2020/06/16 by Yuan-Chuan Zou, Zou, Yuan-Chuan
Engineering · Physics and Astronomy · #Adaptive optics and wavefront sensing #FOS: Physical sciences #Geophysics and Sensor Technology #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Photonic and Optical Devices
paper · pdf · doi:10.48550/arxiv.2006.08874
openalex publication_date 2020/06/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Distance measurement is crucial to astronomy. Here we suggest a new conceptual method to measure the distance by using a local instrument. By engaging the double-slit interference and by considering the phase information of the light, the position of the intensity maximum is related to the distance of the source. Consequently, the precise measurement of the position can be used to measure the distance of the remote source.