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Context. To better understand the observed brightness of low Earth orbit satellites, we must characterize their reflectivity, which in turn depends importantly on their bus designs. The reflectivity of a body can be described by Lambert's…

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

The Steward Observatory LEO Satellite Photometric Survey is a comprehensive observational survey to characterize the apparent brightness of the Starlink and OneWeb low Earth orbit satellites and evaluate the potential impact on astronomy.…

天体物理仪器与方法 · 物理学 2023-11-27 Harrison Krantz , Eric C. Pearce , Adam Block

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

The mean apparent magnitude and the mean of magnitudes adjusted to a standard distance are reported. The illumination phase function for OneWeb satellites is determined and it differs strongly from that of VisorSat spacecraft. Brightness…

天体物理仪器与方法 · 物理学 2022-03-11 Anthony Mallama

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

The population of artificial satellites and space debris orbiting the Earth imposes non-negligible constraints on both space operations and ground-based optical and radio astronomy. The ongoing deployment of several satellite…

天体物理仪器与方法 · 物理学 2021-04-02 Miroslav Kocifaj , Frantisek Kundracik , John C. Barentine , Salvador Bará

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

Modelling techniques for the propagation of light pollution in the atmosphere allow the computation of maps of artificial night sky brightness in any direction of the sky, involving a large number of details from satellite data. Cinzano et…

天体物理仪器与方法 · 物理学 2020-07-02 Pierantonio Cinzano , Fabio Falchi

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 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

On large telescopes trails of MegaConstellation's satellites will appears significantly defocused because of their relatively short distance. Because of such effect their apparent surface brightness will be, under a range of conditions,…

天体物理仪器与方法 · 物理学 2020-10-21 Roberto Ragazzoni

We present a method to map the artificial sky brightness across large territories in astronomical photometric bands with a resolution of approximately 1 km. This is useful to quantify the situation of night sky pollution, to recognize…

天体物理学 · 物理学 2009-10-31 P. Cinzano , F. Falchi , C. D. Elvidge , K. E. Baugh

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

Over the years, the Maltese Islands have seen a marked rise in the prevalence of artificial lighting at night. The most evident type of light pollution arising from this evolution in anthropogenic night-time lighting is artificial skyglow…

天体物理仪器与方法 · 物理学 2020-02-12 Joseph Caruana , Ryan Vella , Daniel Spiteri , Michael Nolle , Sara Fenech , Noel J. Aquilina

We present a project to map the artificial sky brightness in Europe in the main astronomical photometrical bands with a resolution better than 3 km. The aim is to understand the state of night sky pollution in Europe, to quantify the…

天体物理学 · 物理学 2007-05-23 P. Cinzano , F. Falchi , C. D. Elvidge , K. E. Baugh

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

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

Modeling the brightness of satellites in large Low-Earth Orbit (LEO) constellations can not only assist the astronomical community in assessing the impact of reflected light from satellites, optimizing observing schedules and guiding data…

天体物理仪器与方法 · 物理学 2024-05-16 Yao Lu

Artificial light at night is a pollutant that is rising fast, as demonstrated by Kyba et al. (1) work by analyzing ten of thousands observations by citizen scientists in the last 12 years. The study found that the dimmest stars are…

天体物理仪器与方法 · 物理学 2023-07-03 Fabio Falchi , Salvador Bará
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