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This study evaluates the effect of proposed constellations -- ranging from current deployments to mega-constellations and very bright reflector concepts -- on direct trail losses, diffuse background, and scattered sky brightness. We use a…

天体物理仪器与方法 · 物理学 2026-04-13 Olivier R. Hainaut

We study the apparent optical brightness of satellite streaks in ground-based observatory cameras as the orbit height is varied. This is done via simulations. Several factors are in play: the range to the satellite, satellite size and…

天体物理仪器与方法 · 物理学 2025-05-13 Adam Snyder , J. Anthony Tyson

Measuring photometric brightness is a common tool for characterizaing satellites. However, characterizing satellite mega-constellations and their impact on astronomy research requires a new approach and methodology. A few measurements of…

天体物理仪器与方法 · 物理学 2021-10-22 Harrison Krantz , Eric C. Pearce , Adam Block

Megaconstellations of thousands to tens of thousands of artificial satellites (satcons) are rapidly being developed and launched. These satcons will have negative consequences for observational astronomy research, and are poised to…

地球与行星天体物理 · 物理学 2022-01-05 S. M. Lawler , A. C. Boley , H. Rein

The impact of large-scale constellations of satellites, is a concern for ground-based astronomers. In recent years there has been a significant increase in the number of satellites in Low-Earth Orbit and this trend is set to continue. The…

天体物理仪器与方法 · 物理学 2021-11-23 James Osborn , Laurence Blacketer , Matthew J. Townson , Ollie J. D. Farley

The apparent brightness of satellites is calculated as a function of satellite position as seen by a ground-based observer in darkness. Both direct illumination of the satellite by the Sun as well as indirect illumination due to reflection…

天体物理仪器与方法 · 物理学 2023-10-13 Forrest Fankhauser , J. Anthony Tyson , Jacob Askari

Starlink satellites can become extremely bright when sunlight reflects specularly to an observer on the ground. The observed brightness of such flares is consistent with a bidirectional reflectance function of the Starlink satellite…

天体物理仪器与方法 · 物理学 2024-05-24 Anthony Mallama , Richard E. Cole

A model that combines celestial geometry and atmospheric physics is used to calculate the dimming of artificial satellites as they enter and exit the Earth's shadow. Refraction of sunlight by the terrestrial atmosphere can illuminate a…

天体物理仪器与方法 · 物理学 2021-12-16 Anthony Mallama

Large constellations of artificial satellites are beginning to interfere with astronomical observing. Visual magnitude measurements of these spacecraft are useful for monitoring and characterizing their brightness. This paper describes the…

天体物理仪器与方法 · 物理学 2025-05-14 Anthony Mallama

The effect of satellite constellations on observations in the visible and IR domains is estimated, considering 18 constellations in development by SpaceX, Amazon, OneWeb, and others, with over 26,000 satellites, constituting a…

天体物理仪器与方法 · 物理学 2021-08-06 Olivier R. Hainaut , Adrew P. Williams

Artificial satellites orbiting around the Earth, under certain conditions, result to be visible even to the naked eye. The phenomenon of light pollution jeopardises the researching activities of the astronomical community: traces left by…

天体物理仪器与方法 · 物理学 2023-11-07 Gerardo Littoriano , Camilla Colombo , Alessandro Nastasi , Carmelo Falco

I discuss the current low Earth orbit artificial satellite population and show that the proposed `megaconstellation' of circa 12,000 Starlink internet satellites would dominate the lower part of Earth orbit, below 600 km, with a…

天体物理仪器与方法 · 物理学 2020-04-15 Jonathan C. McDowell

The rapid growth of satellite constellations, particularly Starlink, is increasingly affecting ground-based astronomy. In this project, we developed a workflow to detect, identify, and measure the brightness of trails from artificial…

天体物理仪器与方法 · 物理学 2026-03-12 Alexandra Serrano Mendoza , Meredith L. Rawls , Andrés Alejandro Plazas Malagón

Private space companies are increasingly commercializing near-earth space. Some estimates show that more than 100,000 satellites may orbit the Earth by 2030. This increase in the number of satellites has many consequences for science,…

物理与社会 · 物理学 2022-08-09 Sai Charan Petchetti

Radio telescopes observe extremely faint emission from astronomical objects, ranging from compact sources to large scale structures that can be seen across the whole sky. Satellites actively transmit at radio frequencies (particularly at…

天体物理仪器与方法 · 物理学 2025-04-17 M. Peel , S. Eggl , M. L. Rawls , H. Qiu , D. L. Clements

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…

天体物理仪器与方法 · 物理学 2025-05-13 Anthony Mallama , Richard E. Cole , Stephan Hellmich , Roger Spinner , Jeff Warner , Jay Respler

The number of satellites on low orbit has dramatically increased over the past years, raising concerns among the astronomical community about their impact on observations. Spectroscopic observations represent a large fraction of…

天体物理仪器与方法 · 物理学 2024-01-19 Olivier R. Hainaut Sabine Moehler

The mean apparent magnitude of Starlink Mini Direct-To-Cell (DTC) satellites is 4.62 while the mean of magnitudes adjusted to a uniform distance of 1000 km is 5.50. DTCs average 4.9 times brighter than other Starlink Mini spacecraft at a…

天体物理仪器与方法 · 物理学 2024-07-04 Anthony Mallama , Richard E. Cole , Scott Harrington , J. Respler

The impact of mega-constellations of satellites in low-Earth orbit during nighttime optical observations is assessed. Orbital geometry is used to calculate the impact of stellar occultations by satellites on the photometry of individual…

天体物理仪器与方法 · 物理学 2022-11-09 Paul J. Groot

The rapid development of mega-constellations in low Earth orbit (LEO) severely impacts ground-based optical astronomical observations. By combining WorldWide Telescope (WWT) simulations with 2019 and 2023 observational data from the…

天体物理仪器与方法 · 物理学 2026-05-19 Jing Ren , Zhou Fan , Hong-rui Gu , Qi-qian Zhang , Yun-fei Xu , Jun-ju Du , Xiao-han Chen , Lin-ying Mi , Hong Wu
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