Erik Ian Asphaug

Interests

Teaching

Planet formation; Planetary collisions and impact physics; Planetary surfaces; Great papers; Moons; Topical seminars

Research

I study giant impacts that dominate the late stage of planet and satellite formation, such as that which formed the Moon, that can explain why planets are so diverse and sometimes hemispherically dichotomous. I also study the geophysics of asteroids, comets and small moons, the 'small bodies' left over from accretion. I study the strength properties of meteorites and the origin of chondrules. Motivated students have led me to study other topics such as lakes and patterned ground on Mars, the delivery of volatiles to the lunar surface, and Saturn's rings. I am on the science team of NASA's Psyche mission, and ESA's Hera mission to Didymos, and JAXA's MMX mission to the Martian moons. I am Science PI of the SpaceTREx laboratory at U Arizona that is advancing miniaturized space exploration and small cubesat laboratories for low-gravity research.  

Courses

Scholarly Contributions

Chapters

• Asphaug, E., Collins, G., & Jutzi, M. (2015). Global Scale Impacts. In Asteroids IV(pp 661-677).
• Michel, P., Richardson, D., Durda, D., Jutzi, M., & Asphaug, E. (2015). Collisional Formation and Modeling of Asteroid Families. In Asteroids IV(pp 341-354).
• Scott, E., Keil, K., Goldstein, J., Asphaug, E., Bottke, W., & Moskovitz, N. (2015). Early Impact History and Dynamical Origin of Differentiated Meteorites and Asteroids. In Asteroids IV(pp 573-595).

Journals/Publications

• Cambioni, S., Weiss, B. P., Asphaug, E., Volk, K., Emsenhuber, A., Biersteker, J. B., Lin, Z., & Melikyan, R. (2025). Can metal-rich worlds form by giant impacts?. Astronomy and Astrophysics, 696(Issue). doi:10.1051/0004-6361/202450128
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  Context. Astronomical observations revealed the existence of exoplanets whose densities are far higher than what is expected from cosmochemistry. This high-density planetary population may account for 9% of terrestrial planets, suggesting the existence of processes that form planets with compositions dramatically different from their starting materials. Aims. A commonly invoked theory is that these high-density exoplanets are the metallic cores of super- Earth-sized planets whose rocky mantle was stripped by giant impacts. Here we aim to test this hypothesis. Methods. To maximize the likelihood that metal-rich giant-impact remnants form, we model the late orbital instability of tightly packed super-Earths orbiting a host star at small stellocentric distances ("compact systems"). We combine orbital dynamics, impact physics, and machine learning to explore the stability and collisional evolution of 100 observed compact systems. In each unstable compact system, we assume that the super-Earths undergo giant impacts and explore 1000 possible collision scenarios. We repeat the simulations with different initial conditions, such as the initial masses and composition of the super-Earths. Results. We find that giant impacts are capable of stripping the mantles of super-Earths and form metal-rich worlds as massive and large as the observed high-density exoplanets. However, we also find that, in most of the explored scenarios, mantle-stripping giant impacts between super-Earths are unlikely to occur at rates sufficient to explain the size and currently estimated abundance of the observed high-density exoplanets. We explain this as the interplay of three factors: the size of the super-Earths being in most cases smaller than 2 Earth radii; the efficiency of mantle stripping decreasing with increasing planetary size; and the likelihood of compact system instability decreasing with increasing average sizes of the planets in the compact system. Conclusions. We conclude that most of the observed high-density exoplanets are unlikely to be metal-rich giant-impact remnants.
• Denton, C. A., Asphaug, E., Emsenhuber, A., & Melikyan, R. (2025). Capture of an ancient Charon around Pluto. Nature Geoscience, 18(Issue 1). doi:10.1038/s41561-024-01612-0
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  Pluto and Charon are the largest binary system in the known population of trans-Neptunian objects in the outer Solar System. Their shared external orbital axis suggests a linked evolutionary history and collisional origin. Their radii, ~1,200 km and ~600 km, respectively, and Charon’s wide circular orbit of about 16 Pluto radii require a formation mechanism that places a large mass fraction into orbit, with sufficient angular momentum to drive tidal orbital expansion. Here we numerically model the collisional capture of Charon by Pluto using simulations that include material strength. In our simulations, friction distributes impact momentum, leading Charon and Pluto to become temporarily connected, instead of merging, for impacts aligned with the target’s rotation. In this ‘kiss-and-capture’ regime, coalescence of the bodies is prevented by strength. For a prograde target rotation consistent with the system angular momentum, Charon is then tidally decoupled and raised into a near-circular orbit from which it migrates outwards to distances consistent with its present orbit. Charon is captured relatively intact in this scenario, retaining its core and most of its mantle, which implies that Charon could be as ancient as Pluto.
• Dorogy, N., Sava, P., & Asphaug, E. (2025). Seismic interferometry with mobile spaceborne platforms. Advances in Space Research, 76(Issue). doi:10.1016/j.asr.2025.07.020
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  Understanding the deep interior structure of small planetary bodies is crucial for improving planetary formation and evolution theories, deflecting potentially hazardous near-Earth objects, and mapping the distribution of resources vital for sustained human exploration (e.g., water ice). Radar is a commonly-used remote exploration tool, but scattering and attenuation effects can limit its depth of penetration to the near subsurface. Seismic acquisition, however, is well suited to study deep interior structure, although landing seismic instrumentation on a planet or small body is complex and risky. To acquire seismic data remotely, we can use remote sensing seismometers that measure surface motion with laser Doppler vibrometers (LDVs). In lieu of active sources (kinetic impactors and explosives) which could eject debris that are hazardous for spacecraft operation, naturally occurring seismic activity can be used to recover travel times according to the theory of seismic interferometry. However, orbiter-mounted LDVs are mobile and thus sample different points on the ground unlike conventional seismometers that observe a fixed point. In this paper, we adapt the theory of seismic interferometry to account for receiver motion using asteroid 99942 Apophis as a test demonstration. We use artificially stimulated internal sources to mimic natural seismicity thus enabling acquisition with the remote sensing seismometer configuration. This technique provides the ability to remotely collect seismic data without the risks associated with landed instruments and active seismic sources.
