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动力学与控制学报, ISSN 1672-6553, 2017, Volume 15, Issue 5, pp. 476 - 480
研究了近地小行星433 Eros本体悬停轨道的稳定控制问题.用三轴椭球体模型近似Eros引力场分布,建立了航天器在其引力场内的动力学模型,并且应用等加速度变截距时变滑模控制设计了悬停控制器.该方法的滑模面选取与常规滑模控制不同,且不存在到达阶段.仿真分析从不同的初始条件和悬停条件入手,验证控制器的有效性,并讨论了航天器... 
Journal Article
Icarus, ISSN 0019-1035, 11/2018, Volume 314, pp. 299 - 310
•We measured the global surface roughness of 433 Eros.•The surface roughness of Eros is dominated by boulders and craters... 
433 Eros | Asteroids | Topography | Boulders | Impact craters | NEAR-SHOEMAKER | ASTEROID ITOKAWA | SMALL-SCALE TOPOGRAPHY | MOLA DATA | IMPACT | SHAPE | 433-EROS | MARS | ASTRONOMY & ASTROPHYSICS | ALTIMETER | HAYABUSA | Military aspects | Optical range finders | Ponds | Lasers | Analysis | Tectonics (Geology)
Journal Article
Icarus, ISSN 0019-1035, 01/2002, Volume 155, Issue 1, pp. 51 - 74
The NEAR laser rangefinder (NLR) obtained more than 16 million range returns from asteroid 433 Eros... 
Eros | Asteroid surfaces | Tectonics | Asteroids | Regoliths | CALIBRATION | asteroid surfaces | asteroids | RADAR | MOON | 253 MATHILDE | NEARS FLYBY | SHAPE | ASTRONOMY & ASTROPHYSICS | regoliths | 433 EROS | SURFACE | tectonics | Observations | Eros (Asteroid)
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2018, Volume 473, Issue 4, pp. 5050 - 5065
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 438, Issue 3, pp. 2672 - 2682
... (volume, mass, moments of inertia) of asteroids is the polyhedral model method. We rebuild the shape of the asteroid 433 Eros using data from 1998 December observations of the probe Near-Earth-Asteroid-Rendezvous-Shoemaker... 
Minor planets, asteroids | Gravitation | Individual: 433 Eros | Celestial mechanics | Methods: numerical | minor planets | SHAPE | celestial mechanics | MOTION | gravitation | ASTRONOMY & ASTROPHYSICS | DYNAMICS | methods: numerical | GRAVITY | asteroids: individual: 433 Eros
Journal Article
Earth and planetary science letters, ISSN 0012-821X, 2015, Volume 416, pp. 109 - 120
We have mapped the major-element composition of Mercury's surface from orbital MESSENGER X-Ray Spectrometer measurements. These maps constitute the first... 
X-ray fluorescence | geochemistry | spectroscopy | Mercury | MESSENGER | Geochemistry | Spectroscopy | CALORIS BASIN | VOLCANISM | ASTEROID 433 EROS | DICHOTOMY | ABUNDANCE | GEOCHEMISTRY & GEOPHYSICS | ORIGIN | EVOLUTION | SURFACE | EMISSION | Mercury (Planet) | Environmental aspects | Fluorescence | Reservoirs | Magnetism | Chemical properties | X-ray spectroscopy | Maps | Aluminum | Spectrometers | X-rays | Silicon | Magnesium | Solar system | Mercury surface
Journal Article
Icarus, ISSN 0019-1035, 01/2002, Volume 155, Issue 1, pp. 18 - 37
Stereogrammetric measurement of the shape of Eros using images obtained by NEAR's Multispectral Imager provides a survey of the major topographic features and slope processes on this asteroid... 
Eros | Geology | NEAR | Asteroids | Geodesy | asteroids | ASTEROID 433 EROS | geology | GRAVITY | CRATERS | FEATURES | PHOBOS | IMPACT | EJECTA BLOCKS | ASTRONOMY & ASTROPHYSICS | SURFACE | 243-IDA | geodesy | HISTORY | Multispectral photography | Usage | Observations | Eros (Asteroid)
Journal Article
The Astronomical journal, ISSN 1538-3881, 2018, Volume 155, Issue 2, p. 85
Various simplified models have been investigated as a way to understand the complex dynamical environment near irregular asteroids. A dipole segment model is... 
methods: analytical | celestial mechanics | gravitation | minor planets, asteroids: individual (433 Eros) | MOTION | STABILITY | ASTRONOMY & ASTROPHYSICS | LIBRATION POINTS | MASS | BODIES | Errors | Approximation | Dipoles | Approximation method | Asteroids | Process parameters | Mathematical models | Parameter identification | Acceleration | Near-earth objects | Extremities | Elongation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2015, Volume 452, Issue 2, pp. 1316 - 1327
Recent data processing showed the existence of a difference that can reach 25 per cent for the dimensions of asteroid (216) Kleopatra between the radar... 
