[1]2023astro-ph.EPPreprint
Orbital Period Change of Dimorphos Due to the DART Kinetic Impact
Cristina A. Thomas, Shantanu P. Naidu, Peter Scheirich & 46 others
What they foundDART shortened Dimorphos's orbit around Didymos by 33.0 ± 1.0 minutes, far more than the roughly 7 minutes expected from the spacecraft's momentum alone.
Why it mattersIt is the headline result of the first test of deflecting an asteroid.
What they studied
Ground-based light-curve observations before and after the impact.
Source for: Orbit period change from DART
[2]2023astro-ph.EPPreprint
Momentum Transfer from the DART Mission Kinetic Impact on Asteroid Dimorphos
Andrew F. Cheng, Harrison F. Agrusa, Brent W. Barbee & 66 others
What they foundDART slowed Dimorphos's orbital speed by 2.70 ± 0.10 mm/s, and recoil from the ejecta boosted the push well beyond the spacecraft's momentum.
Why it mattersThis 'momentum enhancement' is what makes kinetic impact an effective defence.
What they studied
Analysis based on the measured change in the binary orbit period.
Source for: Along-track speed change
[3]2023astro-ph.EPPreprint
The Dimorphos Boulder Swarm
David Jewitt, Yoonyoung Kim, Jing Li & 1 other
What they foundHubble found a swarm of boulders thrown off by DART, the largest about 7 m across, totalling about 0.1% of Dimorphos's mass.
Why it mattersThe lopsided boulder pattern suggests Dimorphos is a loosely bound rubble pile.
What they studied
Deep Hubble Space Telescope images; 37 boulders were measured.
Source for: Largest ejected boulder
[4]2023astro-ph.EPPreprint
Ejecta from the DART-produced active asteroid Dimorphos
Jian-Yang Li, Masatoshi Hirabayashi, Tony L. Farnham & 61 others
What they foundThe DART ejecta evolved from a cloud shaped by the asteroids' gravity into a tail pushed by sunlight, like a natural active asteroid.
Why it mattersIt is the first time an impact-made asteroid tail was watched forming under known conditions.
What they studied
Hubble images from 15 minutes to 18.5 days after impact.
[5]2024astro-ph.EPPreprint
Physical properties of asteroid Dimorphos as derived from the DART impact
S. D. Raducan, M. Jutzi, A. F. Cheng & 39 others
What they foundThe best-matching impact simulation shows Dimorphos is very weak (cohesion under a few pascals) and less dense than about 2,400 kg/m³.
Why it mattersIt confirms Dimorphos is a rubble pile, like Ryugu and Bennu.
What they studied
Numerical impact simulations matched to DART's measured deflection, ejecta cone and ejected mass.
[6]2021astro-ph.EPPreprint
The Excited Spin State of Dimorphos Resulting from the DART Impact
Harrison F. Agrusa, Ioannis Gkolias, Kleomenis Tsiganis & 12 others
What they foundBefore impact, this study predicted DART could leave Dimorphos wobbling or even tumbling, depending on its shape and the momentum transfer.
Why it mattersA tumbling moon matters for what ESA's Hera finds when it arrives.
What they studied
One analytic and two numerical methods.