• Emsenhuber, A., Mordasini, C., Mayor, M., Marmier, M., Udry, S., Burn, R., Schlecker, M., Mishra, L., Alibert, Y., Benz, W., & Asphaug, E. (2025). The New Generation Planetary Population Synthesis (NGPPS): VII. Statistical comparison with the HARPS/Coralie survey. Astronomy and Astrophysics, 701(Issue). doi:10.1051/0004-6361/202452485
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  Context. Planetary population synthesis is a tool that is used to better understand the key processes of planet formation at the statistical level. Aims. We seek to quantify the fidelity with which modern population syntheses reproduce observations in view of their use as predictive tools. Methods. We compared synthetic populations from the Generation 3 Bern Model of Planet Formation and Evolution (core accretion, solar-type host stars) and the HARPS/Coralie radial velocity sample. We biased the synthetic planet population according to the completeness of the observed data. We then performed quantitative statistical comparisons and systematically identified agreements and differences. Results. Our nominal population reproduces many of the main features of the HARPS planets, such as two main groups of planets in the mass-distance diagram (close-in sub-Neptunes and distant giants), a bimodal mass function with a less populated desert, an observed mean multiplicity of about 1.6, and several key correlations regarding the stellar metallicity dependency, the period ratio distribution, and the eccentricity distribution. Considering that the model was not optimised beforehand to reproduce any particular survey, this indicates that some of the important physical processes governing planetary formation could be captured. The remaining discrepancies that can be quantified thanks to the population synthesis approach point to areas that are not fully captured in the model. For instance, we find that the synthetic population has (1) in absolute terms too many planets by 70%, (2) a desert that is too deep by 60%, (3) a relative excess of giant planets by 40%,(4) planet eccentricities that are on average too low by a factor of about two (median of 0.07 versus 0.15), and (5) a metallicity effect that is too weak. Finally, the synthetic planets are overall too close to the star compared to the HARPS sample. The differences allowed us to find model parameters that better reproduce the observed planet masses, for which we computed additional synthetic populations. We find that decreasing the planet formation efficiency by increasing the planetesimal size re-balances the number of sub-Neptunes versus giant planets. Changing the efficiency of gas-driven migration also affects the sub-Neptune to giant planet ratio, with lower migration rates resulting in more giant planets and fewer sub-Neptunes. Conclusions. However, only modifying the model parameters seems to be insufficient for the model to fully reproduce both the observed mass and distance distributions at the same time. Instead, physical processes appear to be missing. Planets may originate on wider orbits than our model predicts. Mechanisms leading to higher eccentricities and slower disc-limited gas accretion also seem necessary. We also advocate that theoretical models should make a quantitative, rather than merely a qualitative, comparison between the many current and future large surveys and theoretical results to better understand the origins of planetary systems.
• Mohamed, M. M., Hamza, M. H., Garvie, L. A., Cotto-Figueroa, D., Asphaug, E., & Chattopadhyay, A. (2025). Microstructural modeling of the fragmentation of ordinary chondrites. Scientific Reports, 15(Issue 1). doi:10.1038/s41598-025-02724-2
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  The fracture behavior of rocks on asteroids offers insights into the evolution and dynamics of their boulders and regolith while providing critical data for developing hazard mitigation strategies. Information about the mechanical properties of asteroidal boulders primarily comes from laboratory studies of meteorites. This study examines the fracture mechanics of an ordinary chondrite (OC) using an innovative combination of experimental and computational methods to create models for the fragmentation processes of asteroidal materials. This approach illustrates how microstructural features—such as grain spacing and micropores—affect fracture behavior. Our results highlight the importance of microstructure in controlling fracture behavior, with normal stresses surpassing shear stresses in the primary minerals. Micropores accelerate fragmentation by facilitating the formation of multiple cracks. Olivine, plagioclase, and pyroxene demonstrate greater damage than troilite and kamacite, emphasizing differences in load-carrying capacity among these minerals. The findings offer insights for planetary science and the development of planetary defense strategies.
• Prettyman, T. H., Mittlefehldt, D. W., Asphaug, E. I., Binzel, R. P., Courville, S. W., Elkins-Tanton, L. T., Lawrence, D. J., Marchi, S., Merayo, J. M., McCoy, T. J., & Weiss, B. P. (2025). The Psyche Light Elements Investigation. \ssr, 221(8), 110.
• Ballantyne, H. A., Asphaug, E., Denton, C. A., Emsenhuber, A., & Jutzi, M. (2024). Sputnik Planitia as an impactor remnant indicative of an ancient rocky mascon in an oceanless Pluto. Nature Astronomy, 8, 748-755.
• Barnouin, O., Ballouz, R., Marchi, S., Vincent, J., Agrusa, H., Zhang, Y., Ernst, C. M., Pajola, M., Tusberti, F., Lucchetti, A., Daly, R. T., Palmer, E., Walsh, K. J., Michel, P., Sunshine, J. M., Rizos, J. L., Farnham, T. L., Richardson, D. C., Parro, L. M., , Murdoch, N., et al. (2024). The geology and evolution of the Near-Earth binary asteroid system (65803) Didymos. Nature Communications, 15, 6202.
• Cambioni, S., Weiss, B. P., Asphaug, E., Volk, K., Emsenhuber, A., Biersteker, J. B., Lin, Z., & Melikyan, R. (2024). Can metal-rich worlds form by giant impacts?. arXiv e-prints, arXiv:2408.15340.
• Dibb, S. D., Asphaug, E., Bell, J. F., Binzel, R. P., Bottke, W. F., Cambioni, S., Christoph, J. M., Elkins-Tanton, L. T., Jaumann, R., Lawrence, D. J., Oran, R., O'Rourke, J. G., Polansky, C., Weiss, B. P., Wieczorek, M., & Williams, D. A. (2024). A Post-Launch Summary of the Science of NASA's Psyche Mission. AGU Advances, 5(2), e2023AV001077.
• Dibb, S. D., Asphaug, E., Bell, J. F., Binzel, R. P., Bottke, W. F., Cambioni, S., Christoph, J. M., Elkins‐Tanton, L. T., Jaumann, R., Lawrence, D. J., Oran, R., O’Rourke, J. G., Polansky, C., Weiss, B. P., Wieczorek, M., & Williams, D. A. (2024). A Post‐Launch Summary of the Science of NASA's Psyche Mission. AGU Advances, 5(2). doi:10.1029/2023av001077
• Emsenhuber, A., Asphaug, E., Cambioni, S., Gabriel, T. S., Schwartz, S. R., Melikyan, R. E., & Denton, C. A. (2024). A New Database of Giant Impacts over a Wide Range of Masses and with Material Strength: A First Analysis of Outcomes. \psj, 5(3), 59.
• Garvie, L. A., Trif, L., Cotto-Figueroa, D., Asphaug, E., & Hoover, C. G. (2024). High surface area and interconnected nanoporosity of clay-rich astromaterials. Science Communications. doi:10.21203/rs.3.rs-3854166/v1
• Jiao, Y., Cheng, B., Huang, Y., Asphaug, E., Gladman, B., Malhotra, R., Michel, P., Yu, Y., & Baoyin, H. (2024). Asteroid Kamo`oalewa's journey from the lunar Giordano Bruno crater to Earth 1:1 resonance. Nature Astronomy, 8, 819-826.
• Pajola, M., Tusberti, F., Lucchetti, A., Barnouin, O., Cambioni, S., Ernst, C., Dotto, E., Daly, R., Poggiali, G., Hirabayashi, M., Nakano, R., Epifani, E. M., Chabot, N., Della Corte, V., Rivkin, A., Agrusa, H., Zhang, Y., Penasa, L., Ballouz, R. -., , Ivanovski, S., et al. (2024). Author Correction: Evidence for multi-fragmentation and mass shedding of boulders on rubble-pile binary asteroid system (65803) Didymos. Nature Communications, 15(1), 10021.
