Works matching Eros (Asteroid)
Results: 55
Shoemaker crater as the source of most ejecta blocks on the asteroid 433 Eros.
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- Nature, 2001, v. 413, n. 6854, p. 394, doi. 10.1038/35096513
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80 Years Ago: The Asteroid Eros.
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- Mercury, 2010, v. 39, n. 3, p. 7
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Earth today, Eros in a year's time, for asteroid spacecraft.
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- Nature, 1998, v. 391, n. 6666, p. 423, doi. 10.1038/34982
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The orbital evolution of the asteroid Eros and implications for collision with the Earth.
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- Nature, 1996, v. 380, n. 6576, p. 689, doi. 10.1038/380689a0
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The landing of the NEAR-Shoemaker spacecraft on asteroid 433 Eros.
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- Nature, 2001, v. 413, n. 6854, p. 390, doi. 10.1038/35096507
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Computation of Attraction Potential of Asteroid (433) Eros with an Accuracy up to the Terms of the Fourth Order.
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- Doklady Physics, 2020, v. 65, n. 5, p. 164, doi. 10.1134/S1028335820050080
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A Multipole Representation for the Gravitational Field of Asteroid (433) Eros.
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- Cosmic Research, 2024, v. 62, n. 3, p. 286, doi. 10.1134/S0010952524600240
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Detecting crater ejecta-blanket boundaries and constraining source crater regions for boulder tracks and elongated secondary craters on Eros.
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- Meteoritics & Planetary Science, 2012, v. 47, n. 6, p. 1087, doi. 10.1111/j.1945-5100.2012.01380.x
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Experimental investigation of the impact fragmentation of blocks embedded in regolith.
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- Meteoritics & Planetary Science, 2011, v. 46, n. 1, p. 149, doi. 10.1111/j.1945-5100.2010.01163.x
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Eros begins to yield up its secrets.
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- Nature, 2000, v. 403, n. 6772, p. 815, doi. 10.1038/35002736
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Software problem delays US spacecraft's meeting with asteroid.
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- Nature, 1999, v. 397, n. 6714, p. 5, doi. 10.1038/16103
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Seismic resurfacing by a single impact on the asteroid 433 Eros.
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- Nature, 2005, v. 436, n. 7049, p. 366, doi. 10.1038/nature03855
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Once upon an asteroid.
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- Nature, 2001, v. 413, n. 6854, p. 369, doi. 10.1038/35096660
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NASA celebrates as spacecraft homes in on asteroid.
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- Nature, 2001, v. 409, n. 6821, p. 654, doi. 10.1038/35055690
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High precision model of precession and nutation of the asteroids (1) Ceres, (4) Vesta, (433) Eros, (2867) Steins, and (25143) Itokawa.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 565, p. 1, doi. 10.1051/0004-6361/201322905
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Modelling and computation of gravitational attraction, gradient tensors, rotational and horizontal invariants of Asteroid Bennu (101955), Itokawa (25143) and Eros (433) via 2D Non-Uniform FFT.
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- Bulletin of the Mineral Research & Exploration, 2024, v. 173, n. 173, p. 1, doi. 10.19111/bulletinofmre.1251299
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From ACIS to Zamama.
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- Astronomy & Geophysics, 2000, v. 41, n. 4, p. 4.31, doi. 10.1046/j.1468-4004.2000.00431.x
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Effects of ejecta accumulation on the crater population of asteroid 433 Eros.
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- Journal of Geophysical Research. Planets, 2009, v. 114, n. E6, p. n/a, doi. 10.1029/2008JE003229
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Origin and flatness of ponds on asteroid 433 Eros.
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- Meteoritics & Planetary Science, 2014, v. 49, n. 10, p. 1735, doi. 10.1111/maps.12348
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Ponded deposits on asteroid 433 Eros.
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- Meteoritics & Planetary Science, 2002, v. 37, n. 8, p. 1095, doi. 10.1111/j.1945-5100.2002.tb00880.x
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X-ray fluorescence measurements of the surface elemental composition of asteroid 433 Eros.
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- Meteoritics & Planetary Science, 2001, v. 36, n. 12, p. 1673, doi. 10.1111/j.1945-5100.2001.tb01856.x
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Radar constraints on asteroid regolith properties using 433 Eros as ground truth.
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- Meteoritics & Planetary Science, 2001, v. 36, n. 12, p. 1697, doi. 10.1111/j.1945-5100.2001.tb01857.x
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The NEAR magnetic field investigation: Science objectives at asteroid Eros 433 and experimental approach.
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- Journal of Geophysical Research. Planets, 1997, v. 102, n. E10, p. 23751, doi. 10.1029/97JE01161
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Thrust faults and the near-surface strength of asteroid 433 Eros.
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- Geophysical Research Letters, 2011, v. 38, n. 2, p. n/a, doi. 10.1029/2010GL045302
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Fundamentally distinct outcomes of asteroid collisional evolution: Itokawa and Eros.
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- Geophysical Research Letters, 2007, v. 34, n. 9, p. n/a, doi. 10.1029/2007GL029559
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Thermally induced lineations on the asteroid Eros: Evidence of orbit transfer.
