| 期刊全稱 | 3-D Atlas of Stars and Galaxies | | 影響因子2023 | Richard Monkhouse,John Cox | | 視頻video | http://file.papertrans.cn/101/100631/100631.mp4 | | 發(fā)行地址 | Three-dimensional views of the known visible universe!.Three comprehensive full-sky atlases in one book - this is much more than "just" spectacular views *.The distance of any object can be measured o | | 圖書封面 |  | | 影響因子 | The 3-D Atlas of the Stars and Galaxies shows the stars and A star at twice that distance (and showing a parallax of one-half galaxies in three-dimensional space, with the third of a second of arc) is said to be at a distance of‘two parsecs‘; one dimension- distance- dire. ctly apparent to stereoscopic showing a parallax of one-tenth of a second of arc is said to be VISion. The 3-D maps- stereographs- are accurate at a distance of ten parsecs, and so on (1 pc "",3·26 Iy; 10 pc representations constructed from the most recent data available. ~32·6Iy). Because our eyes are set between two and three inches (50 to 80 The accuracy of measurements of parallax depends in part on mm) apart our stereoscopic vision extends to only a few hundred the apparent brightness of the star to be measured, but yards (metres) at most. We use other visual clues, including our ground-based photographic detection is routinely capable of experience of how large a particular object ought to appear when resolutions to plus or minus eight milliarcseconds observed over a particular range, in order to estimate the distance (8/3,600,000 of a degree). The satellite observatory Hipparcos of things that are further | | Pindex | Book 2000 |
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