Ribose and related sugars from ultraviolet irradiation of interstellar ice analogs

Author:

Meinert Cornelia1,Myrgorodska Iuliia12,de Marcellus Pierre3,Buhse Thomas4,Nahon Laurent2,Hoffmann Søren V.5,d’Hendecourt Louis Le Sergeant3,Meierhenrich Uwe J.1

Affiliation:

1. Université Nice Sophia Antipolis, Institut de Chimie de Nice, UMR 7272 CNRS, 28 Avenue Valrose, 06108 Nice, France.

2. Synchrotron SOLEIL, L’Orme des Merisiers, St Aubin BP48, 91192 Gif-sur-Yvette, France.

3. Institut d’Astrophysique Spatiale, CNRS, Université Paris-Sud, Université Paris-Saclay, bât 121, 91405 Orsay, France.

4. Centro de Investigaciones Químicas, Universidad Autónoma del Estado de Morelos, Avenida Universidad 1001, 62209 Cuernavaca, Mexico.

5. Aarhus University, Department of Physics and Astronomy, Ny Munkegade 120, 8000 Aarhus, Denmark.

Abstract

Making ribose in interstellar ices Astrobiologists have long speculated on the origin of prebiotic molecules such as amino acids and sugars. Meinert et al. demonstrated that numerous prebiotic molecules can be formed in an interstellar-analog sample containing a mixture of simple ices of water, methanol, and ammonia. They irradiated the sample with ultraviolet light under conditions similar to those expected during the formation of the solar system. This yielded a wide variety of sugars, including ribose—a major constituent of ribonucleic acid (RNA). Science , this issue p. 208

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference44 articles.

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2. C. Woese The Genetic Code (Harper & Row 1967) pp. 179–195.

3. The origin of the genetic code

4. Evolution of the genetic apparatus

5. Organic Synthesis via Irradiation and Warming of Ice Grains in the Solar Nebula

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