Thursday, October 31, 2013

PC厂商积极推出变形产品

PC厂商积极推出变形产品

PC品牌厂商如惠普,宏碁,联想和华硕电脑都积极推出可变型产品,旨在推动整体消费需求。

宏碁已经在台湾发布了其全新的Android一体机,并预期新设备,以帮助该公司在2014年上半年,成为世界上最大的电脑一体机厂商。

惠普也推出了新款2合1笔记本电脑,型号是Split13x2 ,配备了13英寸显示屏, Windows操作系统,采用专门设计的铰链,该设备可以被分离,成为平板电脑。Split13x2平板电脑拥有一个128GB固态硬盘,键盘基座配备了一个500GB硬盘驱动器,这款产品售价为新台币44900元,大约1528美元。

和平板电脑年出货量增长35-40%相比, 2合1的设备出货量增长幅度预计在2014年达到400% ,因此惠普将重点放在推动相关产品,以扩大其市场份额。

联想最近推出了其Yoga平板电脑,采用8 英寸或10英寸显示屏,联发科MT8125芯片组,内建1.2GHz四核处理器, 1GB内存和16GB存储空间。新瑜伽平板电脑能够在许多不同的角度进行折叠,达到不同的使用目的。




香港南芳实业有限公司(深圳南芳引航科技有限公司)成立于2001年。是一家专业开发、生产、加工、销售各种应用于计算机接口设备连接线手机数据线、车载电子设备、医疗器械等高科技电子设备之连接线的外商独资企业。

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烤线加工等相关线材组立加工。已通过ISO-9001:2008质量管理体系认证和ISO-14001:2004 环境管理体系认证。直接海外美金付款同时可开具17%的增值税发票和提供转厂合同,满足广大客户的需求。


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微软:Surface已掌控未来,竞争对手都在追赶

微软:Surface已掌控未来,竞争对手都在追赶

真的勇士敢于直面惨淡的销量并鄙视对手的产品,当所有人都认为 Surface 2 并不能挽救微软在平板电脑市场的颓势的时候,微软自己显然对这种说法不以为然。

苹果秋季发布的新品 iPad Air 日前刚刚开始发货,因此媒体的焦点很快投向了 Surface 2 和 iPad Air 这两款同月发布的新品的比较上。当微软的英国负责人 Ally Wickham 被问及 Surface 2 与 iPad Air 的比较时,他说:「我们的竞争对手终于跟上了我们的思路,开始意识到用户拿平板不只是为了娱乐。」

Ally Wickham 认为平板的功能不应该只是娱乐,用户应该有更多的选择,平板应该即是娱乐工具又是生产力工具,微软从一开始就意识到了这一点而其他竞争者(指苹果)是刚刚才醒悟,因此微软已经在平板领域里遥遥领先。

Ally Wickham 指的应该是在最近的发布会上苹果宣布全平台 iWorks 免费的消息,苹果此举确实有拓展 iPad 办公性能的意图,但是很显然微软并没有意识到「用户买平板可不只是为了办公」这一事实。

知名导演 Rob Epstein 对这一观点表示认可:「当我们开始周期性的更换价格不菲的平板电脑的时候,我们就会开始思考『为什么我花大价钱买了平板电脑还要另外掏钱买一台笔记本用来工作?』」

虽然不知道究竟有多少用户和微软打的是同样的算盘,不过微软的自信营销一向如此。

目前已经消失在历史的尘埃中的微软 Zune 音乐播放器产品线在刚推出的时候也由比尔盖茨亲自代言:「我从来不让我的家人用 iPod,因为 Zune 已经是一款足够好的产品,它已经超越了苹果的播放器。




香港南芳实业有限公司(深圳南芳引航科技有限公司)成立于2001年。是一家专业开发、生产、加工、销售各种应用于计算机接口设备连接线手机数据线、车载电子设备、医疗器械等高科技电子设备之连接线的外商独资企业。

主要产品为:

线材系列DC电源线USB连接线转接线材HDMI线RCA音视频连接线MHL连接线HDMI高清数据线USB数据线MHL 手机数据线材RCA音频视频线、三星S3 S4转接及数据线、DVI连接线、DB连接线、MINI DIN连接线、弹弓线

