Alpha particle X-ray spectrometer

APXS is also an abbreviation for APache eXtenSion tool, an extension for Apache web servers.

An Alpha Particle X-Ray Spectrometer (APXS) (or Alpha Proton X-Ray Spectrometer for the Pathfinder mission) is a device that analyses the chemical element composition of a sample from the scattered alpha particles, emitted protons (for Pathfinder only), and fluorescent X-rays after the sample is irradiated with alpha particles and X-rays from radioactive sources.[1] Since there are faster methods available which do not use radioactive material to analyse the elemental composition of a sample, this compact and low power method is most often used on space missions.

Over the years several modified versions of the APS (without X-ray spectrometer) or APXS have been flown: Surveyor 5-7,[2] Mars Pathfinder,[3] Mars 96,[4] Mars Exploration Rover,[5] Phobos.[6] APS devices will be included on several upcoming missions: Rosetta/Philae, Mars Science Laboratory and Exomars missions.

Contents

Source

Several forms of radiation are used in APXS. They include alpha particles, protons, and X-rays. Alpha particles, protons, and X-rays are emitted during the radioactive decay of unstable atoms. A common source of alpha particles is curium 244. It emits particles with an energy of 5.8 MeV. X-rays of 14 and 18 keV are emitted in the decay of plutonium 240. The Mars Exploration Rovers' Athena payload uses curium 244 witth a source strength of approximately 30 millicuries (1.1 GBq).[7]

Alpha particles

Some of the alpha particles of a defined energy are backscattered to the detector if they collide with an atomic nucleus. The physical laws for Rutherford backscattering in an angle close to 180° are conservation of energy and conservation of linear momentum. This makes it possible to calculate the mass of the nucleus hit by the alpha particle. Light elements absorb more energy of the alpha particle, while alpha particles are reflected by heavy nuclei nearly with the same energy. The energy spectrum of the scattered alpha particle shows peaks from 25% up to nearly 100% of the initial alpha particles. This spectrum makes it possible to determine the composition of the sample, especially for the lighter elements. The low backscattering rate makes it necessary for elongated irradiation, approx 10 hours.

Protons

Some of the alpha particles are absorbed by the atomic nuclei. The [alpha,proton] process produces protons of a defined energy which are detected. Sodium, magnesium, silicon, aluminium and sulfur can be detected by this method. This method was only used in the Mars Pathfinder APXS. For the Mars Exploration Rovers the proton detector was replaced by a second alpha particle sensor.

X-ray

The alpha particles are also able to eject electrons from the inner shell (K- and L-shell) of an atom. These vacancies are filled by electrons from outer shells, which results in the emission of a characteristic x-ray. This process is termed Particle-Induced X-ray Emission and is relatively easy to detect and has its best sensitivity and resolution for the heavier elements.

References

  1. ^ Economou, T.E. ; Turkevich, A.L. ; Sowinski, K.P. ; Patterson, J.H. ; Franzgrote, E.J. (1970). "The Alpha-Scattering Technique of Chemical Analysis". J. Geophysical Research 75 (32): 6514. Bibcode 1970JGR....75.6514E. doi:10.1029/JB075i032p06514. 
  2. ^ , Patterson, J.H. ; Franzgrote, E.J. ; Turkevich, A.L. ; Anderson, W.A. ; Economou, T.E. ; Griffin, H.E. ; Grotch, S.L. ; Sowinski, K.P. (1969). "Alpha-scattering experiment on Surveyor 7 - Comparison with Surveyors 5 and 6". J. Geophysical Research 74 (25): 6120–48. Bibcode 1969JGR....74.6120P. doi:10.1029/JB074i025p06120. 
  3. ^ R. Rieder, H. Wänke, T. Economou, A. Turkevich (1997). "Determination of the chemical composition of Martian soil and rocks:The alpha proton X ray spectrometer". J. Geophysical Research 102 (E2): 4027–4044. Bibcode 1997JGR...102.4027R. doi:10.1029/96JE03918. 
  4. ^ Rieder, R.; Wanke, H.; Economou, T.; Wanke; Economou (1997). "An Alpha Proton X-Ray Spectrometer for Mars-96 and Mars Pathfinder". American Astronomical Society 28: 1062. Bibcode 1996DPS....28.0221R. 
  5. ^ R. Rieder, R. Gellert, J. Brückner, G. Klingelhöfer, G. Dreibus, A. Yen, S. W. Squyres (2003). "The new Athena alpha particle X-ray spectrometer for the Mars Exploration Rovers". J. Geophysical Research 108 (E12): 8066. Bibcode 2003JGRE..108.8066R. doi:10.1029/2003JE002150. 
  6. ^ Hovestadt, D.; Andreichikov, B.; Brückner, J.; Economou, T.; Klecker, B.; Kunneth, E.; Laeverenz, P.; Mukhin, L.; Prilutskii, A.; Radchenko, V.; REppin, C.; Rieder, R.; Sagdeev, R.; Sastri, C.S.; Turkevich, A.; Vasiliev, V.; Wänke, H.; Andreichikov; Bruckner; Economou; Klecker; Kunneth; Laeverenz; Mukhin et al. (1988). "In-Situ Measurement of the Surface Composition of the Mars Moon Phobos: The Alpha-X Experiment on the Phobos Mission". Abstracts of the Lunar and Planetary Science Conference 19: 511. Bibcode 1988LPI....19..511H. 
  7. ^ unknown (unknown). "Alpha Particle X-Ray Spectrometer (APXS) (2 pages)". http://athena.cornell.edu/pdf/tb_apxs.pdf.