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Results 1 to 25 of 558

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Impact angle influence in high velocity dust collisions during planetesimal formationTEISER, Jens; KÜPPER, Markus; WURM, Gerhard et al.Icarus (New York, N.Y. 1962). 2011, Vol 215, Num 2, pp 596-598, issn 0019-1035, 3 p.Article

Very early collisional evolution in the asteroid beltWEIDENSCHILLING, Stuart J; DAVIS, Donald R; MARZARI, Francesco et al.Earth, planets and space. 2001, Vol 53, Num 11, pp 1093-1097, issn 1343-8832Conference Paper

Les météorites gardent leur mystère = Mystery meteoritesWOOD, John.Recherche (Paris, 1970). 2002, Num 354, pp 52-55, issn 0029-5671Article

Initial sizes of planetesimals and accretion of the asteroidsWEIDENSCHILLING, S. J.Icarus (New York, N.Y. 1962). 2011, Vol 214, Num 2, pp 671-684, issn 0019-1035, 14 p.Article

Does the gas flow through a porous dust aggregate help its growth in a protoplanetary disk?SEKIYA, Minoru; TAKEDA, Hidenori.Icarus (New York, NY). 2005, Vol 176, Num 1, pp 220-223, issn 0019-1035, 4 p.Article

Experimental study on collisional disruption of highly porous icy bodiesSHIMAKI, Yuri; ARAKAWA, Masahiko.Icarus (New York, N.Y. 1962). 2012, Vol 218, Num 2, pp 737-750, issn 0019-1035, 14 p.Article

Compaction and fragmentation of porous gypsum targets from low-velocity impactsFUJII, Yuichi; NAKAMURA, Akiko M.Icarus (New York, N.Y. 1962). 2009, Vol 201, Num 2, pp 795-801, issn 0019-1035, 7 p.Article

Growth of planetesimals by impacts at ∼25 m/sWURM, Gerhard; PARASKOV, Georgi; KRAUSS, Oliver et al.Icarus (New York, NY). 2005, Vol 178, Num 1, pp 253-263, issn 0019-1035, 11 p.Article

Water, heat, bombardment: The evolution and current state of (2) PallasELYCE SCHMIDT, Britney; CASTILLO-ROGEZ, Julie C.Icarus (New York, N.Y. 1962). 2012, Vol 218, Num 1, pp 478-488, issn 0019-1035, 11 p.Article

Impact experiments of porous gypsum―glass bead mixtures simulating parent bodies of ordinary chondrites: Implications for re-accumulation processes related to rubble-pile formationYASUI, Minami; ARAKAWA, Masahiko.Icarus (New York, N.Y. 1962). 2011, Vol 214, Num 2, pp 754-765, issn 0019-1035, 12 p.Article

On oligarchic growth of planets in protoplanetary disksBRUNINI, Adrian; BENVENUTO, Omar G.Icarus (New York, NY). 2008, Vol 194, Num 2, pp 800-810, issn 0019-1035, 11 p.Article

New frontiers in the solar system: trans-Neptunian objects = Les nouvelles frontières du système solaire : les objets transneptuniensBARUCCI, M. Antonietta.Comptes rendus. Physique. 2003, Vol 4, Num 7, issn 1631-0705, 89 p.Serial Issue

A statistical insight into the Edgeworth-Kuiper beltFULCHIGNONI, Marcello; DELSANTI, Audrey C.Comptes rendus. Physique. 2003, Vol 4, Num 7, pp 767-774, issn 1631-0705, 8 p.Article

Discovery of 12 satellites of Saturn exhibiting orbital clusteringGLADMAN, Brett; KAVELAARS, J. J; GRAVY, Tommy et al.Nature (London). 2001, Vol 412, Num 6843, pp 163-166, issn 0028-0836Article

La naissance tumultueuse des planètes : Exoplanètes, nouvelles Terre en vues = Planets birthTERQUEM, Caroline.Pour la science. 2006, Num 347, pp 54-60, issn 0153-4092, 7 p.Article

Discovering and securing TNOs: the CFHTLS Ecliptic surveyPETIT, Jean-Marc; GLADMAN, Brett.Comptes rendus. Physique. 2003, Vol 4, Num 7, pp 743-753, issn 1631-0705, 11 p.Article

Experimental hypervelocity impact effects on simulated planetesimal materialsTEDESCHI, W. J; REMO, J. L; SCHULZE, J. F et al.International journal of impact engineering. 1995, Vol 17, Num 4-6, pp 837-848, issn 0734-743XConference Paper

Density waves in the solar nebula: planetesimal velocitiesWARD, W. R.Icarus (New York, NY). 1993, Vol 106, Num 1, pp 274-287, issn 0019-1035Article

The formation of the Kuiper belt by the outward transport of bodies during Neptune's migrationLEVISON, Harold F; MORBIDELLI, Alessandro.Nature (London). 2003, Vol 426, Num 6965, pp 419-421, issn 0028-0836, 3 p.Article

On the density of EKOs and related objectsALTENHOFF, W. J; BENOLDI, F; MENTEN, K. M et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 441, Num 1, pp L5-L7, issn 0004-6361Article

The discovery and exploration of the trans-Neptunian regionDAVIES, John Keith.Comptes rendus. Physique. 2003, Vol 4, Num 7, pp 733-741, issn 1631-0705, 9 p.Article

New insights on the kuiper beltMORBIDELLI, A.Science (Washington, D.C.). 1998, Vol 280, Num 5372, pp 2071-2073, issn 0036-8075Article

Earth accretionAHRENS, T.J.LPI conference on the origin of the Earth. 1990, pp 211-227Conference Paper

Planetary systems: formation, evolution, and detection. International conferenceBURKE, Bernard F; RAHE, Jürgen H; ROETTGER, Elizabeth E et al.Astrophysics and space science. 1994, Vol 212, Num 1-2, issn 0004-640X, 494 p.Conference Proceedings

HOW NOT TO BUILD TATOOINE: THE DIFFICULTY OF IN SITU FORMATION OF CIRCUMBINARY PLANETS KEPLER 16b, KEPLER 34b, AND KEPLER 35bPAARDEKOOPER, Sijme-Jan; LEINHARDT, ZoË M; THEBAULT, Philippe et al.The Astrophysical journal. 2012, Vol 754, Num 1, issn 0004-637X, L16.1-L16.5, 2Article

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