连接器系列Mini USB接口连接器HDMI接口连接器手机连接器USB接口连接器DIN接口连接器DIN连接器Mini USB连接器HDMI连接器

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红外线感应器系列非接触红外传感器热电堆

二极管系列

烤线加工等相关线材组立加工。已通过ISO-9001:2008质量管理体系认证和ISO-14001:2004 环境管理体系认证。直接海外美金付款同时可开具17%的增值税发票和提供转厂合同,满足广大客户的需求。


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[警告]Mavericks下使用西数外置硬盘会导致数据丢失

[警告]Mavericks下使用西数外置硬盘会导致数据丢失

西部数据(WD)已经向顾客发出警告邮件,通知用户将西数外置硬盘连接至安装有OS X Mavericks的Mac电脑时会导致数据丢失。苹果官方支持论坛、西数支持论坛上有很多用户表示升级至Mavericks后,将西数外置硬盘连接 Mac后会导致数据丢失。

在发送给用户的邮件中,西数警告大家升级至Mavericks前要将WD Drive Manager、WD Raid Manager以及各种相关的软件卸载。如果用户已经升级至Mavericks,西数建议立刻卸载这些应用。目前西数正在紧急调查问题的原因,相信不久之 后就会有解决方案。




香港南芳实业有限公司(深圳南芳引航科技有限公司)成立于2001年。是一家专业开发、生产、加工、销售各种应用于计算机接口设备连接线手机数据线、车载电子设备、医疗器械等高科技电子设备之连接线的外商独资企业。

主要产品为:

线材系列DC电源线USB连接线转接线材HDMI线RCA音视频连接线MHL连接线HDMI高清数据线USB数据线MHL 手机数据线材RCA音频视频线、三星S3 S4转接及数据线、DVI连接线、DB连接线、MINI DIN连接线、弹弓线

连接器系列Mini USB接口连接器HDMI接口连接器手机连接器USB接口连接器DIN接口连接器DIN连接器Mini USB连接器HDMI连接器

热敏电阻系列高耐热性热敏电阻贴片热敏电阻热敏电阻传感器高精度热敏电阻高耐热性电阻

红外线感应器系列非接触红外传感器热电堆

二极管系列

烤线加工等相关线材组立加工。已通过ISO-9001:2008质量管理体系认证和ISO-14001:2004 环境管理体系认证。直接海外美金付款同时可开具17%的增值税发票和提供转厂合同,满足广大客户的需求。


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Former missile-tracking telescope helps reveal fate of baby pulsar

Former missile-tracking telescope helps reveal fate of baby pulsar

The findings are published in the journal Science November 1.

The Crab pulsar is a neutron star which formed in a massive cosmic explosion seen in both Europe and China in AD 1054 as a bright star in the daytime sky. Now rotating 30 times a second, this highly-compact star emits beams of radio waves that, like a lighthouse, produce flashes each time it rotates. The star itself is only about 25 km across but contains the mass of nearly 1 million Earths.

Professor Andrew Lyne and his colleagues from The University of Manchester report on a steady change in these flashes during a 22-year experiment watching the star, telling them about its very strong magnetic field and helping us learn about the otherwise-inaccessible interior of the star.

The flashes, or pulses, come in pairs. The new observations show that the spacing of these pairs ofi pulses is increasing by 0.6 degrees per century, an unexpectedly large rate of evolution. The scientists have shown that this means that the magnetic pole is moving towards the equator.

The astronomers employed a 42-ft telescope that was formerly used to track the Blue Streak missile at the Woomera Rocket Test Range in Australia until 1981, when it was dismantled, transported and re-erected at the Jodrell Bank Observatory in Cheshire, England.

This relatively modest telescope has been used to observe the Crab pulsar almost daily for 31 years, during which time the pulsar has rotated 30 billion times, and Jodrell Bank has kept count of every rotation. The most accurate observations, made since 1991, show the small gradual change in the pulse spacing.

Study lead Andrew Lyne, an Emeritus Professor at Manchester, said that the most surprising aspect of is that this change is happening so rapidly, when the interior of the star is superconducting, and the magnetic field should be frozen in position.

