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Observation of Bose-Einstein condensates in an Earth-orbiting research lab 期刊论文
NATURE, 2020, 582 (7811) : 103-+
作者:  Yamamoto, Keisuke;  Venida, Anthony;  Yano, Julian;  Biancur, Douglas E.;  Kakiuchi, Miwako;  Gupta, Suprit;  Sohn, Albert S. W.;  Mukhopadhyay, Subhadip;  Lin, Elaine Y.;  Parker, Seth J.;  Banh, Robert S.;  Paulo, Joao A.;  Wen, Kwun Wah;  Debnath, Jayanta;  Kim, Grace E.;  Mancias, Joseph D.;  Fearon, Douglas T.;  Perera, Rushika M.;  Kimmelman, Alec C.
收藏  |  浏览/下载:25/0  |  提交时间:2020/07/03

Quantum mechanics governs the microscopic world, where low mass and momentum reveal a natural wave-particle duality. Magnifying quantum behaviour to macroscopic scales is a major strength of the technique of cooling and trapping atomic gases, in which low momentum is engineered through extremely low temperatures. Advances in this field have achieved such precise control over atomic systems that gravity, often negligible when considering individual atoms, has emerged as a substantial obstacle. In particular, although weaker trapping fields would allow access to lower temperatures(1,2), gravity empties atom traps that are too weak. Additionally, inertial sensors based on cold atoms could reach better sensitivities if the free-fall time of the atoms after release from the trap could be made longer(3). Planetary orbit, specifically the condition of perpetual free-fall, offers to lift cold-atom studies beyond such terrestrial limitations. Here we report production of rubidium Bose-Einstein condensates (BECs) in an Earth-orbiting research laboratory, the Cold Atom Lab. We observe subnanokelvin BECs in weak trapping potentials with free-expansion times extending beyond one second, providing an initial demonstration of the advantages offered by a microgravity environment for cold-atom experiments and verifying the successful operation of this facility. With routine BEC production, continuing operations will support long-term investigations of trap topologies unique to microgravity(4,5), atom-laser sources(6), few-body physics(7,8)and pathfinding techniques for atom-wave interferometry(9-12).


  
RARE CHANCE TO REACH ICE GIANTS EXCITES SCIENTISTS 期刊论文
NATURE, 2020, 579 (7797) : 17-17
作者:  Woolston, Chris
收藏  |  浏览/下载:0/0  |  提交时间:2020/07/03
The wide-binary origin of (2014) MU69-like Kuiper belt contact binaries 期刊论文
NATURE, 2020, 580 (7804) : 463-+
作者:  Jiao, Lin;  Howard, Sean;  Ran, Sheng;  Wang, Zhenyu;  Rodriguez, Jorge Olivares;  Sigrist, Manfred;  Wang, Ziqiang;  Butch, Nicholas P.;  Madhavan, Vidya
收藏  |  浏览/下载:66/0  |  提交时间:2020/07/03

Following its flyby and first imaging of the Pluto-Charon binary, the New Horizons spacecraft visited the Kuiper belt object (KBO) 2014 MU69 (also known as (486958) Arrokoth). The imaging showed MU69 to be a contact binary that rotates at a low spin period (15.92 hours), is made of two individual lobes connected by a narrow neck and has a high obliquity (about 98 degrees)(1), properties that are similar to those of other KBO contact binaries inferred through photometric observations(2). However, all scenarios suggested so far for the origins of such configurations(3-5) have failed to reproduce these properties and their probable frequent occurrence in the Kuiper belt. Here we show that semi-secular perturbations(6,7) operating on only ultrawide KBO binaries close to their stability limit can robustly lead to gentle, slow binary mergers at arbitrarily high obliquities but low rotational velocities, reproducing the characteristics of MU69 and other similar oblique contact binaries. Using N-body simulations, we find that approximately 15 per cent of all ultrawide binaries with a cosine-uniform inclination distribution(5,9) are likely to merge through this process. Moreover, we find that such mergers are sufficiently gentle to deform the shape of the KBO only slightly. The semi-secular contact binary formation channel not only explains the observed properties of MU69, but may also apply to other Kuiper belt or asteroid belt binaries and in the Solar System and extra-solar moon systems.


The high obliquity and low rotation period of the Kuiper belt object (2014) MU69 and other similar contact binaries is successfully reproduced from the collision and post-collision characteristics of initially wide binaries.