• Pajola, M., Tusberti, F., Lucchetti, A., Barnouin, O., Cambioni, S., Ernst, C., Dotto, E., Daly, R., Poggiali, G., Hirabayashi, M., Nakano, R., Epifani, E. M., Chabot, N., Della Corte, V., Rivkin, A., Agrusa, H., Zhang, Y., Penasa, L., Ballouz, R. -., , Ivanovski, S., et al. (2024). Evidence for multi-fragmentation and mass shedding of boulders on rubble-pile binary asteroid system (65803) Didymos. Nature Communications, 15, 6205.
• Scott, E. R., Sanders, I. S., Asphaug, E., & Tomlinson, E. L. (2024). Discussion of the unique ``eclogitic'' clast reported from Northwest Africa 801 (CR2) and the possibility of ejection of foundered crust from deep in a molten Moon-sized projectile. \maps, 59(4), 910-920.
• Vincent, J., Asphaug, E., Barnouin, O., Beccarelli, J., Benavidez, P. G., Campo-Bagatin, A., Chabot, N. L., Ernst, C. M., Hasselmann, P. H., Hirabayashi, M., Ieva, S., Karatekin, \., Ka{\v{s}p\'arek}, T., Kohout, T., Lin, Z., Lucchetti, A., Michel, P., Murdoch, N., Pajola, M., , Parro, L. M., et al. (2024). Macroscale Roughness Reveals the Complex History of Asteroids Didymos and Dimorphos. \psj, 5(10), 236.
• Barnouin, O., Ballouz, R., Marchi, S., Vincent, J., Agrusa, H., Zhang, Y., Ernst, C., Pajola, M., Tusberti, F., Lucchetti, A., Daly, R., Palmer, E., Walsh, K., Michel, P., Sunshine, J., Farnham, T., Richardson, D., Parro, L., Murdoch, N., , Robin, C., et al. (2023). The geology and evolution of a the Near-Earth binary asteroid system (65803) Didymos.. Nature Communications. doi:10.21203/rs.3.rs-3399230/v1
• Cheng, B., Asphaug, E., Yu, Y., & Baoyin, H. (2023). Measuring the mechanical properties of small body regolith layers using a granular penetrometer. Astrodynamics, 7(1), 15-29.
• Daly, R. T., Ernst, C. M., Barnouin, O. S., Chabot, N. L., Rivkin, A. S., Cheng, A. F., Adams, E. Y., Agrusa, H. F., Abel, E. D., Alford, A. L., Asphaug, E. I., Atchison, J. A., Badger, A. R., Baki, P., Ballouz, R., Bekker, D. L., Bellerose, J., Bhaskaran, S., Buratti, B. J., , Cambioni, S., et al. (2023). Successful kinetic impact into an asteroid for planetary defence. \nat, 616(7957), 443-447.
• Gowman, G., Cotto-Figueroa, D., Ryan, A., Garvie, L. A., Hoover, C. G., & Asphaug, E. (2023). Roughness and Angularity of Fragments from Meteorite Disruption Experiments. \psj, 4(10), 187.
• Scott, E. R., Sanders, I. S., Asphaug, E., & Tomlinson, E. L. (2023). Discussion of the unique “eclogitic” clast reported from Northwest Africa 801 (CR2) and the possibility of ejection of foundered crust from deep in a molten Moon‐sized projectile. Meteoritics & Planetary Science, 59(4), 910-920. doi:10.1111/maps.14069
• Asphaug, E., & McKinnon, W. B. (2022). H. J. “Jay” Melosh (1947–2020). Vol. 54, Issue 1 (Obituaries, News & Commentaries, Community Reports), 54(1). doi:10.3847/25c2cfeb.01af20d6
• Cheng, B., Asphaug, E., Ballouz, R., Yu, Y., & Baoyin, H. (2022). "Numerical Simulations of Drainage Grooves in Response to Extensional Fracturing: Testing the Phobos Groove Formation Model". psj, 3(11), 249.
• Elkins-Tanton, L. T., Asphaug, E., Bell, J. F., Bierson, C. J., Bills, B. G., Bottke, W. F., Courville, S. W., Dibb, S. D., Jun, I., Lawrence, D. J., Marchi, S., McCoy, T. J., Merayo, J. M., Oran, R., O'Rourke, J. G., Park, R. S., Peplowski, P. N., Prettyman, T. H., Raymond, C. A., , Weiss, B. P., et al. (2022). "Distinguishing the Origin of Asteroid (16) Psyche". ssr, 218(3), 17.
• Marchi, S., Asphaug, E., Bell, J., Bottke, W., Jaumann, R., Park, R., Polanskey, C., Prettyman, T., Williams, D., Binzel, R., Oran, R., Weiss, B., & Russell, C. (2022). "Correction to: Determining the Relative Cratering Ages of Regions of Psyche's Surface". ssr, 218(4), 30.
• Marchi, S., Asphaug, E., Bell, J., Bottke, W., Jaumann, R., Park, R., Polanskey, C., Prettyman, T., Williams, D., Binzel, R., Oran, R., Weiss, B., & Russell, C. (2022). "Determining the Relative Cratering Ages of Regions of Psyche's Surface". ssr, 218(4), 24.
• McKinnon, W. B., & Asphaug, E. (2022). "Obituary: H. J. ``Jay'' Melosh (1947-2020)". baas, 54, 101.
• Michel, P., K{"uppers}, M., Bagatin, A. C., Carry, B., Charnoz, S., Leon, J. d., Fitzsimmons, A., Gordo, P., Green, S. F., H{'erique}, A., Juzi, M., Karatekin, &., Kohout, T., Lazzarin, M., Murdoch, N., Okada, T., Palomba, E., Pravec, P., Snodgrass, C., , Tortora, P., et al. (2022). "The ESA Hera Mission: Detailed Characterization of the DART Impact Outcome and of the Binary Asteroid (65803) Didymos". psj, 3(7), 160.
• Nakajima, M., Genda, H., Asphaug, E., & Ida, S. (2022). "Large planets may not form fractionally large moons". Nature Communications, 13, 568.
• Pajola, M., Barnouin, O., Lucchetti, A., Hirabayashi, M., Ballouz, R. -., Asphaug, E., Ernst, C., Della Corte, V., Farnham, T., Poggiali, G., Sunshine, J., Epifani, E. M., Murdoch, N., Ieva, S., Schwartz, S., Ivanovski, S., Trigo-Rodriguez, J., Rossi, A., Chabot, N., , Zinzi, A., et al. (2022). "Anticipated Geological Assessment of the (65803) Didymos-Dimorphos System, Target of the DART-LICIACube Mission". psj, 3(9), 210.
• Rozehnal, J., Bro{v{z}}, M., Nesvorn{'y}, D., Walsh, K., Durda, D., Richardson, D., & Asphaug, E. (2022). "SPH simulations of high-speed collisions between asteroids and comets". icarus, 383, 115064.
• Vance}, L. D., Thangavelautham, J., Asphaug, E., & Cotto-Figueroa, D. (2022). "Possible particle ejection contributions to the shape and spin stability of small near-Earth asteroids". icarus, 384, 115078.
