The color of the Kuiper belt Core     

Amanda A.S. Gulbis  J.L. Elliot  Julia F. Kane 《Icarus》2006,183(1):168-178

Recent dynamical analyses of the Kuiper belt have introduced a rigorous classification scheme, determined the mean orbital plane, and identified “Core” and “Halo” populations as a function of inclination with respect to this plane (Elliot, J.L., Kern, S.D., Clancy, K.B., Gulbis, A.A.S., Millis, R.L., Buie, M.W., Wasserman, L.H., Chiang, E.I., Jordan, A.B., Trilling, D.E., Meech, K.J., 2005. Astron. J. 129, 1117-1162). Here, we use new observations and existing data to investigate the colors of Kuiper belt objects (KBOs) within this framework. With respect to the bulk KBO color distribution (all objects for which we have B-V and V-R colors; median B-R=1.56), we find that the population of objects classified following (Elliot, J.L., Kern, S.D., Clancy, K.B., Gulbis, A.A.S., Millis, R.L., Buie, M.W., Wasserman, L.H., Chiang, E.I., Jordan, A.B., Trilling, D.E., Meech, K.J., 2005. Astron. J. 129, 1117-1162) as Classical tends to be red (B-R>1.56) while the Scattered Near population is mostly neutral (B-R<1.56). Colors of Scattered Extended and Resonant objects are consistent with the bulk distribution. Separating objects into specific resonances demonstrates that the color of the Resonant sample is dominated by KBOs in the 3:2 resonance, which is consistent with previous findings. Unlike the objects in the 3:2 resonance, however, the majority of objects in the 5:2 resonance are neutral and all but one of the objects in the 4:3, 5:3, 7:4, 2:1, and 7:3 resonances are red. In particular, the objects in the 7:4 resonance are remarkably red. We find that the colors of KBOs in the Core (low-inclination) and Halo (high-inclination) are statistically different, with Core objects being primarily red and Halo objects having a slight tendency to be neutral. Notably, virtually all of the non-Resonant Core objects are red. This combination of low inclination, unperturbed orbits and red colors in the Core may be indicative of a relic grouping of objects.  相似文献   

沂水县龙泉站金矿地质特征及找矿前景     

李洪奎  李英平  田京祥  郝兴中  李秀章 《山东国土资源》2005,(Z1)

沂水县龙泉站金矿位于沂沭断裂带中段,受沂水汤头断裂控制。金矿体产于沂水汤头断裂主裂面下盘的糜棱岩化碎裂岩和花岗质碎裂岩中,已初步圈出6个金矿体。此外,在牛家小河、石崖官庄、郑家庄地区也发现有较好的矿化显示。通过综合研究,认为该地区金矿化与韧性剪切构造带关系密切,且具有较好的找矿前景。  相似文献   

The surface composition of Trojan asteroids: constraints set by scattering theory     

J.P. Emery  R.H. Brown 《Icarus》2004,170(1):131-152

We present the results of spectral modeling of 17 Trojan asteroids. The surface composition of this group of objects (located just beyond the main belt, trapped in Jupiter's stable Lagrange points) remains uncertain due to an absence of diagnostic absorption features in their spectra. We quantitatively analyze spectra of these objects covering the range 0.3-4.0 μm using the formulation for scattering in a particulate medium developed by Hapke. Since the widest spectral range possible is desired to provide the most robust results, recently measured near-IR spectra are combined with previously published visible and near-IR data. These composite spectra are converted to and modeled in terms of geometric albedo to provide the additional constraint of the absolute brightness of the asteroids. It is important that this modeling is performed for a large number of objects, and results are derived based on trends among best-fit models. Under this rigorous examination, we find that it is unlikely that the red spectral slope is a result of organics on the surfaces, due mainly to the lack of absorptions in the L-band. Instead, anhydrous silicates adequately describe the spectral characteristics of this group of objects. A significant fraction of carbonaceous material is also likely present, but is not responsible for the red spectral slope in these models. Also, using these models, we estimate that these surfaces contain at most a few wt% of H₂O ice and no more than 10-30 wt% of hydrated silicates.  相似文献   

河南省西峡北部金矿分布特征浅析     

杨崇辉  韩志勇  张寿广  卢欣祥  董有  常秋玲 《河南国土资源》1994,(4)

从剪切带及原岩建造分析入手，论述了工作区内金矿的分布特征和主要控矿因素。区内的金矿床（点）无论其物质来源和时代如何，就其空间位置而言绝大多数金矿直接产在剪切变形变质带─—脆性及脆－韧性剪切带中。Ｆｅ／（Ｆｅ＋Ｍｇ）高比值的容矿岩石有利于金的沉淀富集。  相似文献   

On The Origin of The High-Perihelion Scattered Disk: The Role of The Kozai Mechanism And Mean Motion Resonances     

Rodney S. Gomes  Tabaré Gallardo  Julio A. Fernández  Adrián Brunini 《Celestial Mechanics and Dynamical Astronomy》2005,91(1-2):109-129

