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哈勃090507:精确测定哈勃常数——逼近暗能量的实质

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 楼主| gohomeman1 发表于 2009-5-10 00:18 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-12-18 20:11 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/

May 25, 1999  11:00 AM (EDT)
News Release Number: STScI-1999-19

太空望远镜科研所1999年第19#新闻公报,美国东部时间1999.5.25 11:00公布。
Hubble Completes Eight-Year Effort to Measure Expanding Universe
哈勃持续8年的测量宇宙膨胀工程完工


                               
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May 25, 1999: The Hubble Space Telescope Key Project team today announced that it has completed efforts to measure precise distances to far-flung galaxies, an essential ingredient needed to determine the age, size and fate of the universe.
1999.5.25:哈勃太空望远镜重点项目团队今天宣布,他们已经完成了精确测量宇宙中广泛分布的星系距离工作,这是确定宇宙大小、年龄以及未来命运必不可少的一步。
The team used the Hubble telescope to observe 19 galaxies out to 108 million light-years. They discovered almost 800 Cepheid variable stars, a special class of pulsating star used for accurate distance measurements. Here is a picture of one of those galaxies. It is the spiral galaxy NGC 4603, the most distant galaxy in which Cepheid variables have been found. It is associated with the Centaurus cluster, one of the most massive assemblages of galaxies in the nearby universe.
团队用哈勃太空望远镜观测了最远达1.08亿光年的19个星系,发现了大约800个造父变星,一类用于精确测定距离的脉动变星。本图是其中一个星系:漩涡星系NGC 4603,本报告中发现造父变星的最远星系。它属于人马座星系团,后者是我们附近宇宙中最大质量的星系团组合之一。
PS:10年前文章,某些观点已经过时在所难免,我翻译时将首先保证“信”,对于明显错误的观点,会在段落中或后边单独说明。——gohomeman1
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 楼主| gohomeman1 发表于 2009-5-10 01:05 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2011-3-22 00:20 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/a/

Image: Distant Spiral Galaxy NGC 4603, Home to Variable Stars
拼接图:遥远的涡旋星系 NGC 4603,造父变星の家



                               
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ABOUT THIS IMAGE:
A NASA Hubble Space Telescope (HST) view of the magnificent spiral galaxy NGC 4603, the most distant galaxy in which a special class of pulsating stars called Cepheid variables have been found. It is associated with the Centaurus cluster, one of the most massive assemblages of galaxies in the nearby universe. The Local Group of galaxies, of which the Milky Way is a member, is moving in the direction of Centaurus at a speed of more than a million miles an hour under the influence of the gravitational pull of the matter in that direction.
哈勃太空望远镜(HST)拍摄的壮丽的漩涡星系NGC 4603,现今发现一类特殊的变星——造父变星的最远的星系。它属于半人马座星系团,后者是我们附近宇宙中最大质量的星系团组合之一。我们银河系所在的本星系群,受半人马座(星系团)方向物质的引力吸引,正以超过百万英里的时速朝半人马座狂奔。
Clusters of young bright blue stars highlight the galaxy's spiral arms. In contrast, red giant stars in the process of dying are also found. Only the very brightest stars in NGC 4603 can be seen individually, even with the unmatched ability of the Hubble Space Telescope to obtain detailed images of distant objects. Much of the diffuse glow comes from fainter stars that cannot be individually distinguished by Hubble. The reddish filaments are regions where clouds of dust obscure blue light from the stars behind them.
亮蓝巨星组成的年轻星团闪耀在星系的旋臂上,同时也发现了垂死的红巨星。由于距离太远,就算哈勃太空望远镜这般无敌的能力,也只能分辨NGC 4603中最亮的单个恒星;更多暗弱的恒星光混合在一起,无法分辨。(后来的ACS就能分辨更多恒星了——译注)泛红的细丝是尘埃云遮蔽、散射了后面巨星的蓝光造成的。
This galaxy was observed by a team affiliated with the HST Key Project on the Extragalactic Distance Scale. Because NGC 4603 is much farther away than the other galaxies studied with Hubble by the Key Project team, 108 million light-years, its stars appear very faint from the Earth, and so accurately measuring their brightness, as is required for distinguishing the characteristic variations of Cepheids, is extremely difficult. At this distance some non-variable stars may by chance appear to grow brighter and fainter in the same fashion as Cepheids due to the physical impossibility of perfect measurements of such dim objects. Determining the distance to the galaxy required an unprecedented statistical analysis based on extensive computer simulations.
星系NGC 4603由隶属于哈勃太空望远镜重大项目组的“河外星系量天尺工程”团队观测。由于它远在1.08亿光年外,远超项目组团队研究的其他星系,故此恒星变得非常黯淡,而任务要求必须正确测定其中的特定变星——造父变星——的光度,显得格外困难。在这个距离上,由于仪器的物理测量极限,测量不可能在完全理想状态下进行(比如仪器本身的热噪点),某些非变星也会显得有时亮有时暗,就如同造父变星的模式似的。确定星系的距离需要基于广泛计算机模拟的前所未有的数学统计分析(模型)。
Researchers found 36-50 Cepheids and used their observed properties to securely determine the distance to NGC 4603. These measurements indicate that when the expansion of the universe and the motion of the Local Group are accounted for, the Centaurus cluster is very nearly at rest compared with the surrounding regions. It is part of the cause of the rapid motions in the nearby universe, rather than being strongly pulled by other concentrations of matter. Observations of distant Cepheids such as those in NGC 4603 also help astronomers to precisely measure the expansion rate of the universe.
搜索者在NGC 4603内发现了36-50个造父变星,利用它们的特性安全的测定了星系距离。这些观测结果表明,在宇宙膨胀、本星系群运动期间,半人马座星系团相比其周围环境,就像几乎不动的。这部分原因是因为附近宇宙的快速膨胀,而并非受到其他物质团强大引力的作用。观测造父变星的距离也有助于天文学家准确测量宇宙膨胀速度。

