Demonstrating Gravitational Lensing Using Solar Eclipses

Author:

Foo Gillian1,Tan Jhoon Yong1,Yuen Edmund1,Arlany Laurentcia1,Yang A.1,Ng S. C. Cindy1,Sow C. H.1,Chan A. H.1

Affiliation:

1. Department of Physics, Faculty of Science, National University of Singapore, Science Drive 3, Singapore 117551, Singapore

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.

Publisher

World Scientific Pub Co Pte Ltd

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