Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Countries citing papers authored by S. J. Weidenschilling
Since
Specialization
Citations
This map shows the geographic impact of S. J. Weidenschilling's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by S. J. Weidenschilling with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. J. Weidenschilling more than expected).
Fields of papers citing papers by S. J. Weidenschilling
This network shows the impact of papers produced by S. J. Weidenschilling. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by S. J. Weidenschilling. The network helps show where S. J. Weidenschilling may publish in the future.
Co-authorship network of co-authors of S. J. Weidenschilling
This figure shows the co-authorship network connecting the top 25 collaborators of S. J. Weidenschilling.
A scholar is included among the top collaborators of S. J. Weidenschilling based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with S. J. Weidenschilling. S. J. Weidenschilling is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Michel, Patrick, C. A. Goodrich, Martin Jutzi, et al.. (2013). Numerical Modeling of Catastrophic Disruption of Molten and Partly Molten Asteroids, with Implications for Breakup of the Ureilite Parent Body. Lunar and Planetary Science Conference. 1300.1 indexed citations
2.
Weidenschilling, S. J.. (2013). Gravitational Diffusion and Mixing During Accretion of the Asteroids. LPI. 2704.1 indexed citations
3.
Hood, L. L., F. J. Ciesla, N. A. Artemieva, & S. J. Weidenschilling. (2008). Nebular Shock Waves Generated by Large-Scale Impacts: Possible Sites for Chondrule Formation. LPI. 2147.1 indexed citations
4.
Weidenschilling, S. J., F. Marzari, & Donald R. Davis. (2004). Accretion of the Outer Planets: Oligarchy or Monarchy?. LPI. 1174.2 indexed citations
5.
Weidenschilling, S. J., et al.. (2001). Origin of the Double Asteroid 90 Antiope: A Continuing Puzzle. LPI. 1890.6 indexed citations
6.
Ghosh, A., S. J. Weidenschilling, & H. Y. McSween. (2001). Thermal Consequences of the Multizone Accretion Code on the Structure of the Asteroid Belt. Lunar and Planetary Science Conference. 1760.1 indexed citations
7.
Weidenschilling, S. J. & F. Marzari. (1999). Supersonic Planetesimals in the Solar Nebula. Lunar and Planetary Science Conference. 1713.1 indexed citations
8.
Weidenschilling, S. J. & F. Marzari. (1998). Did Jupiter Make Chondrules. Meteoritics and Planetary Science. 32.1 indexed citations
9.
Weidenschilling, S. J.. (1997). Planetesimals from Stardust. ASPC. 122. 281.2 indexed citations
10.
Weidenschilling, S. J.. (1997). Growing Jupiter's Core by Runaway Accretion. Lunar and Planetary Science Conference. 1513.4 indexed citations
11.
Farinella, P., Donald R. Davis, & S. J. Weidenschilling. (1995). Collisional Evolution of Kuiper Belt Objects. 27.1 indexed citations
12.
Weidenschilling, S. J. & Donald R. Davis. (1988). Dust to Dust: Low-Velocity Impacts of Fragile Projectiles. Lunar and Planetary Science Conference. 19. 1253.3 indexed citations
13.
Chapman, C. R., Donald R. Davis, & S. J. Weidenschilling. (1987). Impact and cratering processes on asteroids, satellites, and planets. 399.1 indexed citations
14.
Drummond, J., S. J. Weidenschilling, C. R. Chapman, & Donald R. Davis. (1987). Poles and Axial Ratios of 15 Asteroids. Bulletin of the American Astronomical Society. 19. 825.1 indexed citations
15.
Davis, Donald R., et al.. (1986). Experimental Studies of Catastrophic Disruption. Lunar and Planetary Science Conference. 156–157.1 indexed citations
16.
Davis, Donald R., C. R. Chapman, R. Greenberg, & S. J. Weidenschilling. (1983). Asteroid Collisions; Effective Body Strength and Efficiency of Catastrophic Disruption. LPI. 146–147.3 indexed citations
17.
Davis, Donald R. & S. J. Weidenschilling. (1981). Avoiding Close Encounters: Collisional Evolution of Trojan Asteroids. Lunar and Planetary Science Conference. 199–201.5 indexed citations
18.
Weidenschilling, S. J.. (1980). How Fast Can an Asteroid Spin. Bulletin of the American Astronomical Society. 12. 662.2 indexed citations
19.
Weidenschilling, S. J.. (1979). Self-Induced Turbulence and the Onset of Gravitational Instability in a Dust Layer.. Bulletin of the American Astronomical Society. 11. 552.3 indexed citations
20.
Rajan, R. S. & S. J. Weidenschilling. (1977). Dynamics of Small Particles in the Solar System.. Bulletin of the American Astronomical Society. 9. 519.1 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.