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Missing Links in Planet Formation: From Embedded Disks to Planets
작성자 : 한국천문학회 등록일시 : 2026-05-26 13:13:25
첨부파일 :

Dear Colleagues,

The deadline of abstract submission for oral presentations at the international conference “Missing Links in Planet Formation: From Embedded Disks to Planets,” which will be held in Taipei, Taiwan, in November 2026, is approaching: May 31, 2026. The meeting will bring together researchers working on the formation and evolution of protoplanetary disks, with a particular focus on the critical stages linking embedded disks to planet formation.

We warmly invite the community to participate in this conference and look forward to welcoming you to Taipei. Please note that registration may close earlier if the number of participants exceeds approximately 100.

Best regards,
Nagayoshi Ohashi
on behalf of the organizers

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Dear Colleagues,

We are pleased announce that we are organizing an international conference entitled
"Missing Links in Planet Formation: From Embedded Disks to Planets",
which will be held at  Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taipei, Taiwan from  November 9 to 13, 2026.
We expect approximately 100 participants to attend the conference.
Please mark your calendar if you are interested in attending the conference,

Disks around Class 0/I protostars represent the earliest stages of disk assembly, during which mass and angular momentum are still actively exchanged with the surrounding envelopes. These young disks are crucial for understanding how stars and planets form, as they set the initial conditions for subsequent disk evolution and potential early planet formation. Recent observations have revealed a wide diversity in physical and chemical properties of these embedded disks, including substructures and signs of dust evolution, some of which differ significantly from those seen in more evolved Class II disks. These findings suggest that key processes such as grain growth and planet formation may begin much earlier than previously thought. Establishing the link between these embedded disks and the more evolved Class II stage is therefore essential for building a continuous picture of disk evolution and the emergence of planetary systems. By bringing together new observations, theoretical models, and simulations, this conference aims to explore the physical and chemical processes that shape disks from their youngest phases onward.

Key topics of the conference include:
  • Disk formation and early evolution
  • Dust properties and growth
  • Disk physical structures and substructures
  • Early planetesimal and planet formation
  • Magnetic fields and angular momentum transport
  • Accretion mechanisms and episodic accretion
  • Disk chemistry from embedded to evolved stages
SOC
  • Anders Johansen (Globe Institute, University of Copenhagen / Lund University)
  • Jes Jørgensen (Niels Bohr Institute, Denmark)
  • Akimasa Kataoka (NAOJ, Japan)
  • Nagayoshi Ohashi (ASIAA, Taiwan)
  • John Tobin (NRAO, USA)
  • Yusuke Tsukamoto (Kagoshima University, Japan)
  • Coco Zhang (University of Wisconsin–Madison, USA)
LOC
  • Cindy Chiu (ASIAA)
  • Grace Huang (ASIAA)
  • Shirley Huang (ASIAA)
  • Patrick Koch (ASIAA)
  • Tina Lin (ASIAA)
  • Nagayoshi Ohashi (ASIAA)
  • Hsi-Wei Yen (Chair: ASIAA)
More details including the information on the registration will be announced in the 2nd circular. We look forward to seeing you at the conference.
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이전글 [KGO]Gemini Fast Turnaround Deadline: May 31, 2026 NOON HST
다음글 [K-GMT SP UM 2026] K-GMT Science Program Users Meeting 2026: the 1st circular
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