Co-author Professor Sir Francis Graham Smith said: "This pulsar is just 960 years old, so while 22 years gives only a small sample of its lifetime, it is a much larger fraction of a stellar lifetime than astronomers usually get to study."

Dr Christine Jordan, who helps keep the telescope and observations running at Jodrell Bank, said: "It is amazing to think that this relatively small missile-tracking telescope, installed in Australia in 1974 by Marconi and donated to the Jodrell Bank Observatory in 1981 where it was converted to observe pulsars, has proved to be such a boon to astronomers. This is a real sword to ploughshare concept in action."

Dr Patrick Weltevrede, also of The University of Manchester, believes that this result will have important implications for our understanding of the evolution of pulsars and how they emit. He said: "The Crab pulsar is iconic; it is seen across the entire electromagnetic spectrum and is an exemplar and so this result provides vital clues about how these cosmic lighthouses shine and explaining a long-standing mystery about the way pulsars slow down over time."


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Magnetic 'force field' shields giant gas cloud during collision with Milky Way

Magnetic 'force field' shields giant gas cloud during collision with Milky Way

Oct. 31, 2013 — Doom may be averted for the Smith Cloud, a gigantic streamer of hydrogen gas that is on a collision course with the Milky Way Galaxy. Astronomers using the National Science Foundation's Karl G. Jansky Very Large Array (VLA) and Robert C. Byrd Green Bank Telescope (GBT) have discovered a magnetic field deep in the cloud's interior, which may protect it during its meteoric plunge into the disk of our Galaxy.


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This discovery could help explain how so-called high velocity clouds (HVCs) remain mostly intact during their mergers with the disks of galaxies, where they would provide fresh fuel for a new generation of stars.

Currently, the Smith Cloud is hurtling toward the Milky Way at more than 150 miles per second and is predicted to impact in approximately 30 million years. When it does, astronomers believe, it will set off a spectacular burst of star formation. But first, it has to survive careening through the halo, or atmosphere, of hot ionized gas surrounding the Milky Way.

"The million-degree upper atmosphere of the Galaxy ought to destroy these hydrogen clouds before they ever reach the disk, where most stars are formed," said Alex Hill, an astronomer at Australia's Commonwealth Scientific and Industrial Research Organization (CSIRO) and lead author of a paper published in the Astrophysical Journal. "New observations reveal one of these clouds in the process of being shredded, but a protective magnetic field shields the cloud and may help it survive its plunge."

Many hundreds of HVCs zip around our Galaxy, but their obits seldom correspond to the rotation of the Milky Way. This leads astronomers to believe that HVCs are the left-over building blocks of galaxy formation or the splattered remains of a close galactic encounter billions of years ago.

Though massive, the gas that makes up HVCs is very tenuous, and computer simulations predict that they lack the necessary heft to survive plunging through the halo and into the disk of the Milky Way.

"We have long had trouble understanding how HVCs reach the Galactic disk," said Hill. "There's good reason to believe that magnetic fields can prevent their 'burning up' in the halo like a meteorite burning up in Earth's atmosphere."

Despite being the best evidence yet for a magnetic field inside an HVC, the origin of the Smith Cloud's field remains a mystery. "The field we observe now is too large to have existed in its current state when the cloud was formed," said Hill. "The field was probably magnified by the cloud's motion through the halo."

Earlier research indicates the Smith Cloud has already survived punching through the disk of our Galaxy once and -- at about 8,000 light-years from the disk -- is just beginning its re-entry now.

"The Smith Cloud is unique among high-velocity clouds because it is so clearly interacting with and merging with the Milky Way," said Felix J. Lockman, an astronomer at the National Radio Astronomy Observatory (NRAO) in Green Bank, W.Va. "Its comet-like appearance indicates it's already feeling the Milky Way's influence."

Since the Smith Cloud appears to be devoid of stars, the only way to observe it is with exquisitely sensitive radio telescopes, like the GBT, which can detect the faint emission of neutral hydrogen. If it were visible with the naked eye, the Smith Cloud would cover almost as much sky as the constellation Orion.

When the Smith Cloud eventually merges with the Milky Way, it could produce a bright ring of stars similar to the one relatively close to our Sun known as Gould's Belt.

"Our Galaxy is in an incredibly dynamic environment," concludes Hill, "and how it interacts with that environment determines whether stars like the Sun will continue to form."

