42 of the largest asteroids: from spheres to dog bones

More than 650,000 objects orbit in the solar system’s asteroid belt between Mars and Jupiter. Astronomers at the European Southern Observatory ESO imaged 42 of the largest in a large-scale effort from 2017 to 2019; the results have now been published. What did they notice?

Different shapes: By reconstructing the shapes of the objects, the team found that the observed asteroids are divided into two families. Some are almost perfectly spherical, such as Hygiea and Ceres, while others have an elongated shape. The most unusual shape is the «dog bone» asteroid Cleopatra.

Different densities: by combining the shapes of the asteroids with their masses, the researchers found that densities vary significantly within the sample. The four least dense asteroids, including Lamberta and Sylvia, have densities of about 1.3 grams per cubic centimeter, which is about the same as coal or slightly more than the density of water. These asteroids are likely to be composed primarily of ice and clumps of dust. The densest asteroids, Psyche and Calliope, have densities of 3.9 and 4.4 grams per cubic centimeter, respectively, which is more than the density of diamond. Here, a composition of rock is to be assumed.

Variable origin: The large density differences show that also the composition of the asteroids varies strongly. This allows conclusions to be drawn about the origin of the asteroids. «Our observations suggest that these bodies have migrated considerably since their formation. In short, we can only understand this enormous diversity in their composition if the bodies were formed in different regions of the solar system,» explains Josef Hanuš of Charles University in Prague, Czech Republic, one of the study’s authors. In particular, the results support the theory that the lowest-density asteroids must have formed in the remote regions beyond Neptune’s orbit and then migrated to their present location.

This image depicts 42 of the largest objects in the asteroid belt, located between Mars and Jupiter. Most of them are larger than 100 kilometres, with the two biggest asteroids being Ceres and Vesta, which are around 940 and 520 kilometres in diameter, and the two smallest ones being Urania and Ausonia, each only about 90 kilometres. The images of the asteroids have been captured with the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument on ESO’s Very Large Telescope.

Leave a Comment

Tu dirección de correo electrónico no será publicada. Los campos obligatorios están marcados con *

  • BrandonQMorris
  • Brandon Q. Morris es físico y especialista en el espacio. Lleva mucho tiempo preocupado por las cuestiones espaciales, tanto a nivel profesional como privado, y aunque quería ser astronauta, tuvo que quedarse en la Tierra por diversas razones. Le fascina especialmente el "qué pasaría si" y a través de sus libros pretende compartir historias convincentes de ciencia ficción dura que podrían suceder realmente, y que algún día podrían suceder. Morris es autor de varias novelas de ciencia ficción de gran éxito de ventas, como la serie Enceladus.

    Brandon es un orgulloso miembro de la Science Fiction and Fantasy Writers of America y de la Mars Society.