Loading...
Please wait, while we are loading the content...
Similar Documents
The formation of racemic amino acids by uv photolysis of interstellar ice analogs
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Sandford, Scott A. Dworkin, Jason P. Cooper, George Allamandola, Louis J. Bernstein, Max P. |
| Copyright Year | 2001 |
| Description | Small biologically relevant organic molecules including the amino acids glycine, alanine, and marine were formed in the laboratory by the UV (Ultraviolet) photolysis of realistic interstellar ice analogs, composed primarily of H2O, and including CH3OH, NH3, and HCN, under interstellar conditions. N-formyl glycine, cycloserine (4-amino-3-isoxazolidinone), and glycerol were detected before hydrolysis, and glycine, racemic alanine, racemic marine, glycerol, ethanolamine, and glyceric acid were found after hydrolysis. This suggests that some meteoritic amino acids (and other molecules) may be the direct result of interstellar ice photochemistry, expanding the current paradigm that they formed by reactions in liquid water on meteorite parent bodies. |
| File Size | 483955 |
| Page Count | 18 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20020044542 |
| Archival Resource Key | ark:/13960/t0zp9040k |
| Language | English |
| Publisher Date | 2001-01-01 |
| Access Restriction | Open |
| Subject Keyword | Geophysics Water Amino Acids Ice Glycine Hydrolysis Ammonia Meteorites Hydrocyanic Acid Interstellar Chemistry Photolysis Methyl Alcohol Optical Activity Glycerols Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |