Research & Development World

  • R&D World Home
  • Topics
    • Aerospace
    • Automotive
    • Biotech
    • Careers
    • Chemistry
    • Environment
    • Energy
    • Life Science
    • Material Science
    • R&D Management
    • Physics
  • Technology
    • 3D Printing
    • A.I./Robotics
    • Software
    • Battery Technology
    • Controlled Environments
      • Cleanrooms
      • Graphene
      • Lasers
      • Regulations/Standards
      • Sensors
    • Imaging
    • Nanotechnology
    • Scientific Computing
      • Big Data
      • HPC/Supercomputing
      • Informatics
      • Security
    • Semiconductors
  • R&D Market Pulse
  • R&D 100
    • Call for Nominations: The 2025 R&D 100 Awards
    • R&D 100 Awards Event
    • R&D 100 Submissions
    • Winner Archive
    • Explore the 2024 R&D 100 award winners and finalists
  • Resources
    • Research Reports
    • Digital Issues
    • R&D Index
    • Subscribe
    • Video
    • Webinars
  • Global Funding Forecast
  • Top Labs
  • Advertise
  • SUBSCRIBE

Organic Compound Found in Early Stages of Star Formation

By Queen Mary University of London | June 8, 2017

Scientists seeking to understand the origins of life have found a new organic compound in the material from which a star like the Sun is forming.

Researchers from Queen Mary University of London (QMUL) are part of a team that have for the first time detected methyl isocyanate (or CH3NCO) in a solar-type protostar, the kind from which our Sun and the Solar System formed.

Methyl isocyanate (CH3NCO) is one of a family of prebiotic molecules, thought to be the precursors of more complex compounds, such as peptides and amino acids, associated with living organisms on Earth.

“Our findings indicate that the key ingredients for the origin of life could have been produced at an early stage of the Solar System,” said co-author Dr David Quénard from QMUL’s School of Physics and Astronomy.

The team used data from the ALMA telescope (Atacama Large Millimeter/submillimeter Array) in Chile to detect the compound in the warm, dense inner regions of the cocoon of dust and gas around very young stars in the multiple star system IRAS 16293-2422.

Using a new computer model jointly developed by QMUL and University College London (UCL), they were able to use the new observations to understand more about the chemistry in the proto-stellar material and the mechanisms by which this complex molecule is formed.

Earth and the other planets in our Solar System are formed from the material left over after the formation of the Sun. Studying solar-type protostars can therefore open a window to the past for astronomers, allowing them to observe similar conditions that led to the formation of our Solar System over 4.5 billion years ago.

Finding complex molecules such as methyl isocyanate in a solar-type protostar indicates that planets created around the star could begin their existence with a supply of the chemical ingredients needed to make some form of life.

Scientists believe that some basic prebiotic chemistry, involving molecules that form the building blocks of structures associated with life on Earth, could have developed in space. It is believed that molecules created in clouds of interstellar gas and dust during the early stages of star formation could be transferred to planets and smaller bodies (such as asteroids and comets) forming around stars.

Comets, for example, exhibit a wide variety of complex organic molecules that are also commonly detected in matter that lies between the star systems in a galaxy, referred to as the interstellar medium.

Co-author Dr Izaskun Jiménez-Serra from the School of Physics and Astronomy said: “Our results suggest that the chemical composition of comets may be inherited directly from the interstellar medium.”

Related Articles Read More >

Trump lifts 50-year supersonic ban, paving way for 3.5-hour New York–London trips
Europa’s lost decade: What happens to $5 billion‑plus in planetary R&D when missions die?
Artemis III Orion powers on at Kennedy, marking milestone for 2027 Moon-landing push
MIT’s new sodium fuel cell beats lithium three-to-one for regional aviation
rd newsletter
EXPAND YOUR KNOWLEDGE AND STAY CONNECTED
Get the latest info on technologies, trends, and strategies in Research & Development.
RD 25 Power Index

R&D World Digital Issues

Fall 2024 issue

Browse the most current issue of R&D World and back issues in an easy to use high quality format. Clip, share and download with the leading R&D magazine today.

Research & Development World
  • Subscribe to R&D World Magazine
  • Enews Sign Up
  • Contact Us
  • About Us
  • Drug Discovery & Development
  • Pharmaceutical Processing
  • Global Funding Forecast

Copyright © 2025 WTWH Media LLC. All Rights Reserved. The material on this site may not be reproduced, distributed, transmitted, cached or otherwise used, except with the prior written permission of WTWH Media
Privacy Policy | Advertising | About Us

Search R&D World

  • R&D World Home
  • Topics
    • Aerospace
    • Automotive
    • Biotech
    • Careers
    • Chemistry
    • Environment
    • Energy
    • Life Science
    • Material Science
    • R&D Management
    • Physics
  • Technology
    • 3D Printing
    • A.I./Robotics
    • Software
    • Battery Technology
    • Controlled Environments
      • Cleanrooms
      • Graphene
      • Lasers
      • Regulations/Standards
      • Sensors
    • Imaging
    • Nanotechnology
    • Scientific Computing
      • Big Data
      • HPC/Supercomputing
      • Informatics
      • Security
    • Semiconductors
  • R&D Market Pulse
  • R&D 100
    • Call for Nominations: The 2025 R&D 100 Awards
    • R&D 100 Awards Event
    • R&D 100 Submissions
    • Winner Archive
    • Explore the 2024 R&D 100 award winners and finalists
  • Resources
    • Research Reports
    • Digital Issues
    • R&D Index
    • Subscribe
    • Video
    • Webinars
  • Global Funding Forecast
  • Top Labs
  • Advertise
  • SUBSCRIBE