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相关论文: Brightness of the Qianfan Satellites

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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

Based on a large set of visual observations, the mean apparent magnitude of BlueBird satellites is 3.44, while the mean of magnitudes adjusted to a uniform distance of 1000 km is 3.84. Near zenith the spacecraft can be as bright as…

天体物理仪器与方法 · 物理学 2025-05-12 Richard E. Cole , Anthony Mallama , Scott Harrington , Jay Respler

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

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 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

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

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 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

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

Brightness statistics for satellites of the Starlink, BlueBird, Qianfan, Guowang and OneWeb constellations are reported. The means and standard deviations are compared to acceptable limits set by the International Astronomical Union's…

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

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

Observations of BlueWalker 3 (BW3) beginning on December 8 of this year indicate that its apparent brightness had decreased. We postulate that the orbital beta angle and resultant solar power considerations required an adjustment to the…

天体物理仪器与方法 · 物理学 2023-01-05 Anthony Mallama , Richard E. Cole , Scott Tilley

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

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 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 Weizmann Fast Astronomical Survey Telescope (W-FAST) is a 55cm optical survey telescope with a high cadence (25Hz) monitoring of the sky over a wide field of view (~7deg^2). The high frame rate allows detection of sub-second transients…

天体物理仪器与方法 · 物理学 2021-05-26 Guy Nir , Eran O. Ofek , Sagi Ben-Ami , Noam Segev , David Polishook , Ilan Manulis

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

The concept of a measurement of the yet unevaluated Hannay angle, by means of an Earth-bound satellite, adiabatically driven by the Moon, is shown herein. Numerical estimates are given for the angles, the orbital displacements, the…

天体物理学 · 物理学 2009-11-10 Alessandro D. A. M. Spallicci

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
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