We study the transfer process from the scattered disk (SD) to the high-perihelion scattered disk (HPSD) (defined as the population with perihelion distances q > 40 AU and semimajor axes a>50 AU) by means of two different models. One model (Model 1) assumes that SD objects (SDOs) were formed closer to the Sun and driven outwards by resonant coupling with the accreting Neptune during the stage of outward migration (Gomes 2003b, Earth, Moon, Planets 92, 29–42.). The other model (Model 2) considers the observed population of SDOs plus clones that try to compensate for observational discovery bias (Fernández et al. 2004, Icarus , in press). We find that the Kozai mechanism (coupling between the argument of perihelion, eccentricity, and inclination), associated with a mean motion resonance (MMR), is the main responsible for raising both the perihelion distance and the inclination of SDOs. The highest perihelion distance for a body of our samples was found to be q = 69.2 AU. This shows that bodies can be temporarily detached from the planetary region by dynamical interactions with the planets. This phenomenon is temporary since the same coupling of Kozai with a MMR will at some point bring the bodies back to states of lower-q values. However, the dynamical time scale in high-q states may be very long, up to several Gyr. For Model 1, about 10% of the bodies driven away by Neptune get trapped into the HPSD when the resonant coupling Kozai-MMR is disrupted by Neptune’s migration. Therefore, Model 1 also supplies a fossil HPSD, whose bodies remain in non-resonant orbits and thus stable for the age of the solar system, in addition to the HPSD formed by temporary captures of SDOs after the giant planets reached their current orbits. We find that about 12 – 15% of the surviving bodies of our samples are incorporated into the HPSD after about 4 – 5 Gyr, and that a large fraction of the captures occur for up to the 1:8 MMR (a ⋍ 120 AU), although we record captures up to the 1:24 MMR (a ≃ 260 AU). Because of the Kozai mechanism, HPSD objects have on average inclinations about 25°–50°, which are higher than those of the classical Edgeworth–Kuiper (EK) belt or the SD. Our results suggest that Sedna belongs to a dynamically distinct population from the HPSD, possibly being a member of the inner core of the Oort cloud. As regards to 2000 CR₁₀₅ , it is marginally within the region occupied by HPSD objects in the parametric planes (q,a) and (a,i), so it is not ruled out that it might be a member of the HPSD, though it might as well belong to the inner core.  相似文献   

Evolution of regional metamorphism in the Cape Smith Thrust Belt (northern Quebec, Canada): interaction of tectonic and thermal processes     

M. R. ST-ONGE  S. B. LUCAS 《Journal of Metamorphic Geology》1991,9(5):515-534

Abstract Syn-metamorphic re-imbrication of the internal part of thrust belts can result in distinct pressure–temperature–time–deformation ( P–T–t–d ) pathways for different structural–metamorphic domains. In the early Proterozoic Cape Smith Thrust Belt (Canada), an external (piggyback-sequence thrusting) domain is characterized by thermal peak metamorphism occurring after deformation. In contrast, thermal peak metamorphism in an internal domain occurred during re-imbrication by out-of-sequence thrusting. The interactions of tectonic and thermal processes have been studied using three methods: (i) qualitative evaluation of the timing between mineral growth and deformation; (ii) analytical P–T paths from growth-zoned garnet porphyroblasts; and (iii) numerical modelling of vertical heat conduction. Derived P–T–t–d pathways suggest that uplift in the external domain resulted in part from erosion and isostatic unloading. In contrast, paths for the internal domain indicate that the out-of-sequence portion of the thrust belt may have experienced faster unroofing relative to the external domain. This is attributed to thickening by out-of-sequence thrusting and possibly to extensional faulting at (now eroded) higher structural levels. Observations on the timing of metamorphism, coupled with numerical modelling, suggest that the thermal peak metamorphism documented in the external domain is a consequence of the emplacement of the out-of-sequence thrusts stack in the internal portion of the thrust belt.  相似文献   

High pressure metamorphism in the nappes of the Valle dell'Orco traverse (Western Alps collisional belt) *     

U. POGNANTE  F. TALARICO  N. RASTELLI  N. FERRATI 《Journal of Metamorphic Geology》1987,5(3):397-414

Abstract A detailed field and petrological study of rocks from nappes cut by the Valle dell'Orco (Italian Western Alps), in particular the Sesia–Lanzo composite unit, has revealed geological and metamorphic histories which started in pre-alpine times and lasted up to the alpine subduction-collisional processes. During these processes the nappes sustained an early high P–low T stage and a later low P greenschist facies stage, but followed partly distinctive P–T–time trajectories. This paper discusses the kinematic evolution and the thermal history of the alpine belt from the early subduction/underthrust to the later exhumation stage. The metamorphic crystallization is often governed by incomplete and/or local equilibrium, and the pervasive syn-metamorphic deformation and the composition of the syn-metamorphic fluid phase (if present) have exerted an effective local control on reaction kinetics.  相似文献   

