音速黑暗神秘人的个人资料

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自制插件:大陵五(Algol)三合星化插件完全自制(数据来自维基百科)地址(rar zip):http:防删//pan.防删baidu.防删com/防删share/防删link?防删shareid=防删194633&防删uk=防删2165273030防删

(求助)谁能给我做一个超级木星(仙女座卡帕星b)行星纹理超级木星 NASA在仙女座(Andromeda)卡帕(Kappa)星用拍摄法发现了一颗质量大约是木星的12.8倍的行星,在行星和棕矮星的质量分界附近科学家决定称为超级木星. NASA的原图我自己弄了一个,觉得不好求高人制作或找到一个纹理

Gliese 667 cc GJ 667 c是一颗环绕三合星GJ 667中的最小的红矮星Gliese 667 C的适居星球地址http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D109241%26uk%3D2165273030&urlrefer=40110bd17a6d695e8a92006e40dbfd3e @LBV_1806_20 @甘渊 @卩Ghost @happy杀猪6 @楚留香宋甜儿 @小松鼠前辈 @4070011265 @路易九十 @litian

NGC 4349 127系统系统由一个红巨星和一个褐矮星构成距离地球6500光年从地球上看位於NGC 4349附近 http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D108353%26uk%3D2165273030&urlrefer=0d08332f31ccbc50ed706eaa21dca7f7

(自制插件)半人马座阿尔法星Bb

半人马座阿尔法星B发现类地行星! Alpha Centauri Bb is an extrasolar planet orbiting the K-type star Alpha Centauri B approximately 4.37 lightyears away in the southern constellation of Centaurus . On 16 October 2012, a team of European astronomers announced that an Earth-mass planet was detected in orbit around Alpha Centauri B using theradial velocity technique with HARPS at La Silla Observatory , Chile. Over three years of observations were needed for the difficult analysis. The planet is not in the habitable zone, orbiting very close to the host star at just 0.04 AU and completing one orbit every 3.236 days. Subject to uncertainties in Alpha Centauri Bb'salbedo and the likely thickness of its atmosphere, its surface temperature is at least 1500 K , far too hot for liquid water and also above the melting temperatures of many silicate magmas . For comparison, the surface temperature of Venus , the hottest in the solar system , is 735 K. 资料来源:英文维基百科

NGC 4349-127系统

海王星环插件

(求助)怎麼弄celestia恒星数据的赤经和赤纬? rt

(自制插件)C/1996 B2 百武彗星效果图从地球上看经过近日点(从太空中看)扩大插件格式(SSC,STC) 压缩文件格式 (RAR,ZIP) rar文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D61349%26uk%3D2165273030&urlrefer=a226d631544d0a9da7c46cdd74878bc3 zip文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D61350%26uk%3D2165273030&urlrefer=3d6f68d4cc551d1f18ec54cedac3f9c2

NASA正在直播阿姆斯特朗追悼会 http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fwww.nasa.gov%2Fexternalflash%2Farmstrong_memorial%2Findex.html&urlrefer=7180eff2ee1453ecf7904fbeb559914b

celestia直径最大恒星问题看图The Garnet Star的大小有VY CMa(大犬座VY)的近2倍

Algol大陵五三合星化插件 rar文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D25805%26uk%3D2165273030&urlrefer=e27466d4c8a1b410cc8cedd693ed763c zip文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D25804%26uk%3D2165273030&urlrefer=d4485ab58038e951458057dfff68a6a2

(自制插件)Algol(大陵五)三合星化插件 rar文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D25796%26uk%3D2165273030&urlrefer=f2bbe14a0a72df164f101ff57b8eb6c4 zip文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D25797%26uk%3D2165273030&urlrefer=310412d95508eb61b5ae52ed74393f59

(自制插件)北极星三合星化插件 rar文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D25465%26uk%3D2165273030&urlrefer=1a0f8366f1115550a9896fbb3292bbdc zip文件下载地址:http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D25466%26uk%3D2165273030&urlrefer=b010f34140ae903d3b9a97ccd3666fb2 轨道数据来自维基百科

改造插件船底座伊塔星船底座伊塔星(η Car)三合星化插件(我按维基资料修改了celestia插件官网上的船底座伊塔星插件改成了LBV主星高离心率O超巨星伴星和绕O星伴星的沃夫-拉叶星) 插件效果图星系整体图扩大B和C的部份加上1843年观测到的小爆炸时喷出的气体下载地址 zip文件下载地址 http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D9226%26uk%3D2165273030&urlrefer=5f70e8b929e1109c1bdfd214e0a44e26 rar文件下载地址 http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fpan.baidu.com%2Fshare%2Flink%3Fshareid%3D9227%26uk%3D2165273030&urlrefer=c5895af84cf51ed3eaf32b0785a29e33 (注意:删除原来恒星插件在安装插件不用删星云插件)

