Systems, which will be held on Thursday, 19 March 2026 at 15:00 in the library reading room "Dr. Dragan Popović" of the Institute of Physics Belgrade. The talk entitled

From discs of gas and dust to planets and planetesimals

will be given by Marija Janković (Scientific Computing Laboratory, Institute of Physics Belgrade). The abstract of the talk:

Today we know about thousands of planets outside of Solar system. Planets form in discs of gas and dust that surround young stars. In this gas and dust it is small planetesimals that form first, and then the planets. After a few million years, these discs disperse, and what remains are not only planets, but also rings of planetesimals which did not grow - asteroids and comets. Planetesimals and planets continue to evolve for billions of years, due to stellar irradiation, mutual gravitational interactions and mutual collisions. In this talk we will cover numerical research of these and other phenomena that shape planetary systems, and also the most recent astrophysical observations which can be used to test our theories.

References:

M.R. Janković, N. Pawellek, J. Zander, T. Löhne, A.V. Krivov, J. Olofsson, A. Brennan, J. Milli, M. Bonduelle, M.C. Wyatt, A.A. Sefilian, T. Pearce, S. Mac Manamon, Y. Han, S. Marino, L. Matrà, A. Moór, M. Booth, E. Chiang, E. Mansell, P. Weber, A.M. Hughes, D.J. Wilner, P. Luppe, B. Zawadzki, C. del Burgo, Á. Kóspál, S. Pérez, J.M. Carpenter, Th. Henning, The ALMA survey to Resolve exoKuiper belt Substructures (ARKS). X. Interpreting the peculiar dust rings around HD 131835, A&A 705, A204 (2026)

Marija R. Janković, Mark C. Wyatt, Torsten Löhne, Collisional damping in debris discs: Only significant if collision velocities are low, A&A, 691, A302 (2024)

Marija R. Janković, Subhanjoy Mohanty, James E. Owen, Jonathan C. Tan, MRI-active inner regions of protoplanetary discs – II. Dependence on dust, disc, and stellar parameters, MNRAS 509, 4, 5974–5991 (2022)

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