-
作者:Cordiner, Martin; Roth, Nathan X.; Micheli, Marco; Villanueva, Geronimo; Farnocchia, Davide; Charnley, Steven; Biver, Nicolas; Bockelee-Morvan, Dominique; Bodewits, Dennis; Chandler, Colin Orion; Crovisier, Jacques; Drozdovskaya, Maria N.; Furuya, Kenji; Kelley, Michael S. P.; Milam, Stefanie; Noonan, John W.; Opitom, Cyrielle; Schwamb, Megan E.; Thomas, Cristina A.
作者单位:National Aeronautics & Space Administration (NASA); NASA Goddard Space Flight Center; Catholic University of America; American University; California Institute of Technology; National Aeronautics & Space Administration (NASA); NASA Jet Propulsion Laboratory (JPL); Sorbonne Universite; CY Cergy Paris Universite; Universite Paris Cite; Centre National de la Recherche Scientifique (CNRS); Universite PSL; Observatoire de Paris; Auburn University System; Auburn University; University of Washington; University of Washington Seattle; Northern Arizona University; University of Bern; University System of Maryland; University of Maryland College Park; University of Edinburgh
摘要:Interstellar objects provide the only directly observable samples of icy planetesimals formed around other stars, and can therefore provide insight into the diversity of physical and chemical conditions occurring during exoplanet formation1, 2-3. Here we report isotopic measurements of the interstellar comet 3I/ATLAS, which reveal an elemental composition unlike any Solar System body. The water in 3I/ATLAS is enriched in deuterium, at a level of D/H = (0.98 +/- 0.06)%, which is more than an or...
-
作者:Cooke, Megan
作者单位:University of Colorado System; University of Colorado Boulder
-
作者:Ronning, E. K.; Richard, A. L.; Liddick, S. N.; Spyrou, A.; Ringle, R.; Arora, H.; Berg, H. C.; Berkman, J. M.; Bleuel, D. L.; Bosmpotinis, K.; Campbell, S. E.; Chen, X.; Crider, B. P.; Coleman, R. J.; DeYoung, P. A.; Doetsch, A. A.; Erington, H.; Gaballah, T.; Gamage, N. D.; Good, E. C.; Greaves, B.; Hartley, A. C.; Huffman, J.; Ireland, C. M.; Izzo, C.; Jain, R.; Larsen, A. C.; Larsson, J. E. L.; Lubna, R. S.; Maier, F. M.; Mogannam, M. J.; Mucher, D.; Mumpower, M. R.; Owens-Fryar, G.; Ogunbeku, T. H.; Scriven, D. P.; Smith, M. K.; Sumithrarachchi, C. S.; Sweet, A.; Taft, K.; Tsantiri, A.; Uthayakumaar, S.; Wiedeking, M.
作者单位:Michigan State University; Michigan State University; University System of Ohio; Ohio University; United States Department of Energy (DOE); Lawrence Livermore National Laboratory; Michigan State University; Central Michigan University; Institute for Basic Science - Korea (IBS); Mississippi State University; University of Guelph; Hope College; United States Department of Energy (DOE); Pacific Northwest National Laboratory; University of Oslo; Technical University of Darmstadt; Helmholtz Association; GSI Helmholtz-Center for Heavy Ion Research; Air Force Institute of Technology (AFIT); University of Cologne; University of Notre Dame; United States Department of Energy (DOE); Los Alamos National Laboratory; University of Regina; University of Victoria; United States Department of Energy (DOE); Lawrence Berkeley National Laboratory
摘要:The transition of an atomic nucleus from an excited state to a state of lower energy is typically accompanied by the emission of photons. The likelihood of photon emission is a function of the photon energy and of properties of the initial and final nuclear states and is known as the photon (or gamma-ray) strength function (gamma SF)1,2. Of the features present in the gamma SF, an enhancement in the low-energy region has been observed in some nuclei, but the electromagnetic nature of this enha...
-
作者:[Anonymous]
-
作者:Fieldhouse, Rachel
-
作者:Mitchinson, Andrew
-
作者:Simms, Chris
-
作者:Hoekstra, Steven
作者单位:University of Groningen; FOM National Institute for Subatomic Physics
摘要:The response of the nucleus of a deuterium atom to electric fields shows no evidence of asymmetry, which is consistent with conventional theories of particle physics.
-
作者:Callaway, Ewen
-
作者:Hoy, Kevin; Zurlo, Alice; Pena R, Pablo A.; Kohler, Jana; Desidera, Silvano; Gratton, Raffaele; Lazzoni, Cecilia; Petrus, Simon; Rodler, Florian; Smoker, Jonathan; D'Orazi, Valentina; Carleo, Ilaria; Giovannini, Ilaria
作者单位:University Diego Portales; European Southern Observatory; Istituto Nazionale Astrofisica (INAF); National Aeronautics & Space Administration (NASA); NASA Goddard Space Flight Center; University of Rome Tor Vergata; Istituto Nazionale Astrofisica (INAF); University of Padua
摘要:Brown dwarfs occupy the mass regime between planets and stars. In systems containing both a star and a substellar companion (be it a brown dwarf or an exoplanet), a third object orbiting the companion can be called an exosatellite. Exoplanet satellites can be easily described as exomoons, but it is not clear if satellites of brown dwarf companions can be called the same, as the term lacks a formal definition. Despite more than 6,000 exoplanets being discovered1, no exomoon has ever been confid...