(新闻)Dawn号探测器准备前往1号小行星(矮行星)Ceres NASA's Dawn Prepares for Trek Toward Dwarf Planet08.30.12 A simulated flyover of the most intriguing landmarks on giant asteroid Vesta, as seen by NASA's Dawn spacecraft. › Download video http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fwww.nasa.gov%2Fmultimedia%2Fvideogallery%2Findex.html%3Fmedia_id%3D151381721&urlrefer=5f39139897672122bd39f02212c20e53This image of NASA's Dawn spacecraft and the giant asteroid Vesta is an artist's concept. Dawn arrived at Vesta on July 15, 2011 PDT (July 16, 2011 EDT) and is set to depart on Sept. 4, 2012 PDT (Sept. 5, 2012 EDT). Image credit: NASA/JPL-Caltech › Larger view PASADENA, Calif. – NASA's Dawn spacecraft is on track to become the first probe to orbit and study two distant solar system destinations, to help scientists answer questions about the formation of our solar system. The spacecraft is scheduled to leave the giant asteroid Vesta on Sept. 4 PDT (Sept. 5 EDT) to start its two-and-a-half-year journey to the dwarf planet Ceres. Dawn began its 3-billion-mile (5-billion kilometer) odyssey to explore the two most massive objects in the main asteroid belt in 2007. Dawn arrived at Vesta in July 2011 and will reach Ceres in early 2015. Dawn's targets represent two icons of the asteroid belt that have been witness to much of our solar system's history. To make its escape from Vesta, the spacecraft will spiral away as gently as it arrived, using a special, hyper-efficient system called ion propulsion. Dawn's ion propulsion system uses electricity to ionize xenon to generate thrust. The 12-inch-wide ion thrusters provide less power than conventional engines, but can maintain thrust for months at a time. "Thrust is engaged, and we are now climbing away from Vesta atop a blue-green pillar of xenon ions," said Marc Rayman, Dawn's chief engineer and mission director, at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "We are feeling somewhat wistful about concluding a fantastically productive and exciting exploration of Vesta, but now have our sights set on dwarf planet Ceres. Dawn's orbit provided close-up views of Vesta, revealing unprecedented detail about the giant asteroid. The mission revealed that Vesta completely melted in the past, forming a layered body with an iron core. The spacecraft also revealed the scarring from titanic collisions Vesta suffered in its southern hemisphere, surviving not one but two colossal impacts in the last two billion years. Without Dawn, scientists would not have known about the dramatic troughs sculpted around Vesta, which are ripples from the two south polar impacts. "We went to Vesta to fill in the blanks of our knowledge about the early history of our solar system," said Christopher Russell, Dawn's principal investigator, based at the University of California Los Angeles (UCLA). "Dawn has filled in those pages, and more, revealing to us how special Vesta is as a survivor from the earliest days of the solar system. We can now say with certainty that Vesta resembles a small planet more closely than a typical asteroid." The mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory in Pasadena, Calif., for the agency's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, which is managed by NASA's Marshall Space Flight Center in Huntsville, Ala. UCLA is responsible for the overall Dawn mission science. Orbital Sciences Corp. of Dulles, Va., designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are part of the mission's team. The California Institute of Technology in Pasadena manages JPL for NASA. For more information about Dawn, visit: http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fwww.nasa.gov%2Fdawn&urlrefer=5ac8c77d36c2b6541e54194476472740 and http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fdawn.jpl.nasa.gov&urlrefer=e040d8a9b36e2fb6957dd5cde8998ba7 . Jia-Rui Cook 818-354-0850 Jet Propulsion Laboratory, Pasadena, Calif. [email protected] Dwayne Brown 202-358-1726 NASA Headquarters, Washington [email protected] 2012-271

