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dc.contributor.authorMorgado, B E
dc.contributor.authorSicardy, B
dc.contributor.authorBraga-Ribas, F
dc.contributor.authorOrtiz, J L
dc.contributor.authorSalo, H
dc.contributor.authorVachier, F
dc.contributor.authorDesmars, J
dc.contributor.authorPereira, C L
dc.contributor.authorSantos-Sanz, P
dc.contributor.authorSfair, R
dc.contributor.authorde Santana, T
dc.contributor.authorAssafin, M
dc.contributor.authorVieira-Martins, R
dc.contributor.authorGomes-Júnior, A R
dc.contributor.authorMargoti, G
dc.contributor.authorDhillon, V S
dc.contributor.authorFernández-Valenzuela, E
dc.contributor.authorBroughton, J
dc.contributor.authorBradshaw, J
dc.contributor.authorLangersek, R
dc.contributor.authorBenedetti-Rossi, G
dc.contributor.authorSouami, D
dc.contributor.authorHoller, B J
dc.contributor.authorKretlow, M
dc.contributor.authorBoufleur, R C
dc.contributor.authorCamargo, J I B
dc.contributor.authorDuffard, R
dc.contributor.authorBeisker, W
dc.contributor.authorMorales, N
dc.contributor.authorLecacheux, J
dc.contributor.authorRommel, F L
dc.contributor.authorHerald, D
dc.contributor.authorBenz, W
dc.contributor.authorJehin, E
dc.contributor.authorJankowsky, F
dc.contributor.authorMarsh, T R
dc.contributor.authorLittlefair, S P
dc.contributor.authorBruno, G
dc.contributor.authorPagano, I
dc.contributor.authorBrandeker, A
dc.contributor.authorCollier-Cameron, A
dc.contributor.authorFlorén, H G
dc.contributor.authorHara, N
dc.contributor.authorOlofsson, G
dc.contributor.authorWilson, T G
dc.contributor.authorBenkhaldoun, Z
dc.contributor.authorBusuttil, R
dc.contributor.authorBurdanov, A
dc.contributor.authorFerrais, M
dc.contributor.authorGault, D
dc.contributor.authorGillon, M
dc.contributor.authorHanna, W
dc.contributor.authorKerr, S
dc.contributor.authorKolb, U
dc.contributor.authorNosworthy, P
dc.contributor.authorSebastian, D
dc.contributor.authorSnodgrass, C
dc.contributor.authorTeng, J P
dc.contributor.authorde Wit, J
dc.identifier.citationMorgado , B E , Sicardy , B , Braga-Ribas , F , Ortiz , J L , Salo , H , Vachier , F , Desmars , J , Pereira , C L , Santos-Sanz , P , Sfair , R , de Santana , T , Assafin , M , Vieira-Martins , R , Gomes-Júnior , A R , Margoti , G , Dhillon , V S , Fernández-Valenzuela , E , Broughton , J , Bradshaw , J , Langersek , R , Benedetti-Rossi , G , Souami , D , Holler , B J , Kretlow , M , Boufleur , R C , Camargo , J I B , Duffard , R , Beisker , W , Morales , N , Lecacheux , J , Rommel , F L , Herald , D , Benz , W , Jehin , E , Jankowsky , F , Marsh , T R , Littlefair , S P , Bruno , G , Pagano , I , Brandeker , A , Collier-Cameron , A , Florén , H G , Hara , N , Olofsson , G , Wilson , T G , Benkhaldoun , Z , Busuttil , R , Burdanov , A , Ferrais , M , Gault , D , Gillon , M , Hanna , W , Kerr , S , Kolb , U , Nosworthy , P , Sebastian , D , Snodgrass , C , Teng , J P & de Wit , J 2023 , ' A dense ring of the trans-Neptunian object Quaoar outside its Roche limit ' , Nature , vol. 614 , no. 7947 , pp. 239-243 .
dc.identifier.otherPURE: 283371089
dc.identifier.otherPURE UUID: 94c5622f-7a66-41e3-b3ab-f85f52f6943b
dc.identifier.otherPubMed: 36755175
dc.identifier.otherORCID: /0000-0002-8863-7828/work/129147667
dc.identifier.otherORCID: /0000-0001-8749-1962/work/129147845
dc.identifier.otherScopus: 85147724719
dc.descriptionFunding: This work was carried out under the Lucky Star umbrella that agglomerates the efforts of the Paris, Granada and Rio teams, which is funded by the ERC under the European Community’s H2020 (ERC grant agreement no. 669416). A.C.-C. and T.G.W. acknowledge support from STFC consolidated grant nos. ST/R000824/1 and ST/V000861/1, and UK Space Agency grant no. ST/R003203/1.en
dc.description.abstractPlanetary rings are observed not only around giant planets, but also around small bodies such as the Centaur Chariklo and the dwarf planet Haumea. Up to now, all known dense rings were located close enough to their parent bodies, being inside the Roche limit, where tidal forces prevent material with reasonable densities from aggregating into a satellite. Here we report observations of an inhomogeneous ring around the trans-Neptunian body (50000) Quaoar. This trans-Neptunian object has an estimated radius of 555 km and possesses a roughly 80-km satellite (Weywot) that orbits at 24 Quaoar radii. The detected ring orbits at 7.4 radii from the central body, which is well outside Quaoar's classical Roche limit, thus indicating that this limit does not always determine where ring material can survive. Our local collisional simulations show that elastic collisions, based on laboratory experiments, can maintain a ring far away from the body. Moreover, Quaoar's ring orbits close to the 1/3 spin-orbit resonance with Quaoar, a property shared by Chariklo's and Haumea's rings, suggesting that this resonance plays a key role in ring confinement for small bodies.
dc.rightsCopyright © 2023 the Authors. This work has been made available online in accordance with the Rights Retention Strategy This accepted manuscript is distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. The final published version of this work is available at
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleA dense ring of the trans-Neptunian object Quaoar outside its Roche limiten
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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