...
  • 主题
高级搜索  >
历史搜索 清空历史
首页> 外文期刊>Journal of Physics & Astronomy >Moon, Super-Moon, Planets of the Solar System and Star Vega: Brightness and Size
【24h】

Moon, Super-Moon, Planets of the Solar System and Star Vega: Brightness and Size

机译：月亮，超级月亮，太阳系和维加星系：亮度和大小

获取原文
           
页面导航
  • 摘要
  • 著录项
  • 相似文献
  • 相关主题

摘要

The Moon, moonlight and phases of the Moon and its relatively simple recurring cycle have been of interest since time immemorial to human beings, navigators, astronomers and astrologers. The fact that the Moon’s orbit is close to the plane of the ecliptic and not to Earth's equatorial plane leads to new Moon to full Moon and solar and lunar eclipses also. During the phase of the full Moon, the luminous flux and its apparent size will depend on its distance from the Earth; when the full Moon is at farthest point called lunar apogee, it will be smallest full moon or micro full moon and whilst it is closest to us termed as lunar perigee will appear macro full moon-better known as super-moon, a term coined by astrologer Richard Nolle in 1979. The expressions for the lunar luminous fluxes on the Earth for the extreme positions lunar apogee and lunar perigee are derived for the first time from the students’ point of view. Furthermore, estimates for apparent magnitudes and apparent sizes of full moons corresponding to these positions are also examined. It is shown that full perigee Moon is about 29% brighter and 14% bigger than the full apogee Moon consistent with numbers available in literature. This paper will motivate the students to apply the techniques learnt here to the case of planets which are revolving around the Sun in their respective elliptical orbits having equivalent extreme positions aphelion and perihelion. In addition, students can also assess apparent magnitude of the reference star Vega.
机译：自从远古时代以来，人类，航海家，天文学家和占星家就开始关注月球，月光和月相及其相对简单的重复周期。月球的轨道靠近黄道平面，而不是地球的赤道平面，这一事实导致了新月到满月以及日食和月食。在满月阶段，光通量及其表观大小将取决于其距地球的距离。当满月位于最远的月球顶点时，它将是最小的满月或微型满月，而距我们最近的月球近地点会出现宏观的月球，被称为超级月球，这是由1979年的占星家理查德·诺尔（Richard Nolle）。这是第一次从学生的角度得出地球上月球顶点和近地点的极端位置的光通量表达式。此外，还检查了对应于这些位置的满月的视在大小和视在大小的估计。结果表明，近地点满月的亮度比近地点满月的亮度大约高29％，比前者大14％，这与文献中的数字一致。本文将激励学生将此处学到的技术应用于在各自的椭圆轨道上绕太阳旋转的行星的情况，这些椭圆轨道具有相等的极端位置阿菲尔和近日点。此外，学生还可以评估参考星Vega的视星等。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱：kefu@zhangqiaokeyan.com

京公网安备：11010802029741号 ICP备案号：京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有

  • 客服微信

  • 服务号