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Microspherulite

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450:). They may be made up of organic-inorganic compounds and provided with different properties. In fact, commercially, microspheres can be found manufactured from materials such as glass, polymers (polyethylene, polystyrene) or ceramic. Microspheres can be solid or hollow, and so their density will be very different as well as their applications. Hollow microspheres usually are added to reduce the density of a material. Solid microspheres have numerous applications depending on their size and their manufacture material. Solid glass microspheres are used in fields such as roads and streets signaling (Figure 3). They are added to paintings used for traffic signs and roadway surface signaling to incorporate the retroreflective effect. So they improve the night visibility of the way. 90: 412: 226: 557: 504: 541: 343:(subaerial environment) can have pisolitic structure. They usually reach 5–8 mm in diameter and for this reason they can not strictly be considered microspherulites. Dunham (1969) considered them associated to caliches, while Pray and Esteban (1977) suggested they were formed by inorganic precipitation from 150:
Impact spherulites occur when a large extraterrestrial object strikes Earth at cosmic velocity, melts and vaporizes, silicate materials can condense into high spheroidal, sand-sized particles deposited around the point of impact. Unaltered impact spherulites consist entirely of glass
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of material in solution, much as salt crystallizes from water during evaporation. In the former case they have thin concentric layers, and in the latter they have radiating sprays of crystals. However, a combination of both processes can be found. Microbes could contribute to their
147:. During this melt stage a significant loss of mass can occur through holes in their surface. The degree of heating and their original composition determine that only a few minerals have been founded in micrometeorites. They have not yet been properly classified. 367:. Chondrules range in diameter from a few micrometres to over 1 cm. They are formed by rapid heating of solid precursor material and subsequent melting, followed by slow cooling. Their main composition is silicate minerals such as olivine and 527:
facies Permian Reef complex, Guadalupe Mountains, New Mexico and West Texas. 1977 Field Conference Guidebook. Society of Economic Paleontologists and Mineralogists, Permian Basin Section, Publication 77-16: 479-483.
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Glass, B.P., Burns, C.A., Crosbie, J.R., DuBois, D.L., 1985. Late Eocene North American Microtektites and Clinopyroxene-Bearing Spherules, Proceedings of the Sixteenth Lunar and Planetary Science Conference. Part 1.
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Verrecchia, E.P., Freytet, P., Verrecchia, K.E., Dumont, J.L., 1995. Spherulites in calcrete laminar crusts: biogenic CaCO3, precipitation as a major contributor to crust formation. J. Sed. Research A65, 690–700.
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Dunham, R.J., 1969. Vadose pisolites in the Capitan Reefs (Permian) New Mexico and Texas, in Depositional Environments in carbonate rocks: Soc. Econ. Palaeontologists and Mineralogists Spec. Publ. 14, 182-191.
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Artefacts are spherules intentionally produced spherical particles for use in industry or medicine. The shape is often perfectly spherical, truly uniform and size ranging ~ 50 nm to 1000 nm (
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combustion processes of fuels, and may be coated with a layer of adsorbed hydrocarbons, sulfates or both. These particles are hollow microspherules that are black in colour, and made up of carbon or
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Biolites are biologically produced, many organisms can produce mineral particles dubbed in general biolites. Their shape, size and composition may be very varied. As examples we can cite
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of well-defined minerals, together with non-crystalline compounds, with axial geometry and a characteristic depression (vortex), structured around a coarse-grained core with a
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Bubbles include frequently unstable spherules which may be produced by the dispersion of two immiscible fluids forming an emulsion. Usually this term is applied to air-water
