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Magnitudes for the VisorSat and Original-design types were analyzed separately and by time. Mean values are compared with those from other large-scale photometric studies, and some signficant differences are noted. The illumination phase…

天体物理仪器与方法 · 物理学 2021-11-19 Anthony Mallama

A large dataset of visual magnitudes for all three designs of Starlink satellites is analyzed. Brightness phase functions are derived for the Original, VisorSat and Post-VisorSat models. Similarities and differences between the functions…

天体物理仪器与方法 · 物理学 2022-11-01 Anthony Mallama , Jay Respler

Visual magnitudes and sky coordinates are projected for the full constellation of Starlink satellites. The results are presented in the form of sky maps and numerical tables. Observer latitudes from the equator to 60 degrees are considered.…

天体物理仪器与方法 · 物理学 2022-09-27 Anthony Mallama

Observations of Starlink V2 Mini satellites during orbit-raising suggest that SpaceX applies brightness mitigation when they reach a height of 357 km. The mean apparent magnitudes for objects below that height threshold is 2.68 while the…

天体物理仪器与方法 · 物理学 2024-05-21 Anthony Mallama , Richard E. Cole , Jay Respler , Scott Harrington , Ron Lee , Aaron Worley

Starlink Generation 2 Mini satellites are fainter than Gen 1 spacecraft despite their larger size. The mean of apparent magnitudes for satellites in brightness mitigation mode is 7.06 +/- 0.10. When these magnitudes are adjusted to a…

天体物理仪器与方法 · 物理学 2023-06-13 Anthony Mallama , Richard E. Cole , Scott Harrington , Andreas Hornig , Jay Respler , Aaron Worley , Ron Lee

The mean of 830 visual magnitudes adjusted to a distance of 550 km (the operational altitude) is 4.63 +/-0.02. The data on DarkSat, the low-albedo satellite, indicate that it is fainter than the others by 1.6 magnitudes or 78%. However,…

地球与行星天体物理 · 物理学 2020-06-16 Anthony Mallama

The Starlink satellites are shaped like flat panels. The flat sides face zenith and nadir during normal operations. Their brightness is determined by the product of the solar illumination on the downward facing side of the panel multiplied…

天体物理仪器与方法 · 物理学 2020-03-18 Anthony Mallama

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

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

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 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 rapid increase in satellite launches in recent years, and the pressure of launches planned into the next decade, demands an improvement in the efficiency of space domain awareness facilities. Optical facilities form an important…

天体物理仪器与方法 · 物理学 2025-06-16 Sarah E. Caddy , Lee R. Spitler

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

Photometric characteristics for all models of Starlink satellites launched to date are reviewed. The Original design that lacked brightness mitigation is the most luminous. SpaceX installed a sunshade on the VisorSat model which reduced its…

天体物理仪器与方法 · 物理学 2023-10-04 Anthony Mallama , Andreas Hornig , Richard E. Cole , Scott Harrington , Jay Respler , Ron Lee , Aaron Worley

The mean of 430 visual magnitudes of VisorSats adjusted to a distance of 550-km (the operational altitude) is 5.92 +/-0.04. This is the characteristic brightness of these satellites when observed at zenith. VisorSats average 1.29 magnitudes…

天体物理仪器与方法 · 物理学 2021-01-05 Anthony Mallama

The mean apparent magnitude of Starlink Mini Direct-To-Cell (DTC) satellites observed in brightness mitigation mode is 5.16, while the mean of magnitudes adjusted to a uniform distance of 1,000 km is 6.47. The DTCs have faded since early in…

天体物理仪器与方法 · 物理学 2025-02-07 Anthony Mallama , Richard E. Cole , Jay Respler , Scott Harrington

The new Starlink V2 satellites incorporate improvements to the chassis brightness through dielectric mirrors, off-pointing solar arrays, and black paint on exposed components. For the general case in which the reflectivities are initially…

天体物理仪器与方法 · 物理学 2025-06-25 Phanindra Kandula , J. Anthony Tyson , Jacob Askari , Forrest Fankhauser

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

Starlink is a low-Earth orbit (LEO) satellite constellation operated by Space Exploration Technologies Corp. (SpaceX) which aims to provide global satellite internet access. Thus far, most photometric observations of Starlink satellites…

地球与行星天体物理 · 物理学 2022-08-08 Grace Halferty , Vishnu Reddy , Tanner Campbell , Adam Battle , Roberto Furfaro

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
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