Object Name: NGC 4603
对象名称:NGC 4603
Image Type: Astronomical
对象类型:天体
Credit: Jeffrey Newman (Univ. of California at Berkeley) and NASA
图片版权:美国宇航局,美国加州大学伯克利分校的杰弗里.纽曼
互相尊重,互相理解,共同提高
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 楼主| gohomeman1 发表于 2009-5-10 01:08 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2011-3-22 22:49 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/text/

Hubble Completes Eight-Year Effort to Measure Expanding Universe
The full news release story:

《哈勃持续8年的测量宇宙膨胀工程完工》新闻稿全文
The Hubble Space Telescope Key Project team today announced that it has completed efforts to measure precise distances to far-flung galaxies, a nessential ingredient needed to determine the age, size and fate of theuniverse.
哈勃太空望远镜重点项目团队今天宣布,他们已经完成了精确测量宇宙中广泛分布的星系距离工作,这是确定宇宙大小、年龄以及未来命运必不可少的一步。
"Before Hubble, astronomers could not decide if the universe was 10 billion or 20 billion years old. The size scale of the universe had a range so vast that it didn't allow astronomers to confront with any certainty many of the most basic questions about the origin and eventual fate of the cosmos," said team leader Wendy Freedman, of the Observatories of the Carnegie Institution of Washington. "After allthese years, we are finally entering an era of precision cosmology.Now we can more reliably address the broader picture of the universe'sorigin, evolution and destiny."
“哈勃太空望远镜上天前,天文学家甚至无法确定宇宙已经100亿岁还是200亿岁了。宇宙大小的变动范围是如此之大,以致于天文学家无法直面任何关于宇宙起源和未来命运的基本问题。”团队带头人、美国华盛顿卡内基研究院附属天文台的温蒂. 弗里德曼说。
The team's precise measurements are the key to learning about the expansion rate of the universe, called the Hubble constant. Measuring the Hubble constant was one of the three major goals for NASA's Hubble Space Telescope before it was launched in 1990.  
团队精确的测量值是研究宇宙膨胀速率——哈勃常数的钥匙。测定哈勃常数是哈勃天文望远镜在1990年发射前就预定的三大重要目标之一。
For the past 70 years astronomers have sought a precise measurement of the Hubble constant, ever since astronomer Edwin Hubble realized that galaxies were rushing away from each other at a rate proportional to their distance, i.e. the farther away, the faster the recession. For many years, right up until the launch of the Hubble telescope - the range of measured values for the expansion rate was from 50 to 100 kilometers per second per megaparsec (a megaparsec, or mpc, is 3.26million light-years).
70多年前的过去,埃德温.哈勃发现星系彼此远离速率与它们间的距离成正比,也就是说,距离越远,后退越快。此后多年来,天文学家持续寻求更精准的哈勃常数。但直到哈勃望远镜发射前,哈勃常数的值还在每百万秒差距50~100km/s这么大范围内(百万秒差距缩写为mpc,相当于326万光年)。

