Search Results - "WEIDENSCHILLING, Stuart J"

Origin and history of ureilitic material in the solar system: The view from asteroid 2008 TC3 and the Almahata Sitta meteorite by Goodrich, Cyrena Anne, Hartmann, William K., O'Brien, David P., Weidenschilling, Stuart J., Wilson, Lionel, Michel, Patrick, Jutzi, Martin

“…Asteroid 2008 TC3 (approximately 4 m diameter) was tracked and studied in space for approximately 19 h before it impacted Earth's atmosphere, shattering at…”
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The effect of multiple particle sizes on cooling rates of chondrules produced in large-scale shocks in the solar nebula by Morris, Melissa A., Weidenschilling, Stuart J., Desch, Steven J.

“…Chondrules represent one of the best probes of the physical conditions and processes acting in the early solar nebula. Proposed chondrule formation models are…”
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The planetesimal bow shock model for chondrule formation: A more quantitative assessment of the standard (fixed Jupiter) case by HOOD, Lon L., WEIDENSCHILLING, Stuart J.

“…– One transient heating mechanism that can potentially explain the formation of most meteoritic chondrules 1–3 Myr after CAIs is shock waves produced by…”
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Particles in the nebular midplane: Collective effects and relative velocities by WEIDENSCHILLING, Stuart J.

“…– In the absence of global turbulence, solid particles in the solar nebula tend to settle toward the midplane, forming a layer with enhanced solids/gas ratio…”
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Gravitational scattering as a possible origin for giant planets at small stellar distances by Weidenschilling, Stuart J, Marzari, Francesco

“…The recent discoveries of massive planetary companions orbiting several solar-type stars pose a conundrum. Conventional models for the formation of giant…”
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Formation of Planetesimals and Accretion of the Terrestrial Planets by Weidenschilling, Stuart J

“…Planetesimals formed in the solar nebula by collisional coagulation. Dust aggregates settled toward the central plane, the larger ones growing by sweeping up…”
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Nebular shock waves generated by planetesimals passing through Jovian resonances: Possible sites for chondrule formation by HOOD, Lon L., CIESLA, Fred J., ARTEMIEVA, Natalia A., MARZARI, Francesco, WEIDENSCHILLING, Stuart J.

“…— The primordial asteroid belt contained at least several hundred and possibly as many as 10,000 bodies with diameters of 1000 km or larger. Following the…”
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Growth of Jupiter: Enhancement of core accretion by a voluminous low-mass envelope by D’Angelo, Gennaro, Weidenschilling, Stuart J., Lissauer, Jack J., Bodenheimer, Peter

“…•We study the formation of Jupiter’s core from an evolving disk of planetesimals.•The growth of an envelope around the core includes an accurate determination…”
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Evaluating planetesimal bow shocks as sites for chondrule formation by CIESLA, Fred J., HOOD, Lon L., WEIDENSCHILLING, Stuart J.

“…— We investigate the possible formation of chondrules by planetesimal bow shocks. The formation of such shocks is modeled using a piecewise parabolic method…”
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Very early collisional evolution in the asteroid belt by WEIDENSCHILLING, Stuart J, DAVIS, Donald R, MARZARI, Francesco

“…The asteroids probably experienced significant collisional evolution while the solar nebula was present. Planetesimals were brought into resonances with…”
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Growth of Jupiter: Formation in disks of gas and solids and evolution to the present epoch by D'Angelo, Gennaro, Weidenschilling, Stuart J., Lissauer, Jack J., Bodenheimer, Peter

“…The formation of Jupiter is modeled via core-nucleated accretion, and the planet's evolution is simulated up to the present epoch. Throughout the phases when…”
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Importance of the accretion process in asteroid thermal evolution: 6 Hebe as an example by Ghosh, Amitabha, Weidenschilling, Stuart J., McSween Jr, Harry Y.

“…— Widespread evidence exists for heating that caused melting, thermal metamorphism, and aqueous alteration in meteorite parent bodies. Previous simulations of…”
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Growth of Jupiter: Formation in disks of gas and solids and evolution to the present epoch by D'Angelo, Gennaro, Weidenschilling, Stuart J., Lissauer, Jack J., Bodenheimer, Peter

“…The formation of Jupiter is modeled via core-nucleated accretion, and the planet's evolution is simulated up to the present epoch. Throughout the phases when…”
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Saturn Ring Particles as Dynamic Ephemeral Bodies by Davis, Donald R., Weidenschilling, Stuart J., Chapman, Clark R., Greenberg, Richard

“…Although Saturn's rings are within the Roche zone, the accretion of centimeter-sized particles into large aggregates many meters in diameter occurs readily, on…”
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Origin and history of ureilitic material in the solar system: The view from asteroid 2008 TC sub(3) and the Almahata Sitta meteorite by Goodrich, Cyrena Anne, Hartmann, William K, O'Brien, David P, Weidenschilling, Stuart J, Wilson, Lionel, Michel, Patrick, Jutzi, Martin

“…Asteroid 2008 TC sub(3) (approximately 4 m diameter) was tracked and studied in space for approximately 19 h before it impacted Earth's atmosphere, shattering…”
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Origin and history of ureilitic material in the solar system: The view from asteroid 2008 TC 3 and the Almahata Sitta meteorite by Goodrich, Cyrena Anne, Hartmann, William K., O'Brien, David P., Weidenschilling, Stuart J., Wilson, Lionel, Michel, Patrick, Jutzi, Martin

“…Asteroid 2008 TC 3 (approximately 4 m diameter) was tracked and studied in space for approximately 19 h before it impacted Earth's atmosphere, shattering at…”
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A possible origin for the grooves of Phobos by Weidenschilling, Stuart J

“…A hypothesis that the age and distribution of grooves on the surface of Phobos may be explained by a hybrid origin due to varying tidal stresses induced after…”
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Growth of Jupiter: Formation in Disks of Gas and Solids and Evolution to the Present Epoch by D'Angelo, Gennaro, Weidenschilling, Stuart J, Lissauer, Jack J, Bodenheimer, Peter

“…Icarus 355 (2021) 114087 [Abridged] The formation of Jupiter is modeled via core-nucleated accretion, and the planet's evolution is simulated up to the present…”
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Looking for Planets: Planetary Systems . Formation, Evolution, and Detection. Bernard F. Burke, Jurgen H. Rahe, and Elizabeth Roettger, Eds. Kluwer, Norwell, MA, 1994. xii, 486 pp., illus. $217 or £148.50 or Dfl. 380. From a conference, Pasadena, CA, Dec. 1992. Reprinted from Astrophysics and Space Science , vol. 212, nos. 1-2 by Weidenschilling, Stuart J.

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Looking for planets -- Planetary Systems. Formation, Evolution, and Detection edited by Bernard F. Burke, Jurgen H. Rahe and Elizabeth Roettger by Weidenschilling, Stuart J

“…Review…”
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