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44 Nysa
Asteroid Observations with the Hubble Space Telescope? FGS??
Arizona-Based Astronomers Characterize One of the Smallest Known Asteroids
Asteroid Photometric and Polarimetric Phase Curves: Joint Linear-Exponential Modeling
Hungaria Asteroid Family As the Source of Aubrite Meteorites ⇑ Matija C´ Uk A, , Brett J
Mineralogical Variations Among High Albedo E-Type Asteroids: Implications for Asteroid Igneous Processes
2-Meter Diameter Near-Earth Asteroid 2015 TC25: a Possible Boulder from E-Type Asteroid (44) Nysa
E-Type Apollo Asteroid (3103) 1982Bb: a Hungaria-Derived Near-Earth Source Body for the Aubrites
The Minor Planet Bulletin, We Feel Safe in Al., 1989)
Radar Observations of E-Class Asteroids 44 Nysa and 434 Hungaria
Asteroid Models from Combined Sparse and Dense Photometric Data
Anticipating Formation Trends of Binary and Multiple Asteroids in The
Asteroid Families: Statistical Identification of New Families and Determination of Size Distributions of the Families’ Members
Pole Orientation of Asteroid 44 Nysa Via Photometric Astrometry, Including a Discussion of the Method's Application and Its Limitations
Polarimetric Observations of Hungaria Asteroids
1 Asteroids, Second Part. Summary Asteroid Surface Mineralogy A
An Unusual E-Type Asteroid
University Microfilms International 300 N
Astronomy Astrophysics
Top View
The Minor Planet Bulletin (Warner Et Al., 2008)
Asteroid Photometric and Polarimetric Phase Effects
The Trajectory Optimization & Space Logistics of Asteroid Mining Missions
Ny8-29012 PRECEDING PAGE BLANK NOT FILMED
Photometric Analysis for the Spin and Shape Parameters of the C-Type Main-Belt Asteroids \(171\) Ophelia and \(360\) Carlova
Establishing Asteroid–Meteorite Links
(10302) 1989 ML Michael Mueller, Alan W
Ultraviolet Spwtra and Geometric Albecios of 45 Asteroids
New Findings on Asteroid Spin-Vector Distributions
UBV Photometry of the Asteroid 44 Nysa