QQ登录

只需一步,快速开始

重磅出击:大西洋月刊——欧洲南方天文台

[复制链接]
人与自然 发表于 2013-1-24 14:03 | 显示全部楼层 |阅读模式 来自: 中国–广东–中山 电信

马上注册,结交更多好友,享用更多功能,让你轻松玩转社区。

您需要 登录 才可以下载或查看,没有账号?加入牧夫(请注明天文爱好者,否则无法通过审核,请勿使用gmail/outlook/aol/icloud邮箱注册)

×
本帖最后由 人与自然 于 2013-1-24 17:54 编辑

欧洲南方天文台官网:http://www.eso.org/public/
欧洲南方天文台:维基百科http://zh.wikipedia.org/wiki/%E6%AC%A7%E6%B4%B2%E5%8D%97%E6%96%B9%E5%A4%A9%E6%96%87%E5%8F%B0

以下图片来自欧洲南方天文台官网,
图片较大,另外下载再看吧
gerd_huedepohl_2.jpg

lombardi-vlt.jpg

potw1051a.jpg

gerd_huedepohl_4.jpg

eso1210a.jpg

eso0812c.jpg

ats.jpg

potw1118a.jpg
欧洲南方天文台 (The European Southern Observatory,ESO) 是为在南半球研究天文学,在government间组织的一个研究机构,由15个国家组成和支援的一个天文研究组织。它成立于1962年,目的是为欧洲的天文学家提供先进的设施和捷径以研究南方的天空。这个组织的总部设在德国慕尼黑附近的加兴,雇用了约700名工作人员,每年并接受成员国约135亿欧元的经费。
欧洲南方天文台建设和经营一些已知规模最大和技术最先进的望远镜,包括首创主动光学技术的新技术望远镜、和由4个8米等级的望远镜和4个1.8米辅助望远镜组成的甚大望远镜。目前由ESO进行的计划包括亚他加马大型毫米波阵列和欧洲极大望远镜。
ALMA是下一个十年最大的地面天文专案,将成为在毫米与次毫米波尺度下观测的主要新工具。他的建设正在进行中,预计于2013年完成。ALMA专案是欧洲各国、亚洲、北美洲和智利之间的国际合作计划。欧洲的执行权由ESO代表行使,并且还主持ALMA区域中心。
E-ELT是40米等级的望远镜,目前还在细部设计阶段,将是世界上观测天空最大的巨眼。 欧洲极大望远镜,它将极有力的推动天文物理学的知识,能够仔细研究的天体,包括围绕着其它恒星的行星、宇宙中的第一个天体、超大质量黑洞、和主宰宇宙的暗物质与暗能量的自然本质和分布。从2005年底,ESO就一直与工作和使用社群的欧洲天文学家和天文物理学家共同来定义此新的聚型望远镜。
ESO的观测机构已经作出许多重大的天文发现和一些天体目录[4]。最近的研究结果包括发现最遥远的伽玛射线暴和我们的星系,银河系,中心有黑洞的证据。在2004年,甚大望远镜让天文学家获得第一张在173光年外环绕着的棕矮星的系外行星2M1207b轨道的绝佳影像。安装在ESO另一架望远镜上的仪器,高精度径向速度行星搜索器发现许多的系外行星,包括迄今发现最小的系外行星格利泽581c。甚大望远镜还发现了迄今距离人类最遥远星系的候选者阿贝尔1835 IR1916。

ESO的总部始终都在德国,而它的望远镜和仪器都在智利。这个组织运作著一些世界上规模最大、最先进的观测设施都在该国北部的三个地点:
拉西拉:新技术望远镜的主机,
帕瑞纳:甚大望远镜设置在此地,
拉诺德查南托:此处是亚他加马探路者实验 ( Atacama Pathfinder Experiment,APEX)、次毫米望远镜和亚他加马大型毫米波阵列的所在地;ALMA目前正在建设中。
这些都是南半球的天文观测最佳地点。

ESO最有野心勃勃的计划是欧洲极大望远镜,追随着势不可挡的巨大望远镜观念,以5个创新的镜面设计为基础的一架口径42米的望远镜。如果完成了, E-ELT将是世界上最大的光学/近红外线望远镜。ESO在2006年初开始设计阶段,期望在2011年开始建造[15]在2010年4月26日决定,第四个场所,阿玛逊斯山将是E-ELT的落脚处。
每一年,大约有2,000件企划申请使用ESO的望远镜,超过可以使用夜晚的四至六倍。使用这些仪器设备完成的论文出现在许多同行评审的科学年报中,单单在2009年,基于ESO的资料出版的论文就超过了650篇