• Asphaug, E., Buratti, B., Bauer, J., Bellerose, J., Blewett, D., Bottke, W., Britt, D., Castillo-Rogez, J., Denk, T., Haghighipour, N., Li, J., Nesvorny, D., Rivkin, A., Scheeres, D., Sykes, M. V., Thomas, P., Verbiscer, A., Vilas, F., Yano, H., , Cartwright, R., et al. (2021). The Small Satellites of the Solar System: Priorities for the Decadal Study. Bulletin of the AAS, 53(4). doi:10.3847/25c2cfeb.298c2878
• Asphaug, E., Emsenhuber, A., Cambioni, S., Gabriel, T. S., & Schwartz, S. R. (2021). Collision Chains among the Terrestrial Planets. III. Formation of the Moon. \psj, 2(5), 200.
• Asphaug, E., Haynes, M., Virkki, A., Venditti, F., Hickson, D., Pinilla-Alonso, N., Brisset, J., Benner, L., Raymond, C., Lazio, J., Freeman, A., Castillo-Rogez, J., Taylor, P., Herique, A., Kofman, W., Sava, P., Pajola, M., Lucchetti, A., Pra, M. N., & Rivera-Valentin, E. (2021). Asteroids Inside Out: Radar Tomography. Bulletin of the AAS, 53(4). doi:10.3847/25c2cfeb.6ef5e6e8
• Asphaug, E., Miyamoto, H., Niihara, T., Wada, K., Ogawa, K., Senshu, H., Michel, P., Kikuchi, H., Hemmi, R., Nakamura, T., Nakamura, A. M., Hirata, N., Sasaki, S., Britt, D. T., Abell, P. A., Ballouz, R., Barnouin, O. S., Barsei, N., Barucci, M. A., , Biele, J., et al. (2021). Surface Environment of Phobos and Phobos Simulant UTPS. Planetary and Space Science. doi:10.21203/rs.3.rs-150345/v1
• Asphaug, E., Rabbi, M. F., Garvie, L. A., Cotto‐Figueroa, D., Khafagy, K. H., Datta, S., & Chattopadhyay, A. (2021). Understanding asteroidal failure through quasi‐static compression testing and 3‐D digital image correlation of the Aba Panu (L3) chondrite. Meteoritics & Planetary Science, 56(12), 2131-2143. doi:10.1111/maps.13761
• Cambioni, S., Delbo, M., Poggiali, G., Avdellidou, C., Ryan, A., Deshapriya, J., Asphaug, E., Ballouz, R. -., Barucci, M., Bennett, C., Bottke, W., Brucato, J., Burke, K., Cloutis, E., DellaGiustina, D., Emery, J., Rozitis, B., Walsh, K., & Lauretta, D. (2021). Fine-regolith production on asteroids controlled by rock porosity. \nat, 598(7879), 49-52.
• Cambioni, S., Jacobson, S. A., Emsenhuber, A., Asphaug, E., Rubie, D. C., Gabriel, T. S., Schwartz, S. R., & Furfaro, R. (2021). The Effect of Inefficient Accretion on Planetary Differentiation. \psj, 2(3), 93.
• Cheng, B., Yu, Y., Asphaug, E., Michel, P., Richardson, D. C., Hirabayashi, M., Yoshikawa, M., & Baoyin, H. (2021). Reconstructing the formation history of top-shaped asteroids from the surface boulder distribution. Nature Astronomy, 5, 134-138.
• Emsenhuber, A., Asphaug, E., Cambioni, S., Gabriel, T. S., & Schwartz, S. R. (2021). Collision Chains among the Terrestrial Planets. II. An Asymmetry between Earth and Venus. \psj, 2(5), 199.
• Emsenhuber, A., Mordasini, C., Burn, R., Alibert, Y., Benz, W., & Asphaug, E. (2021). The New Generation Planetary Population Synthesis (NGPPS). I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems. \aap, 656, A69.
• Emsenhuber, A., Mordasini, C., Burn, R., Alibert, Y., Benz, W., & Asphaug, E. (2021). The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical results. \aap, 656, A70.
• Miyamoto, H., Niihara, T., Wada, K., Ogawa, K., Senshu, H., Michel, P., Kikuchi, H., Hemmi, R., Nakamura, T., Nakamura, A. M., Hirata, N., Sasaki, S., Asphaug, E., Britt, D. T., Abell, P. A., Ballouz, R., Banouin, O. S., Baresi, N., Barucci, M. A., , Biele, J., et al. (2021). Surface environment of Phobos and Phobos simulant UTPS. Earth, Planets and Space, 73(1), 214.
• Rabbi, M., Garvie, L., Cotto-Figueroa, D. .., Asphaug, E., Khafagy, K., Datta, S., & Chattopadhyay, A. (2021). Understanding asteroidal failure through quasi-static compression testing and 3-D digital image correlation of the Aba Panu (L3) chondrite. \maps, 56(12), 2131-2143.
• Springmann, A., Swindle, T. D., Asphaug, E., Nolan, M., Michel, P., Venditti, F. C., Samarasinha, N., Sugita, S., Perry, M. E., Daly, R. T., Binzel, R. P., Sanchez-Vahamonde, C. R., Devogele, M., Hickson, D. C., Masiero, J., Busch, M. W., Brozovic, M., Becker, T. M., Marshall, S. E., , Virkki, A. K., et al. (2021). Near-Earth Objects. Bulletin of the AAS, 53(4). doi:10.3847/25c2cfeb.babe6f0d
• Asphaug, E. (2020). Book Review: Evolving Theories on the Origin of the Moon. Journal of Astronomical History and Heritage, 23(3), 701-702.
• Asphaug, E. (2020). Eye of a skull reveals details of cometary materials. \nat, 586(7831), 675-676.
• Asphaug, E. (2020). Interiors of small bodies and moons. Nature Communications, 11, 1564.
• Asphaug, E., Elkins‐Tanton, L. T., Bell, J. F., Bercovici, H., Bills, B., Binzel, R., Bottke, W. F., Dibb, S., Lawrence, D. J., Marchi, S., McCoy, T. J., Oran, R., Park, R. S., Peplowski, P. N., Polanskey, C. A., Prettyman, T. H., Russell, C. T., Schaefer, L., Weiss, B. P., , Wieczorek, M. A., et al. (2020). Observations, Meteorites, and Models: A Preflight Assessment of the Composition and Formation of (16) Psyche. Journal of Geophysical Research: Planets, 125(3). doi:10.1029/2019je006296
• Ballouz, R. -., Walsh, K., Barnouin, O., DellaGiustina, D., Asad, M. A., Jawin, E., Daly, M., Bottke, W., Michel, P., Avdellidou, C., Delbo, M., Daly, R., Asphaug, E., Bennett, C., Bierhaus, E., Connolly, H., Golish, D., Molaro, J., Nolan, M., , Pajola, M., et al. (2020). Bennu's near-Earth lifetime of 1.75 million years inferred from craters on its boulders. \nat, 587(7833), 205-209.
• Elkins-Tanton, L., Asphaug, E., Bell, J., Bercovici, H., Bills, B., Binzel, R., Bottke, W., Dibb, S., Lawrence, D., Marchi, S., McCoy, T., Oran, R., Park, R., Peplowski, P., Polanskey, C., Prettyman, T., Russell, C., Schaefer, L., Weiss, B., , Wieczorek, M., et al. (2020). Observations, Meteorites, and Models: A Preflight Assessment of the Composition and Formation of (16) Psyche. Journal of Geophysical Research (Planets), 125(3), e06296.
