[1]2010astro-ph.EPPreprint
Triplicity and Physical Characteristics of Asteroid (216) Kleopatra
Pascal Descamps, F. Marchis, J. Berthier & 16 others
What they foundKleopatra has two small moons; their orbits give a system mass of about 4.64 × 10¹⁸ kg and a density of about 3.6 g/cm³, implying significant porosity.
Why it mattersIt confirmed the dog-bone shape and showed Kleopatra is not solid metal.
What they studied
Keck adaptive-optics images, Spitzer spectra and past occultations.
Source for: System mass
[2]2021astro-ph.EPPeer-reviewed
(216) Kleopatra, a low density critically rotating M-type asteroid
F. Marchis, L. Jorda, P. Vernazza & 36 others
What they foundKleopatra's shape is close to an equilibrium dumbbell and it spins near the limit at which it would start shedding material; its density is lower than a previous 5 g/cm³ estimate.
Why it mattersA lower density makes the dumbbell shape easier to explain.
What they studied
VLT/SPHERE images from 2017–2018 plus light curves, occultations and radar.
[3]2013astro-ph.EPPreprint
Analysis of Asteroid (216) Kleopatra using dynamical and structural constraints
Masatoshi Hirabayashi & Daniel J. Scheeres
What they foundKleopatra won't shed surface material at its current 5.385-hour spin, but its neck may be close to structural failure.
Why it mattersSo its moons probably didn't form by simple surface shedding.
What they studied
Stability calculations using its radar shape and measured mass.
Source for: Spin period
[4]2014astro-ph.EPPeer-reviewed
Dumb-bell-shaped equilibrium figures for fiducial contact-binary asteroids and EKBOs
Pascal Descamps
What they foundDumbbell-shaped equilibrium figures fit Kleopatra's light curves and give new density estimates.
Why it mattersThis shape family is a better model for peanut-shaped asteroids than two separate spheres.
What they studied
Mathematical models tested on Kleopatra, Trojan asteroid Hektor and a Kuiper belt object.