11-15 May 2020
Leibniz Institute for Astrophysics Potsdam (AIP)
Europe/Berlin timezone

An Origin of Misaligned Disks and Planetary Orbits: Angular Momentum Accretion in Star Formation Process

15 May 2020, 09:50
20m
Lecture Hall (Leibniz Institute for Astrophysics Potsdam (AIP))

Lecture Hall

Leibniz Institute for Astrophysics Potsdam (AIP)

An der Sternwarte 16 14482 Potsdam, Germany
Oral presentation Main conference Transition Disks & Irregular Structure

Speaker

Prof. Shu-ichiro Inutsuka (Nagoya University)

Description

I try to explain the primordial origin of misalignment between the disk rotation and host star’s rotation from the context of the disk formation. Theoretical and observational investigations have provided convincing evidence for the formation of molecular cloud cores by the gravitational fragmentation of filamentary molecular clouds, which has important implication for the origin of the stellar initial mass function. On the other hand, the size and total angular momentum of a protoplanetary disk are supposed to be directly related to the rotational property of the parental molecular cloud core where the central protostar and surrounding disk are born. Our recent analysis concludes that both the mass function and angular momentum distribution of molecular cloud core are the natural outcome of transonic turbulence with Kolmogorov spectrum in parental filamentary molecular clouds. The implication of this identification is non-homogeneous angular momentum distribution inside a molecular cloud core. The actual angular momentum accretion onto a young stellar object in the core should create misalignment of disk surrounding the star. We show the probability distribution of the misalignment as a function of disk mass. This finding may explain the origin of misaligned planets created in those disks.

Primary author

Prof. Shu-ichiro Inutsuka (Nagoya University)

Presentation Materials

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