The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.



Welcome to SUV System Ltd!

SUV System Ltd is ISO 90012008 Certified electronics distributor with 10 years of experiences.

We have built up long term business relationship with about many companies which are stockers and authorized agents. we have a steady and reliable supply to meet customer's demands to the greatest extent .Confidently, we are able to lower your cost and support your business with our years of professional service.

SUV System Ltd is Electronic Components Distributor Supplies,Find Quality Electronic Components Supplies Products IC(Integrated Circuits),Connectors,Capacitor,Resistors,Diodes,Transistors,LED at Suvsystem.com. Sourcing Other Energy, Environment, Excess Inventory Products from Manufacturers and Suppliers at Suvsystem.com

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Connectors Distributor:http://www.suvsystem.com/l/Connectors-1.html

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Capacitor Distributor:http://www.suvsystem.com/l/Capacitor-1.html

Transistor Distributor:http://www.suvsystem.com/l/Transistors-1.html

Resistor Distributor:http://www.suvsystem.com/l/Resistors-1.html

Diode Distributor:http://www.suvsystem.com/l/Diodes-1.html

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New techniques produce cleanest graphene yet

New techniques produce cleanest graphene yet

The study is published in Science on November 1, 2013.

"This is an exciting new paradigm in materials engineering where instead of the conventional approach of layer by layer growth, hybrid materials can now be fabricated by mechanical assembly of constituent 2D crystals," says Electrical Engineering Professor Ken Shepard, co-author of the paper. "No other group has been able to successfully achieve a pure edge-contact geometry to 2D materials such as graphene."

He adds that earlier efforts have looked at how to improve 'top contacts' by additional engineering such as adding dopants: "Our novel edge-contact geometry provides more efficient contact than the conventional geometry without the need for further complex processing. There are now many more possibilities in the pursuit of both device applications and fundamental physics explorations."

First isolated in 2004, graphene is the best-studied 2D material and has been the subject of thousands of papers studying its electrical behavior and device applications. "But in nearly all of this work, the performance of graphene is degraded by exposure to contamination," notes Mechanical Engineering Professor James Hone who is also a co-author of the study. "It turns out that the problems of contamination and electrical contact are linked. Any high-performance electronic material must be encapsulated in an insulator to protect it from the environment. Graphene lacks the ability to make out-of-plane bonds, which makes electrical contact through its surface difficult, but also prevents bonding to conventional 3D insulators such as oxides. Instead, the best results are obtained by using a 2D insulator, which does not need to make bonds at its surface. However, there has been no way to electrically access a fully-encapsulated graphene sheet until now."

In this work, says Cory Dean, who led the research as a postdoc at Columbia and is now an assistant professor at The City College of New York, the team solved both the contact and contamination problems at once. "One of the greatest assets of 2D materials such as graphene is that being only one atom thick, we have direct access to its electronic properties. At the same time, this can be one of its worst features since this makes the material extremely sensitive to its environment. Any external contamination quickly degrades performance. The need to protect graphene from unwanted disorder, while still allowing electrical access, has been the most significant roadblock preventing development of graphene-based technologies. By making contact only to the 1D edge of graphene, we have developed a fundamentally new way to bridge our 3D world to this fascinating 2D world, without disturbing its inherent properties. This virtually eliminates external contamination and finally allows graphene to show its true potential in electronic devices"

The researchers fully encapsulated the 2D graphene layer in a sandwich of thin insulating boron nitride crystals, employing a new technique in which crystal layers are stacked one-by-one. "Our approach for assembling these heterostructures completely eliminates any contamination between layers," Dean explains, "which we confirmed by cross-sectioning the devices and imaging them in a transmission electron microscope with atomic resolution."

Once they created the stack, they etched it to expose the edge of the graphene layer, and then evaporated metal onto the edge to create the electrical contact. By making contact along the edge, the team realized a 1D interface between the 2D active layer and 3D metal electrode. And, even though electrons entered only at the 1D atomic edge of the graphene sheet, the contact resistance was remarkably low, reaching 100 Ohms per micron of contact width -- a value smaller than what can be achieved for contacts at the graphene top surface.