  
Nightside condensation of iron in an ultrahot giant exoplanet 期刊论文
NATURE, 2020, 580 (7805) : 597-+
作者:  Lu, Zhihao;  Zou, Jianling;  Li, Shuang;  Topper, Michael J.;  Tao, Yong;  Zhang, Hao;  Jiao, Xi;  Xie, Wenbing;  Kong, Xiangqian;  Vaz, Michelle;  Li, Huili;  Cai, Yi;  Xia, Limin;  Huang, Peng;  Rodgers, Kristen;  Lee, Beverly;  Riemer, Joanne B.;  Day, Chi-Ping;  Yen, Ray-Whay Chiu;  Cui, Ying;  Wang, Yujiao;  Wang, Yanni;  Zhang, Weiqiang;  Easwaran, Hariharan;  Hulbert, Alicia;  Kim, KiBem;  Juergens, Rosalyn A.;  Yang, Stephen C.;  Battafarano, Richard J.;  Bush, Errol L.;  Broderick, Stephen R.;  Cattaneo, Stephen M.;  Brahmer, Julie R.;  Rudin, Charles M.;  Wrangle, John;  Mei, Yuping;  Kim, Young J.;  Zhang, Bin;  Wang, Ken Kang-Hsin;  Forde, Patrick M.;  Margolick, Joseph B.;  Nelkin, Barry D.;  Zahnow, Cynthia A.;  Pardoll, Drew M.;  Housseau, Franck;  Baylin, Stephen B.;  Shen, Lin;  Brock, Malcolm V.
收藏  |  浏览/下载:57/0  |  提交时间:2020/07/03

Ultrahot giant exoplanets receive thousands of times Earth'  s insolation(1,2). Their high-temperature atmospheres (greater than 2,000 kelvin) are ideal laboratories for studying extreme planetary climates and chemistry(3-5). Daysides are predicted to be cloud-free, dominated by atomic species(6) and much hotter than nightsides(5,7,8). Atoms are expected to recombine into molecules over the nightside(9), resulting in different day and night chemistries. Although metallic elements and a large temperature contrast have been observed(10-14), no chemical gradient has been measured across the surface of such an exoplanet. Different atmospheric chemistry between the day-to-night ('  evening'  ) and night-to-day ('  morning'  ) terminators could, however, be revealed as an asymmetric absorption signature during transit(4,7,15). Here we report the detection of an asymmetric atmospheric signature in the ultrahot exoplanet WASP-76b. We spectrally and temporally resolve this signature using a combination of high-dispersion spectroscopy with a large photon-collecting area. The absorption signal, attributed to neutral iron, is blueshifted by -11 +/- 0.7 kilometres per second on the trailing limb, which can be explained by a combination of planetary rotation and wind blowing from the hot dayside(16). In contrast, no signal arises from the nightside close to the morning terminator, showing that atomic iron is not absorbing starlight there. We conclude that iron must therefore condense during its journey across the nightside.


Absorption lines of iron in the dayside atmosphere of an ultrahot giant exoplanet disappear after travelling across the nightside, showing that the iron has condensed during its travel.


  
Where I work 期刊论文
NATURE, 2020, 583 (7815) : 324-324
作者:  Dance, Amber;  Ousnamer, Zach
收藏  |  浏览/下载:3/0  |  提交时间:2020/07/03

Engineer and roboticist Zach Ousnamer is helping to prepare NASA'  s Perseverance rover for its launch to the red planet.


Engineer and roboticist Zach Ousnamer is helping to prepare NASA'  s Perseverance rover for its launch to the red planet.


  
Evidence for extremely rapid magma ocean crystallization and crust formation on Mars 期刊论文
NATURE, 2018, 558 (7711) : 586-+
作者:  Bouvier, Laura C.;  Costa, Maria M.;  Connelly, James N.;  Jensen, Ninna K.;  Wielandt, Daniel;  Storey, Michael;  Nemchin, Alexander A.;  Whitehouse, Martin J.;  Snape, Joshua F.;  Bellucci, Jeremy J.;  Moynier, Frederic;  Agranier, Arnaud;  Gueguen, Bleuenn;  Schonbachler, Maria;  Bizzarro, Martin
收藏  |  浏览/下载:9/0  |  提交时间:2019/11/27
Turbulent convective length scale in planetary cores 期刊论文
NATURE, 2019, 570 (7761) : 368-+
作者:  Guervilly, Celine;  Cardin, Philippe;  Schaeffer, Nathanael
收藏  |  浏览/下载:1/0  |  提交时间:2019/11/27
In situ X-ray diffraction measurement of shock-wave-driven twinning and lattice dynamics 期刊论文
NATURE, 2017, 550 (7677) : 496-+
作者:  Wehrenberg, C. E.;  McGonegle, D.;  Bolme, C.;  Higginbotham, A.;  Lazicki, A.;  Lee, H. J.;  Nagler, B.;  Park, H. -S.;  Remington, B. A.;  Rudd, R. E.;  Sliwa, M.;  Suggit, M.;  Swift, D.;  Tavella, F.;  Zepeda-Ruiz, L.;  Wark, J. S.
收藏  |  浏览/下载:11/0  |  提交时间:2019/11/27
PLANETARY SCIENCE Earth's building blocks 期刊论文
NATURE, 2017, 541 (7638) : 468-470
作者:  Carlson, Richard W.
收藏  |  浏览/下载:5/0  |  提交时间:2019/11/27
Penitentes as the origin of the bladed terrain of Tartarus Dorsa on Pluto 期刊论文
NATURE, 2017, 541 (7636) : 188-+
作者:  Moores, John E.;  Smith, Christina L.;  Toigo, Anthony D.;  Guzewich, Scott D.
收藏  |  浏览/下载:6/0  |  提交时间:2019/04/09