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A remnant planetary core in the hot-Neptune desert 期刊论文
NATURE, 2020, 583 (7814) : 39-+
作者:  David J. Armstrong;  Thé;  o A. Lopez;  Vardan Adibekyan;  Richard A. Booth;  Edward M. Bryant;  Karen A. Collins;  Magali Deleuil;  Alexandre Emsenhuber;  Chelsea X. Huang;  George W. King;  Jorge Lillo-Box;  Jack J. Lissauer;  Elisabeth Matthews;  Olivier Mousis;  Louise D. Nielsen;  Hugh Osborn;  Jon Otegi;  Nuno C. Santos;  ;  rgio G. Sousa;  Keivan G. Stassun;  Dimitri Veras;  Carl Ziegler;  Jack S. Acton;  Jose M. Almenara;  David R. Anderson;  David Barrado;  Susana C. C. Barros;  Daniel Bayliss;  Claudia Belardi;  Francois Bouchy;  ;  sar Briceñ;  o;  Matteo Brogi;  David J. A. Brown;  Matthew R. Burleigh;  Sarah L. Casewell;  Alexander Chaushev;  David R. Ciardi;  Kevin I. Collins;  Knicole D. Coló;  n;  Benjamin F. Cooke;  Ian J. M. Crossfield;  Rodrigo F. Dí;  az;  Elisa Delgado Mena;  Olivier D. S. Demangeon;  Caroline Dorn;  Xavier Dumusque;  Philipp Eigmü;  ller;  Michael Fausnaugh;  Pedro Figueira;  Tianjun Gan;  Siddharth Gandhi;  Samuel Gill;  Erica J. Gonzales;  Michael R. Goad;  Maximilian N. Gü;  nther;  Ravit Helled;  Saeed Hojjatpanah;  Steve B. Howell;  James Jackman;  James S. Jenkins;  Jon M. Jenkins;  Eric L. N. Jensen;  Grant M. Kennedy;  David W. Latham;  Nicholas Law;  Monika Lendl;  Michael Lozovsky;  Andrew W. Mann;  Maximiliano Moyano;  James McCormac;  Farzana Meru;  Christoph Mordasini;  Ares Osborn;  Don Pollacco;  Didier Queloz;  Liam Raynard;  George R. Ricker;  Pamela Rowden;  Alexandre Santerne;  Joshua E. Schlieder;  Sara Seager;  Lizhou Sha;  Thiam-Guan Tan;  Rosanna H. Tilbrook;  Eric Ting;  Sté;  phane Udry;  Roland Vanderspek;  Christopher A. Watson;  Richard G. West;  Paul A. Wilson;  Joshua N. Winn;  Peter Wheatley;  Jesus Noel Villasenor;  Jose I. Vines;  Zhuchang Zhan
收藏  |  浏览/下载:93/0  |  提交时间:2020/07/06

The interiors of giant planets remain poorly understood. Even for the planets in the Solar System, difficulties in observation lead to large uncertainties in the properties of planetary cores. Exoplanets that have undergone rare evolutionary processes provide a route to understanding planetary interiors. Planets found in and near the typically barren hot-Neptune '  desert'  (1,2)(a region in mass-radius space that contains few planets) have proved to be particularly valuable in this regard. These planets include HD149026b(3), which is thought to have an unusually massive core, and recent discoveries such as LTT9779b(4)and NGTS-4b(5), on which photoevaporation has removed a substantial part of their outer atmospheres. Here we report observations of the planet TOI-849b, which has a radius smaller than Neptune'  s but an anomalously large mass of39.1-2.6+2.7Earth masses and a density of5.2-0.8+0.7grams per cubic centimetre, similar to Earth'  s. Interior-structure models suggest that any gaseous envelope of pure hydrogen and helium consists of no more than3.9-0.9+0.8 per cent of the total planetary mass. The planet could have been a gas giant before undergoing extreme mass loss via thermal self-disruption or giant planet collisions, or it could have avoided substantial gas accretion, perhaps through gap opening or late formation(6). Although photoevaporation rates cannot account for the mass loss required to reduce a Jupiter-like gas giant, they can remove a small (a few Earth masses) hydrogen and helium envelope on timescales of several billion years, implying that any remaining atmosphere on TOI-849b is likely to be enriched by water or other volatiles from the planetary interior. We conclude that TOI-849b is the remnant core of a giant planet.


