https://arxiv.org/abs/2409.20432 Skip to main content Cornell University We gratefully acknowledge support from the Simons Foundation, member institutions, and all contributors. Donate arxiv logo > astro-ph > arXiv:2409.20432 [ ] Help | Advanced Search [All fields ] Search arXiv logo Cornell University Logo [ ] GO quick links * Login * Help Pages * About Astrophysics > Instrumentation and Methods for Astrophysics arXiv:2409.20432 (astro-ph) [Submitted on 30 Sep 2024] Title:Brightness of the Qianfan Satellites Authors:Anthony Mallama, Richard E. Cole, Bram Dorreman, Scott Harrington, Nick James View a PDF of the paper titled Brightness of the Qianfan Satellites, by Anthony Mallama and 3 other authors View PDF Abstract:Observed magnitudes of Qianfan spacecraft range from 4 when they are near zenith to 8 when low in the sky. Nearly all of the observations can be modeled with a nadir-facing flat antenna panel and the underside of a zenith-facing solar array, both with Lambertian reflectance properties. These satellites will impact astronomical research unless their brightness is reduced. Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM) Cite as: arXiv:2409.20432 [astro-ph.IM] (or arXiv:2409.20432v1 [astro-ph.IM] for this version) https://doi.org/10.48550/arXiv.2409.20432 Focus to learn more arXiv-issued DOI via DataCite Submission history From: Anthony Mallama [view email] [v1] Mon, 30 Sep 2024 15:53:36 UTC (1,744 KB) Full-text links: Access Paper: View a PDF of the paper titled Brightness of the Qianfan Satellites, by Anthony Mallama and 3 other authors * View PDF * Other Formats license icon view license Current browse context: astro-ph.IM < prev | next > new | recent | 2024-09 Change to browse by: astro-ph References & Citations * NASA ADS * Google Scholar * Semantic Scholar a export BibTeX citation Loading... BibTeX formatted citation x [loading... ] Data provided by: Bookmark BibSonomy logo Reddit logo (*) Bibliographic Tools Bibliographic and Citation Tools [ ] Bibliographic Explorer Toggle Bibliographic Explorer (What is the Explorer?) [ ] Litmaps Toggle Litmaps (What is Litmaps?) [ ] scite.ai Toggle scite Smart Citations (What are Smart Citations?) ( ) Code, Data, Media Code, Data and Media Associated with this Article [ ] Links to Code Toggle CatalyzeX Code Finder for Papers (What is CatalyzeX?) [ ] DagsHub Toggle DagsHub (What is DagsHub?) [ ] GotitPub Toggle Gotit.pub (What is GotitPub?) [ ] Links to Code Toggle Papers with Code (What is Papers with Code?) [ ] ScienceCast Toggle ScienceCast (What is ScienceCast?) ( ) Demos Demos [ ] Replicate Toggle Replicate (What is Replicate?) [ ] Spaces Toggle Hugging Face Spaces (What is Spaces?) [ ] Spaces Toggle TXYZ.AI (What is TXYZ.AI?) ( ) Related Papers Recommenders and Search Tools [ ] Link to Influence Flower Influence Flower (What are Influence Flowers?) [ ] Connected Papers Toggle Connected Papers (What is Connected Papers?) [ ] Core recommender toggle CORE Recommender (What is CORE?) [ ] IArxiv recommender toggle IArxiv Recommender (What is IArxiv?) * Author * Venue * Institution * Topic ( ) About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs. Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?) * About * Help * Click here to contact arXiv Contact * Click here to subscribe Subscribe * Copyright * Privacy Policy * Web Accessibility Assistance * arXiv Operational Status Get status notifications via email or slack