                               
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The team measured the Hubble constant at 70 km/sec/mpc, with an uncertainty of 10 percent. This means that a galaxy appears to be moving 160 thousand miles per hour faster for every 3.3 light-years away from Earth.
团队测得哈勃常数是70km/sec/mpc,不确定性约10%。这意味着离地球每隔3.3光年,星系就以16万英里以上的(平均叠加)时速退离我们。
"The truth is out there, and we will find it," said Dr. Robert Kirshner,of Harvard University. "We used to disagree by a factor of 2; now we are just as passionate about 10 percent. A factor of two is like being unsure if you have one foot or two. Ten percent is like arguing aboutone toe. It's a big step forward."
“真相就在那里,而我们将发现它,”哈佛大学罗伯特.科什纳博士说。 “过去我们常常都不能确定因子是取1还是2,现在我们的不确定性只有10%了。是1还是2就像你搞不清自己有一只脚还是两只脚一样(糊涂),而10%就像在讨论脚趾头数目这种细节了。这是一个巨大的进步。”
Adds Dr. Robert Kennicutt of the University of Arizona, a co-leader of the team: "Things are beginning to add up. The factor of two controversy is over."  
团队协同领导人、亚利桑那州大学的罗伯特.肯尼柯特博士补充说:“事情正在变得合乎情理,因子取1还是2的辩论已经结束了。”
The team used the Hubble telescope to observe 18 galaxies out to 65 million light-years. They discovered almost 800 Cepheid variable stars,a special class of pulsating star used for accurate distance measurement. Although Cepheids are rare, they provide a very reliable"standard candle" for estimating intergalactic distances. The team used the stars to calibrate many different methods for measuring distances.
团队使用哈勃太空望远镜观测了6500万光年外的18个星系。他们发现了差不多800个造父变星,一种用于准确测量距离的特殊变星。虽然造父变星数量稀少,它们是估计银河系间距离的一种非常可靠的“标准烛光”。团队使用它们校准各种不同的测距方法。
"Our results are a legacy from Hubble telescope that will be used in a variety of future research," said Dr. Jeremy Mould, of the Australian National University, also a co-leader of the team. "It's exciting to see the different methods of measuring galaxy distances converge, calibrated by the Hubble Space Telescope."
另一位团队协同领导人、澳大利亚国立大学杰里米.模特博士说:“我们的研究结论将成为哈勃遗产,在未来多种研究中有用。经哈勃太空望远镜校准,不同的测量星系距离的方法逐步汇集一点,真令人兴奋。”
Combining the Hubble constant measurement with estimates for the density of the universe, the team determined that the universe is approximately 12 billion years old - similar to the oldest stars. This discovery clears up a nagging paradox that arose from previous age estimates. The researchers emphasize that the age estimate holds true if the universeis below the so-called "critical density" where it is delicately balanced between expanding forever or collapsing. Or, the universe is pervaded by a mysterious force pushing the galaxies farther apart, in which case the Hubble measurements point to an even older universe.
结合哈勃常数和当前宇宙密度估值,团队确定宇宙大约有120亿岁了——与最老的恒星寿命一致。这个发现同时澄清了以前那些估值引起的似是而非的唠叨。研究者强调,如果宇宙刚好在“临界密度”之下,那么年龄估计有效;或者,星系被充斥宇宙各处的神秘力量推动而互相远离,那么哈勃望远镜观测结果将指向一个更古老的宇宙。所谓“临界密度”是指宇宙平均密度刚好在持续膨胀与最终收缩之间。
The universe's age is calculated using the expansion rate from precise distance measurements, and the calculated age is refined based on whether the universe appears to be accelerating or decelerating, given the amount of matter observed in space. A rapid expansion rate indicates the universe did not require as much time to reach its present size, and so it is younger than if it were expanding more slowly.
宇宙年龄的计算基于精准距离测量导出的宇宙膨胀速率,准确性同时基于根据空间物质数量观测结果——宇宙到底是在加速膨胀还是减速膨胀。一个快速膨胀的宇宙意味着宇宙不需要很多时间就能到达现在大小,自然比非常慢膨胀会更年轻。
The Hubble Space Telescope Key Project team is an international group of 27 astronomers from 13 different U.S. and international institutions.The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc. for NASA, under contract with NASA's Goddard Space Flight Center in Greenbelt, MD.
哈勃太空望远镜重点项目团队是有来自13个国家、组织的27位天文学家组成的国际团队。太空望远镜科研所由美国大学天文研究协会(AURA,向NASA负责)负责运作,并与马里兰州格林贝尔市的美国航空航天局戈达德太空飞行中心长期协作。