• Emsenhuber, A., Cambioni, S., Asphaug, E., Gabriel, T. S., Schwartz, S. R., & Furfaro, R. (2020). Realistic On-the-fly Outcomes of Planetary Collisions. II. Bringing Machine Learning to N-body Simulations. \apj, 891(1), 6.
• Emsenhuber, A., Mordasini, C., Burn, R., Alibert, Y., Benz, W., & Asphaug, E. (2020). The New Generation Planetary Population Synthesis (NGPPS). I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems. arXiv e-prints, arXiv:2007.05561.
• Emsenhuber, A., Mordasini, C., Burn, R., Alibert, Y., Benz, W., & Asphaug, E. (2020). The New Generation Planetary Population Synthesis (NGPPS). II. Planetary population of solar-like stars and overview of statistical results. arXiv e-prints, arXiv:2007.05562.
• Gabriel, T. S., Jackson, A. P., Asphaug, E., Reufer, A., Jutzi, M., & Benz, W. (2020). Gravity-dominated Collisions: A Model for the Largest Remnant Masses with Treatment for ``Hit and Run'' and Density Stratification. \apj, 892(1), 40.
• Marchi, S., Durda, D., Polanskey, C., Asphaug, E., Bottke, W., Elkins-Tanton, L., Garvie, L., Ray, S., Chocron, S., & Williams, D. (2020). Hypervelocity Impact Experiments in Iron-Nickel Ingots and Iron Meteorites: Implications for the NASA Psyche Mission. Journal of Geophysical Research (Planets), 125(2), e05927.
• Marsset, M., Bro{\v{z}}, M., Vernazza, P., Drouard, A., Castillo-Rogez, J., Hanu{\v{s}}, J., Viikinkoski, M., Rambaux, N., Carry, B., Jorda, L., {\v{S}eve\v{c}ek}, P., Birlan, M., Marchis, F., Podlewska-Gaca, E., Asphaug, E., Bartczak, P., Berthier, J., Cipriani, F., Colas, F., , Dudzi{\'nski}, G., et al. (2020). The violent collisional history of aqueously evolved (2) Pallas. Nature Astronomy, 4, 569-576.
• McKinnon, W. B., & Asphaug, E. (2020). H. J. Melosh. Nature Astronomy, 4, 1118-1119.
• Nallapu, R. T., Schwartz, S. R., Asphaug, E., & Thangavelautham, J. (2020). Robust Spin Control Design for the AOSAT+ Mission Concept. IEEE Journal on Miniaturization for Air and Space Systems, 1(1), 10-31.
• Wright, E., Quillen, A. C., South, J., Nelson, R. C., S{\'anchez}, P., Martini, L., Schwartz, S. R., Nakajima, M., & Asphaug, E. (2020). Boulder stranding in ejecta launched by an impact generated seismic pulse. \icarus, 337, 113424.
• Cambioni, S., Asphaug, E., Emsenhuber, A., Gabriel, T. S., Furfaro, R., & Schwartz, S. R. (2019). Realistic On-the-fly Outcomes of Planetary Collisions: Machine Learning Applied to Simulations of Giant Impacts. \apj, 875(1), 40.
• Cambioni, S., Delbo, M., Ryan, A. J., Furfaro, R., & Asphaug, E. (2019). Constraining the thermal properties of planetary surfaces using machine learning: Application to airless bodies. \icarus, 325, 16-30.
• Dellagiustina}, D., Emery, J., Golish, D., Rozitis, B., Bennett, C., Burke, K., Ballouz, R. -., Becker, K., Christensen, P., Drouet, D. C., Hamilton, V., Reuter, D., Rizk, B., Simon, A., Asphaug, E., Bandfield, J., Barnouin, O., Barucci, M., Bierhaus, E., , Binzel, R., et al. (2019). Properties of rubble-pile asteroid (101955) Bennu from OSIRIS-REx imaging and thermal analysis. Nature Astronomy, 3, 341-351.
• Emsenhuber, A., & Asphaug, E. (2019). Fate of the Runner in Hit-and-run Collisions. \apj, 875(2), 95.
• Emsenhuber, A., & Asphaug, E. (2019). Graze-and-merge Collisions under External Perturbers. \apj, 881(2), 102.
• Sava, P., & Asphaug, E. (2019). Seismology on small planetary bodies by orbital laser Doppler vibrometry. Advances in Space Research, 64(2), 527-544.
• Walsh}, K., Jawin, E., Ballouz, R. -., Barnouin, O., Bierhaus, E., Connolly, H., Molaro, J., McCoy, T., Delbo', M., Hartzell, C., Pajola, M., Schwartz, S., Trang, D., Asphaug, E., Becker, K., Beddingfield, C., Bennett, C., Bottke, W., Burke, K., , Clark, B., et al. (2019). Craters, boulders and regolith of (101955) Bennu indicative of an old and dynamic surface. Nature Geoscience, 12(4), 242-246.
• Walsh}, K., Jawin, E., Ballouz, R. -., Barnouin, O., Bierhaus, E., Connolly, H., Molaro, J., McCoy, T., Delbo', M., Hartzell, C., Pajola, M., Schwartz, S., Trang, D., Asphaug, E., Becker, K., Beddingfield, C., Bennett, C., Bottke, W., Burke, K., , Clark, B., et al. (2019). Publisher Correction: Craters, boulders and regolith of (101955) Bennu indicative of an old and dynamic surface. Nature Geoscience, 12(5), 399-399.
• Asphaug, E., & Emsenhuber, A. (2018). Giant Impacts Around Saturn. European Planetary Science Congress, 12, EPSC2018-569.
• Asphaug, E., Perera, V., Jackson, A. P., & Elkins‐Tanton, L. T. (2018). Effect of Reimpacting Debris on the Solidification of the Lunar Magma Ocean. Journal of Geophysical Research: Planets, 123(5), 1168-1191. doi:10.1029/2017je005512
• Belton, M., Zou, X., Li, J., & Asphaug, E. (2018). On the origin of internal layers in comet nuclei. \icarus, 314, 364-375.
• Benavidez, P., Durda, D., Enke, B., Campo Bagatin, A., Richardson, D., Asphaug, E., & Bottke, W. (2018). Impact simulation in the gravity regime: Exploring the effects of parent body size and internal structure. \icarus, 304, 143-161.
• Cambioni, S., Gabriel, T., Asphaug, E., Furfaro, R., Emsenhuber, A., & Schwartz, S. (2018). Application of Machine Learning to Giant Impact Studies. European Planetary Science Congress, 12, EPSC2018-121.
• Emsenhuber, A., & Asphaug, E. (2018). Sequential Giant Impacts. European Planetary Science Congress, 12, EPSC2018-196.
• Golabek, G., Emsenhuber, A., Jutzi, M., Asphaug, E., & Gerya, T. (2018). Coupling SPH and thermochemical models of planets: Methodology and example of a Mars-sized body. \icarus, 301, 235-246.
