[小说文学] 短篇小说集：坐窗观风景[第405页]

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[小说文学]短篇小说集：坐窗观风景[第405页]

作者:San若梦

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    【The Great Galaxy of the Andromeda Constellation, Galaxy M31 is the brightest and the largest galaxy of the northern sky. You can see it take the shape of a mist surrounded by stars even with the naked eye in suburban skies. Under a dark sky, it can’t be missed, even if you’re just accidentally “scanning” the Andromeda Constellation. When you get hold of a large telescope it becomes picturesque. Its view takes a breath away, especially once you realize what you’re looking at. The photographs took about 20 hours of total exposure. Photons were collected through several nights in the artist's private observatory. The quality of this photography makes it one of the best of this type in the world. Photo resolution exceeds 65 mpix. Artist: Adam Jesionkiewicz (Founder of Astrography)】—摘自ASTROGRAPHY

    【仙女座星系（Andromeda Galaxy，M31和NGC 224）是一个螺旋星系，距离地球大约250万光年，是除麦哲伦云（地球所在的银河系的伴星系）以外最近的星系。位于仙女座的方向上，是人类肉眼可见（3.4等星）最远的深空天体。仙女座星系在适度黑暗的天空环境下很容易用肉眼看见，但是肉眼看见的仙女座星系非常小，因为它只有中心一小块的区域有足够的亮度，但是这个星系完整的角直径有满月的七倍大。】

    【Stephan’s Quintet is a group consisting of four interacting galaxies – NGC 7317, NGC 7318A, NGC 7318B and NGC 7319 – and a visual companion, the spiral galaxy NGC 7320. The galaxies are located in Pegasus constellation. The four interacting galaxies are members of the first compact galaxy group ever discovered, the Hickson Compact Group 92. Compact groups are typically groups of about five galaxies in close proximity and isolated from other galaxies.】—摘自网络

    【史蒂芬五重星系是由五个视觉可见的星系组成的星系群，其中四个形成一个致密星系群。这个群位于飞马座，是爱德华·史提芬于1877年在马赛天文台发现的。这个星系群是所有致密星系群中研究最多的。群中最亮的成员（也是唯一的假成员）是螺旋星系NGC 7320，它有大量被确认为电离氢区的红点，在那些区域正在发生活跃的恒星形成。史蒂芬五重星系中的四个有物理上的关联性，是一个真正的星系群，称为希克斯92，未来很可能合并成一个超星系。】—摘自维基百科

    【Messier 53 (also known as M53 or NGC 5024) is a globular cluster in the Coma Berenices constellation. It was discovered by Johann Elert Bode in 1775. M53 is one of the more outlying globular clusters, being about 60,000 light-years (18.4 kpc) away from the Galactic Center, and almost the same distance (about 58,000 light-years (17.9 kpc)) from the Solar System.】

    【M53（也称为NGC 5024）是约翰·埃勒特·巴德于1775年在后发座发现的一个球状星团。M53是比较偏远的球状星团之一，距离银河中心约60,000光年（18.4千秒差距），与太阳系的距离也相似，大约是58,000光年（17.9千秒差距）。】—分别摘自维基百科英文、中文版

    【NGC 6946, also known as the Fireworks Galaxy, is an intermediate spiral galaxy in Cepheus. NGC 6946 is one of the nearest giant spiral galaxies beyond the local group. It has a high level of star formation throughout its disk in addition to a strong nuclear starburst region. NGC 6946 has a peculiar multiple arm spiral structure which coalesces into four dominant spiral arms. NGC 6946 has an unusually large halo of neutral gas that extends out of the plane of the disk, rotating at a slower velocity than the disk.】—摘自网络

    【NGC 6946，也是所知的焰火星系 (Fireworks Galaxy)，Arp 29，和 Caldwell 12"，是个距离大约一千万光年远的中间螺旋星系，位置界于仙王座和天鹅座交界处，是威廉·赫歇尔在1798年9月9日发现的。NGC 6946因为紧挨着银道面，因此受到银河系的星际物质严重的遮蔽。在NGC 6946这个星系中已经发现了10颗超新星，这使得它成为在100年内，这种类型事件最多产的已知星系。相比之下，银河系，恒星数量是NGC 6946的2倍，每个世纪却只有一颗超新星的事件。它还拥有一颗失败的超新星，形成潜在黑洞的N6946-BH1。】摘自维基百科