(新闻)Dawn号准备开始前往1号小行星(矮行星)Ceres NASA's Dawn Prepares for Trek Toward Dwarf Planet 08.30.12 A simulated flyover of the most intriguing landmarks on giant asteroid Vesta, as seen by NASA's Dawn spacecraft. › Download video http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fwww.nasa.gov%2Fmultimedia%2Fvideogallery%2Findex.html%3Fmedia_id%3D151381721&urlrefer=5f39139897672122bd39f02212c20e53This image of NASA's Dawn spacecraft and the giant asteroid Vesta is an artist's concept. Dawn arrived at Vesta on July 15, 2011 PDT (July 16, 2011 EDT) and is set to depart on Sept. 4, 2012 PDT (Sept. 5, 2012 EDT). Image credit: NASA/JPL-Caltech › Larger view PASADENA, Calif. – NASA's Dawn spacecraft is on track to become the first probe to orbit and study two distant solar system destinations, to help scientists answer questions about the formation of our solar system. The spacecraft is scheduled to leave the giant asteroid Vesta on Sept. 4 PDT (Sept. 5 EDT) to start its two-and-a-half-year journey to the dwarf planet Ceres. Dawn began its 3-billion-mile (5-billion kilometer) odyssey to explore the two most massive objects in the main asteroid belt in 2007. Dawn arrived at Vesta in July 2011 and will reach Ceres in early 2015. Dawn's targets represent two icons of the asteroid belt that have been witness to much of our solar system's history. To make its escape from Vesta, the spacecraft will spiral away as gently as it arrived, using a special, hyper-efficient system called ion propulsion. Dawn's ion propulsion system uses electricity to ionize xenon to generate thrust. The 12-inch-wide ion thrusters provide less power than conventional engines, but can maintain thrust for months at a time. "Thrust is engaged, and we are now climbing away from Vesta atop a blue-green pillar of xenon ions," said Marc Rayman, Dawn's chief engineer and mission director, at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "We are feeling somewhat wistful about concluding a fantastically productive and exciting exploration of Vesta, but now have our sights set on dwarf planet Ceres. Dawn's orbit provided close-up views of Vesta, revealing unprecedented detail about the giant asteroid. The mission revealed that Vesta completely melted in the past, forming a layered body with an iron core. The spacecraft also revealed the scarring from titanic collisions Vesta suffered in its southern hemisphere, surviving not one but two colossal impacts in the last two billion years. Without Dawn, scientists would not have known about the dramatic troughs sculpted around Vesta, which are ripples from the two south polar impacts. "We went to Vesta to fill in the blanks of our knowledge about the early history of our solar system," said Christopher Russell, Dawn's principal investigator, based at the University of California Los Angeles (UCLA). "Dawn has filled in those pages, and more, revealing to us how special Vesta is as a survivor from the earliest days of the solar system. We can now say with certainty that Vesta resembles a small planet more closely than a typical asteroid." The mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory in Pasadena, Calif., for the agency's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, which is managed by NASA's Marshall Space Flight Center in Huntsville, Ala. UCLA is responsible for the overall Dawn mission science. Orbital Sciences Corp. of Dulles, Va., designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are part of the mission's team. The California Institute of Technology in Pasadena manages JPL for NASA. For more information about Dawn, visit: http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fwww.nasa.gov%2Fdawn&urlrefer=5ac8c77d36c2b6541e54194476472740 and http://tieba.baidu.com/mo/q/checkurl?url=http%3A%2F%2Fdawn.jpl.nasa.gov&urlrefer=e040d8a9b36e2fb6957dd5cde8998ba7 . Jia-Rui Cook 818-354-0850 Jet Propulsion Laboratory, Pasadena, Calif. [email protected] Dwayne Brown 202-358-1726 NASA Headquarters, Washington [email protected] 2012-271

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瞎打

谁帮我检查一下我朋友这个出错的三合星系统 Barycenter "Kostania Stars"{RA288.9214Dec47.8725Distance711.1166} Barycenter "Kostania Media And Kostania Borealis" { OrbitBarycenter "Kostania Stars" EllipticalOrbit { Period 16234.9785 SemiMajorAxis 6618.1558757# Combined mass Kostania Australis = 1.89 x Sol,Kostania Media-Kostania Borealis Combined Mass = 8.34 x Sol Eccentricity 0.001362 Inclination 100 AscendingNode 56.072 ArgOfPericenter 213.139 MeanAnomaly 0 } "Kostania Australis"{ OrbitBarycenter "Kostania Stars"SpectralType"B1V"Radius5312402 AppMag3.922 EllipticalOrbit { Period 16234.9785 SemiMajorAxis 1499.7979143 Eccentricity 0.001362 Inclination 100 AscendingNode 56.072 ArgOfPericenter 213.139 MeanAnomaly 0 } } "Kostania Media"{ OrbitBarycenter "Kostania Media And Kostania Borealis" SpectralType "G2V" Radius689754.8743 AppMag 11.542 EllipticalOrbit { Period 853.2342 SemiMajorAxis 89.8989 Eccentricity 0.0009 Inclination 100 AscendingNode 56.072 ArgOfPericenter 213.139 MeanAnomaly 0 }} "Kostania Borealis"{ OrbitBarycenter "Kostania Media And Kostania Borealis" SpectralType "K1V" Radius689754.8743 AppMag 12.524 EllipticalOrbit { Period 853.2342 SemiMajorAxis 99.9999 Eccentricity 0.0009 Inclination 100 AscendingNode 56.072 ArgOfPericenter 213.139 MeanAnomaly 0 }}

匿名功能被禁止了

你认为哪颗恒星最出名格式(不知道相应数据打问号) 恒星名称恒星光谱视星等绝对星等自转周期年龄直径(太阳为1) 质量(太阳为1) 亮度(太阳为1) 赤经赤纬距离表面温度认为最出名原因

目前已知最大的小行星(包括矮行星)是什么(有争议)

太阳系的矮行星从大到小 1 Eris(阋神星) 2 Pluto(冥王星) 3 Haumea(任神星) 4 Makemake(鸟神星) 5 Ceres(谷神星) (冥王星有可能比阋神星大,鸟神星有可能比任神星打大) (冥王星和阋神星的直径估计值都是2320KM左右)

哪种光谱类型的恒星(不包括棕矮星)在所有恒星中占的比例最大?

宇宙中百分之多少的恒星是联星系统中的一员?

大家从哪个台看Discovery节目

你认为除了太阳(目前)离地球最近的恒星/褐矮星是什麽?

你认为哪颗行星或卫星最有可能存在外星生物?

大家哪个Discovery节目