潼峪金矿区成矿断裂构造特征     

钱壮志  胡正国 《地球科学与环境学报》1992,(3)

潼峪金矿区发育过冲剪滑型、平移剪张型和平移剪滑型三种不同性质、不同方向成矿断裂,分布在金罗斑背形的不同部位,其形成有先后差异,但变形环境大体相同,具脆-韧性变形特征。空间上一般不超越褶皱主体。三类断裂中,前两者具石英脉型金矿化,后者形成构造蚀变岩型及小规模石英脉型金矿化。矿化差异与断裂产出的褶皱部位及其相应的应力应变条件的不同有关。  相似文献   

Blue amphiboles and their significance for the metamorphic history of the Pan-African Gariep belt, Namibia     

H. E. FRIMMEL  C. J. H. HARTNADY 《Journal of Metamorphic Geology》1992,10(5):651-669

The metamorphic history of mafic exotic blocks from a tectonic melange zone within an allochthonous ophiolitic terrane (Marmora Terrane) of the Pan-African Gariep orogenic belt in south-western Namibia was studied, based on mineral parageneses and amphibole composition. Glaucophane described previously from these rocks could not be verified. Instead, two types of blue amphiboles were distinguished: (i) rims of (ferro-) edenitic to pargasitic to barroisitic hornblende composition around brownish amphibole phenocrysts replacing magmatic clinopyroxene, and (ii) deep blue porphyroblasts of magnesio-riebeckite with little ferro-glaucophane component in a highly metasomatized albite-rich rock. Textural and mineralogical evidence, particularly the existence of up to three different amphibole generations in metagabbro samples, supports a multiphase metamorphic history experienced by these exotic blocks. The first metamorphic event, M1, is interpreted as very low- P hydrothermal oceanic metamorphism that affected the igneous protoliths at up to amphibolite facies temperatures. Subsequent M2 metamorphism was syntectonic and is characterized by temperatures similar to those attained during M1 but higher pressures indicating burial to 15–20 km. This event is related to a subduction process. The third metamorphic event, M3, was low grade and of regional nature. It is the only one recorded in the sedimentary envelope of the exotic blocks. The formation of magnesio-riebeckite is considered a retrograde reaction at greenschist facies during M2. The results indicate that in the Gariep belt subduction and subsequent obduction have occurred, although blueschist facies metamorphism has not been reached.  相似文献   

Pressure-Temperature Evolution of a Late Palaeozoic Paired Metamorphic Belt in North-Central Chile (34{degrees}-35{degrees}30'S)     

WILLNER  ARNE P. 《Journal of Petrology》2005,46(9):1805-1833

In the Chilean Coastal Cordillera, two units, the Western andEastern Series, constitute coeval parts of a Late Palaeozoicpaired metamorphic belt dominated by siliciclastic metasediments.The Western Series also contains rocks from the upper oceaniccrust and represents an accretionary prism. Omnipresent high-pressureconditions are reflected by Na–Ca-amphibole and phengitein greenschists. Peak PT conditions of 7·0–9·3kbar, 380–420°C point to a metamorphic gradient of11–16°C/km. Three unique occurrences of blueschistyield deviating conditions of 9·5–10·7 kbar,350–385°C and are interpreted as relics from the lowermostpart of the basal accretion zone preserving the original gradientof 9–11°C/km along the subducting slab. Pervasiveductile deformation related to basal accretion occurred nearpeak PT conditions. Deformation and PT evolution of the metapsammopeliticrocks is similar to that of the metabasites. However, a raregarnet mica-schist yields peak PT conditions of 9·6–14·7kbar, 390–440°C reflecting a retrograde stage aftercooling from a high-temperature garnet-forming stage. It isconsidered to be an exhumed relic from the earliest siliciclasticrocks subducted below a still hot mantle wedge. A retrogradeoverprint of all rock types occurred at 300–380°C.Continuous reactions caused crystal growth and recrystallizationwith abundant free water mostly under strain-free conditions.They record a pressure release of 3–4 kbar without erasingpeak metamorphic mineral compositions. The Eastern Series lacksmetabasite intercalations and represents a less deformed retro-wedgearea. In the study area it was entirely overprinted at a uniformdepth at 3 ± 0·5 kbar with temperatures progressivelyrising from 400°C to 720°C towards the coeval Late Palaeozoicmagmatic arc batholith. The interrelated pattern of PT datapermits a conceptual reconstruction of the fossil convergentmargin suggesting a flat subduction angle of 25° with continuousbasal accretion at a depth of 25–40 km and a short mainintrusion pulse in the magmatic arc. The latter was accompaniedby the formation of a thermal dome in the retro-wedge area,which remained stable relative to the vertically growing accretionaryprism characterized by cyclic mass flow. KEY WORDS: paired metamorphic belt; greenschist; blueschist; central Chile; thermobarometry  相似文献