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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:19/0  |  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.


  
Antarctic Surface Mass Balance: Natural Variability, Noise, and Detecting New Trends 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (12)
作者:  King, Matt A.;  Watson, Christopher S.
收藏  |  浏览/下载:8/0  |  提交时间:2020/06/16
WHY POLLUTION IS FALLING IN SOME CITIES - BUT NOT OTHERS 期刊论文
NATURE, 2020, 580 (7803) : 313-313
作者:  Sulkowski, Parker L.;  Oeck, Sebastian;  Dow, Jonathan;  Economos, Nicholas G.;  Mirfakhraie, Lily;  Liu, Yanfeng;  Noronha, Katelyn;  Bao, Xun;  Li, Jing;  Shuch, Brian M.;  King, Megan C.;  Bindra, Ranjit S.;  Glazer, Peter M.
收藏  |  浏览/下载:14/0  |  提交时间:2020/07/03
Increased drought severity tracks warming in the United States' largest river basin 期刊论文
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2020, 117 (21) : 11328-11336
作者:  Martin, Justin T.;  Pederson, Gregory T.;  Woodhouse, Connie A.;  Cook, Edward R.;  McCabe, Gregory J.;  Anchukaitis, Kevin J.;  Wise, Erika K.;  Erger, Patrick J.;  Dolan, Larry;  McGuire, Marketa;  Gangopadhyay, Subhrendu;  Chase, Katherine J.;  Littell, Jeremy S.;  Gray, Stephen T.;  George, Scott St.;  Friedman, Jonathan M.;  Sauchyn, David J.;  St-Jacques, Jeannine-Marie;  King, John
收藏  |  浏览/下载:14/0  |  提交时间:2020/05/13
drought severity  streamflow  temperature  precipitation  water resources  
Spectroscopic confirmation of a mature galaxy cluster at a redshift of 2 期刊论文
NATURE, 2020, 577 (7788) : 39-+
作者:  Willis, J. P.;  Canning, R. E. A.;  Noordeh, E. S.;  Allen, S. W.;  King, A. L.;  Mantz, A.;  Morris, R. G.;  Stanford, S. A.;  Brammer, G.
收藏  |  浏览/下载:12/0  |  提交时间:2020/07/03

Galaxy clusters are the most massive virialized structures in the Universe and are formed through the gravitational accretion of matter over cosmic time(1). The discovery(2) of an evolved galaxy cluster at redshift z = 2, corresponding to a look-back time of 10.4 billion years, provides an opportunity to study its properties. The galaxy cluster XLSSC 122 was originally detected as a faint, extended X-ray source in the XMM Large Scale Structure survey and was revealed to be coincident with a compact over-density of galaxies(2) with photometric redshifts of 1.9 +/- 0.2. Subsequent observations3 at millimetre wavelengths detected a Sunyaev-Zel'  dovich decrement along the line of sight to XLSSC 122, thus confirming the existence of hot intracluster gas, while deep imaging spectroscopy from the European Space Agency'  s X-ray Multi-Mirror Mission (XMM-Newton) revealed(4) an extended, X-ray-bright gaseous atmosphere with a virial temperature of 60 million Kelvin, enriched with metals to the same extent as are local clusters. Here we report optical spectroscopic observations of XLSSC 122 and identify 37 member galaxies at a mean redshift of 1.98, corresponding to a look-back time of 10.4 billion years. We use photometry to determine a mean, dust-free stellar age of 2.98 billion years, indicating that star formation commenced in these galaxies at a mean redshift of 12, when the Universe was only 370 million years old. The full range of inferred formation redshifts, including the effects of dust, covers the interval from 7 to 13. These observations confirm that XLSSC 122 is a remarkably mature galaxy cluster with both evolved stellar populations in the member galaxies and a hot, metal-rich gas composing the intracluster medium.


