Jul 2026· Publications of the Astronomical Society of the Pacific· Vol 138, pp. 074508· 1 citation· 50 references
Physics
Abstract
Satellite mega-constellations have overtaken the population of spacecraft since the first Starlink launch in 2019, but the regulation on mega-constellations has lagged. The brightness and quantity of mega-constellation satellites can interfere with astronomical surveys, add naked-eye visible objects to the sky, congest low-Earth orbit, and their launches add pollutants to the atmosphere. Quantitative measurements of the brightness of these mega-constellations are lacking since their high relative motion makes them challenging to track with scientific instruments. We present measurements of AST SpaceMobile’s five Block 1 BlueBird satellites: an average V magnitude of 3.9 ± 1.1, with the brightest observation reaching V magnitude 1.2 ± 0.3 and the faintest V magnitude 6.4 ± 0.3. Our measurements reveal an average brightness seven times brighter than mitigation targets cited in FCC filings and peak values over 200 times brighter than the International Astronomical Union’s recommended threshold (V magnitude 7). Now, AST SpaceMobile is expected to deploy over 200 Block 2 satellites that are each three times larger (199 m2) which would be three times brighter than Block 1 (all else being equal), and regulations have not changed. The brightness of the current mega-constellations highlights the lack of enforceable photometric standards and environmental reporting, marking a critical regulatory gap that impacts both space and ground-based astronomy.
Satellite megaconstellations in low Earth orbit interfere with ground-based optical astronomy, but the scale of that interference has been hard to measure. Here we report an uncued photometric survey from a mid-northern latitude site in late 2024 which recorded some 25,000 tracks of 5,118 individual satellites to a lim...
Jack Rayworth, D. Vida, P. Barmby et al.· 0 citations
Optical Space Domain Awareness (SDA) operations have traditionally relied on Sunlit passes near the terminator, limiting continuous tracking of low-Earth orbit (LEO) satellites. In this work, we show that by accounting for all four major illumination sources: Sunlight, Earthshine, Moonlight, and Lunar-Earthshine, large...
Sarah E. Caddy, Stephen Catsamas, Michele Trenti et al.· 0 citations
The mean apparent magnitude for BlueBird 6, the first Block 2 satellite of the BlueBird constellation, is 3.85 +/- 0.10 while that for Block 1 spacecraft is 3.30 +/- 0.07. So, BlueBird 6 is 0.55 magnitudes fainter. Likewise, the means of apparent magnitudes adjusted to a uniform distance of 1,000 km are 4.32 +/- 0.08 a...
Photometric observations of satellites, rockets and space debris brighter than magnitudes 6.0, 7.0 and 8.0 are characterized. Those magnitudes pertain to different levels of interference with astronomy as defined by the International Astronomical Union. The densities of objects per square degree of sky and brighter tha...
Anthony Mallama, S. Karpov, Richard E. Cole· 0 citations
Studies with 1-m class telescopes have now established that glints from satellites and space debris are the main obstacles to searches for sub-minute optical transients. Here, we report a study of this foreground using observations from the Legacy Survey of Space and Time (LSST) with the Simonyi 8.4-m telescope at the...
G. M. Homar, S. R. Kulkarni, C. Lage et al.· 0 citations
The detection of orbiting exoplanets by way of astrometric monitoring of the host star to reveal gravitationally induced reflex motion requires extreme precision and measurement stability when targeting Earth-mass objects. Despite this, astrometry is widely regarded as the most promising avenue for the most desired of...
P. Tuthill, George Ayad, Donald G. Dansereau et al.· Astronomical Telescopes + In...· 0 citations
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