Interplanetary dust, micrometeorites, and meteorites: Chemistry, mineralogy and atmospheric interactions of meteors

37th Aerospace Sciences Meeting and Exhibit

Volumn , Issue , 1999, Pages

  Flynn, George J ^a  

^a STATE UNIVERSITY OF NEW YORK   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

AEROSPACE ENGINEERING; CHEMICAL ANALYSIS; DUST; IONIZATION OF GASES; METEORITES; MINERALS; PARTICLE SIZE ANALYSIS; SILICATES; ZINC;

ATMOSPHERIC ENTRY; ATMOSPHERIC INTERACTION; CHEMICAL COMPOSITIONS; INTERPLANETARY DUST; INTERPLANETARY DUST PARTICLES; LABORATORY ANALYSIS; MINERALOGICAL PROPERTIES; VOLATILE ELEMENTS;

ATMOSPHERIC CHEMISTRY;

EID: 84983140791     PISSN: None     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.2514/6.1999-500     Document Type: Conference Paper

References (40)

1. Anders, E. and Grevesse, N. (1989) Abundances of the elements: Meteoritic and solar, Geochim. Cosmochim. Acta, 53, 197-214.
2. Bandt, D. T. and Consohnagno, G. J. (1997) The porosity of meteorites and asteroids: Results from the Vatican collection, Lunar andPlanet. Sci. XWIII, 159-160.
3. Brownlee, D. E. (1978) Microparticle studies by sampling techniques, in Cosmic Dust (ed. J. A. M. McDonnell), John Wiley 8~ Sons, New York, 295336.
4. Brownlee, D. E., Joswiak, D. J., Love, S. G., Nier, A.O., Schlutter, D. J., and Bradley, J. P. (1993) Identification of cometary and asteroidal particles in stratospheric IDP collections, Lunar andPlanetary Science 115, 205-206.
5. Bums, J. A., Lamy, P. L., and Soter, S. (1979) radiation forces on small particles in the Solar System, Icarus, 40, l-48.
6. Davis, A. M. and Brownlee, D. E. (1993) Iron and nickel isotopic mass fractionation in deep-sea spherules. Lunar h Planet. Sci. 114, 373-374.
7. Durda, D. D., and Flynn, G. J. (1997) Impact disruption of a porous, inhomogeneous target, Meteoritics and Planetay Science, A36-A31.
8. Flynn, G. J. (1989) Atmospheric entry heating: a criterion to distinguish between asteroidal and cometary sources of interplanetary dust. Icarus, 77,287-3 10.
9. Flynn, G. J. (1990) The near-earth enhancement of asteroidal over cometary dust, Proceedings ofthe 2dh Lunar and Planeta y Science Conference, 363-37 1.
10. Flynn, G. J. (1994) Cometary dust: A thermal crietrion to identify cometary samples among the interplanetary dust collected from the stratosphere. In Analysis of Interplanetary Dust (eds., M. E. Zolensky, T. L. Wilson, F. J. M. Rietmeijer, G. J. Flynn), AIP Conference Proc. 3 10, American Institute of Physics, New York, 223-230.
11. Flynn, G. J. (1992) Atmospheric entry survival of large micrometeorites: Implications for their sources and for the cometary contribution to the Zodiacal Cloud, in Asteroids, Comets, and Meteors 1991 (eds. A. W. Harris and E. Bowell), Lunar and Planetary Institute, Houston, TX.
12. Flynn, G. J. and Sutton, S. R. (1991) Cosmic dust particle densities: Evidence for two populations of stony meteorites. Proc. Lunar andPlanet. Sci., 22, 171-184.
13. Flynn, G. J, Sutton, S. R., Bajt, S., Kandk, W., Thomas, K. L., and Keller, L. P. (1993) The volatile content of anhydrous interplanetary dust, Meteoritics, 28, 349-350.
14. Flynn, G. J., Bajt, S., Sutton, S. R., Zolensky, M. E., Thomas, K. L., and Keller, L. P. (1996). The abundance pattern of elements having low nebular condensation temperatures in interplanetary dust particles: Evidence for a new type of chondritic material. In Physics, Chemistry, and Dynamics of Interplanetary Dust (eds. B. A. S. Gustafson and M. S. Hanner), ASP Conference Series, Vol. 104, Astronomical Society of the Pacific, 291-204.
15. Flynn, G. J. and Klack, W. (1998) Densities and porosities of meteorites: implications for the porosities of asteroids, Lunar and Planetaly Science 11…, in press.
16. Flynn, G. J., Keller, L. P., Jacobsen, C, and Wirick, S. (1998a) Carbon and potassium mapping and carbon bonding state measurements on interplanetary dust, Meteoritics, 33, A50.
17. Flynn, G. J., Keller, L. P, Miller, M. A. (1998b) FTIR detection of organic carbon in interplanetary dust particles, Lunar and Planet. Sci. XYIX, in press.