• Herique, A., Agnus, B., Asphaug, E., Barucci, A., Beck, P., Bellerose, J., Biele, J., Bonal, L., Bousquet, P., Bruzzone, L., Buck, C., Carnelli, I., Cheng, A., Ciarletti, V., Delbo, M., Du, J., Du, X., Eyraud, C., Fa, W., , Gil Fernandez, J., et al. (2018). Direct observations of asteroid interior and regolith structure: Science measurement requirements. Advances in Space Research, 62, 2141-2162.
• Jackson, A., Gabriel, T., & Asphaug, E. (2018). Constraints on the pre-impact orbits of Solar system giant impactors. \mnras, 474, 2924-2936.
• Michel, P., Kueppers, M., Sierks, H., Carnelli, I., Cheng, A., Mellab, K., Granvik, M., Kestil{\"a}, A., Kohout, T., Muinonen, K., N{\"asil\"a}, A., Penttila, A., Tikka, T., Tortora, P., Ciarletti, V., H{\'erique}, A., Murdoch, N., Asphaug, E., Rivkin, A., , Barnouin, O., et al. (2018). European component of the AIDA mission to a binary asteroid: Characterization and interpretation of the impact of the DART mission. Advances in Space Research, 62, 2261-2272.
• Perera, V., Jackson, A., Elkins-Tanton, L., & Asphaug, E. (2018). Effect of Reimpacting Debris on the Solidification of the Lunar Magma Ocean. Journal of Geophysical Research (Planets), 123, 1168-1191.
• Perera, V., Jackson, A., Elkins-Tanton, L., Asphaug, E., & Gabriel, T. (2018). Cratering and Penetration of the Early Lunar Crust. LPI Contributions, 2107, 2024.
• Sava, P., & Asphaug, E. (2018). 3D radar wavefield migration of comet interiors. Advances in Space Research, 62, 1146-1164.
• Sava, P., & Asphaug, E. (2018). 3D radar wavefield tomography of comet interiors. Advances in Space Research, 61, 2198-2213.
• Schwartz, S., Asphaug, E., Thanga, J., Nallapu, R., & Vance, L. (2018). An Ultra-Low-Gravity Centrifuge in Low-Earth Orbit. European Planetary Science Congress, 12, EPSC2018-421.
• Stopar, J., Jolliff, B., Speyerer, E., Asphaug, E., & Robinson, M. (2018). Potential impact-induced water-solid reactions on the Moon. \planss, 162, 157-169.
• Thangavelautham, J., & Asphaug, E. (2018). DRAGON: the Deimos Reconnaissance And Geological ObservatioN CubeSat. European Planetary Science Congress, 12, EPSC2018-567.
• Vernazza, P., Brozv, M., Drouard, A., Hanusv, J., Viikinkoski, M., Marsset, M., Jorda, L., Fetick, R., Carry, B., Marchis, F., Birlan, M., Fusco, T., Santana-Ros, T. .., Podlewska-Gaca, E. .., Jehin, E., Ferrais, M., Bartczak, P., Dudzinski, G., Berthier, J., , Castillo-Rogez, J. .., et al. (2018). VizieR Online Data Catalog: SPHERE/ZIMPOL (89) Julia images (Vernazza+, 2018). VizieR Online Data Catalog, 361.
• Vernazza, P., Bro{\v, z. M., Drouard, A., Hanu{\v, s. J., Viikinkoski, M., Marsset, M., Jorda, L., Fetick, R., Carry, B., Marchis, F., Birlan, M., Fusco, T., Santana-Ros, T. .., Podlewska-Gaca, E. .., Jehin, E., Ferrais, M., Bartczak, P., Dudzi{\'nski}, G., Berthier, J., , Castillo-Rogez, J. .., et al. (2018). The impact crater at the origin of the Julia family detected with VLT/SPHERE?. \aap, 618, A154.
• Benavidez, P., Durda, D., Enke, B., Campo Bagatin, A., Richardson, D., Asphaug, E., & Bottke, W. (2017). Large asteroid families modelled by impact events. European Planetary Science Congress, 11, EPSC2017-924.
• Golabek, G., Emsenhuber, A., Jutzi, M., Gerya, T., & Asphaug, E. (2017). Coupling giant impacts and long-term evolution models. European Planetary Science Congress, 11, EPSC2017-524.
• Lightholder, J., Thoesen, A., Adamson, E., Jakubowski, J., Nallapu, R., Smallwood, S., Raura, L., Klesh, A., Asphaug, E., & Thangavelautham, J. (2017). Asteroid Origins Satellite (AOSAT) I: An On-orbit Centrifuge Science Laboratory. Acta Astronautica, 133, 81-94.
• Asphaug, E. (2016). Rise and fall of the Martian moons. Nature Geoscience, 9, 568-569.
• Cotto-Figueroa, D. .., Asphaug, E., Garvie, L., Rai, A., Johnston, J., Borkowski, L., Datta, S., Chattopadhyay, A., & Morris, M. (2016). Scale-dependent measurements of meteorite strength: Implications for asteroid fragmentation. \icarus, 277, 73-77.
• Gabriel, T., Asphaug, E., Reufer, A., & Jackson, A. (2016). Mantle Fraction Enhancement in Targets of Giant Impacts. AGU Fall Meeting Abstracts, P51A-2117.
• Hurford, T., Asphaug, E., Spitale, J., Hemingway, D., Rhoden, A., Henning, W., Bills, B., Kattenhorn, S., & Walker, M. (2016). Tidal disruption of Phobos as the cause of surface fractures. Journal of Geophysical Research (Planets), 121, 1054-1065.
• Movshovitz, N., Nimmo, F., Korycansky, D., Asphaug, E., & Owen, J. (2016). Impact disruption of gravity-dominated bodies: New simulation data and scaling. \icarus, 275, 85-96.
• Nayak, M., & Asphaug, E. (2016). Sesquinary catenae on the Martian satellite Phobos from reaccretion of escaping ejecta. Nature Communications, 7, 12591.
• Perera, V., Jackson, A., Asphaug, E., & Ballouz, R. (2016). The spherical Brazil Nut Effect and its significance to asteroids. \icarus, 278, 194-203.
• Rozehnal, J., Bro{\v, z. M., Nesvorn{\'y}, D., Durda, D., Walsh, K., Richardson, D., & Asphaug, E. (2016). Hektor - an exceptional D-type family among Jovian Trojans. \mnras, 462, 2319-2332.
• Spitale, J. N., Asphaug, E., Hurford, T. A., Hemingway, D., Rhoden, A. R., Henning, W. G., Bills, B. G., Kattenhorn, S. A., & Walker, M. (2016). Tidal disruption of Phobos as the cause of surface fractures: Tidal Disruption of Phobos. Journal of Geophysical Research: Planets, 121(6), 1054-1065. doi:10.1002/2015je004943
• Asphaug, E., & Reufer, A. (2015). The Missing Mantle Paradox, and the Statistical Argument for Repeated Hit and Run Collisions. European Planetary Science Congress, 10, EPSC2015-797.
• Asphaug, E., Hurford, T., Spitale, J., Hemingway, D., Rhoden, A., Henning, W., Bills, B., & Walker, M. (2015). Tidal Disruption of Phobos as Cause of Surface Fractures. European Planetary Science Congress, 10, EPSC2015-796.