会员国及加入时间
比利时 1962年
德国 1962年
法国 1962年
荷兰 1962年
瑞典 1962年
丹麦 1967年
瑞士 1981年
意大利 1982年5月24日
葡萄牙 2000年6月27日
英国 2002年7月8日
芬兰 2004年7月1日
西班牙 2006年7月1日
捷克 2007年1月1日
奥地利 2008年7月1日
巴西 2010年12月29日

2000px-ESO_member_states.jpg


评分

参与人数 1牧夫币 +10 威望 +1 收起 理由
张紫恒 + 10 + 1 赞一个!

查看全部评分

 楼主| 人与自然 发表于 2013-1-24 14:04 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:15 编辑

大西洋月刊
http://www.theatlantic.com/infocus/2013/01/the-european-southern-observatory/100444/

High in the Atacama Desert of northern Chile, the European Southern Observatory (ESO) has built several collections of telescopes and observatories on remote, arid mountaintops. The locations are ideal for ground-based astronomy -- far from city lights, high above sea level, with more than 350 cloudless days a year. The ESO is an intergovernmental research organization with 15 member states, founded in 1962. It has been making observations from the southern hemisphere since 1966, and continues to expand its facilities to this day. The sites are La Silla, which hosts the New Technology Telescope (NTT); Paranal, home to the Very Large Telescope (VLT); and Llano de Chajnantor, which hosts the APEX submillimeter telescope and the Atacama Large Millimeter/submillimeter Array (ALMA). Construction on the newest project in Chile's desert -- the European Extremely Large Telescope (E-ELT), a 40-meter-class telescope -- is due to start later this year in Cerro Armazones. I've collected below some amazing images of the ESO's observatories, and a few of the astronomical images they've been able to make over the years. [34 photos total]

As the full Moon sets, the Sun is about to rise on the opposite horizon. The ESO's Very Large telescope (VLT) has already closed its eyes after a long night of observations, and telescope operators and astronomers sleep while technicians, engineers and day astronomers wake up for a new day of work. Operations never stop at the most productive astronomical ground-based observatory in the world. ESO staff member Gordon Gillet welcomed the new day by capturing this stunning image from 14 km away, on the road to the nearby Cerro Armazones. (ESO/Gordon Gillet)


                               
登录/注册后可看大图
2
This view of the Chajnantor Plateau shows the site of the Atacama Large Millimeter/submillimeter Array (ALMA), taken from near the peak of Cerro Chico. Babak Tafreshi, an ESO Photo Ambassador, has succeeded in capturing the feeling of solitude experienced at the ALMA site, 5,000 meters above sea level in the Chilean Andes. When the telescope is completed in 2013, there will be a total of 66 such antennas in the array, operating together. ALMA is already revolutionizing how astronomers study the Universe at millimeter and submillimeter wavelengths. Even with a partial array of antennas, ALMA is more powerful than any previous telescope at these wavelengths, giving astronomers an unprecedented capability to study the cool Universe -- molecular gas and dust as well as the relic radiation of the Big Bang. (ESO/Babak Tafreshi) #


                               
登录/注册后可看大图
3
A glowing laser shines forth from the VLT, piercing the dark Chilean skies, its mission is to help astronomers explore the far reaches of the cosmos. We have all gazed up at the night sky and seen the stars gently twinkle as the Earth's turbulent atmosphere causes their light to shimmer. While it's a beautiful sight, it causes problems for astronomers, who want the crispest possible views. To help them achieve this, professional stargazers use something that sounds as though it has come from science fiction: a laser guide star that creates an artificial star 90 km above the surface of the Earth. The laser energizes sodium atoms high in the Earth's mesosphere, causing them to glow and creating a bright dot that appears to be a man-made star. Observations of how this "star" twinkles are fed into the VLT's adaptive optics system, controlling a deformable mirror in the telescope to restore the image of the star to a sharp point. By doing this, the system also compensates for the distorting effect of the atmosphere in the region around the artificial star. The end result is an exceptionally crisp view of the sky, allowing ESO astronomers to make stunning observations of the Universe, almost as though the VLT were above the atmosphere in space. (ESO/G. Huedepohl)