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Díaz-Hernández, J.L., Párraga, 2008. The nature and tropospheric formation of iberulites: Pinkish mineral microspherulites. Geochimica et Cosmochimica Acta 72, 3883–3906.
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Díaz-Hernández, J.L., 2000. Aportaciones sólidas a la atmósfera originadas por un incendio forestal en el ámbito mediterráneo. Estudios Geológicos 56, 153–161.
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are microscopic spherical particles with diameter less than two mm, usually in the 100 micrometre range, mainly consisting of mineral material (the Greek
407:, spherical to ellipsoidal in shape and with sizes between 0.03 and 0.15 mm. They are thought to be faecal particles from aquatic organisms. 352:
Aerolite is a generic term indicating lithogenic elements gathered from the atmosphere. This term does not imply sphericity or microscopic size.
253:-water-gas interactions. The modal size is in the 60-90 micrometre range, and the shapes are almost perfect spheres. Their name comes from the 116:(egg). They are formed by growing larger and accreting material as they move around. They accomplish this either (a) by physical attachment of 481:
Smit, J., 1999: The global stratigraphy of the. Cretaceous-Tertiary boundary impact ejecta. Annu. Rev. Earth Planetary Science, 27: 75-113.
155:) or a combination of glass and crystals grown in flight (microkrystites). Primary crystals are only common in microspherulites from two 41:
this contribution is possible) or human activity, are considered to be microspherulites. Generally speaking, the common feature (
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Several types of these forms are found in nature. Depending on the formational environment, microspherulites can be classed as
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Pisolites are spheroidal particles, larger in size and commonly more distorted than ooids. The name derives from the Greek
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means "stone"). Only bodies created by natural physico-chemical processes, with no contribution of either biological (in
139:, whose dimensions must range from tens of micrometres to one millimetre. They correspond to pieces of extraterrestrial 493: 561: 469: 229:
Figure 2: Group of iberulites observed under Scanning Electron Microscope (SEM). The arrows show vortex position.
529: 257:, indicating the place where they were discovered. They are related to intrusions of aerosol plumes from the 45:) indicates that each sphere represents an internal equilibrium of forces within a fluid medium (water, air). 582: 164: 17: 135:
Micrometeorites are typically metallic microspherules (iron or iron and nickel) but can also be formed by
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Figure 3: Solid glass microspheres used like ingredients in road and street signaling paintings.
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Esteban, M., Pray, L.C., 1977. Origin of the pisolite facies of the shelf crest. In: Upper
432: 364: 8: 577: 424:, but it is also valid for water-air (hazes, drops) or other liquid fluids (oil-water). 270: 387: 340: 254: 136: 99: 403:
Pellets are those homogeneous aggregates with no internal structure, consisting of
294: 310: 290: 282: 395: 261:. The mineralogy of the core (tens of micrometres thick) is commonly formed by 214: 120:
material as they roll around, much in the manner of a snowball, and (b) by the
58: 398:. Studies have confirmed that microorganisms are able to precipitate minerals. 571: 278: 277:, while the most frequent minerals of the rind (a few micrometres thick) are 258: 242: 160: 89: 443: 524: 447: 411: 246: 156: 117: 245:
rind, and pinkish colour (Figure 2). They are formed at present in the
201: 196: 184: 140: 42: 371:, surrounded by feldspars (crystalline or glassy); minor minerals are 225: 391: 360: 356: 234: 111: 103: 74: 70: 62: 436: 421: 368: 336: 332: 306: 274: 210: 188: 180: 110:
ranges between 0.25 and 2 mm. The name derives from the Greek
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Figure 1: Oolites observed with a transmitted light microscope.
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Oolites are internally structured spheres, composed mainly by
