grovel 发表于 2025-3-23 09:56:57
The Galilean Moons of Jupiter,he other planets from an unfavorable perch on our own moving planet, their movements in our sky are somewhat complicated (see Chapters 7 and 8). Consequently, the brightest of Jupiter’s moons are incomparably better for demonstrating the third Keplerian law quantitatively.水汽 发表于 2025-3-23 16:48:57
The Speed and Color of Light,eous; thus when a smooth-surfaced body of water is exposed to a starlit sky, images of stars and sky immediately descend and are seen in the water. Even in Lucretius’s time, the stars were at the extreme of the heavens.急性 发表于 2025-3-23 19:37:51
http://reply.papertrans.cn/23/2235/223499/223499_13.png抵押贷款 发表于 2025-3-24 00:44:07
Mikrobiomische Selbstwirksamkeitrdless of angular diameter, takes the same length-a sidereal day-to complete. The stars also maintain the same positions relative to each other. In the past when people assumed the Earth to be motionless, the easiest way to account for such a phenomenon was to imagine that the stars were embedded on a great rotating sphere.逗留 发表于 2025-3-24 06:23:28
https://doi.org/10.1007/978-3-8350-9568-7enith. A change in the latitude of the observer will show up as a shift in the displacement of the diurnal paths of the stars in the field of view of the exposure. For a displacement of 2 mm on an exposure taken with a camera lens of 135-mm focal length, a north-south displacement of 100 km is needed.发源 发表于 2025-3-24 07:02:35
http://reply.papertrans.cn/23/2235/223499/223499_16.pngAffiliation 发表于 2025-3-24 10:50:15
https://doi.org/10.1007/978-3-642-96838-9 the sky. The looping or zigzag movement of a planet at opposition is seen to result from a combination of the planet’s orbital motion and from the parallactic shifts caused by the motion of the Earthbound viewer.违抗 发表于 2025-3-24 15:10:35
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http://reply.papertrans.cn/23/2235/223499/223499_19.pngdiskitis 发表于 2025-3-25 02:09:52
Astronomy of the Spheres,rdless of angular diameter, takes the same length-a sidereal day-to complete. The stars also maintain the same positions relative to each other. In the past when people assumed the Earth to be motionless, the easiest way to account for such a phenomenon was to imagine that the stars were embedded on a great rotating sphere.