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相关论文: Brightness Characterization for Starlink Direct-to…

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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

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

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

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

Second-generation Starlink Direct-to-Cell (DTC) satellites carry an additional payload for direct cellular phone connectivity whose unintended electromagnetic radiation (UEMR) at sub-300 MHz frequencies has not been individually…

信号处理 · 电气工程与系统科学 2026-05-19 Haofan Dong , Houtianfu Wang , Hanlin Cai , Ozgur B. Akan

The mean visual magnitude of OneWeb satellites at the standard satellite distance of 1,000 km is 7.18 +/-0.03 . When this value is adjusted to the nominal 1,200 km altitude of a OneWeb satellite in orbit it corresponds to magnitude 7.58…

天体物理仪器与方法 · 物理学 2020-12-10 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

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 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 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 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

The brightness of Starlink satellites during orbit parking and orbit raising decreased significantly in 2020 when the operator modified their orientation. The mean apparent magnitude before the change was 3.90 +/- 0.18, while afterward it…

天体物理仪器与方法 · 物理学 2023-03-03 Anthony Mallama , Jay Respler

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

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

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

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

The mean apparent magnitude of Amazon Leo satellites is 6.28 based on 1,938 observations. For spacecraft in their operational mode, 92% exceeded the brightness limit recommended by the IAU for interference with research, while 25% distract…

天体物理仪器与方法 · 物理学 2026-01-13 Anthony Mallama , Richard E. Cole , Hui Zhi , Brad Young , Jay Respler , Olga Zamora , Michelle Dadighat

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

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
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