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Results 1 to 25 of 58

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Geophysical evolution of the Themis family parent bodyCASTILLO-ROGEZ, Julie C; SCHMIDT, B. E.Geophysical research letters. 2010, Vol 37, Num 10, issn 0094-8276, L10202.1-L10202.5Article

Efficient delivery of meteorites to the Earth from a wide range of asteroid parent bodiesVOKROUHILCKY, D; FARINELLA, P.Nature (London). 2000, Vol 407, Num 6804, pp 606-608, issn 0028-0836Article

Impact process of boulders on the surface of asteroid 25143 Itokawa-fragments from collisional disruptionNAKAMURA, A. M; MICHIKAMI, T; HONDA, C et al.Earth, planets and space. 2008, Vol 60, Num 1, pp 7-12, issn 1343-8832, 6 p.Conference Paper

Discovery of a basaltic asteroid in the outer main beltLAZZARO, D; MICHTCHENKO, T; CARVANO, J. M et al.Science (Washington, D.C.). 2000, Vol 288, Num 5473, pp 2033-2035, issn 0036-8075Article

Fundamentally distinct outcomes of asteroid collisional evolution: Itokawa and ErosCHENG, A. F; BAMOUIN-JHA, O; HIRATA, N et al.Geophysical research letters. 2007, Vol 34, Num 9, issn 0094-8276, L09201.1-L09201.5Article

EVOLUTION OF CARBONACEOUS CHONDRITE PARENT BODIES = EVOLUTION DES CORPS PARENTAUX DE CHONDRITE CARBONEERAO MN; NAUTIYAL CM; PADIA JT et al.1981; METEORITICS; ISSN 0026-1114; USA; DA. 1981; VOL. 16; NO 4; PP. 380; BIBL. 3 REF.Conference Paper

THE DIMMITT H CHONDRITE REGOLITH BRECCIA AND IMPLICATIONS FOR THE STRUCTURE OF THE H CHONDRITE PARENT BODY = LA BRECHE A REGOLITHE DE LA CHONDRITE H DIMMITT ET IMPLICATIONS POUR LA STRUCTURE DU CORPS PARENTAL DES CHONDRITES HRUBIN ALAN E; SCOTT ERD; TAYLOR G JEFFREY et al.1981; METEORITICS; ISSN 0026-1114; USA; DA. 1981; VOL. 16; NO 4; PP. 382-383; BIBL. 1 REF.Conference Paper

CHEMISTRY OF THE SHERGOTTY PARENT BODY = CHIMIE DU MASSIF D'ORIGINE DE SHERGOTTYDREIBUS GERLIND; PALME H; RAMMENSEE W et al.1981; METEORITICS; ISSN 0026-1114; USA; DA. 1981; VOL. 16; NO 4; PP. 310; BIBL. 7 REF.; 1 TAB. ; ILL.Conference Paper

THE ABEE CONSORTIUM; PROBING THE PARENT BODY OF ENSTATITE METEORITES = CONSORTIUM ABEE; EXPLORATION DU CORPS PARENTAL DE METEORITES A ENSTATITEMARTI KURT; ANONYMOUS.1981; METEORITICS; ISSN 0026-1114; USA; DA. 1981; VOL. 16; NO 4; PP. 354; BIBL. 5 REF.Conference Paper

TL sensitivity of single chondrules from type 3 chondrites : Thermal metamorphism of chondrules in a nebular environment?BANERJEE, D; MAHALINGAM, V; PANDA, D. K et al.Radiation measurements. 2008, Vol 43, Num 2-6, pp 406-409, issn 1350-4487, 4 p.Conference Paper

Iron meteorites as remnants of planetesimals formed in the terrestrial planet regionBOTTKE, William F; NESVORNY, David; GRIMM, Robert E et al.Nature (London). 2006, Vol 439, Num 7078, pp 821-824, issn 0028-0836, 4 p.Article

Widespread magmatic activities on the angrite parent body at 4562 Ma agoSUGIURA, Naoji; MIYAZAKI, Akiko; YANAI, Keizo et al.Earth, planets and space. 2005, Vol 57, Num 12, issn 1343-8832, e13-e16Article

Chondrites and the solar nebulaBREARLEY, A.Science (Washington, D.C.). 1997, Vol 278, Num 5335, pp 76-77, issn 0036-8075Article

Structures induced by small moonlets in Saturn's rings : Implications for the Cassini MissionSEISS, M; SPAHN, F; SREMCEVIC, M et al.Geophysical research letters. 2005, Vol 32, Num 11, pp L11205.1-L11205.4, issn 0094-8276Article

The influence of temperature on the spectra of the A-asteroids and implications for their silicate chemistryLUCEY, P. G; KEIL, K; WHITELY, R et al.Journal of geophysical research. 1998, Vol 103, Num E3, pp 5865-5871, issn 0148-0227Article

Plasma conditions and the structure of the Jovian ringHORANYI, Mihály; JUHASZ, Antal.Journal of geophysical research. 2010, Vol 115, Num A9, issn 0148-0227, A09202.1-A09202.12Article

Measuring pickup ions to characterize the surfaces and exospheres of planetary bodies : Applications to the MoonHARTLE, Richard E; KILLEN, Rosemary.Geophysical research letters. 2006, Vol 33, Num 5, issn 0094-8276, L05201.1-L05201.5Article

The crystallization age of eucrite zirconSRINIVASAN, G; WHITEHOUSE, M. J; WEBER, I et al.Science (Washington, D.C.). 2007, Vol 317, Num 5836, pp 345-347, issn 0036-8075, 3 p.Article

Energetics of asteroid dynamos and the role of compositional convectionNIMMO, F.Geophysical research letters. 2009, Vol 36, Num 10, issn 0094-8276, L10201.1-L10201.6Article

Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroidsHARDERSEN, Paul S; GALLEY, Michael J; ABELL, Paul A et al.Icarus (New York, NY). 2005, Vol 175, Num 1, pp 141-158, issn 0019-1035, 18 p.Article

Late Accretion on the Earliest Planetesimals Revealed by the Highly Siderophile ElementsDALE, Christopher W; BURTON, Kevin W; GREENWOOD, Richard C et al.Science (Washington, D.C.). 2012, Vol 336, Num 6077, pp 72-75, issn 0036-8075, 4 p.Article

Analysis of interplanetary dust particles by soft and hard X-ray microscopyFLYNN, G. J; KELLER, L. P; WIRICK, S et al.Journal de physique. IV. 2003, Vol 104, pp 367-372, issn 1155-4339, 6 p.Conference Paper

Possible in situ formation of meteoritic nanodiamonds in the early Solar SystemDAI, Z. R; BRADLEY, J. P; JOSWIAK, D. J et al.Nature (London). 2002, Vol 418, Num 6894, pp 157-159, issn 0028-0836Article

Detrital remanent magnetization in the solar nebulaFU, Roger R; WEISS, Benjamin P.Journal of geophysical research. 2012, Vol 117, Num E2, issn 0148-0227, E02003.1-E02003.19Article

FINE-GRAINED SERPENTINE IN CM2 CARBONACEOUS CHONDRITES AND ITS IMPLICATIONS FOR THE EXTENT OF AQUEOUS ALTERATION ON THE PARENT BODY: A REVIEWVELBEL, Michael A; PALMER, Eric E.Clays and clay minerals. 2011, Vol 59, Num 4, pp 416-432, issn 0009-8604, 17 p.Article

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