18. Fraundorf, P., Brownlee, D. E., and Walker, R. M. (1982) Laboratory studies of interplanetary dust. In Comets (ed. L. Wilkening), U. of Arizona Press, Tucson, 383-409.
19. Greshake, A., KlGck, W., Flynn Amdt P, Maetz, M. and Bischoff, A. (1995). Volatile element abundances in micrometeorites: Evidence for the loss of copper, germanium, and zinc during atmospheric entry, Lunar and Planetary Science 224, 509-510.
20. Greshake, A., IUBck, W., Arndt, P., Maetz, M., and Bischoff, A. (1996). Pulse-heating of fragments from Orgueil (CI): Simulation of atmospheric entry heating of micrometeorites. In The Interstellar Dust Connection (editor. J. M. Greenberg), Kluwer Academic Publishers, Dordrecht, Netherlands, 303-311.
21. Greshake, A., Kliick, W., Amdt, P. Mae@ M., Flynn, G. J., Bajt, S., and Bischoff, A. (1998). Heating experiments simulating atmospheric entry heating of micrometeorites: Clues to their parent body sources. Meteoritics and Planetary Science, 33,267-290.
22. Gtin, E. and Jessberger, E. K. (1990). “Dust,” in Physics and Chemistry of Comets (ed. W. F. Huebner) Springer-Verlag, New York, 113-176.
23. Jackson, A. and Zook, H. A. (1992) Orbital evolution of dust particles from comets and asteroids. Icarus, 97,70-84.
24. Jenniskens, P. (1995) Meteor stream activity: II. Meteor outbursts, Astronomy and Astrophysics, 295, 206-235.
25. Kliick, W., Flynn, G. J., Sutton, S. R., Bajt, S., and Neuking, K. (1994). Heating experiments simulating atmospheric entry of micrometeorites, Lunar andPlanetaiy Science 141, 713-714.
26. Lipschutz, M. E. and Wollum, D. S. (1988). “Highly Labile Elements,” in Meteorites and the Early Solar System (eds. J. F. Kerridge, and M. S. Matthews), University of Arizona Press, Tucson, Arizona, 462-487.
27. Love, S. G. and Brownlee, D. E. (1993) A direct measurement of the terrestrial mass accretion rate of cosmic dust. Science, 262, 550-353.
28. Love, S. G. and Brownlee, D. E. (1994) Peak atmospheric entry temperatures of micrometeorites, Meteoritics, 29, 60-7 1.
29. Love, S. G., Joswiak, D. J., and Brownlee, D. E. (1993). Densities of 5 to 15 pm interplanetary dust particles, Lunar andPlaneta y Science 122, 90I-902. Low, F. J., Beintema, D. A., Gautier, T. N.
30. Gillett, F. C., Beichman, C. A., Neugebauer, G., Young, E., Aumann, H. H., Boggess, N, Walker, R. G., and Wesselius, P. R. (1984) Infrared cirrus: new components of the extended infrared emission. Astrophys. J., 278, Ll9-L22.
31. Mackinnon, I. D. R. and Rietrneijer, F. J. M. (1987) Mineralogy of chondritic interplanetary dust particles, Reviews Geophys., 25, 1527-1553.
32. Maurette, M, Olinger, C., ChristopheMichel-Levy, M., Vincent, C., and Kurat, G. (1991) A collection of diverse micrometeorites recovered from 100 tonnes of Antarctic blue ice, Nature, 351,44-47.
33. Nishiizumi, K. et al., (1991) Exposure histories of individual cosmic particles. Earth and Planet. Sci. Lett., 104, 315.
34. Opik, E. J., (1951) Collisional probabilities with planets and the distribution of interplanetary matter, Proc. R. Irish Acad., 54, Sect A., 165-199.
35. Scott, E. R. D. and Newsom, H. E. (1989) Planetary compositions - Clues from meteorites and asteroids, Zeitschrzftftir Naturforschung, 44a, 924-934.
36. Steel, D. (1998) The Leonid meteors: compositions and consequences, Astronomy and Geophysics, 39,24-26.
37. Sykes, M. V., Lobofsky, L. A., Hunten, D. M., and Low, F. (1986) The discovery of dust trails in the orbits of periodic comets. Science, 232, 1115 1117.
38. Thomas, K. L., L. P. Keller, G. E. Blanford, and D. S. McKay (1994), Quantitative analysis of carbon in anhydrous and hydrated interplanetary dust particles, in Analysis of Interplanetary Dust (eds. M. E. Zolensky, T. L. Wilson, F. J. M. Rielmeijer, and G. J. Flynn), AIP Cod Proc. 310, AIP Press, New York, 165-172.
39. Vemiani, F. (1969) Structure and fragmentation of meteoroids. Space Sci. Rev., 10,230-261.
40. Wetherill, G. W. (1974) Solar system sources of meteorites and large meteoroids, Annual Reviews of Earth and Planeta y Science, 2,303-33 1.