With the two new techniques -- the contact architecture through the 1D edge and the stacking assembly method that prevents contamination at the interfaces -- the team was able to produce what they say is the "cleanest graphene yet realized." At room temperature, these devices exhibit previously unachievable performance, including electron mobility at least twice as large as any conventional 2D electron system, and sheet resistivity less than 40 Ohms when sufficient charges are added to the sheet by electrostatic "gating." Amazingly, this 2D sheet resistance corresponds to a "bulk" 3D resistivity smaller than that of any metal at room temperature. At low temperature, electrons travel through the team's samples without scattering, a phenomenon known as ballistic transport. Ballistic transport, had previously been observed in samples close to one micrometer in size, but this work demonstrates the same behavior in samples as large as 20 micrometers. "So far this is limited purely by device size," says Dean, "indicating that the true 'intrinsic' behavior is even better."

The team is now working on applying these techniques to develop new hybrid materials by mechanical assembly and edge contact of hybrid materials drawing from the full suite of available 2D layered materials, including graphene, boron nitride, transition metal dichlcogenides (TMDCs), transition metal oxides (TMOs), and topological insulators (TIs). "We are taking advantage of the unprecedented performance we now routinely achieve in graphene-based devices to explore effects and applications related to ballistic electron transport over fantastically large length scales," Dean adds. "With so much current research focused on developing new devices by integrating layered 2D systems, potential applications are incredible, from vertically structured transistors, tunneling based devices and sensors, photoactive hybrid materials, to flexible and transparent electronics."

"This work results from a wide collaboration of researchers interested in both pure and applied science," says Hone. "The unique environment at Columbia provides an unparalleled opportunity for these two communities to interact and build off one another."

The Columbia team demonstrated the first technique to mechanically layer 2D materials in 2010. These two new techniques, which are critical advancements in the field, are the result of interdisciplinary efforts by Lei Wang (PhD student, Electrical Engineering, Hone group) and Inanc Meric (Postdoc, Electrical Engineering, Shepard group), co-lead authors on this project who worked with the groups of Philip Kim (Physics and Applied Physics and Applied Mathematics, Columbia), James Hone (Mechanical Engineering, Columbia), Ken Shepard (Electrical Engineering, Columbia) and Cory Dean (Physics, City College of New York).


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A first step in learning by imitation, baby brains respond to another's actions

A first step in learning by imitation, baby brains respond to another's actions

Now researchers from the University of Washington and Temple University have found the first evidence revealing a key aspect of the brain processing that occurs in babies to allow this learning by observation.

The findings, published online Oct. 30 by PLOS ONE, are the first to show that babies' brains showed specific activation patterns when an adult performed a task with different parts of her body. When 14-month-old babies simply watched an adult use her hand to touch a toy, the hand area of the baby's brain lit up. When another group of infants watched an adult touch the toy using only her foot, the foot area of the baby's brain showed more activity.

"Babies are exquisitely careful people-watchers, and they're primed to learn from others," said Andrew Meltzoff, co-author and co-director of the UW Institute for Learning & Brain Sciences. "And now we see that when babies watch someone else, it activates their own brains. This study is a first step in understanding the neuroscience of how babies learn through imitation."

The study took advantage of how the brain is organized. The sensory and motor area of the cortex, the outer portion of the brain known for its creased appearance, is arranged by body part with each area of the body represented in identifiable neural real estate. Prick your finger, stick out your tongue, or kick a ball and distinct areas of the brain light up according to a somatotopic map.

Other studies show that adults show this somatotopic brain activation while watching someone else use different body parts, suggesting that adults understand the actions of others in relation to their own bodies. The researchers wondered whether the same would be true in babies.

The 70 infants in the study wore electroencephalogram, or EEG, caps with embedded sensors that detected brain activity in the regions of the cortex that respond to movement or touch of the feet and hands. Sitting on a parent's lap, each baby watched as an experimenter touched a toy placed on a low table between the baby and the experimenter.

The toy had a clear plastic dome and was mounted on a sturdy base. When the experimenter pressed the dome with her hand or foot, music played and confetti in the dome spun. The experimenter repeated the action -- taking breaks after every four presses -- until the baby lost interest.