                               
登录/注册后可看大图
32
The reflection nebula Messier 78, captured using the Wide Field Imager camera on the MPG/ESO 2.2-meter telescope at the La Silla Observatory, Chile. This color picture was created from many monochrome exposures taken through blue, yellow/green and red filters, supplemented by exposures through a filter that isolates light from glowing hydrogen gas. (ESO/Igor Chekalin) #


                               
登录/注册后可看大图
33
This evocative image shows a dark cloud where new stars are forming along with a cluster of brilliant stars that have already emerged from their dusty stellar nursery. This cloud is known as Lupus 3 and it lies about 600 light-years from Earth in the constellation of Scorpius (The Scorpion). It is likely that the Sun formed in a similar star formation region more than four billion years ago. This picture was taken with the MPG/ESO 2.2-meter telescope at the La Silla Observatory in Chile and is the best image ever taken of this little-known object. (ESO/F. Comeron) #


                               
登录/注册后可看大图
34
This aerial view shows beautifully the Chilean Atacama Desert around the ESO Paranal Observatory, home to the VLT (at bottom right). Close to the VLT, one can see the dome of the VISTA survey telescope, and to the right, the Paranal Residence and basecamp. The high peak in the distance is the 6,739-meter high Andean volcano named Llullaillaco. Also in the image, to the middle left, one can see an isolated peak with a curvy road leading to its summit. This is Cerro Armazones, the selected home for the future European Extremely Large Telescope (E-ELT). (ESO/M. Tarenghi)
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:05 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:16 编辑


                               
登录/注册后可看大图
4
This color-composite image of the Helix Nebula (NGC 7293) was created from images obtained using the Wide Field Imager (WFI), an astronomical camera attached to the 2.2-meter Max-Planck Society/ESO telescope at the La Silla observatory in Chile. The blue-green glow in the center of the Helix comes from oxygen atoms shining under effects of the intense ultraviolet radiation of the 120 000 degree Celsius central star and the hot gas. Further out from the star and beyond the ring of knots, the red colour from hydrogen and nitrogen is more prominent. A careful look at the central part of this object reveals not only the knots, but also many remote galaxies seen right through the thinly spread glowing gas. (ESO) #


                               
登录/注册后可看大图
5
Many billions of years old, but still sparkling brightly, NGC 2257 is a globular cluster, the name given to the roughly spherical concentrations of stars that orbit galactic cores, but are often found far out from the centers in the halo areas of galaxies. NGC 2257 lies on the outskirts of the Large Magellanic Cloud (LMC), a satellite galaxy of our own Milky Way. The image is made from data taken with the Wide Field Imager instrument on the 2.2-meter MPG/ESO telescope at La Silla, as part of the ESO Imaging Survey project, which was planned to make public imaging surveys to identify targets for follow-up observations with the VLT. (ESO) #


                               
登录/注册后可看大图
6
A view of the Chajnantor plateau, showing the ALMA antennas ranged across the unearthly landscape. Some familiar celestial objects can be seen in the night sky behind them. These crystal-clear night skies explain why Chile is the home of not only ALMA, but also several other astronomical observatories. In the foreground, the 12-meter diameter ALMA antennas are in action, working as one giant telescope. On the far left, a cluster of smaller 7-meter antennas for ALMA's compact array can be seen illuminated. The crescent Moon, although not visible in this image, casts stark shadows over all the antennas. In the sky above the antennas, the most prominent bright "star", on the left of the image, is in fact the planet Jupiter. The Large Magellanic Cloud can also be clearly seen on the right, just above the rightmost antenna. On the far left of the image, just left of the foreground antennas, is the elongated smudge of the Andromeda galaxy. This galaxy, more than ten times further away than the Magellanic Clouds, is our closest major neighboring galaxy. Even though only its most central region is apparent in this image, the galaxy spans the equivalent of six full Moons in the sky. (ESO/Babak Tafreshi) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:07 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:16 编辑

full Moons in the sky. (ESO/Babak Tafreshi) #

                               
登录/注册后可看大图
7
The ALMA correlator, one of the most powerful supercomputers in the world, fully installed and tested at its remote, high altitude site in the Andes of northern Chile. This wide-angle view shows some of the racks of the correlator in the ALMA Array Operations Site Technical Building. This photograph shows one of four quadrants of the correlator. The full system has four identical quadrants, with over 134 million processors, performing up to 17 quadrillion operations per second. (ESO) #


