Brightness Characteristics of the Qianfan Satellites and Evidence That Some Are Tumbling

Fuente: arXiv
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Autori principali: Mallama, Anthony, Cole, Richard E., Hellmich, Stephan, Spinner, Roger, Warner, Jeff, Respler, Jay
Natura: Preprint
Pubblicazione: 2025
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author Mallama, Anthony
Cole, Richard E.
Hellmich, Stephan
Spinner, Roger
Warner, Jeff
Respler, Jay
author_facet Mallama, Anthony
Cole, Richard E.
Hellmich, Stephan
Spinner, Roger
Warner, Jeff
Respler, Jay
contents The mean apparent magnitude of the Qianfan satellites is 5.76 +/- 0.04, while the mean of magnitudes adjusted to a distance of 1,000 km is 5.24 +/- 0.04, based on 1,161 observations. Light curves of several spacecraft display rapid periodic fluctuations which indicate that they are tumbling. Nearly all of the non-tumbling satellite observations can be modeled with diffusely reflecting, Earth-facing surfaces. The Qianfan constellation will impact astronomical research and aesthetic appreciation of the night sky unless their brightness is mitigated.
format Preprint
id arxiv_https___arxiv_org_abs_2505_07194
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Brightness Characteristics of the Qianfan Satellites and Evidence That Some Are Tumbling
Mallama, Anthony
Cole, Richard E.
Hellmich, Stephan
Spinner, Roger
Warner, Jeff
Respler, Jay
Instrumentation and Methods for Astrophysics
The mean apparent magnitude of the Qianfan satellites is 5.76 +/- 0.04, while the mean of magnitudes adjusted to a distance of 1,000 km is 5.24 +/- 0.04, based on 1,161 observations. Light curves of several spacecraft display rapid periodic fluctuations which indicate that they are tumbling. Nearly all of the non-tumbling satellite observations can be modeled with diffusely reflecting, Earth-facing surfaces. The Qianfan constellation will impact astronomical research and aesthetic appreciation of the night sky unless their brightness is mitigated.
title Brightness Characteristics of the Qianfan Satellites and Evidence That Some Are Tumbling
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2505.07194