"Our findings show that when babies see others produce actions with a particular body part, their brains are activated in a corresponding way," said Joni Saby, lead author and a psychology graduate student at Temple University in Philadelphia. "This mapping may facilitate imitation and could play a role in the baby's ability to then produce the same actions themselves."

One of the basics for babies to learn is how to copy what they see adults do. In other words, they must first know that it is indeed their hand and not their foot, mouth or other body part that is needed.

The new study shows that babies' brains are organized in a somatotopic way that helps crack the interpersonal code. The connection between doing and seeing actions maps hand to hand, foot to foot, all before they can name those body parts through language.

"The reason this is exciting is that it gives insight into a crucial aspect of imitation," said co-author Peter Marshall, an associate psychology professor at Temple University. "To imitate the action of another person, babies first need to register what body part the other person used. Our findings suggest that babies do this in a particular way by mapping the actions of the other person onto their own body."

Meltzoff added, "The neural system of babies directly connects them to other people, which jump-starts imitation and social-emotional connectedness and bonding. Babies look at you and see themselves."

The National Institutes of Health and the National Science Foundation funded the study.


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AMD显卡全球份额不断攀升 有望占领40%市场

AMD显卡全球份额不断攀升 有望占领40%市场

台湾显卡厂商指出,R9/R7系列发布以来,AMD的全球份额不断攀升,有望在未来半年内升至40%。根据市调机构JRP此前的数据,今年第二季度的全球独立显卡市场上,AMD的份额为38.0%,环比增加了2.3个百分点,但不如去年同期的40.3%。

如果厂商的预言成真,那对AMD来说也没什么特别值得高兴的,仅仅是经过两年的挣扎,回到了当初的较高水平而已。

第三季度,AMD取得了4800万美元的净利润,定制芯片和稳定的桌面出货量是主要动力,但是笔记本相关产品出货量大幅下滑,移动GPU收入也在倒退。

市场观察人士大多对AMD第四季度的业绩持保守态度,不过也有人期待AMD的显卡业务可以推动其盈利能力。

此外,AMD日前还曾经表示会努力提高FirePro专业显卡的份额,目前区区的18%显然无法令人满意。




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微软:杀毒软件无法保护Windows XP

微软:杀毒软件无法保护Windows XP

微软计划在2014年年初淘汰Windows XP,因此Windows XP很快便会成为不安全的操作系统,微软一直说服Windows XP的用户不要再使用此系统。

微软发布过信息图表展示安全性威胁的进化和发展,强调第三方反病毒软件无法保护没有补丁的Windows XP。

微软还表示Windows XP受恶意攻击的可能性是Win8的21倍,进而表明微软最新的系统才是用户的明智选择。




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Wednesday, October 30, 2013

How the universe's violent youth seeded cosmos with iron

How the universe's violent youth seeded cosmos with iron

New evidence that iron is spread evenly between the galaxies in one of the largest galaxy clusters in the universe supports the theory that the universe underwent a turbulent and violent youth more than 10 billion years ago. That explosive period was responsible for seeding the cosmos with iron and other heavy elements that are critical to life itself.

Researchers from the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), jointly run by Stanford University and the Department of Energy's SLAC National Accelerator Laboratory, shed light on this important era by analyzing 84 sets of X-ray telescope observations from the Japanese-US Suzaku satellite. Their results appear in the Oct. 31 issue of the journal Nature.

In particular, the researchers looked at iron distribution throughout the Perseus cluster, a large grouping of galaxies about 250 million light-years away.

"We saw that iron is spread out between the galaxies remarkably smoothly," said Norbert Werner, an astrophysicist at KIPAC and lead author of the paper. "That means it had to be present in the intergalactic gas before the Perseus cluster formed."

The even distribution of these elements supports the idea that they were created at least 10 billion to 12 billion years ago. According to the paper, during this time of intense star formation, billions of exploding stars created vast quantities of heavy elements in the alchemical furnaces of their own destruction. This was also the epoch when black holes in the hearts of galaxies were at their most energetic.

"The combined energy of these cosmic phenomena must have been strong enough to expel most of the metals from the galaxies at early times and to enrich and mix the intergalactic gas," said co-author and KIPAC graduate student Ondrej Urban.