                               
登录/注册后可看大图
8
Scientists work at the radio telescope control station of the ALMA project, in the Chajnantor plateau, Atacama desert, some 1,500 km north of Santiago, Chile, on October 1, 2011. (Martin Bernetti/AFP/Getty Images) #


                               
登录/注册后可看大图
9
One of most famous spiral galaxies is Messier 104, widely known as the "Sombrero" because of its particular shape. It is located towards the constellation Virgo, at a distance of about 30 million light-years. (ESO/IDA/Danish 1.5 m/R. Gendler and J.-E. Ovaldsen) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:09 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:17 编辑


                               
登录/注册后可看大图
10
A composite color image of the Horsehead Nebula and its immediate surroundings, based on three exposures in the visual part of the spectrum with the FORS2 multi-mode instrument at the 8.2-m KUEYEN telescope at Paranal. It was produced from three images, obtained on February 1, 2000. (ESO) #


                               
登录/注册后可看大图
11
This image, taken with the VLT Survey Telescope (VST) shows a wide variety of interacting galaxies in the young Hercules galaxy cluster. The sharpness of the picture and the sheer number of objects captured -- across a full square degree -- in less than three hours of observations attest to the great power of the VST and its OmegaCAM camera to explore the nearby Universe. (ESO/INAF-VST/OmegaCAM) #


                               
登录/注册后可看大图
12
The residence for astronomers of the European Southern Observatory (ESO) at the Cerro Paranal Observatory, photographed on September 15, 2008. The residence was built below ground to minimize the impact on the environment and to avoid the artificial light to spoil the night sky. This site was also used as one of the locations for the 2008 James Bond film "Quantum of Solace". (Martin Bernetti/AFP/Getty Images) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:10 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:18 编辑


                               
登录/注册后可看大图

13
The swimming pool inside the residence for ESO astronomers at the Cerro Paranal Observatory, photographed on September 15, 2008. (Martin Bernetti/AFP/Getty Images) #


                               
登录/注册后可看大图
14
The Atacama Large Millimeter/submillimeter Array, under construction. ALMA will be initially composed of 66 antennas, consisting a main array of fifty 12-meter antennas that can be spread over distances from 150 metres to 16 kilometers. In addition to the main array, ALMA will also have a compact array, composed of four 12-meter antennas plus twelve 7-meter antennas. By using the technique of interferometry, ALMA will work as a single giant telescope, enabling astronomers to observe the cold universe with unprecedented sensitivity and resolution. (ESO/NAOJ/NRAO/W. Garnier) #


                               
登录/注册后可看大图
15
Spain's Crown Prince Felipe and his wife Princess Letizia visit Paranal observatory of ESO in Cerro Paranal, on November 24, 2011. (Reuters/Felipe Trueba) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:11 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:18 编辑


                               
登录/注册后可看大图
16
The KMOS spectrograph, shown when it was undergoing tests at the UK Astronomy Technology Center in Edinburgh, before it was shipped to Chile to become a powerful new instrument on the VLT. The 24 robotic arms are visible. (STFC/UKATC/ESO) #


                               
登录/注册后可看大图
17
The prominent tail of Comet McNaught made a spectacular view over the VLT platform in January of 2007. (ESO/H.H.Heyer) #


                               
登录/注册后可看大图
18
Radio telescope antennas of the ALMA project, in the Chajnantor plateau, on October 1, 2011. (Martin Bernetti/AFP/Getty Images) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:12 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:19 编辑


                               
登录/注册后可看大图
19
In this image released April 25, 2011, taken atop Cerro Paranal, the 2,600-meter-high mountain in Chile's Atacama Desert, home to the VLT, the atmospheric conditions are so exceptional that fleeting events such as the "green flash" of the setting Sun are seen relatively frequently. ESO Electronics Engineer Gerhard Hudeepohl captured an even rarer sight: a green flash from the Moon, instead of the Sun. (Reuters/ESO/G.Huedepohl) #


                               
登录/注册后可看大图
20
The 8.2m diameter main mirror of Antu, the first Unit Telescope of ESO's Very Large Telescope, is cleaned using carbon dioxide snow. While the telescope enclosure is maintained extremely clean, the mirrors are exposed to the elements during the observations. Consequently, dust from the desert slowly accumulates over the surface of the mirror, making it less reflective over time. The mirror's surface is so delicate that normal cleaners used for household mirrors are not appropriate. Observatories have developed other methods, such as this one using carbon dioxide snow. The tiny CO2 snowflakes in the white plume have a temperature of minus 80 degrees Celsius; when they land on the mirror, which is at room temperature, they cause minuscule 'explosions' that detach the dust grains from the surface. The dust then floats away, leaving the mirror clean. (ESO/Y. Beletsky) #


