Table of Contents



The molecular universe

I. Introduction

This section starts with the role of molecules in space.

Then the developments of how to detect molecules in space are briefly stated.

II. The molecular inventory of the interstellar medium

Interstellar medium is where the further generations of stars are created.

Selected papers


# The most stable conformer of glycine
import ssl
ssl._create_default_https_context = ssl._create_unverified_context
from import pubchem_atoms_search

atoms = pubchem_atoms_search(cid=750)
atoms.write('', plain=True)



2020 - Nat Astron - PH3

PH3 is thought to be a biosignature, since the production of PH3 on Earth is often related with the activities of microorganisms. In addition, PH3 gets easily oxidized under Venus's atmosphere and is unstable. The confirmation of PH3 on Venus's atmosphere means that there must be a stable mechanism to generate PH3.

2020 - Nat Astron - An experimental study of the surface formation of methane in interstellar molecular clouds

This paper is the first experimental proof of solid-state CH4 formation by atomic C and H under conditions mimicking those of interstellar molecular cloud environments. It starts with the existence of CH4 in space and interstellar environments where CH4 is detected. Experimentalists have tried to reproduce interstellar environments in laboratories to reveal how CH4 is formed in space. The new part of this work is that it solves a technical issue which is the combination between an atomic carbon source and a ultrahigh vacuum (UHV) set-up. This special design is necessary to study atom-induced surface reactions under molecular cloud conditions.

What is the guess for CH4 formation from observational point of view?

CH4 is expected to be formed by the hydrogenation of C on dust grains, and CH4 ice is strongly correlated with solid H2O.

What systems are investigated in laboratories and what are found by experiments?

Three layers structure: Species/Surface/Substrate

Species Surface Substrate
atomic C + atomic H amorphous carbon (carbonaceous surface) Inert gold substrate (10 K)
atomic C + atomic H + H2O amorphous carbon (carbonaceous surface) Inert gold substrate (10 K)

How to understand the role of H2O?

The Abundance of C2H4 in the Circumstellar Envelope of IRC+10216