• Asphaug, E., Movshovitz, N., Nimmo, F., Korycansky, D. G., & Owen, J. M. (2015). Disruption and reaccretion of midsized moons during an outer solar system Late Heavy Bombardment. Geophysical Research Letters, 42(2), 256-263. doi:10.1002/2014gl062133
• Cotto-Figueroa, D. .., Asphaug, E., Garvie, L., Morris, M., Rai, A., Chattopadhyay, A., Johnston, J., & Borkowski, L. (2015). Scale-Dependent Measurements of Meteorite Strength and Fragmentation: Tamdakht (H5) and Allende (CV3).. AGU Fall Meeting Abstracts, NH11A-1889.
• Golabek, G., Emsenhuber, A., Jutzi, M., Gerya, T., & Asphaug, E. (2015). Coupling giant impacts and long-term evolution models. European Planetary Science Congress, 10, EPSC2015-48.
• Golabek, G., Jutzi, M., Emsenhuber, A., Gerya, T., & Asphaug, E. (2015). Coupling giant impacts and long-term evolution models. AGU Fall Meeting Abstracts, P11A-2059.
• Jutzi, M., & Asphaug, E. (2015). The shape and structure of cometary nuclei as a result of low-velocity accretion. Science, 348, 1355-1358.
• Liu, S., Hori, Y., Lin, D., & Asphaug, E. (2015). Giant Impact: An Efficient Mechanism for the Devolatilization of Super-Earths. \apj, 812, 164.
• Movshovitz, N., Nimmo, F., Korycansky, D., Asphaug, E., & Owen, J. (2015). Disruption and reaccretion of midsized moons during an outer solar system Late Heavy Bombardment. \grl, 42, 256-263.
• Movshovitz, N., Nimmo, F., Korycansky, D., Asphaug, E., & Owen, M. (2015). Collisional Disruption of Gravity Dominated Bodies: New Data and Scaling. AGU Fall Meeting Abstracts, P11A-2058.
• Winebrenner, D., Gary, D., Sahr, J., & Asphaug, E. (2015). On Using Solar Radio Emission to Probe Interiors of Asteroids and Comets. AGU Fall Meeting Abstracts, P51C-2083.
• Asphaug, E. (2014). Impact Origin of the Moon?. Annual Review of Earth and Planetary Sciences, 42(1), 551-578. doi:10.1146/annurev-earth-050212-124057
• Asphaug, E. (2014). Impact Origin of the Moon?. Annual Review of Earth and Planetary Sciences, 42, 551-578.
• Asphaug, E., & Reufer, A. (2014). Making an Iron Planet: The Case for Repeated Hit and Run Collisions. AGU Fall Meeting Abstracts, P44A-03.
• Asphaug, E., & Reufer, A. (2014). Mercury and other iron-rich planetary bodies as relics of inefficient accretion. Nature Geoscience, 7, 564-568.
• Clenet, H., Jutzi, M., Barrat, J., Asphaug, E., Benz, W., & Gillet, P. (2014). A Deep Moho in ``Small Planet'' Vesta and Implication Regarding the Chondritic Nature of Protoplanets. AGU Fall Meeting Abstracts, P51D-3971.
• Clenet, H., Jutzi, M., Barrat, J., Asphaug, E., Benz, W., & Gillet, P. (2014). A deep crust-mantle boundary in the asteroid 4 Vesta. \nat, 511, 303-306.
• Gim, Y., Heggy, E., Arumugam, D., Wu, X., & Asphaug, E. (2014). 3D Synthetic Aperture Radar Imaging of the Interior of the Cometary Nucleus. AGU Fall Meeting Abstracts, P51C-3962.
• Golabek, G., Jutzi, M., Gerya, T., & Asphaug, E. (2014). Towards Coupled Giant Impact and Long Term Interior Evolution Models. AGU Fall Meeting Abstracts, P51A-3904.
• Golabek, G., Jutzi, M., Gerya, T., & Asphaug, E. (2014). Towards coupled giant impact and long term interior evolution models. European Planetary Science Congress, 9, EPSC2014-433.
• Movshovitz, N., Nimmo, F., Korycansky, D., Asphaug, E., & Owen, M. (2014). Destruction and Re-Accretion of Mid-Size Moons During an Outer Solar System Late Heavy Bombardment. AGU Fall Meeting Abstracts, P43B-3991.
• Rivkin, A., Asphaug, E., & Bottke, W. (2014). The case of the missing Ceres family. \icarus, 243, 429-439.
• Asphaug, E. (2013). Planetary science: Go and catch a falling star. Nature Geoscience, 6, 422-423.
• Asphaug, E., & Reufer, A. (2013). Diversity of Planets in the Aftermath of Late Stage Accretion (Invited). AGU Fall Meeting Abstracts, P51H-01.
• Asphaug, E., & Reufer, A. (2013). Late origin of the Saturn system. \icarus, 223, 544-565.
• Asphaug, E., Orloff, T., & Kreslavsky, M. (2013). Distribution of polygon characteristic scale in Martian patterned ground terrain in the northern hemisphere using the Fourier transform: MARS PATTERNED GROUND SCALE DISTRIBUTION. Journal of Geophysical Research: Planets, 118(7), 1558-1566. doi:10.1002/jgre.20111
• Golabek, G., Jutzi, M., Gerya, T., & Asphaug, E. (2013). Towards coupled giant impact and long term interior evolution models. AGU Fall Meeting Abstracts, P51A-1721.
• Jutzi, M., Asphaug, E., Gillet, P., Barrat, J., & Benz, W. (2013). The structure of the asteroid 4 Vesta as revealed by models of planet-scale collisions. \nat, 494, 207-210.
• Movshovitz, N., Nimmo, F., Korycansky, D., Asphaug, E., & Owen, J. (2013). SPH Simulations of Volatiles Loss from Icy Satellites During a Late Heavy Bombardment. AGU Fall Meeting Abstracts, P43A-2007.
• Orloff, T., Kreslavsky, M., & Asphaug, E. (2013). Distribution of polygon characteristic scale in Martian patterned ground terrain in the northern hemisphere using the Fourier transform. Journal of Geophysical Research (Planets), 118, 1558-1566.
• Orloff, T., Kreslavsky, M., & Asphaug, E. (2013). Possible mechanism of boulder clustering on Mars. \icarus, 225, 992-999.
• Wenkert, D., Elkins-Tanton, L., Asphaug, E., Bairstow, S., Bell, J., Bercovici, D., Bills, B., Binzel, R., Bottke, W., Jun, I., Landau, D., Marchi, S., Oh, D., Weiss, B., & Zuber, M. (2013). Journey to a metal world: Concept for a Discovery mission to Psyche. AGU Fall Meeting Abstracts, P51A-1729.
• Kraal, E. R., Asphaug, E., Moore, J. M., & Lorenz, R. D. (2006). Quantitative geomorphic modeling of Martian bedrock shorelines. Journal of Geophysical Research: Planets, 111(E3). doi:10.1029/2005je002567
• Greenberg, R. J., {Melosh}, H., Asphaug, E. I., & Nolan, M. C. (1996). Impact Craters on Asteroids: Does Gravity or Strength Control Their Size?. Icarus, 124, 359-371.