                               
登录/注册后可看大图
21
The dynamism of ESO's Very Large Telescope in operation is wonderfully encapsulated in this unusual photograph, taken just after sunset at the moment Unit Telescope 1 starts work. An extended exposure time of 26 seconds has allowed ESO Photo Ambassador Gerhard Huedepohl to record the movement of the dome, looking out through the opening from within, as the system swings into action. The rotating walls of the dome look like an ethereal swirl through which a slice of the Atacama Desert can be glimpsed, while the crisp dusk sky provides a splash of cool blue. (ESO/Gerhard Huedepohl) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:13 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:20 编辑


                               
登录/注册后可看大图
22
Color composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy's central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870-micron submillimeter data, from LABOCA on APEX, are shown in orange. X-ray data from the Chandra X-ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the stars and the galaxy's characteristic dust lane in close to "true colour". (ESO/WFI, Optical; MPIfR/ESO/APEX/A.Weiss et al., Submillimeter; NASA/CXC/CfA/R.Kraft et al., X-ray) #


                               
登录/注册后可看大图
23
Observations using the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed an unexpected spiral structure in the material around the old star R Sculptoris. This feature has never been seen before and is probably caused by a hidden companion star orbiting the star. This slice through the new ALMA data reveals the shell around the star, which shows up as the outer circular ring, as well as a very clear spiral structure in the inner material. (ALMA/ESO/NAOJ/NRAO/M. Maercker) #


                               
登录/注册后可看大图
24
A color composite of visible and near-infrared images of the dark cloud Barnard 68. It was obtained with the 8.2-m VLT ANTU telescope and the multimode FORS1 instrument in March 1999. At these wavelengths, the small cloud is completely opaque because of the obscuring effect of dust particles in its interior. (ESO) #


                               
登录/注册后可看大图

25
The barren Atacama Desert in northern Chile, with part of the ESO's VLT observatory visible. The four 8.2-meter Unit Telescopes stand out to the right on the summit of Mount Paranal. To the left looms the 4.1-meter Visible and Infrared Survey Telescope for Astronomy (VISTA), the largest survey telescope in operation. (ESO/G.Huedepohl) #
回复 顶~ 砸~

使用道具 举报

 楼主| 人与自然 发表于 2013-1-24 14:15 | 显示全部楼层 来自: 中国–广东–中山 电信
本帖最后由 人与自然 于 2013-1-24 15:21 编辑


                               
登录/注册后可看大图
26
High in the Chilean Andes, at 5,000 metres above sea level, one of the giant Atacama Large Millimeter/submillimeter Array (ALMA) antenna transporters contemplates an unexpected sight -- a delicate dusting of snow whitens the landscape of the Chajnantor plateau. Snow is a very rare event at this extremely arid site and is a consequence of the Altiplanic winter, caused when the jet stream reverses and comes from the chill east. Chajnantor is one of the driest sites in the world, making it excellent for astronomical observations. The hill in the background is Toco, a 5600-meter mountain toward the north. This image was taken on 30 April 2010. The ALMA transporters, two giant custom-built vehicles, can move the antennas across the Chajnantor plateau, allowing different configurations of the array. (ESO/NAOJ/NRAO) #


                               
登录/注册后可看大图
27
Star trails over the ESO 3.6-meter Telescope, which hosts HARPS, the High Accuracy Radial velocity Planet Searcher, the world's foremost exoplanet hunter. (ESO/A.Santerne) #


                               
登录/注册后可看大图
28
This VISTA image shows the spectacular 30 Doradus star-forming region, also called the Tarantula Nebula. At its core is a large cluster of stars known as R 136, in which some of the most massive stars known are located. This infrared image, made with ESO's VISTA survey telescope. (ESO/M.-R. Cioni/VISTA Magellanic Cloud survey)