CONTACT
联系人
Donald Savage
唐纳德.萨维奇   (野蛮人唐老鸭叔叔?)   
NASA Headquarters, Washington, DC,
华盛顿特区 美国航空航天局总部

Phone: 202/358-1547)

Nancy Neal
南希.尼尔  
Goddard Space Flight Center, Greenbelt, MD,
马里兰州 格林贝尔市 戈达德太空飞行中心 (绿化带市?)  
Phone: 301/286-0039)

Ray Villard
雷·维兰德
Space Telescope Science Institute, Baltimore, MD,
马里兰州 巴尔的摩市 太空望远镜科研所
Phone: 410/338-4514)

PS:本文的人名、地名又比较特殊,有野蛮人Savage、有自由民(获释奴隶)Freeman,Mould虽然不是女模特的意思,但也是模具、模型的意思。至于Wendy,英文还有勇于冒险的少女之意。Donald,大家都知道唐老鸭吧。 Greenbelt,绿化隔离带。
我们现在知道,主流观点是宇宙充斥着暗能量,宇宙年龄大概137亿年,误差小于5%。
根据本文最后一句话,Space Telescope Science Institute将继续翻译为太空望远镜科学学会。——gohomeman1
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 楼主| gohomeman1 发表于 2009-5-10 01:10 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 15:42 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/b/

Image: Spiral Galaxy NGC 4603
http://imgsrc.hubblesite.org/hu/db/images/hs-1999-19-b-full_jpg.jpg

由于当年的图像技术不够发达,大家可以看到图像存在明显的拼合痕迹。

                               
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 楼主| gohomeman1 发表于 2009-5-10 01:16 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 10:19 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/c/

Image: Spiral Galaxy NGC 4603 With Location of Cepheids Marked
标注出造父变星位置的涡旋星系NGC 4603


                               
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 楼主| gohomeman1 发表于 2009-5-10 01:53 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 10:23 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/d/ ~http://hubblesite.org/newscenter/archive/releases/1999/19/image/g/

NGC 4603中的造父变星1~4的放大图
Cepheid 1 NGC 4603

                               
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Cepheid 2 NGC 4603

                               
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Cepheid 3 NGC 4603

                               
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Cepheid 4 NGC 4603

                               
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 楼主| gohomeman1 发表于 2009-5-10 01:55 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 10:28 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/h/

Image: Ground-Based Image of Supernova 1994D in Galaxy NGC 4526
图:地面望远镜拍摄的超新星1994D和宿主星系NGC 4526

                               
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Object Names: Supernova 1994D, NGC 4526
对象名称:NGC 4526,超新星1994D
Image Type: Astronomical
对象类型:天体
Credit: NASA, ESA and the Hubble Key Project Team
图片版权:美国宇航局,欧洲航天局,哈勃太空望远镜重大项目团队
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 楼主| gohomeman1 发表于 2009-5-10 01:58 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 11:27 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/i/

Image: Supernova 1994D in Galaxy NGC 4526
爆发于NGC 4526星系的超新星1994D
http://imgsrc.hubblesite.org/hu/db/images/hs-1999-19-i-full_tif.tif