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- Geophysical Research Letters, 2002, v. 29, n. 16, p. 65-1, doi. 10.1029/2002GL015181
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The nature of ponded deposits on Eros.
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- Nature, 2001, v. 413, n. 6854, p. 396, doi. 10.1038/35096518
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A multiresolution model for small-body gravity estimation.
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- Celestial Mechanics & Dynamical Astronomy, 2011, v. 111, n. 3, p. 309, doi. 10.1007/s10569-011-9374-y
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Approximation of the Attractive Field of a Body Close to Dynamically Symmetrical Using the Attractive Field of Three Balls.
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- Doklady Physics, 2023, v. 68, n. 3, p. 87, doi. 10.1134/S1028335823030023
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Space Weathering‐Induced Formation of Hydrogen Sulfide (H<sub>2</sub>S) and Hydrogen Disulfide (H<sub>2</sub>S<sub>2</sub>) in the Murchison Meteorite.
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- Journal of Geophysical Research. Planets, 2019, v. 124, n. 11, p. 2772, doi. 10.1029/2018JE005913
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Asteroids: Shaken on impact.
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- Nature, 2005, v. 436, n. 7049, p. 335, doi. 10.1038/436335a
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Mascon distribution techniques for asteroids and comets.
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- Celestial Mechanics & Dynamical Astronomy, 2022, v. 134, n. 6, p. 1, doi. 10.1007/s10569-022-10115-2
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Analytic orbit theory with any arbitrary spherical harmonic as the dominant perturbation.
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- Celestial Mechanics & Dynamical Astronomy, 2019, v. 131, n. 10, p. N.PAG, doi. 10.1007/s10569-019-9923-3
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Evaluation of the spherical harmonic coefficients for the external potential of a polyhedral body with linearly varying density.
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- Celestial Mechanics & Dynamical Astronomy, 2019, v. 131, n. 2, p. 1, doi. 10.1007/s10569-019-9885-5
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Easily retrievable objects among the NEO population.
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- Celestial Mechanics & Dynamical Astronomy, 2013, v. 116, n. 4, p. 367, doi. 10.1007/s10569-013-9495-6
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The Method of Determination of the Gravitational Field Model of an Asteroid Using a Group of Small Spacecrafts.
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- Cosmic Research, 2022, v. 60, n. 3, p. 185, doi. 10.1134/S0010952522030091
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Using the К-Means Method for Aggregating the Masses of Elongated Celestial Bodies.
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- Cosmic Research, 2019, v. 57, n. 4, p. 266, doi. 10.1134/S0010952519040026
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Mykola Evdokymov (1868–1941): Founder of Astrometric Research at Kharkiv Astronomical Observatory.
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- Kinematics & Physics of Celestial Bodies, 2022, v. 38, n. 2, p. 114, doi. 10.3103/S0884591322020027
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Ludwig von Struve (1858–1920): Development of Positional Astronomy at the Kharkiv Astronomical Observatory.
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- Kinematics & Physics of Celestial Bodies, 2021, v. 37, n. 5, p. 269, doi. 10.3103/S0884591321050032
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Attitude dynamics and control of satellites orbiting rotating asteroids.
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- Acta Mechanica, 2008, v. 198, n. 1-2, p. 99, doi. 10.1007/s00707-007-0508-y
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Accurate Calculation of Geodetic Heights of a Celestial Body's Surface Points Relative to the Triaxial Ellipsoid.
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- Doklady Earth Sciences, 2019, v. 486, n. 2, p. 663, doi. 10.1134/S1028334X19060035
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Multiple-hopping trajectories near a rotating asteroid.
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- Astrophysics & Space Science, 2017, v. 362, n. 3, p. 1, doi. 10.1007/s10509-017-3026-y
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Hydrogen and major element concentrations on 433 Eros: Evidence for an L- or LL-chondrite-like surface composition.
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- Meteoritics & Planetary Science, 2015, v. 50, n. 3, p. 353, doi. 10.1111/maps.12434
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Eros's extended family.
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- Nature, 1997, v. 388, n. 6642, p. 516, doi. 10.1038/41423
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Exact Determination of the Lunar Mass by means of Selenoid Satellites.
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- Nature, 1961, v. 192, n. 4801, p. 442, doi. 10.1038/192442a0
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Change of boundary: towards a mathematical foundation of global gravity models.
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- Journal of Geodesy, 2023, v. 97, n. 6, p. 1, doi. 10.1007/s00190-023-01748-8
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Evaluation Procedures for the Potential Harmonic Coefficients of a Generally Shaped Polyhedron.
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- Surveys in Geophysics, 2024, v. 45, n. 2, p. 315, doi. 10.1007/s10712-023-09802-y
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Spherical Harmonic Expansions for the Gravitational Field of a Polyhedral Body with Polynomial Density Contrast.
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- Surveys in Geophysics, 2019, v. 40, n. 2, p. 197, doi. 10.1007/s10712-019-09515-1
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FORMATION OF FE WHISKERS THROUGH SIMULATED MICROMETEOROID BOMBARDMENT.
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- Meteoritics & Planetary Science, 2022, v. 57, p. 6045
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Astronomers reveal the secrets of the name game.
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- Nature, 2000, v. 406, n. 6798, p. 819
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