Show simple item record

dc.contributor.authorBernardinelli, Pedro H.
dc.contributor.authorBernstein, Gary M.
dc.contributor.authorMontet, Benjamin T.
dc.contributor.authorWeryk, Robert
dc.contributor.authorWainscoat, Richard
dc.contributor.authorAguena, M.
dc.contributor.authorAllam, S.
dc.contributor.authorAndrade-Oliveira, F.
dc.contributor.authorAnnis, J.
dc.contributor.authorAvila, S.
dc.contributor.authorBertin, E.
dc.contributor.authorBrooks, D.
dc.contributor.authorBurke, D. L.
dc.contributor.authorCarnero Rosell, A.
dc.contributor.authorKind, M. Carrasco
dc.contributor.authorCarretero, J.
dc.contributor.authorCawthon, R.
dc.contributor.authorConselice, C.
dc.contributor.authorCostanzi, M.
dc.contributor.authorda Costa, L. N.
dc.contributor.authorPereira, M. E. S.
dc.contributor.authorDe Vicente, J.
dc.contributor.authorDiehl, H. T.
dc.contributor.authorEverett, S.
dc.contributor.authorFerrero, I.
dc.contributor.authorFlaugher, B.
dc.contributor.authorFrieman, J.
dc.contributor.authorGarcía-Bellido, J.
dc.contributor.authorGaztanaga, E.
dc.contributor.authorGerdes, D. W.
dc.contributor.authorGruen, D.
dc.contributor.authorGruendl, R. A.
dc.contributor.authorGschwend, J.
dc.contributor.authorGutierrez, G.
dc.contributor.authorHinton, S. R.
dc.contributor.authorHollowood, D. L.
dc.contributor.authorHonscheid, K.
dc.contributor.authorJames, D. J.
dc.contributor.authorKuehn, K.
dc.contributor.authorKuropatkin, N.
dc.contributor.authorLahav, O.
dc.contributor.authorMaia, M. A. G.
dc.contributor.authorMarshall, J. L.
dc.contributor.authorMenanteau, F.
dc.contributor.authorMiquel, R.
dc.contributor.authorMorgan, R.
dc.contributor.authorOgando, R. L. C.
dc.contributor.authorPaz-Chinchón, F.
dc.contributor.authorPieres, A.
dc.contributor.authorMalagón, A. A. Plazas
dc.contributor.authorRodriguez-Monroy, M.
dc.contributor.authorRomer, A. K.
dc.contributor.authorRoodman, A.
dc.contributor.authorSanchez, E.
dc.contributor.authorSchubnell, M.
dc.contributor.authorSerrano, S.
dc.contributor.authorSevilla-Noarbe, I.
dc.contributor.authorSmith, M.
dc.contributor.authorSoares-Santos, M.
dc.contributor.authorSuchyta, E.
dc.contributor.authorSwanson, M. E. C.
dc.contributor.authorTarle, G.
dc.contributor.authorTo, C.
dc.contributor.authorTroxel, M. A.
dc.contributor.authorVarga, T. N.
dc.contributor.authorWalker, A. R.
dc.contributor.authorZhang, Y.
dc.date.accessioned2021-11-09T11:00:36Z
dc.date.available2021-11-09T11:00:36Z
dc.date.issued2021-11-09
dc.date.submitted2021-09-20
dc.identifier.issn2041-8205
dc.identifier.otherapjlac32d3
dc.identifier.otherac32d3
dc.identifier.otheraas34873
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/330491
dc.description.abstractAbstract: Comet C/2014 UN271 (Bernardinelli-Bernstein), incoming from the Oort cloud, is remarkable in having the brightest (and presumably largest) nucleus of any well-measured comet and having been discovered at the heliocentric distance r h ≈ 29 au, farther than any Oort cloud comet. In this work, we describe the discovery process and observations and the properties that can be inferred from images recorded until the first reports of activity in 2021 June. The orbit has i = 95°, with a perihelion of 10.97 au to be reached in 2031 and a previous aphelion at 40,400 ± 260 au. Backward integration of the orbit under a standard Galactic tidal model and known stellar encounters suggests a perihelion of q ≈ 18 au on its previous perihelion passage 3.5 Myr ago; hence, the current data could be the first ever obtained of a comet that has not been inside Uranus’s orbit