376: 344: 428: 107: 167:(K/T boundary) layer. Other crystalline phases may be 439:. The size ranges from tens to a hundred micrometres. 81:, pellets, bubbles, or carbonaceous microspherules. 431:particle floating in the atmosphere, produced by 159:impact layers: the Upper Eocene microkrystite or 569: 355:Chondrules are the microscopic constituents of 102:(Figure 1). They are a type of constituent in 427:Carbonaceous microspherules are a type of 183:. Frequently the crystals are replaced by 394:) and the calculi resulting from various 410: 224: 88: 14: 570: 317: 84: 129: 24: 533: 517: 508: 497: 486: 475: 461: 25: 594: 549: 446:), or 1 ÎĽm to 1000 ÎĽm ( 363:that fall to the Earth per the 48: 555: 281:, mainly smectites (beidellite, 470:Journal of Geophysical Research 327:(pea). Mineral concentrations ( 13: 1: 454: 165:Cretaceous-Paleogene boundary 112: 7: 10: 599: 359:that represent 80% of the 163:spherule layer and the 39:sedimentary environments 416: 230: 122:chemical precipitation 94: 61:, impact spherulites, 414: 375:, metallic Fe-Ni and 228: 92: 583:Atmospheric sciences 564:at Wikimedia Commons 365:Meteoritical Society 339:) and the pedogenic 293:and impregnation of 106:. The size of these 318:Other related terms 85:Aqueous environment 417: 386:(compounds of the 231: 145:Earth’s atmosphere 130:Aerial environment 95: 560:Media related to 388:vestibular system 255:Iberian Peninsula 137:silicate minerals 100:calcium carbonate 16:(Redirected from 590: 559: 543: 537: 531: 521: 515: 512: 506: 501: 495: 490: 484: 479: 473: 472:90, D 175-D 196. 465: 405:micritic calcite 396:histopathologies 295:sulfate minerals 173:Fe-rich pyroxene 115: 28:Microspherulites 21: 598: 597: 593: 592: 591: 589: 588: 587: 568: 567: 562:Microspherulite 552: 547: 546: 538: 534: 522: 518: 513: 509: 502: 498: 491: 487: 480: 476: 466: 462: 457: 320: 283:montmorillonite 239:co-associations 187:phases such as 132: 87: 59:micrometeorites 51: 23: 22: 15: 12: 11: 5: 596: 586: 585: 580: 566: 565: 551: 550:External links 548: 545: 544: 532: 516: 507: 496: 485: 474: 459: 458: 456: 453: 452: 451: 440: 425: 409: 408: 400: 399: 380: 353: 349: 348: 319: 316: 315: 314: 223: 222: 148: 131: 128: 127: 126: 86: 83: 50: 49:Classification 47: 9: 6: 4: 3: 2: 595: 584: 581: 579: 576: 575: 573: 563: 558: 554: 553: 542: 536: 530: 526: 520: 511: 505: 500: 494: 489: 483: 478: 471: 464: 460: 449: 445: 441: 438: 434: 433:anthropogenic 430: 426: 423: 419: 418: 413: 406: 402: 401: 397: 393: 389: 385: 381: 378: 374: 370: 366: 362: 358: 354: 351: 350: 346: 342: 338: 334: 330: 326: 322: 321: 312: 308: 304: 300: 296: 292: 288: 284: 280: 279:clay minerals 276: 272: 268: 264: 260: 259:Sahara desert 256: 252: 248: 244: 240: 236: 233: 232: 227: 220: 216: 212: 208: 204: 203: 198: 194: 190: 186: 182: 178: 174: 170: 166: 162: 161:clinopyroxene 158: 154: 153:microtektites 149: 146: 142: 138: 134: 133: 123: 119: 114: 109: 105: 101: 97: 96: 91: 82: 80: 76: 72: 68: 64: 60: 56: 46: 44: 40: 37: 33: 29: 19: 18:Microspherule 535: 519: 510: 499: 488: 477: 463: 448:microspheres 372: 324: 289:, amorphous 238: 218: 200: 172: 125:development. 118:fine-grained 52: 31: 27: 26: 525:Guadalupian 444:nanospheres 249:by complex 247:troposphere 202:K-feldspars 157:Phanerozoic 578:Mineralogy 572:Categories 455:References 373:Fe-sulfide 361:meteorites 357:chondrites 235:Iberulites 219:carbonates 197:glauconite 185:diagenetic 141:meteoroids 75:chondrules 63:iberulites 43:sphericity 422:emulsions 392:inner ear 337:siderites 333:limonites 311:chlorides 275:feldspars 181:feldspars 104:limestone 71:aerolites 67:pisolites 437:graphite 384:otolites 369:pyroxene 341:caliches 329:bauxites 307:jarosite 297:(mainly 271:dolomite 243:smectite 215:chlorite 211:sericite 189:goethite 79:biolites 390:of the 303:alunite 267:calcite 251:aerosol 177:spinels 169:olivine 55:oolites 36:aqueous 377:oxides 345:brines 309:) and 299:gypsum 291:silica 287:illite 285:) and 263:quartz 217:, and 207:quartz 193:pyrite 325:pisos 113:ooion 108:ooids 32:litos 429:soot 305:and 273:and 237:are 179:and 574:: 335:, 331:, 301:, 269:, 265:, 213:, 209:, 205:, 199:, 195:, 191:, 175:, 171:, 77:, 73:, 69:, 65:, 57:, 379:. 347:. 313:. 221:. 151:( 20:)

Index

Microspherule
aqueous
sedimentary environments
sphericity
oolites
micrometeorites
iberulites
pisolites
aerolites
chondrules
biolites

calcium carbonate
limestone
ooids
fine-grained
chemical precipitation
silicate minerals
meteoroids
Earth’s atmosphere
microtektites
Phanerozoic
clinopyroxene
Cretaceous-Paleogene boundary
olivine
spinels
feldspars
diagenetic
goethite
pyrite

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