  
Spatial heterogeneity in CO2, CH4, and energy fluxes: insights from airborne eddy covariance measurements over the Mid-Atlantic region 期刊论文
ENVIRONMENTAL RESEARCH LETTERS, 2020, 15 (3)
作者:  Hannun, Reem A.;  Wolfe, Glenn M.;  Kawa, S. Randy;  Hanisco, Thomas F.;  Newman, Paul A.;  Alfieri, Joseph G.;  Barrick, John;  Clark, Kenneth L.;  DiGangi, Joshua P.;  Diskin, Glenn S.;  King, John;  Kustas, William P.;  Mitra, Bhaskar;  Noormets, Asko;  Nowak, John B.;  Thornhill, K. Lee;  Vargas, Rodrigo
收藏  |  浏览/下载:13/0  |  提交时间:2020/07/02
airborne eddy covariance  CO2 and CH4  fluxes  biosphere-atmosphere exchange  
The Role of Individual Heterogeneity in Collective Animal Behaviour 期刊论文
TRENDS IN ECOLOGY & EVOLUTION, 2020, 35 (3) : 278-291
作者:  Jolles, Jolle W.;  King, Andrew J.;  Killen, Shaun S.
收藏  |  浏览/下载:1/0  |  提交时间:2020/07/02
Initial results from the InSight mission on Mars 期刊论文
NATURE GEOSCIENCE, 2020, 13 (3) : 183-+
作者:  Banerdt, W. Bruce;  Smrekar, Suzanne E.;  Banfield, Don;  Giardini, Domenico;  Golombek, Matthew;  Johnson, Catherine L.;  Lognonne, Philippe;  Spiga, Aymeric;  Spohn, Tilman;  Perrin, Clement;  Staehler, Simon C.;  Antonangeli, Daniele;  Asmar, Sami;  Beghein, Caroline;  Bowles, Neil;  Bozdag, Ebru;  Chi, Peter;  Christensen, Ulrich;  Clinton, John;  Collins, Gareth S.;  Daubar, Ingrid;  Dehant, Veronique;  Drilleau, Melanie;  Fillingim, Matthew;  Folkner, William;  Garcia, Raphael F.;  Garvin, Jim;  Grant, John;  Grott, Matthias;  Grygorczuk, Jerzy;  Hudson, Troy;  Irving, Jessica C. E.;  Kargl, Guenter;  Kawamura, Taichi;  Kedar, Sharon;  King, Scott;  Knapmeyer-Endrun, Brigitte;  Knapmeyer, Martin;  Lemmon, Mark;  Lorenz, Ralph;  Maki, Justin N.;  Margerin, Ludovic;  McLennan, Scott M.;  Michaut, Chloe;  Mimoun, David;  Mittelholz, Anna;  Mocquet, Antoine;  Morgan, Paul;  Mueller, Nils T.;  Murdoch, Naomi;  Nagihara, Seiichi;  Newman, Claire;  Nimmo, Francis;  Panning, Mark;  Pike, W. Thomas;  Plesa, Ana-Catalina;  Rodriguez, Sebastien;  Rodriguez-Manfredi, Jose Antonio;  Russell, Christopher T.;  Schmerr, Nicholas;  Siegler, Matt;  Stanley, Sabine;  Stutzmann, Eleanore;  Teanby, Nicholas;  Tromp, Jeroen;  Van Driel, Martin;  Warner, Nicholas;  Weber, Renee;  Wieczorek, Mark
收藏  |  浏览/下载:25/0  |  提交时间:2020/05/13
The seismicity of Mars 期刊论文
NATURE GEOSCIENCE, 2020, 13 (3) : 205-+
作者:  Giardini, D.;  Lognonne, P.;  Banerdt, W. B.;  Pike, W. T.;  Christensen, U.;  Ceylan, S.;  Clinton, J. F.;  van Driel, M.;  Staehler, S. C.;  Boese, M.;  Garcia, R. F.;  Khan, A.;  Panning, M.;  Perrin, C.;  Banfield, D.;  Beucler, E.;  Charalambous, C.;  Euchner, F.;  Horleston, A.;  Jacob, A.;  Kawamura, T.;  Kedar, S.;  Mainsant, G.;  Scholz, J. -R.;  Smrekar, S. E.;  Spiga, A.;  Agard, C.;  Antonangeli, D.;  Barkaoui, S.;  Barrett, E.;  Combes, P.;  Conejero, V.;  Daubar, I.;  Drilleau, M.;  Ferrier, C.;  Gabsi, T.;  Gudkova, T.;  Hurst, K.;  Karakostas, F.;  King, S.;  Knapmeyer, M.;  Knapmeyer-Endrun, B.;  Llorca-Cejudo, R.;  Lucas, A.;  Luno, L.;  Margerin, L.;  McClean, J. B.;  Mimoun, D.;  Murdoch, N.;  Nimmo, F.;  Nonon, M.;  Pardo, C.;  Rivoldini, A.;  Manfredi, J. A. Rodriguez;  Samuel, H.;  Schimmel, M.;  Stott, A. E.;  Stutzmann, E.;  Teanby, N.;  Warren, T.;  Weber, R. C.;  Wieczorek, M.;  Yana, C.
收藏  |  浏览/下载:11/0  |  提交时间:2020/05/13
Bacterial coexistence driven by motility and spatial competition 期刊论文
NATURE, 2020, 578 (7796) : 588-+
作者:  Micke, P.;  Leopold, T.;  King, S. A.;  Benkler, E.;  Spiess, L. J.;  Schmoeger, L.;  Schwarz, M.;  Crespo Lopez-Urrutia, J. R.;  Schmidt, P. O.
收藏  |  浏览/下载:8/0  |  提交时间:2020/07/03

Elucidating elementary mechanisms that underlie bacterial diversity is central to ecology(1,2) and microbiome research(3). Bacteria are known to coexist by metabolic specialization(4), cooperation(5) and cyclic warfare(6-8). Many species are also motile(9), which is studied in terms of mechanism(10,11), benefit(12,13), strategy(14,15), evolution(16,17) and ecology(18,19). Indeed, bacteria often compete for nutrient patches that become available periodically or by random disturbances(2,20,21). However, the role of bacterial motility in coexistence remains unexplored experimentally. Here we show that-for mixed bacterial populations that colonize nutrient patches-either population outcompetes the other when low in relative abundance. This inversion of the competitive hierarchy is caused by active segregation and spatial exclusion within the patch: a small fast-moving population can outcompete a large fast-growing population by impeding its migration into the patch, while a small fast-growing population can outcompete a large fast-moving population by expelling it from the initial contact area. The resulting spatial segregation is lost for weak growth-migration trade-offs and a lack of virgin space, but is robust to population ratio, density and chemotactic ability, and is observed in both laboratory and wild strains. These findings show that motility differences and their trade-offs with growth are sufficient to promote diversity, and suggest previously undescribed roles for motility in niche formation and collective expulsion-containment strategies beyond individual search and survival.


In mixed bacterial populations that colonize nutrient patches, a growth-migration trade-off can lead to spatial exclusion that provides an advantage to populations that become rare, thereby stabilizing the community.