                               
登录/注册后可看大图
29
The NGC 1365 galaxy, also known as the Great Barred Spiral Galaxy, in an image that combines observations performed through three different filters with the 1.5-meter Danish telescope at the European Southern Observatory (ESO) in Chile, on September 22, 2010. The galaxy, at 60 million light-years from Earth, 200,000 light-years across and about twice the size of the Milky Way, is one of the largest known to astronomers. (Reuters/ESO/IDA/Danish 1.5 m/ R. Gendler, J-E. Ovaldsen, C. Thsne, and C. Feron) #


                               
登录/注册后可看大图
30
Work takes place on one of the ESO's 12-meter radio telescopes in the Atacama desert. (AP Photo) #


                               
登录/注册后可看大图
31
As soon as the Sun sets over the Chilean Atacama Desert, ESO's VLT begins catching light from the far reaches of the Universe. The VLT has four 8.2-meter Unit Telescopes such as the one shown in the photograph. Many of the photons that are collected have traveled through space for billions of years before reaching the telescope's primary mirror. The giant mirror acts like a high-tech "light bucket", gathering as many photons as possible and sending them to sensitive detectors. Careful analysis of the data from these instruments allows astronomers to unravel the mysteries of the cosmos. (ESO/Jose Francisco Salgado)
回复 顶~ 砸~

使用道具 举报

无毒 发表于 2013-1-24 14:16 | 显示全部楼层 来自: 中国–浙江–金华 电信
提示: 该帖被管理员或版主屏蔽
回复 顶~ 砸~

使用道具 举报

星星猎手 发表于 2013-1-24 14:45 | 显示全部楼层 来自: 中国–辽宁–葫芦岛 联通
提示: 该帖被管理员或版主屏蔽
回复 顶~ 砸~

使用道具 举报

whw5555 发表于 2013-1-24 14:52 | 显示全部楼层 来自: 中国–北京–北京 联通
提示: 该帖被管理员或版主屏蔽
回复 顶~ 砸~

使用道具 举报

君临天下 发表于 2013-1-24 15:08 | 显示全部楼层 来自: 中国–黑龙江–哈尔滨 联通
真壮观!中国的科研和教育经费都在government的接待费中喝到畜生肚子了!

点评

☭的政策好啊 。乌拉。无啦  详情 回复 发表于 2013-1-24 20:57
多捞多得的基本国厕不改,脚踏实地的科学精神永远不会亲近我们  发表于 2013-1-24 16:52
回复 顶~ 砸~

使用道具 举报

无毒 发表于 2013-1-24 16:19 | 显示全部楼层 来自: 中国–浙江–金华 电信
无毒 发表于 2013-1-24 14:16
**** 该帖被屏蔽 ****

我还跟着你一起水  结果屏蔽了 额
回复 顶~ 砸~

使用道具 举报

adamdyj 发表于 2013-1-24 16:19 | 显示全部楼层 来自: 中国–陕西–西安 联通
壮观!那道激光漂亮

点评

用于抵消大气扰动的,不过只用一个激光源的效果很有限。 新一代的AO已经采用多轭技术了,ESO这次动作不够快。  详情 回复 发表于 2013-1-24 20:20
那个貌似是金星  详情 回复 发表于 2013-1-24 17:51
回复 顶~ 砸~

使用道具 举报

feb22 发表于 2013-1-24 16:24 | 显示全部楼层 来自: 中国–上海–上海–青浦区 电信
漂亮啊!马头的细节……
回复 顶~ 砸~

使用道具 举报

danming 发表于 2013-1-24 16:34 | 显示全部楼层 来自: 中国–山西–忻州 联通
提示: 作者被禁止或删除 内容自动屏蔽
回复 顶~ 砸~

使用道具 举报

晒月亮的老花猫 发表于 2013-1-24 17:02 | 显示全部楼层 来自: 中国–安徽–合肥 电信
中国对这方面是不是受限制啊!
回复 顶~ 砸~

使用道具 举报

vwuvwu 发表于 2013-1-24 17:36 | 显示全部楼层 来自: 中国–广东–广州 电信
高端器材出猛片啊
回复 顶~ 砸~

使用道具 举报

本版积分规则

APP下載|手机版|爱牧夫天文淘宝店|牧夫天文网 ( 公安备案号21021102000967 )|网站地图|辽ICP备19018387号

GMT+8, 2024-11-22 00:36 , Processed in 0.196775 second(s), 26 queries , Gzip On, Redis On.

Powered by Discuz! X3.5 Licensed

Copyright © 2001-2020, Tencent Cloud.

快速回复 返回顶部 返回列表