Proceedings Publications

• Baijal, N., Asphaug, E., Adeene Denton, C., Jutzi, M., Raducan, S., & Cambioni, S. (2025, sep). Collisional Modification of Metal\ensuremath{-}Rich Asteroids and the Influence of Pre\ensuremath{-}impact Rotation. In EPSC-DPS Joint Meeting 2025, 2025.
• Cambioni, S., Weiss, B., Asphaug, E., Baijal, N., Biersteker, J., Bottke, W., Courville, S., Elkins-Tanton, L., Lawrence, D., Merayo, J., Raymond, C., Wieczorek, M., & Zuber, M. (2025, mar). Formation of Asteroid (16) Psyche by a Giant Impact. In 56th Lunar and Planetary Science Conference, 3090.
• Denton, C., Asphaug, E., Emsenhuber, A., & Melikyan, R. (2025, mar). Kiss-and-Capture Preserves an Ancient Charon Around Pluto. In 56th Lunar and Planetary Science Conference, 3090.
• Jiao, Y., Cheng, B., Dai, W., Asphaug, E., Jutzi, M., Raducan, S., Yan, X., Yu, Y., & Baoyin, H. (2025, sep). Giant Craters on Asteroid Mathilde Revealing a Cohesive Porous Interior of C-type Parent Bodies. In EPSC-DPS Joint Meeting 2025, 2025.
• Lagnado, M., Denton, C., Asphaug, E., & Baijal, N. (2025, mar). Effects of Layering and Impact Angle on the Crater Morphology of Asteroid (16) Psyche. In 56th Lunar and Planetary Science Conference, 3090.
• Miyamoto, H., Kobayashi, M., Murakami, T., Takekura, S., Toida, A., Shimizu, Y., Takemura, T., Yoshimitsu, T., Usami, N., Otsuki, M., Kunii, Y., Maeda, T., Kumamoto, A., Nakauchi, Y., Heldmann, J., Hurley, D., Niihara, T., Usui, T., Nagaoka, H., , Saiki, K., et al. (2025, mar). High-Precision Permittivity Measurements by LDA: Probing Bulk Regolith Density and Putative Lunar Ice. In 56th Lunar and Planetary Science Conference, 3090.
• Mohamed, M., Hamza, M., Garvie, L., Cotto-Figueroa, D. .., Asphaug, E., & Chattopadhyay, A. (2025, mar). Fracture Modeling of the Hammadah al Hamra 346 (L6) Meteorite: Insights into the Mechanical Behavior of Ordinary Chondrites. In 56th Lunar and Planetary Science Conference, 3090.
• Mohamed, M., Ranade, R., Garvie, L., Cotto-Figueroa, D. .., Asphaug, E., & Chattopadhyay, A. (2025, mar). Fragmentation Insights in the Hammadah al Hamra 346 (L6) Meteorite: Porosity and Surface Topology Charaterization. In 56th Lunar and Planetary Science Conference, 3090.
• Raducan, S., Bickel, V., Ernst, C., Michel, P., Asphaug, E., Almeida, M., Jutzi, M., & Thomas, N. (2025, mar). Insights into Deimos Formation from Impact Simulations and New Fly-by Data. In 56th Lunar and Planetary Science Conference, 3090.
• Vance, L., Thukral, H., Vernekar, H., Thangelautham, J., & Asphaug, E. (2025, apr). An Apophis Precursor Mission to Establish High Resolution Topography Prior to 2029 Earth Flyby. In Apophis T-4 Years, 3083.
• Baijal, N., Asphaug, E., Denton, C., Jutzi, M., Cambioni, S., Raducan, S., Marchi, S., Elkins-Tanton, L., Bierson, C., & Binzel, R. (2024, mar). Effect of Asteroid Shape on Basin-Scale Collisions: Implications for (16) Psyche. In 55th Lunar and Planetary Science Conference, 3040.
• Ballouz, R. -., Ryan, A., Macke, R., Aebersold, J., Asphaug, E., Barnouin, O., Bierhaus, E., Blumenfeld, E., Delbo, M., Eckley, S., Fulford, R., Golish, D., Hildebrand, A., Hoover, C., Jardine, K., Jawin, E., Lunning, N., McCubbin, F., Michel, P., , Molaro, J., et al. (2024, mar). Investigating the Physical Modification of the Bennu Sample During Entry, Descent, and Landing. In 55th Lunar and Planetary Science Conference, 3040.
• Bhatt, S., Davis, T., Cotto-Figueroa, D. .., Asphaug, E., Garvie, L., & Hoover, C. (2024, mar). Nano-Chemo-Mechanical Behavior of the Carbonaceous Chondrite Meteorite TARDA (C2-UNG): Implications for Planetary Defense. In 55th Lunar and Planetary Science Conference, 3040.
• Cambioni, S., Weiss, B., Asphaug, E., Volk, K., Emsenhuber, A., Melikyan, R., Biersteker, J., & Lin, Z. (2024, mar). A Size Barrier to Forming Metal-Rich Worlds by Giant Impacts. In 55th Lunar and Planetary Science Conference, 3040.
• Denton, C. A., Asphaug, E., & Melikyan, R. (2024, aug). Groundhog Day in the Kuiper Belt? How strength can trap KBOs in a collisional loop. In AAS/Division of Dynamical Astronomy Meeting, 56.
• Jiao, Y., Asphaug, E., Cheng, B., & Baoyin, H. (2024, sep). Effect of Giant Cratering Impacts on the Slow Rotation of Asteroid Mathilde. In European Planetary Science Congress.
• Jiao, Y., Cheng, B., Huang, Y., Asphaug, E., Gladman, B., Malhotra, R., Michel, P., Yu, Y., & Baoyin, H. (2024, mar). Dynamical Constraints Linking Earth Co-Orbital Asteroid Kamo`oalewa to the Lunar Giordano Bruno Impact. In 55th Lunar and Planetary Science Conference, 3040.
• Pajola, M., Tusberti, F., Lucchetti, A., Barnouin, O., Cambioni, S., Ernst, C., Dotto, E., Daly, R., Poggiali, G., Hirabayashi, M., Nakano, R., Mazzotta Epifani, E., Chabot, N., Della Corte, V., Rivkin, A., Agrusa, H., Zhang, Y., Penasa, L., Ballouz, R., , Ivanovski, S., et al. (2024, mar). The Didymos and Dimorphos Global Boulder Size-Frequency Distributions: Implications on Their Mutual Origin. In 55th Lunar and Planetary Science Conference, 3040.
• Purdie, Z., Baijal, N., Spring, I., Mallik, A., Asphaug, E., Melikyan, R., Denton, C., Cambioni, S., & Emsenhuber, A. (2024, mar). Applying Laboratory Studies to 3D Modeling Results of Thermodynamic Evolution During Planet-Forming Collisions. In 55th Lunar and Planetary Science Conference, 3040.
• Asphaug, E. (2023, mar). Hysteretic Evolution of Accreting Planetary Interiors. In LPI Contributions, 2806.
• Asphaug, E., Thirupathi Raj, A., Qiu, J., Vilvanathan, V., Xu, Y., & Thangavelautham, J. (2023). Systems Engineering of Using Sandbags for Site Preparation and Shelter Design for a Modular Lunar Base. In IAC.
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