Demonstrating Gravitational Lensing Using Solar Eclipses

Gillian Foo, Jhoon Yong Tan, E. Yuen, L. Arlany, A. Yang, S. Ng, C. Sow, A. H. Chan
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引用次数: 0

Abstract

As encouraged by the interesting paper “Solar eclipses as a teaching opportunity in relativity” by Overduin et al.,awe made measurements of the angular deflections of neighboring stars during the 9 March 2016 total solar eclipse as imaged by National University of Singapore (NUS) students, to verify a result of general relativity. In this project, we used these images and measured the stars’ pixel positions and transformed them to equatorial coordinates using a similar approach to Overduin et al., with a few modifications. Instead of solving to determine the pixel scale and rotation, we performed a plate solution using the software AstroImageJ which enables accounting for the image’s higher order distortion. This data is found in the image’s Flexible Image Transport System (FITS) header. Image star pair separations were then compared to their database separations after determining how the individual deflections affect angular separation. Our experimental results have large uncertainties and were deemed imprecise to confirm the effects of gravitational light deflection. We include a detailed analysis and discussion on this educational project.
利用日食演示引力透镜效应
受Overduin等人的有趣论文“日食作为相对论的教学机会”的鼓舞,我们测量了2016年3月9日新加坡国立大学(NUS)学生拍摄的日全食期间邻近恒星的角偏转,以验证广义相对论的结果。在这个项目中,我们使用这些图像并测量恒星的像素位置,并使用与Overduin等人类似的方法将它们转换为赤道坐标,并进行了一些修改。而不是解决确定像素尺度和旋转,我们执行了一个板解决方案,使用AstroImageJ软件,使计算图像的高阶失真。该数据在图像的灵活图像传输系统(FITS)标题中找到。然后在确定单个偏转如何影响角分离之后,将图像星对分离与数据库分离进行比较。我们的实验结果有很大的不确定性,被认为是不精确的,以确认重力光偏转的影响。我们对这个教育项目进行了详细的分析和讨论。
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CiteScore
0.60
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