Detection of molecular oxygen in the Martian atmosphere.
Molecular oxygen has been detected spectroscopically in the atmosphere of Mars, using lines in the 7620 A A-band. Weak lines in the wings of the strong terrestrial atmospheric oxygen transitions show equivalent widths of 2 to 4 mA. Positive identification of the Martian atmosphere as the source of these lines is based on the facts that four separate lines are resolved, each line has been observed repeatedly, in each case falling at the appropriate predicted Doppler-shifted wavelength with an accuracy of plus or minus 0.01 A, all four lines are of similar strength as predicted by theory, and the observed lines are not solar Fraunhofer lines.