To settle the question of whether the heavy elements created by supernovae remain mostly in their home galaxies or are spread out through intergalactic space, the researchers looked through the Perseus cluster in eight different directions. They focused on the hot, 10-million-degree gas that fills the spaces between galaxies and found the spectroscopic signature of iron reaching all the way to the cluster's edges.

The researchers estimate that the amount of iron in the cluster is roughly equivalent to the mass of 50 billion suns.

"We think most of the iron came from a single type of supernovae, called Type Ia supernovae," said former KIPAC member and co-author Aurora Simionescu, who is currently with the Japanese Aerospace Exploration Agency as an International Top Young Fellow.

In a Type Ia supernova, a star explodes and releases all its material to the void. The researchers believe that at least 40 billion Type Ia supernovae must have exploded within a relatively short period on cosmological time scales in order to release that much iron and have the force to drive it out of the galaxies.

The results suggest that the Perseus cluster is probably not unique and that iron -- along with other heavy elements -- is evenly spread throughout all massive galaxy clusters, said Steven Allen, a KIPAC associate professor and head of the research team.

"You are older than you think -- or at least, some of the iron in your blood is older, formed in galaxies millions of light years away and billions of years ago," Simionescu said.

The researchers are now looking for iron in other clusters and eagerly awaiting a mission capable of measuring the concentrations of elements in the hot gas with greater accuracy.

"With measurements like these, the Suzaku satellite is having a profound impact on our understanding of how the largest structures in our universe grow," Allen said. "We're really looking forward to what further data can tell us."

The research was supported by the Japanese Aerospace Exploration Agency and by the US Department of Energy.


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Lava world baffles astronomers: Planet Kepler-78b 'shouldn't exist'

Lava world baffles astronomers: Planet Kepler-78b 'shouldn't exist'

Oct. 30, 2013 — Kepler-78b is a planet that shouldn't exist. This scorching lava world circles its star every eight and a half hours at a distance of less than one million miles -- one of the tightest known orbits. According to current theories of planet formation, it couldn't have formed so close to its star, nor could it have moved there.


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"This planet is a complete mystery," says astronomer David Latham of the Harvard-Smithsonian Center for Astrophysics (CfA). "We don't know how it formed or how it got to where it is today. What we do know is that it's not going to last forever."

"Kepler-78b is going to end up in the star very soon, astronomically speaking," agrees CfA astronomer Dimitar Sasselov.

Not only is Kepler-78b a mystery world, it is the first known Earth-sized planet with an Earth-like density. Kepler-78b is about 20 percent larger than Earth, with a diameter of 9,200 miles, and weighs almost twice as much. As a result it has a density similar to Earth's, which suggests an Earth-like composition of iron and rock.

The tight orbit of Kepler-78b poses a challenge to theorists. When this planetary system was forming, the young star was larger than it is now. As a result, the current orbit of Kepler-78b would have been inside the swollen star.

"It couldn't have formed in place because you can't form a planet inside a star. It couldn't have formed further out and migrated inward, because it would have migrated all the way into the star. This planet is an enigma," explains Sasselov.

According to Latham, Kepler-78b is a member of a new class of planets recently identified in data from NASA's Kepler spacecraft. These newfound worlds all orbit their stars with periods of less than 12 hours. They're also small, about the size of Earth. Kepler-78b is the first planet in the new class to have its mass measured.

"Kepler-78b is the poster child for this new class of planets," notes Latham.

The team studied Kepler-78b using a newly commissioned, high-precision spectrograph known as HARPS-North, at the Roque de los Muchachos Observatory on La Palma. They coordinated their work with a second, independent team using the HIRES spectrograph at the Keck Observatory. The teams' measurements agreed with each other, increasing their confidence in the result.

Kepler-78b is a doomed world. Gravitational tides will draw it even closer to its star. Eventually it will move so close that the star's gravity will rip the world apart. Theorists predict that Kepler-78b will vanish within three billion years.

Interestingly, our solar system could have held a planet like Kepler-78b. If it had, the planet would have been destroyed long ago leaving no signs for astronomers today.

Kepler-78b orbits a Sun-like G-type star located 400 light-years from Earth in the constellation Cygnus.



