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.
The Provenances of Asteroids, and Their Contributions to the Volatile Inventories of the Terrestrial Planets
2012475 citationsC. M. O'd. Alexander, R. Bowden et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of K. T. Howard'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 K. T. Howard with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. T. Howard more than expected).
This network shows the impact of papers produced by K. T. Howard. 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 K. T. Howard. The network helps show where K. T. Howard may publish in the future.
Co-authorship network of co-authors of K. T. Howard
This figure shows the co-authorship network connecting the top 25 collaborators of K. T. Howard.
A scholar is included among the top collaborators of K. T. Howard 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 K. T. Howard. K. T. Howard is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Weisberg, M. K., et al.. (2021). Abundances and Isotopic Compositions of Volatile H, N, C in Unequilibrated Enstatite Chondrites and the Volatile Inventories of the Terrestrial Planets. Lunar and Planetary Science Conference. 2116.1 indexed citations
3.
Takir, D., K. T. Howard, K. R. Stockstill‐Cahill, et al.. (2020). Spectroscopy and Mineralogy of Aguas Zarcas. Lunar and Planetary Science Conference. 2533.2 indexed citations
4.
Zolensky, M. E., et al.. (2020). Petrologic Evidence of Hydrothermal Activity on the EL3 Parent Asteroid. Lunar and Planetary Science Conference. 1683.2 indexed citations
5.
Greenwood, R. C., K. T. Howard, A. J. King, et al.. (2019). Oxygen Isotope Evidence for Multiple CM Parent Bodies: What Will We Learn from the Hayabusa2 and OSIRIS-REx Sample Return Missions?. LPI. 3191.5 indexed citations
6.
Howard, K. T. & B. Zanda. (2019). Why is the Degree of Aqueous Alteration Variable. 82(2157). 6178.1 indexed citations
7.
Sunshine, J. M., et al.. (2015). Aqueous Alteration in CR Meteorites as Seen with VIS/NIR and MIR Spectroscopy. LPI. 2540.2 indexed citations
8.
Nehru, C. E., M. K. Weisberg, K. T. Howard, et al.. (2014). An Unusual Dark Inclusion from the Bencubbin Breccia and Deformation in an Asteroid Regolith. LPI. 1437.1 indexed citations
9.
Howard, K. T. & C. M. O'd. Alexander. (2013). A New Classification Scheme for Aqueously Altered Carbonaceous Chondrites Based on Total Phyllosilicate Abundance. LPI. 2598.4 indexed citations
10.
Howard, K. T., G. K. Benedix, P. A. Bland, et al.. (2013). Non-Progressive Aqueous Alteration of CM Carbonaceous Chondrites: The Perspective of Modal Mineralogy and Bulk O-Isotopes. Lunar and Planetary Science Conference. 2520.1 indexed citations
11.
Sunshine, J. M., et al.. (2013). Fe and Mg Compositional Variations of CM/CI Meteorites and Dark Asteroids. LPI. 1048.1 indexed citations
12.
Alexander, C. M. O'd., R. Bowden, Marilyn L. Fogel, & K. T. Howard. (2013). Carbonate Abundances and Isotopic Compositions in Chondrites. LPI. 2788.2 indexed citations
13.
Alexander, C. M. O'd., R. Bowden, Marilyn L. Fogel, K. T. Howard, & C. D. K. Herd. (2012). The Origin of Water in Chondrites and Volatiles in the Terrestrial Planet Region. Lunar and Planetary Science Conference. 1929.1 indexed citations
14.
Howard, K. T., et al.. (2010). Correlated modal mineralogy, aqueous alteration and oxygen isotope composition of CM Chondrites. Open Research Online (The Open University). 1595.3 indexed citations
15.
Vernazza, Pierre, F. Cipriani, C. A. Dukes, et al.. (2010). Origin of the Martian moons: Investigating their surface composition. 262.3 indexed citations
16.
Vernazza, Pierre, F. Cipriani, C. A. Dukes, et al.. (2010). Meteorite Analogs for Phobos and Deimos: Unraveling the Origin of the Martian Moons. Meteoritics and Planetary Science Supplement. 73. 5076.4 indexed citations
17.
Howard, K. T., G. K. Benedix, P. A. Bland, & G. Cressey. (2010). Aqueous Alteration, `Serpentinization' and the CM-C2ung-CI Connection by PSD-XRD. Meteoritics and Planetary Science Supplement. 73. 5186.5 indexed citations
18.
Howard, K. T., et al.. (2009). Spherical carbonaceous inclusions in (Darwin) impact glass and co-genetic mineral (SiO 2 + TiO 2 ) growth under impact conditions. LPI. 1603.1 indexed citations
19.
Howard, K. T.. (2003). Geochemical Systematics in Darwin Impact Glass. Meteoritics and Planetary Science Supplement. 38. 5079.2 indexed citations
20.
Howard, K. T., et al.. (2000). The 770 Ka Tektite Producing Impact Event: Evidence for Distal Environmental Effects in NE Thailand. Lunar and Planetary Science Conference. 1308.2 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.