    【is a barred spiral galaxy located in the constellation Dorado. It was discovered by the astronomer James Dunlop in November 5, 1826. It was originally unclear whether it was a member of the Dorado Group, with some sources finding it to be a member and other sources rejecting its membership. However, recent tip of the red-giant branch (TRGB) measurements indicate that NGC 1672 is located at the same distance as other members, suggesting it is indeed a member of the Dorado Group.】—摘自维基百科

    【NGC 1672是位于剑鱼座的一个棒旋星系。它最初被认为是剑鱼座星系团的成员[2]，然而，稍后就被排除了[3]。NGC 1672有个巨大的棒，估计长达20,000秒差距。】— 摘自维基百科

【三角座星系是位于三角座，距离地球300万光年的一个螺旋星系，它被编入梅西耶33，NGC 598，M33。三角座星系继仙女座星系和银河系之后，是本星系群第三大的星系，也是长久以来以肉眼可以看见的最遥远天体。这个星系是本星系群中最小的螺旋星系，并且因为与仙女座星系的有交互作用、速度，与在夜空中互相靠近而被认为是仙女座星系的一个卫星星系。】—摘自维。基。百科

    【A panorama of the center of the Galaxy portion of the southern hemisphere Milky Way, from Crux at right to Aquila at left. Note the sweep of bright blue stars from Scorpius to Orion but angled above then across and below the Milky Way, this is Gould's Belt of new hot stars near us.】—摘自网络

    这是银河系在南半球部份的全景式图片，南十字座在右、天鹰座在左。那些从天蝎座漫延至猎户座的明亮的蓝星们，由上至下穿过银河系，就是由我们近邻的新生恒星组成的古尔德带。—若梦译介

    【古尔德带是横跨3,000光年直径，由恒星组成的星环的一部分，包含许多O型和B型的OB星恒星，从银河盘面翘起16至20°。古尔德带被怀疑是包含太阳在内的螺旋臂，太阳距离旋臂中心约325光年。估计存在的时间约3,000至5,000万年，但来源还未知，名称则得自1879年发现它的美国天文学家本杰明·阿普索普·古尔德。古尔德带包含了许多星系中的亮星包括仙王座，蝎虎座，英仙座，猎户座，座，船尾座，船帆座，船底座，南十字座，半人马座，豺狼座，天蝎座。在天空中可见的银河系也经过这些星座中的大部分，但在豺狼座的东南部。】—摘自维基百科

    【The Pleiades, also known as The Seven Sisters, Messier 45, and other names by different cultures, is an asterism and an open star cluster containing middle-aged, hot B-type stars in the north-west of the constellation Taurus. It is among the star clusters nearest to Earth, it is the nearest Messier object to Earth, and is the cluster most obvious to the naked eye in the night sky】—摘自维基百科

    【昴宿星团，简称昴星团，又称七姊妹星团，M45，是一个大而明亮的疏散星团，位于金牛座，裸眼就可以轻易看见，肉眼通常见到有九颗亮星。昴星团的视直径约2°，形成斗状。成员星数在200个以上，是一个很年轻的星团。昴星团也是一个移动星团。昴宿星团的云气是最接近地球的星云之一，并且可能是最著名的。它有时被称为玛亚女神的星云，这种错误或许是因为反射星光的云气本质上是环绕在迈亚的四周所造成的。】— 摘自维基百科

    Stars And The Milky Way — 银河系和星星

    这个没啥说明，选它纯因好看～～：）

    【Part of the M42 nebula in Orion - Space photograph of a large, bright nebula of swirling clouds dotted with stars in the constellation of Orion. The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated in the Milky Way, being south of Orion's Belt in the constellation of Orion. It is one of the brightest nebulae and is visible to the naked eye in the night sky. It is 1,344 ± 20 light-years (412.1 ± 6.1 pc) away and is the closest region of massive star formation to Earth. The M42 nebula is estimated to be 24 light-years across. It has a mass of about 2,000 times that of the Sun. Older texts frequently refer to the Orion Nebula as the Great Nebula in Orion or the Great Orion Nebula.】—摘自维基百科

