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相关论文: Assessment of Brightness Mitigation Practices for …

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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

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 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

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

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

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

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

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

This study provides the results of simultaneous multicolor observations for the first Visorsat (STARLINK-1436) and the ordinary Starlink satellite, STARLINK-1113 in the $U$, $B$, $V$, $g'$, $r$, $i$, $R_{\rm C}$, $I_{\rm C}$, $z$, $J$, $H$,…

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

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 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

A model of the brightness of the visorsat Starlink spacecraft is presented based on published information on the engineering design and from analysis of 131 observations of individual visorsats in late 2020. Comments are offered on the…

天体物理仪器与方法 · 物理学 2021-07-14 Richard E Cole

We report studies on the mitigation of optical effects of bright low-Earth-orbit (LEO) satellites on Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST). These include options for pointing the telescope to avoid…

We present observations of 23 Starlink satellites in the $g'$ bandpass, obtained from the Dominion Astrophysical Observatory's Plaskett 1.8 metre telescope. The targets include a mixture of satellites with and without brightness mitigation…

天体物理仪器与方法 · 物理学 2022-04-13 Aaron C. Boley , Ewan Wright , Samantha Lawler , Paul Hickson , Dave Balam

SpaceX recently proposed to orbit 19,440 Starlink internet satellites at a low altitude of 350 km instead of the current 550 km. The distribution in the sky and the apparent magnitudes of these spacecraft are simulated in this paper. During…

天体物理仪器与方法 · 物理学 2024-06-25 Anthony Mallama

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 illumination phase functions for Starlink Mini satellites are determined for times of twilight and darkness. Those functions are then evaluated to give apparent magnitudes over a grid of points across the sky and over a range of solar…

天体物理仪器与方法 · 物理学 2024-01-04 Anthony Mallama , Richard E. Cole , Jay Respler , Cees Bassa , Scott Harrington , Aaron Worley

Magnitudes recorded from 2021 through 2026 for Starlink VisorSats reveal brightening of 0.6 magnitudes, while those of OneWeb show dimming of 0.4. Both trends are significant at 3 sigma. This study is based on 1.6 million magnitudes…

天体物理仪器与方法 · 物理学 2026-04-16 Anthony Mallama

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
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