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The secret math of plants: Biologists uncover rules that govern leaf design

The secret math of plants: Biologists uncover rules that govern leaf design

The UCLA team discovered the mathematical relationships using "allometric analysis," which looks at how the proportions of parts of an organism change with differences in total size. This approach has been used by scientists since Galileo but had never before been applied to the interior of leaves.

Reporting in the October issue of the American Journal of Botany, the biologists focused on how leaf anatomy varies across leaves of different sizes. They examined plant species from around the world, all grown on the UCLA campus.

While it is easy to observe major differences in leaf surface area among species, they said, differences in leaf thickness are less obvious but equally important.

"Once you start rubbing leaves between your fingers, you can feel that some leaves are floppy and thin, while others are rigid and thick," said Grace John, a UCLA doctoral student in ecology and evolutionary biology and lead author of the research. "We started with the simplest questions -- but ones that had never been answered clearly -- such as whether leaves that are thicker or larger in area are constructed of different sizes or types of cells."

The researchers embedded pieces of leaf in plastic and cut cross-sections thinner than a single cell to observe each leaf's microscopic layout. This allowed them to test the underlying relationship between cell and tissue dimensions and leaf size across species.

Leaves are made up of three basic tissues, each containing cells with particular functions: the outer layer, or epidermis; the mesophyll, which contains cells that conduct photosynthesis; and the vascular tissue, whose cells are involved in water and sugar transport. The team found that the thicker the leaf, the larger the size of the cells in all of its tissues -- except in the vascular tissue.

These relationships also applied to the components of the individual cells. Plant cells, unlike animal cells, are surrounded by carbohydrate-based cell walls, and the scientists discovered that the larger cells of thicker leaves are surrounded by thicker cell walls, in a strict proportionality.

The team was surprised by the "extraordinary" strength of the relationships linking cell size, cell-wall thickness and leaf thickness across diverse and distantly related plant species. These relationships can be described by new, simple mathematical equations, effectively allowing scientists to predict the dimension of cells and cell walls based on the thickness of a leaf. In most cases, the relationships the team found were what is known as "isometric."

"This means that if a leaf has a larger cell in one tissue, it has a larger cell in another tissue, in direct proportion, as if you blew up the leaf and all its cells using Photoshop," said Christine Scoffoni, a doctoral student at UCLA and member of the research team.

By contrast, a leaf's area is unrelated to the sizes of the cells inside. This allows plants to produce leaves with a huge range of surface areas without the need for larger cells, which would be inefficient in function, the researchers said.

The team hypothesized that these strong mathematical relationships arise from leaf development -- the process by which leaves form on the branch, growing from a few cells that divide into many, with cells then expanding until the leaf is fully mature. Because light can penetrate only so many layers of cells, leaves cannot vary much in the number of cells arranged vertically. The expansion of individual cells and their cell walls occurs simultaneously and is reflected in the thickness of the whole leaf. On the other hand, the number of cells arranged horizontally in the leaf continues to increase as leaves expand, regardless of the size of the individual cells.

The new ability to predict the internal anatomy of leaves from their thickness can give clues to the function of the leaf, because leaf thickness affects both the overall photosynthetic rate and the lifespan, said Sack.

"A minor difference in thickness tells us more about the layout inside the leaf than a much more dramatic difference in leaf area," John said.

The design of the leaf provides insights into how larger structures can be constructed without losing function or stability.

"Fundamental discoveries like these highlight the elegant solutions evolved by natural systems," Sack said. "Plant anatomy often has been perceived as boring. Quantitative discoveries like these prove how exciting this science can be. We need to start re-establishing skill sets in this type of fundamental science to extract practical lessons from the mysteries of nature.

"There are so many properties of leaves we cannot yet imitate synthetically," he added. "Leaves are providing us with the blueprints for bigger, better things. We just have to look close enough to read them."

The new allometric equations are an important step toward understanding the design of leaves on a cellular basis, John said. And because leaves are so diverse, she said, there is much to learn. In future research, the group will study species that are very closely related in an effort to uncover any evolutionary relationships between leaf design and function.

"What makes the cross-sections especially exciting is the huge variation from one species to the next," John said. "Some have relatively enormous cells in certain tissues, and cell shapes vary from cylindrical to star-shaped. Each species is beautiful in its distinctiveness. All of this variation needs decoding."


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