Observations of TOI-849b reveal a radius smaller than Neptune'  s but a large mass of about 40 Earth masses, indicating that the planet is the remnant core of a gas giant.


  
Nuclear force probed at short distances 期刊论文
NATURE, 2020, 578 (7796) : 524-525
作者:  Shukla, Aditi;  Yen, Jenny;  Pagano, Daniel J.;  Dodso, Anne E.;  Fei, Yuhan;  Gorham, Josh;  Seidman, J. G.;  Wickens, Marvin;  Kennedy, Scott
收藏  |  浏览/下载:23/0  |  提交时间:2020/07/03

The dense soup of matter in the core of neutron stars is hard to model, but particle-accelerator experiments in which energetic electrons scatter off atomic nuclei could help to explore this high-density regime.


A test of effective nucleon-nucleon interactions at short separations.


  
Novel tau filament fold in corticobasal degeneration 期刊论文
NATURE, 2020, 580 (7802) : 283-+
作者:  Izumi, Natsuko;  Shoji, Keisuke;  Suzuki, Yutaka;  Katsuma, Susumu;  Tomari, Yukihide
收藏  |  浏览/下载:19/0  |  提交时间:2020/07/03

Cyro-electron microscopy of tau filaments from people with corticobasal degeneration reveals a previously unseen four-layered fold, distinct from the filament structures seen in Alzheimer'  s disease, Pick'  s disease and chronic traumatic encephalopathy.


Corticobasal degeneration (CBD) is a neurodegenerative tauopathy-a class of disorders in which the tau protein forms insoluble inclusions in the brain-that is characterized by motor and cognitive disturbances(1-3). The H1 haplotype of MAPT (the tau gene) is present in cases of CBD at a higher frequency than in controls(4,5), and genome-wide association studies have identified additional risk factors(6). By histology, astrocytic plaques are diagnostic of CBD7,8  by SDS-PAGE, so too are detergent-insoluble, 37 kDa fragments of tau(9). Like progressive supranuclear palsy, globular glial tauopathy and argyrophilic grain disease(10), CBD is characterized by abundant filamentous tau inclusions that are made of isoforms with four microtubule-binding repeats(11-15). This distinguishes such '  4R'  tauopathies from Pick'  s disease (the filaments of which are made of three-repeat (3R) tau isoforms) and from Alzheimer'  s disease and chronic traumatic encephalopathy (CTE) (in which both 3R and 4R isoforms are found in the filaments)(16). Here we use cryo-electron microscopy to analyse the structures of tau filaments extracted from the brains of three individuals with CBD. These filaments were identical between cases, but distinct from those seen in Alzheimer'  s disease, Pick'  s disease and CTE17-19. The core of a CBD filament comprises residues lysine 274 to glutamate 380 of tau, spanning the last residue of the R1 repeat, the whole of the R2, R3 and R4 repeats, and 12 amino acids after R4. The core adopts a previously unseen four-layered fold, which encloses a large nonproteinaceous density. This density is surrounded by the side chains of lysine residues 290 and 294 from R2 and lysine 370 from the sequence after R4.


  
Phase Stability and Thermal Equation of State of Iron Carbide Fe3C to 245 GPa 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2019
作者:  Hu, Xiaojun;  Fei, Yingwei;  Yang, Jing;  Cai, Yang;  Ye, Shijia;  Qi, Meilan;  Liu, Fusheng;  Zhang, Mingjian
收藏  |  浏览/下载:26/0  |  提交时间:2019/11/27
Earth core  shockwave compression  iron carbide  core density  core composition  
Nitrogen Content in the Earth's Outer Core 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2019, 46 (1) : 89-98
作者:  Bajgain, Suraj K.;  Mookherjee, Mainak;  Dasgupta, Rajdeep;  Ghosh, Dipta B.;  Karki, Bijaya B.
收藏  |  浏览/下载:18/0  |  提交时间:2019/04/09
Earth'  s outer core  light elements  density of molten Fe-N alloy  compressional velocity of molten Fe-N alloy