Artist concept of Haumea, with the correct proportions of the main body and the ring. The ring is at a distance of 2287 kilometers from the center of the main body and is darker than the surface of the dwarf planet itself.
At the ends of the Solar System, beyond the orbit of Neptune, there is a belt of objects composed of ice and rocks, among which four dwarf planets stand out: Pluto, Eris, Makemake and Haumea. The latter is the least well known of the four and was recently the object of an international observation campaign which was able to establish its main physical characteristics. The study, led by astronomers from the Institute of Astrophysics of Andalusia and published in Nature, reveals the presence of a ring around the planet.
“We predicted that Haumea would pass in front of a star on the 21st of January 2017, and twelve telescopes from ten different European observatories converged on the phenomenon,” says José Luis Ortiz, researcher at the Institute of Astrophysics of Andalusia (IAA-CSIC) in charge of the study. “This deployment of technical means allowed us to reconstruct with a very high precision the shape and size of dwarf planet Haumea, and discover to our surprise that it is considerably bigger and less reflecting than was previously believed. It is also much less dense than previously thought, which answered questions that had been pending about the object.”
Haumea is an interesting object: it rotates around the Sun in an elliptic orbit which takes it 284 years to complete (it presently lies fifty times further from the Sun than the Earth), and it takes 3.9 hours to rotate around its axis, much less than any other body measuring more than a hundred kilometers long in the entire Solar System. This rotational speed causes it to flatten out, giving it an ellipsoid shape similar to a rugby ball. The recently published data reveal that Haumea measures 2,320 kilometers in its largest axis — almost the same as Pluto — but lacks the global atmosphere that Pluto has.
First Trans-Neptunian Object With a Ring
“One of the most interesting and unexpected findings was the discovery of a ring around Haumea. Until a few years ago we only knew of the existence of rings around the giant planets; then, recently, our team discovered that two small bodies situated between Jupiter and Neptune, belonging to a group called centaurs, have dense rings around them, which came as a big surprise. Now we have discovered that bodies even farther away than the centaurs, bigger and with very different general characteristics, can also have rings,” says Pablo Santos-Sanz, another member of the IAA-CSIC team.
According to the data obtained from the stellar occultation, the ring lies on the equatorial plane of the dwarf planet, just like its biggest satellite, Hi´iaka, and it displays a 3:1 resonance with respect to the rotation of Haumea, which means that the frozen particles which compose the ring rotate three times slower around the planet than it rotates around its own axis.
“There are different possible explanations for the formation of the ring; it may have originated in a collision with another object, or in the dispersal of surface material due to the planet’s high rotational speed,” says Ortiz (IAA-CSIC). It is the first time a ring has been discovered around a trans-neptunian object, and it shows that the presence of rings could be much more common than was previously thought, in our Solar System as well as in other planetary systems.
This study has been possible thanks to the national funding of the AYA program and to EU funding under its H2020 program (SBNAF project, Small Bodies Near and Far).
Story Source: Materials provided by Instituto de Astrofísica de Andalucía (IAA-CSIC) Original written by Whitney Clavin.Note: Content may be edited for style and length.
J. L. Ortiz, P. Santos-Sanz, B. Sicardy, G. Benedetti-Rossi, D. Bérard, N. Morales, R. Duffard, F. Braga-Ribas, U. Hopp, C. Ries, V. Nascimbeni, F. Marzari, V. Granata, A. Pál, C. Kiss, T. Pribulla, R. Komžík, K. Hornoch, P. Pravec, P. Bacci, M. Maestripieri, L. Nerli, L. Mazzei, M. Bachini, F. Martinelli, G. Succi, F. Ciabattari, H. Mikuz, A. Carbognani, B. Gaehrken, S. Mottola, S. Hellmich, F. L. Rommel, E. Fernández-Valenzuela, A. Campo Bagatin, S. Cikota, A. Cikota, J. Lecacheux, R. Vieira-Martins, J. I. B. Camargo, M. Assafin, F. Colas, R. Behrend, J. Desmars, E. Meza, A. Alvarez-Candal, W. Beisker, A. R. Gomes-Junior, B. E. Morgado, F. Roques, F. Vachier, J. Berthier, T. G. Mueller, J. M. Madiedo, O. Unsalan, E. Sonbas, N. Karaman, O. Erece, D. T. Koseoglu, T. Ozisik, S. Kalkan, Y. Guney, M. S. Niaei, O. Satir, C. Yesilyaprak, C. Puskullu, A. Kabas, O. Demircan, J. Alikakos, V. Charmandaris, G. Leto, J. Ohlert, J. M. Christille, R. Szakáts, A. Takácsné Farkas, E. Varga-Verebélyi, G. Marton, A. Marciniak, P. Bartczak, T. Santana-Ros, M. Butkiewicz-Bąk, G. Dudziński, V. Alí-Lagoa, K. Gazeas, L. Tzouganatos, N. Paschalis, V. Tsamis, A. Sánchez-Lavega, S. Pérez-Hoyos, R. Hueso, J. C. Guirado, V. Peris, R. Iglesias-Marzoa. The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation. Nature, 2017; 550 (7675): 219 DOI: 10.1038/nature24051