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Related papers: Multicolor and multi-spot observations of Starlink…

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We present the $g'$-, $R_{\rm c}$-, and $I_{\rm c}$-band magnitudes and associated colors of the Starlink's STARLINK-1113 (one of the standard Starlink satellites) and 1130 (Darksat) with a darkening treatment to its surface. By the 105 cm…

Instrumentation and Methods for Astrophysics · Physics 2020-12-16 Takashi Horiuchi , Hidekazu Hanayama , Masatoshi Ohishi

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…

Instrumentation and Methods for Astrophysics · Physics 2025-06-25 Phanindra Kandula , J. Anthony Tyson , Jacob Askari , Forrest Fankhauser

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…

Earth and Planetary Astrophysics · Physics 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,…

Earth and Planetary Astrophysics · Physics 2020-06-16 Anthony Mallama

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…

Instrumentation and Methods for Astrophysics · Physics 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…

Instrumentation and Methods for Astrophysics · Physics 2021-01-05 Anthony Mallama

Four observations of Starlink's LEO communication satellites, Darksat and STARLINK-1113, were conducted on two nights with two telescopes. The Chakana 0.6\,m telescope at the Ckoirama observatory (Chile) observed both satellites on…

Measure the Sloan g' magnitudes of the Starlink's STARLINK-1130 (Darksat) and 1113 LEO communication satellites and determine the effectiveness of the Darksat darkening treatment at 475.4\,nm. Two observations of the Starlink's Darksat LEO…

Instrumentation and Methods for Astrophysics · Physics 2020-05-06 J. Tregloan-Reed , A. Otarola , E. Ortiz , V. Molina , J. Anais , R. González , J. P. Colque , E. Unda-Sanzana

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…

Instrumentation and Methods for Astrophysics · Physics 2021-11-19 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…

Instrumentation and Methods for Astrophysics · Physics 2021-07-14 Richard E Cole

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…

Instrumentation and Methods for Astrophysics · Physics 2022-11-01 Anthony Mallama , Jay Respler

The development of low earth orbit (LEO) mega-constellation fundamentally threatens ground-based optical astronomical observations. To study the photometric properties of the LEO mega-constellations, we used the Xinglong 50 cm telescope to…

Instrumentation and Methods for Astrophysics · Physics 2024-03-11 Hui Zhi , Xiaojun Jiang , Jianfeng Wang

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…

Instrumentation and Methods for Astrophysics · Physics 2020-03-18 Anthony Mallama

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…

The impact of large-scale constellations of satellites, is a concern for ground-based astronomers. In recent years there has been a significant increase in the number of satellites in Low-Earth Orbit and this trend is set to continue. The…

Instrumentation and Methods for Astrophysics · Physics 2021-11-23 James Osborn , Laurence Blacketer , Matthew J. Townson , Ollie J. D. Farley

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…

Instrumentation and Methods for Astrophysics · Physics 2024-05-21 Anthony Mallama , Richard E. Cole , Jay Respler , Scott Harrington , Ron Lee , Aaron Worley

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…

Instrumentation and Methods for Astrophysics · Physics 2022-04-13 Aaron C. Boley , Ewan Wright , Samantha Lawler , Paul Hickson , Dave Balam

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…

Instrumentation and Methods for Astrophysics · Physics 2024-01-19 Olivier R. Hainaut Sabine Moehler

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…

Instrumentation and Methods for Astrophysics · Physics 2023-10-13 Forrest Fankhauser , J. Anthony Tyson , Jacob Askari

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.…

Instrumentation and Methods for Astrophysics · Physics 2023-11-27 Harrison Krantz , Eric C. Pearce , Adam Block
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