                               
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Object Names: Supernova 1994D, NGC 4526
对象名称:NGC 4526,超新星1994D
Image Type: Astronomical
对象类型:天体
Credit: NASA, ESA, The Hubble Key Project Team, and The High-Z Supernova Search Team
图片版权:美国宇航局,欧洲航天局,哈勃太空望远镜重大项目团队,高红移超新星搜索团队

PS:这是WFPC2的图像,21世纪初的地面望远镜也能达到如此清晰度了。但比起WFC3和ACS来,还是比不过的。——gohomeman1
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 楼主| gohomeman1 发表于 2009-5-10 02:01 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 15:40 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/j/

Image: Hubble Diagram for Cepheids
哈勃图解造父变星

                               
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ABOUT THIS IMAGE:
This is a plot of galaxy distance versus the velocity that the galaxy appears to be receding from Earth. It is based on data collected by the Hubble Space Telescope Key Project team. The distances have been measured using Cepheid variables. The slope in the plot measures the expansion rate of the universe, a quantity called the Hubble constant. The best fit to the data yields a Hubble constant of 70 kilometers/second/megaparsec. The dashed lines indicate Hubble constant values of 77 and 63 and do not fit the data as well. This plot is analogous to that obtained by Carnegie astronomer Edwin Hubble that led to his discovery of the expansion of the universe. With the Hubble Space Telescope, it is now possible to measure Cepheid distances over 30 times farther away than Hubble was able to do.
本图表示意星系的退行速度与离地球距离的关系,它由哈勃太空望远镜重大项目团队收集的数据汇总而成。星系的距离由造父变星测定。根据测量值拟合的斜率表示宇宙的膨胀速率,一个称为哈勃常数的量。得出的最佳拟合值是70km/s/Mpc。虚线对应的哈勃常数分别是77、63,不是最佳值。这与当年埃德温.哈勃发现宇宙膨胀时测得的值类似。使用哈勃太空望远镜后,现在我们能够观测比埃德温.哈勃当年观测远30倍的造父变星。

Image Type: Illustration
对象类型:图解
Credit: NASA, ESA and STScI
图片版权:美国宇航局,欧洲航天局,太空望远镜科学研究所

PS:本段其实是这个发现的关键段,但是其中一句话明显不对吧。当年哈勃测得的数值大多了,导致宇宙只有20~30亿岁的推论。——gohomeman1
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 楼主| gohomeman1 发表于 2009-5-10 02:04 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 15:22 编辑

http://hubblesite.org/newscenter/archive/releases/1999/19/image/k/

Image: Possible Models of the Expanding Universe
图解:膨胀宇宙的几种可能的模型

                               
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Image Type: Illustration
对象类型:图解
Credit: NASA, ESA and STScI
图片版权:美国宇航局,欧洲航天局,太空望远镜科学研究所

PS:本图很好理解,看图就知道了,文字就不翻译了。最近的观测趋向于后两种。——gohomeman1
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 楼主| gohomeman1 发表于 2009-5-10 02:05 | 显示全部楼层 来自: 中国–浙江–宁波 电信
http://hubblesite.org/newscenter/archive/releases/1999/19/fastfacts/

Technical facts about this news release:
  
About the Object      
Object Name:NGC 4603
Object Description:Spiral Galaxy
Position (J2000):R.A. 12h 40m 55.70s
Dec. -40° 58' 34.0"
Constellation:Centaurus
Distance:108 million light-years (33 million parsecs)
   
About the Data      
Instrument:WFPC2
Exposure Date(s):May - July, 1996; June - July, 1997
   
About the Image      
Image Credit:NASA and J. Newman (UC Berkeley)
Release Date:May 25, 1999
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 楼主| gohomeman1 发表于 2009-5-10 02:07 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2010-1-11 23:43 编辑

Technical facts about this news release:
本报告相关科学事实

About the Object  研究对象
Object Name:   NGC 4603
对象名称:NGC 4603
Object Description:   Spiral Galaxy
对象类型:漩涡星系
Position (J2000): R.A. 12h 40m 55.70s    Dec.  -40° 58' 34.0"
坐标(儒略纪元2000星历表): 赤经 12时40分55.70秒,赤纬 -40°58′34.0″
Constellation:  Centaurus
星座:人马座
Distance:   108 million light-years (33 megaparsecs)
距离:1.08亿光年(0.33亿秒差距)

