Kleopatra / Science

Science · Kleopatra

What the research says about Kleopatra

These are six research papers, all free to read on arXiv, about Kleopatra. We summarize each one in plain English from its abstract.

  • Papers 6
  • Topics 3
  • Reviewed Oct 24, 2026
  • Source arXiv.org
Illustrative · not to scale

Our own artist's impression. No figures are taken from the papers.

Known so far

Every number links to the paper it comes from.

System mass
4.64 × 10¹⁸kg1From the orbits of its two moons (± 0.02).
Spin period
5.385hours3Used to test whether it sheds material (it doesn’t, at this spin).
01

Size, shape & spin

4 papers

How big Kleopatra is, what shape it has and how it spins.

[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.

02

Orbit & dynamics

1 paper

How Kleopatra moves, and the gravity and sunlight forces that shape its path.

[5]2021astro-ph.EPPeer-reviewed

Observed tidal evolution of Kleopatra's outer satellite

M. Brož, J. Ďurech, B. Carry & 8 others

What they foundLinking observations from 1980 to 2018 needs tidal effects that slowly widen the orbit of the outer moon, Alexhelios.

Why it mattersIt is a rare case of tides seen working on an asteroid's moon.
What they studied

Orbit modelling with an occultation from 1980 and VLT/SPHERE astrometry.

03

Missions

1 paper

Spacecraft that have visited, or are planned to study, Kleopatra.

[6]2025astro-ph.EPPreprint

Radio Science Investigations for the Heavy Metal Mission to Asteroid (216) Kleopatra

Paolo Tortora, Riccardo Lasagni Manghi, Edoardo Gramigna & 3 others

What they foundA proposed 'Heavy Metal' mission could measure Kleopatra's mass to one part in ten million and map its gravity well enough to tell interior models apart.

Why it mattersIt shows what a visit could reveal about metal-rich asteroids.
What they studied

Simulations of radio-tracking and imaging for the mission concept.

New research

New papers on Kleopatra, checked weekly, summarized after a person reads it.

RSS feed

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How we choose papers

We search arXiv for Kleopatra papers and keep the ones that add something new, are clearly written up and are relevant to a general reader. A person reads every abstract.

Our own words, our own drawings

Summaries are written by us from each paper’s abstract, not copied. Diagrams are our own simplified drawings, not figures from the papers.

Preprint vs. peer-reviewed

“Peer-reviewed” means arXiv lists a journal reference for the paper. Everything else is marked “Preprint”: shared openly, possibly before or without journal review.

Paper metadata courtesy of arXiv. Summaries written by us; read the original papers via the links. Paper metadata from arXiv.org, which does not endorse this site.