    【猎户座大星云（M42，NGC 1976）是一个位于猎户座的弥漫星云，距地球1344 ± 20光年，为最接近我们的一个恒星形成区。它的亮度相当高，在全天仅次于船底座星云，在无光害的地区用肉眼就可观察。对于天文爱好者而言，M42是一个相当值得一看的深空天体：只要一枝小望远镜或双筒望远镜就可以观赏了。对于天文学家而言，这个星云是一个热门的研究对象，由大型的地基望远镜，到哈勃太空望远镜（HST）都指向它。猎户座大星云还是天文摄影爱好者和天文台的大望远镜最主要的拍摄对象之一。】—摘自维基百科

【The Orion Nebula Region - The Orion Nebula, M42 and M43, with surrounding associated nebulae and star clusters, such as the Running Man Nebula above (NGC 1975) and blue star cluster above it, NGC 1981...】—摘自网络

    【 is an emission nebula of about 125 light-years across in the Large Magellanic Cloud, a small companion galaxy to our own Milky Way which lies about 157,000 light-years away in the southern constellation of Dorado, while it is receding from us at approximately 278 kilometers per second. The nebula is surrounding an association of young stars. N44C is part of the larger N44 (LHA 120-N 44) complex, which includes young, hot, massive stars, nebulae, and a “superbubble” blown out by multiple supernova explosions. 】—摘自网络

    【N44C是个发射星云，位在我们银河系的卫星星系——大麦哲伦星云内。离明亮云气区相当远的流动五彩云气带和黝黑尘埃带，可能是更大范围的N44云气团之一部份。光大约要用上125年才能越过N44C。发出奇异的辉光，虽然看起像是造成这个发光星云的恒星，很年轻也很明亮，不过它的温度并没有高到能够产生上面影像的某些颜色。】—摘自百度百科

    【Pillars of Creation: Probably the most famous and iconic picture of the cosmos made by the Hubble Space Telescope. Pillars of Creation is a photograph taken by the Hubble Space Telescope of elephant trunks of interstellar gas and dust in the Eagle Nebula, specifically the Serpens constellation, some 6,500–7,000 light years from Earth. They are named so because the gas and dust are in the process of creating new stars, while also being eroded by the light from nearby stars that have recently formed. Taken on April 1, 1995, it was named one of the top ten photographs from Hubble. The region was rephotographed by ESA’s Herschel Space Observatory in 2011, and again by the Hubble in 2014 with a newer camera.】— 摘自ASTROGRAPHY

    【创生之柱指的是哈伯太空望远镜拍摄在鹰星云内圆柱形的星际气体和尘埃的一张影像。它是在1995年4月1日拍摄的，被Space.com评定为哈伯太空望远镜拍摄的最佳前十名的照片之一。在2015年，天文学家使用更高分辨率重新拍摄了照片。这张由32张不同影像合成的照片来自哈伯太空望远镜第二代广域和行星照相机的四架不同的相机。这张影像是由不同元素发射的光合成的，在星云中不同的元素以不同的颜色表示：绿色的是氢、单独的红色是电离的硫、蓝色是少了两个电子的氧原子。】—摘自维基百科

    【The universe is 13.7 billion years old, and the XDF reveals galaxies that span back 13.2 billion years in time. The eXtreme Deep Field, or XDF, was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field. The is an image of a small area of space in the constellation Fornax, created using Hubble Space Telescope data from 2003 and 2004. By collecting faint light over many hours of observation, it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken at that time. The new full-color XDF image reaches much fainter galaxies, and includes very deep exposures in red light from Hubble's new infrared camera, enabling new studies of the earliest galaxies in the universe. The XDF contains about 5,500 galaxies even within its smaller field of view. 】— 摘自ASTROGRAPHY

    【哈勃超深空（英文：Hubble Ultra Deep Field，HUDF）是一张外太空照片，显示的是天炉座的一小部分。该照片由哈勃空间望远镜于2003年9月24日至2004年1月16日期间得到的数据累积而成的，相当于113天的曝光。它是截至2006年为止以可见光拍摄的最深远的宇宙影象，显示的是超过130亿年前的情况。此中估计有10,000个星系。】—摘自维基百科

总算把做好的14个星空图给整理好，这项DIY完成了三分之二。还有9张图片在路上，都是尺寸稍小的，做起来会很容易，我歇一会儿～～：）

    @周一沉 2021-12-09 13:30:05
    还是花好，叶也好，草也好，嘿嘿
    -----------------------------

最后一张～～

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