Oral: A panel discussion on Hot Corinos and protoplanetary disks
ORAL
Abstract
Hot Corinos and the regions of planet formation, protoplanetary disks are reservoirs of organic molecules predicted by chemical models and confirmed by observations. The organic inventory of hot Corinos and protoplanetary disks will be discussed in a panel discussion. The broad topics of the discussion session will be the chemical inventory of Hot corinos and protopanetary disks: An observer’s view, a modelers’ view and an experimentalists’ view.
1. How can we enhance our understanding of the chemistry and physics of hot corinos and protoplanetary disks to improve the interpretation of observational data?
2. What are the primary challenges and opportunities in the field of molecular spectroscopic measurements and ab initio studies for hot corinos and protoplanetary disks?
3. How can we create an inclusive workplace environment that encompasses a broad range of perspectives and backgrounds?
1. How can we enhance our understanding of the chemistry and physics of hot corinos and protoplanetary disks to improve the interpretation of observational data?
2. What are the primary challenges and opportunities in the field of molecular spectroscopic measurements and ab initio studies for hot corinos and protoplanetary disks?
3. How can we create an inclusive workplace environment that encompasses a broad range of perspectives and backgrounds?
* NASA ROSES Emerging Worlds NNH20ZDA001N-EWThe Production ofAstrobiologically Important Organics During Early Planetary System Formation and Evolution”, NASA Work Package.
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Presenters
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Partha P Bera
NASA Ames Research Center
Authors
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Partha P Bera
NASA Ames Research Center
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Alexander Tielens
University of Leiden, Leiden Univ, Leiden University