in 4 Gyr. The photometric data show an unresolved nucleus with absolute magnitude H r = 8.0, colors that are typical of comet nuclei or Damocloids, and no secular trend as it traversed the range 34–23 au. For the r-band geometric albedo p r , this implies a diameter of 150(pr/0.04)−0.5 km. There is strong evidence of brightness fluctuations at the ±0.2 mag level, but no rotation period can be discerned. A coma, nominally consistent with a “stationary” 1/ρ surface brightness distribution, grew in scattering cross section at an exponential rate from A f ρ ≈ 1 to ≈150 m as the comet approached from 28 to 20 au. The activity rate is consistent with a very simple model of sublimation of a surface species in radiative equilibrium with the Sun. The inferred enthalpy of sublimation matches those of CO2 and NH3. More volatile species, such as N2, CH4, and CO, must be far less abundant on the sublimating surfaces.
dc.languageen
dc.publisherThe American Astronomical Society
dc.titleC/2014 UN 271 (Bernardinelli-Bernstein): The Nearly Spherical Cow of Comets
dc.typeArticle
dc.date.updated2021-11-09T11:00:36Z
prism.issueIdentifier2
prism.publicationNameThe Astrophysical Journal Letters
prism.volume921
dc.identifier.doi10.17863/CAM.77935
dcterms.dateAccepted2021-10-22
rioxxterms.versionofrecord10.3847/2041-8213/ac32d3
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
dc.contributor.orcidBernardinelli, Pedro H. [0000-0003-0743-9422]
dc.contributor.orcidBernstein, Gary M. [0000-0002-8613-8259]
dc.contributor.orcidMontet, Benjamin T. [0000-0001-7516-8308]
dc.contributor.orcidWeryk, Robert [0000-0002-0439-9341]
dc.contributor.orcidWainscoat, Richard [0000-0002-1341-0952]
dc.contributor.orcidAguena, M. [0000-0001-5679-6747]
dc.contributor.orcidAnnis, J. [0000-0002-0609-3987]
dc.contributor.orcidBertin, E. [0000-0002-3602-3664]
dc.contributor.orcidBrooks, D. [0000-0002-8458-5047]
dc.contributor.orcidCarretero, J. [0000-0002-3130-0204]
dc.contributor.orcidCawthon, R. [0000-0003-2965-6786]
dc.contributor.orcidConselice, C. [0000-0003-1949-7638]
dc.contributor.orcidCostanzi, M. [0000-0001-8158-1449]
dc.contributor.orcidDiehl, H. T. [0000-0002-8357-7467]
dc.contributor.orcidGarcía-Bellido, J. [0000-0002-9370-8360]
dc.contributor.orcidGaztanaga, E. [0000-0001-9632-0815]
dc.contributor.orcidGerdes, D. W. [0000-0001-6942-2736]
dc.contributor.orcidGruendl, R. A. [0000-0002-4588-6517]
dc.contributor.orcidGschwend, J. [0000-0003-3023-8362]
dc.contributor.orcidHinton, S. R. [0000-0003-2071-9349]
dc.contributor.orcidHollowood, D. L. [0000-0002-9369-4157]
dc.contributor.orcidKuehn, K. [0000-0003-0120-0808]
dc.contributor.orcidMarshall, J. L. [0000-0003-0710-9474]
dc.contributor.orcidMenanteau, F. [0000-0002-1372-2534]
dc.contributor.orcidMiquel, R. [0000-0002-6610-4836]
dc.contributor.orcidMorgan, R. [0000-0002-7016-5471]
dc.contributor.orcidPaz-Chinchón, F. [0000-0003-1339-2683]
dc.contributor.orcidPieres, A. [0000-0001-9186-6042]
dc.contributor.orcidRoodman, A. [0000-0001-5326-3486]
dc.contributor.orcidSevilla-Noarbe, I. [0000-0002-1831-1953]
dc.contributor.orcidSwanson, M. E. C. [0000-0002-1488-8552]
dc.contributor.orcidTarle, G. [0000-0003-1704-0781]
dc.contributor.orcidTo, C. [0000-0001-7836-2261]
dc.identifier.eissn2041-8213
pubs.funder-project-idNational Science Foundation (NSF) (AST-1515804)
pubs.funder-project-idNational Science Foundation (NSF) (AST-2009210)
pubs.funder-project-idU.S. Department of Energy (DOE) (DE-SC0007901)


Files in this item

Thumbnail
Thumbnail

This item appears in the following Collection(s)

Show simple item record