Minor planets | Gravitation | Asteroids: individual: Kleopatra | Celestial mechanics | Methods: numerical | minor planets | RADAR OBSERVATIONS | MODEL | methods: numerical | DENSITY | celestial mechanics | EVOLUTION | gravitation | ASTRONOMY & ASTROPHYSICS | LUTETIA | MASS | 433 EROS | DYNAMICS | IRAS | asteroids: individual: Kleopatra
Journal Article
Icarus, ISSN 0019-1035, 01/2002, Volume 155, Issue 1, pp. 104 - 118
Preliminary measurements of craters and boulders have been made in various locations on Eros from images acquired during the first nine months of NEAR Shoemaker's orbital mission, including... 
Impact processes | Cratering | Surfaces, asteroids | Asteroids, Eros | Geological processes | EARTH | cratering | asteroids | CROSSING ASTEROIDS | ASTEROID 433 EROS | impact processes | SPECTRAL PROPERTIES | SIMULATION | Eros | SHAPE | surfaces | geological processes | SMALL-SCALE FEATURES | S-TYPE ASTEROIDS | ASTRONOMY & ASTROPHYSICS | LASER IRRADIATION | ORDINARY CHONDRITE | Craters | Observations | Asteroids | Eros (Asteroid)
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2018, Volume 477, Issue 2, pp. 1782 - 1802
Journal Article
Icarus (New York, N.Y. 1962), ISSN 0019-1035, 2008, Volume 195, Issue 2, pp. 622 - 629
The X-ray spectrometer of the Near-Earth Asteroid Rendezvous (NEAR) mission discovered a low abundance of sulfur on the surface of asteroid Eros... 
Impact processes | Experimental techniques | Asteroid Eros | Near-Earth objects | Asteroids | asteroids | BOMBARDMENT | near-Earth objects | ASTEROID 433 EROS | impact processes | PYRRHOTITE | IMPACT | asteroid Eros | 433-EROS | ASTRONOMY & ASTROPHYSICS | RAY SPECTROMETER | ELEMENTAL COMPOSITION | SURFACE | experimental techniques | SCATTERING | REGOLITH | Sulfur | Sulfur compounds
Journal Article
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, ISSN 1364-503X, 05/2017, Volume 375, Issue 2094, p. 20150384
Of the potential volatile sources for the terrestrial planets, the CI and CM carbonaceous chondrites are closest to the planets' bulk H and N isotopic... 
Terrestrial planets | Water | Chondrites | Volatiles | Asteroids | Grand Tack | PARENT BODY | asteroids | MULTIDISCIPLINARY SCIENCES | DEUTERATED WATER | MAGMA OCEAN | chondrites | ASTEROID 433 EROS | terrestrial planets | OXYGEN ISOTOPIC COMPOSITION | water | DIFFERENTIATED PLANETESIMALS | MURCHISON METEORITE | AMINO-ACIDS | NOBLE-GAS-ANALYSES | CARBONACEOUS CHONDRITES | volatiles | 169 | 1000 | Review
Journal Article
Icarus, ISSN 0019-1035, 2004, Volume 172, Issue 2, pp. 415 - 431
A photometric model of (433) Eros at wavelengths from 450 to 1050 nm is constructed using the combination of the images from the multispectral imager (MSI... 
433 Eros | NEAR | Asteroids | Photometry | Asteroids, 433 Eros | asteroids, 433 Eros | photometry | INFLIGHT CALIBRATION | COHERENT BACKSCATTER | CURVES | PHASE-ANGLE | REFLECTANCE SPECTRA | 433-EROS | ASTRONOMY & ASTROPHYSICS | ASTEROID LIGHTCURVE OBSERVATIONS | GALILEO PHOTOMETRY | MULTISPECTRAL IMAGER | SCATTERING | Composition | Astronomical photometry | Observations | Analysis | Eros (Asteroid)
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 01/2017, Volume 464, Issue 3, pp. 3552 - 3560
One of the most accurate models currently used to represent the gravity field of irregular bodies is the polyhedral approach. In this model, the mass of the... 
TARGET | 21-LUTETIA | SMALL BODIES | ROTATING 2ND-DEGREE | VESTA | EQUILIBRIUM POINTS | PERIODIC-ORBITS | celestial mechanics | gravitation | ORDER GRAVITY FIELDS | ASTRONOMY & ASTROPHYSICS | ROSETTA MISSION | 433 EROS | minor planets, asteroids: individual: Lutetia | Physics - Earth and Planetary Astrophysics | Earth and Planetary Astrophysics | Physics | Astrophysics
Journal Article
Icarus, ISSN 0019-1035, 01/2014, Volume 228, pp. 217 - 246
•We find no correlation between band parameters and ExploreNEOs albedos and diameters.•There is no universal phase angle–Band Area Ratio correlation.•For NIR... 
Spectroscopy | Asteroids, composition | Near-Earth objects | Asteroids | astro-ph.EP | DAWN MISSION | ASTEROID SPECTROSCOPIC SURVEY | MINERALOGICAL CHARACTERIZATION | SPACE-TELESCOPE | REFLECTANCE SPECTRA | INFRARED TELESCOPE FACILITY | S-TYPE ASTEROIDS | SOURCE REGIONS | ASTRONOMY & ASTROPHYSICS | 433 EROS | ORDINARY CHONDRITE | Physics - Earth and Planetary Astrophysics
Journal Article