About the Data   数据来源
Instrument:  WFPC2
仪器:宽视野行星相机2#  WFPC2
Exposure Date(s):May - July, 1996; June - July, 1997
拍摄时间:分别是 1996.5~1996.7,1997.6~1997.7

About the Image  关于本图               
Image Credit:    NASA and J. Newman (UC Berkeley)
图片版权:美国宇航局,美国加州大学伯克利分校的J.纽曼
Release Date:   May 25, 1999
报告发表时间:1999.05.25
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 楼主| gohomeman1 发表于 2009-5-10 02:14 | 显示全部楼层 来自: 中国–浙江–宁波 电信
本帖最后由 gohomeman1 于 2009-5-10 02:45 编辑

1999.5.25文章所附的几段视频
http://hubblesite.org/newscenter/archive/releases/1999/19/video/a/

Video: SSU Webcast: Hubble's Yardstick of the Universe
视频:宇宙学知识更新网上直播——哈勃望远镜测定宇宙的新尺码
http://imgsrc.hubblesite.org/hu/db/videos/hs-1999-19-a-low_real.ram

What is a Space Science Update?
什么是宇宙学知识更新SSU?
Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update(SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media.
NASA TV节目——哈勃望远镜的重大发现:天文学家在召开新闻发布会讲解哈勃望远镜的发现并在美国航空航天局电视台播出,谓之SSU。SSU节目还包括媒体记者问答时间。
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 楼主| gohomeman1 发表于 2009-5-10 02:34 | 显示全部楼层 来自: 中国–浙江–宁波 电信
我使用IE8的时间比较少,但某些网页错误,不用IE还难于纠正。今天用IE8一看才发现,在Firefox中显示大小舒服的网页文字,在IE8中却小了一号。不知道大家看了感觉如何,我明天用IE7和其他浏览器看看显示效果如何,如果也是小1号的,还是取消font=2的设置吧。
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幽哎浮欧 发表于 2009-5-10 15:14 | 显示全部楼层 来自: 中国–四川–达州 电信
话说,暗物质是看不到的吧
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 楼主| gohomeman1 发表于 2009-5-10 16:13 | 显示全部楼层 来自: 中国–浙江–宁波 电信
话说,暗物质是看不到的吧
幽哎浮欧 发表于 2009-5-10 15:14


是啊,看不到的,但通过引力透镜、物质团聚等现象可以探测到。现在能探测到暗物质的唯一手段就是它们的各种引力效应,而暗能量更搞不清,是为了解释宇宙膨胀而人为设置的,因为最近10几年的观测表明宇宙在加速膨胀,这是无法用惯性解释的。
不过,本文开头的那段我倒是认为是个思路,如果只是整个可见宇宙的一部分在加速膨胀,那么还好理解些。
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zhl91 发表于 2009-5-10 17:07 | 显示全部楼层 来自: 中国–福建–福州–鼓楼区 有线通
好文章啊,谢谢LZ的分享
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 楼主| gohomeman1 发表于 2009-5-10 22:29 | 显示全部楼层 来自: 中国–浙江–宁波 电信
终于全文完成,从本文尤其是第2页内容看,哈勃望远镜确实对当代天文学做出了杰出贡献。
2天后哈勃维修任务就开始了,希望哈勃望远镜整修后能够继续带来全新的科学发现!
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SamuelHan 发表于 2009-6-20 23:02 | 显示全部楼层 来自: 中国–广东–珠海 联通
不错不错,谢谢!
如果能把他们之前那八年以来的公布也翻出来就好了。
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 楼主| gohomeman1 发表于 2009-6-20 23:46 | 显示全部楼层 来自: 中国–浙江–宁波 电信
实在太多了,我没时间也没精力一个个去翻译,其实许多我也不知道,所以才有人家问哈勃是否拍过月球,我还说应该没人去申请使用哈勃望远镜拍摄月球的。事实是,官网中就公布了2次拍摄图像。
还有些哈勃拍摄的照片公布在APOD中或其他地方。
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